20xx Vol. xx No. x, XXX 11institutetext:  National Astronomical Observatories,
Chinese Academy of Sciences, Beijing 100101, China;
22institutetext: University of Chinese Academy of Sciences, Beijing 100049,
China<EMAIL_ADDRESS>
33institutetext: Research Center for Intelligent Computing Platforms, Zhejiang
Laboratory, Hangzhou 311100, China;
44institutetext: Department of Physics and Astronomy, University of Nevada,
Las Vegas, NV 89154, USA<EMAIL_ADDRESS>
55institutetext: Nevada Center for Astrophysics, University of Nevada, Las
Vegas, NV 89154, USA;
66institutetext: CSIRO Space and Astronomy, PO Box 76, Epping, NSW 1710,
Australia;
77institutetext: Xinjiang Astronomical Observatory, Chinese Academy of
Sciences, Urumqi, Xinjiang 830011, China;
88institutetext: Kavli Institute for Astronomy and Astrophysics, Peking
University, Beijing 100871, China;
99institutetext: Department of Astronomy, Peking University, Beijing 100871,
China;
Received 20xx XXX; accepted 20xx XXX

# FAST observations of an extremely active episode of FRB 20201124A:
II. Energy Distribution

Yong-Kun Zhang 112233 Pei Wang 11 Yi Feng 33 Bing Zhang 445*5* Di Li 11223*3*
Chao-Wei Tsai 11 Chen-Hui Niu 11 Rui Luo 66 Ju-Mei Yao 77 Wei-Wei Zhu 11 J. L.
Han 1122 Ke-Jia Lee 88 De-Jiang Zhou 1122 Jia-Rui Niu 1122 Jin-Chen Jiang 88
Wei-Yang Wang 8899 Chun-Feng Zhang 88 Heng Xu 88 Bo-Jun Wang 88 Jiang-Wei Xu
88

###### Abstract

We report the properties of more than 800 bursts detected from the repeating
fast radio burst (FRB) source FRB 20201124A with the Five-hundred-meter
Aperture Spherical radio Telescope (FAST) during an extremely active episode
on UTC September 25-28, 2021 in a series of four papers. In this second paper
of the series, we study the energy distribution of 881 bursts (defined as
significant signals separated by dips down to the noise level) detected in the
first four days of our 19-hour observational campaign spanning 17 days. The
event rate initially increased exponentially but the source activity stopped
within 24 hours after the 4th day. The detection of 542 bursts in one hour
during the fourth day marked the highest event rate detected from one single
FRB source so far. The bursts have complex structures in the time-frequency
space. We find a double-peak distribution of the waiting time, which can be
modeled with two log-normal functions peaking at 51.22 ms and 10.05 s,
respectively. Compared with the emission from a previous active episode of the
source detected with FAST, the second distribution peak time is smaller,
suggesting that this peak is defined by the activity level of the source. We
calculate the isotropic energy of the bursts using both a partial bandwidth
and a full bandwidth and find that the energy distribution is not
significantly changed. We find that an exponentially connected broken-power-
law function can fit the cumulative burst energy distribution well, with the
lower and higher-energy indices being $-1.22\pm 0.01$ and $-4.27\pm 0.23$,
respectively. Assuming a radio radiative efficiency of $\eta_{r}=10^{-4}$, the
total isotropic energy of the bursts released during the four days when the
source was active is already $3.9\times 10^{46}$ erg, exceeding $\sim 23\%$ of
the available magnetar dipolar magnetic energy. This challenges the magnetar
models invoking an inefficient radio emission (e.g. synchrotron maser models).

###### keywords:

transients: fast radio bursts - stars: individual (FRB 20201124A) - methods:
data analysis

##  1 Introduction

Fast Radio Bursts (FRBs) are short-duration bright transients in radio band.
Since the first discovery (Lorimer et al. 2007), more than 600 FRB sources
have been detected (Petroff et al. 2016; CHIME/FRB Collaboration et al. 2021).
While most of the FRBs were detected once, more than 20 sources have been
observed to emit repeated bursts 111https://www.wis-tns.org/. Whether FRBs can
be divided into repeaters and non-repeaters is still an open question. The
engine to power FRB sources and the physical mechanism to generate coherent
radio emission are subject to intense study (Zhang 2020).

Emitted energy is a fundamental property of FRBs. For the FRB population, the
luminosity function is usually assumed to be a power law function with an
exponential high-energy cutoff (also called Schechter function Schechter
1976). In the literature, the power law index $\alpha$ of the Schechter
luminosity function ($dN/dL$) has been constrained by different groups using
different FRB samples (Lu & Kumar 2016, 2019; Luo et al. 2018; Bhandari et al.
2018; Macquart & Ekers 2018; Golpayegani et al. 2019; Luo et al. 2020; Zhang
et al. 2021; Hashimoto et al. 2022), with $\alpha$ constrained to the range
from -1.5 to -2.2. Lu et al. (2020) showed that an index $\sim-1.8$ can
account for FRBs down to the low-luminosity Galactic FRB 200418. The observed
FRB population is a convolution of the luminosity function and redshift
distribution. For sources in Euclidean geometry with constant space density,
the observed fluence distribution should follow a power-law distribution with
an index $-1.5$ (Vedantham et al. 2016). As cosmological sources, FRBs spatial
distribution deviates from this simple law and the unknown redshift
distribution may play a role in shaping the observed population. If the
progenitors of FRBs are young, the number density of FRBs should track the
cosmic star formation history (Madau & Dickinson 2014; Nicholl et al. 2017)
towards redshift about $z\sim 2$. Some studies have shown that the FRB samples
show the trend of deviating from the star formation history (Hashimoto et al.
2020b; Zhang et al. 2021; Arcus et al. 2021; James et al. 2022). In
particular, the CHIME first catalog sample seems to suggest a redshift
distribution that is delayed from the star formation history (Zhang & Zhang
2022; Hashimoto et al. 2022), suggesting that a good fraction of FRB
progenitors are likely old, with the number density decrease towards high
redshift. In any case, various studies showed that the derived
luminosity/energy functions are consistent with each other regardless of the
assumption of redshift distribution (Lu & Kumar 2016, 2019; Luo et al. 2018;
Bhandari et al. 2018; Macquart & Ekers 2018; Golpayegani et al. 2019; Luo et
al. 2020; Zhang et al. 2021; Zhang & Zhang 2022; Hashimoto et al. 2022).

For repeating FRBs, the energy/luminosity functions of individual sources can
been studied in great detail. Detailed studies on the two well-known sources
FRB 20121102A and FRB 20180916B suggested that they can be modeled by a power
law function with the power-law indices ranging from $-2.8$ to $-1.7$ for
bright bursts (Law et al. 2017; Wang & Zhang 2019; Gourdji et al. 2019; Cruces
et al. 2021; Aggarwal et al. 2021; CHIME/FRB Collaboration et al. 2020). These
results can imply some differences for the two kinds of FRBs in respect to
luminosity/energy functions (Hashimoto et al. 2020a). Owing to the high
sensitivity of the Five-hundred-meter Aperture Spherical radio Telescope
(FAST, Nan et al. 2011), Li et al. (2021) revealed a detailed energy function
using more than 1600 bursts for the repeater FRB 20121102A. They found that
the energy function cannot be fitted with one single power law, but requires a
two-component model to fit the data. Besides the rough power law component in
the high-energy end, there exists a log-normal low-energy component with
characteristic values at $\sim 4.8\times 10^{37}$ erg. It is unclear whether
such a feature is universal among repeaters.

FRB 20201124A was first discovered by the Canadian Hydrogen Intensity Mapping
Experiment Fast Radio Burst (CHIME/FRB) on 2020 November 24 and entered a
high-active period in March 2021 (CHIME/FRB Collabortion 2021). Hundreds of
bursts were reported during this period with a variety of radio telescopes
(Hilmarsson et al. 2021; Marthi et al. 2021; Lanman et al. 2022; Kumar et al.
2022; Law et al. 2021; Xu et al. 2021). In particular, our previous FAST
observations (Xu et al. 2021) detected 1863 bursts that revealed significant
short-term evolution of the rotation measure (RM). Multiple independent
follow-up observations with radio interferometers localized this source to a
host galaxy, which has a spectroscopic redshift of $z=0.0979$, corresponding
to a luminosity distance of $451$ Mpc with $h=0.7$, $\Omega_{\Lambda}=0.7$ and
$\Omega_{m}=0.3$ (Fong et al. 2021; Ravi et al. 2022; Piro et al. 2021a; Nimmo
et al. 2022). Follow-up observations using the Keck optical telescope revealed
that the host galaxy is a Milky-Way-like, metal rich, barred spiral galaxy
with the FRB source residing in a low stellar density, interarm region at an
intermediate galactocentric distance (Xu et al. 2021). This source also shows
its diversity in the burst properties, such as extremely high brightness and
complex structure (Kumar et al. 2022; Marthi et al. 2021), high degree of
circular polarization and variation in the polarization position angle
(Hilmarsson et al. 2021; Kumar et al. 2022; Xu et al. 2021), and obvious
scintillation (Main et al. 2021). This previous active phase lasted until the
end of May, 2021.

CHIME/FRB reported a new burst from FRB20201124A on September 21,
2021222https://www.chime-frb.ca/repeaters. Triggered by this event, we started
to use FAST to monitor this source since September 25, 2021. The observations
lasted until October 17 for a total of 17 days, leading to the detection of
more than 700 bursts during the first four days. In this paper, we mainly
focus on the energy distribution of FRB 20201124A. The morphology,
polarization and periodicity search using the same set of data are discussed
in paper I (Zhou et al. 2022), III (Jiang et al. 2022) and IV (Niu et al.
2022), respectively. Section 2 describes our observations, burst detection and
data reduction procedures. Section 3 describes the results of our analysis on
the burst energies and the energetics of this source. Section 4 discusses the
comparison of the luminosity/energy function between this source and other
sources. In Section 5, we present our conclusions.

##  2 Observations and Data Processing

The observations of FRB 20201124A were carried out with the FAST’s L-band
receiver Array of 19-beams (FLAN, Li et al. 2018; Jiang et al. 2020, covering
a frequency bandwidth of $1-1.5$ GHz, from 2021 September 25 to October 17
with a total of 19 hours of the observation time.

###  2.1 Burst Detection

The data recorded by FAST are in fits format with 4096 frequency channels and
a time resolution of 49.152 $\mu s$. We first perform de-dispersion processing
on the time-frequency data according to different DM values to construct new
time-DM data. We then use the trained object detection model to identify the
arrival time and DM of the bursts in the data. According to the DM value and
burst arrival time, the data of pulse candidates are cut from the original
data, and a binary classification neural network is used to determine whether
they are true bursts or false signals. We also searched for bursts in
dedispersed time series using a matched filtering algorithm as implemented by
the presto program (Ransom 2001). We combined the bursts detected by the two
search methods as the final sample.

###  2.2 DM Optimization

Since DM is the integral of electron density along the path, we assume that
the DM does not change significantly within an hour. We first use a uniform DM
value of $413\ \rm pc/cm^{3}$ to select the pulses detected in one day from
the data. Under 8 times down-sampling of time, bursts with a signal-to-noise
ratio greater than 10 are selected. We then change the DM trials ranging from
$-5\ \rm pc/cm^{3}$ to $5\ \rm pc/cm^{3}$ from the central value for de-
dispersion to maximize the structure of all the burst profiles, and reapply
this DM value to all bursts on this day.

###  2.3 Flux Calibration

For each burst, we estimate the peak flux density with the radiometer equation

$S_{\nu}=\frac{{\rm SNR}\times T_{sys}}{G\sqrt{n_{p}\times BW\times
t_{samp}}},$ (1)

where $T_{sys}$ is the system temperature and $G$ is the gain of the
telescope, which is modeled as a function of the zenith angle and observation
frequency in Jiang et al. (2020), $n_{p}=2$ is the number of polarization
summed, $t_{samp}$ is the sampling time, $BW$ is the used bandwidth for
calibration.

Repeating FRBs tend to have a narrow emission bandwidth compared with apparent
non-repeating events (Pleunis et al. 2021). The bandwidth may be related to
the telescope sensitivity. For these narrow-band bursts, usually the energy is
calculated using the flux density defined by the full bandwidth to be
multiplied by the full bandwidth. Alternatively, the energy can be calculated
using the flux defined with the narrow band in which the burst is detected and
multiplied by this narrow band. We roughly estimate the emission bandwidth of
each burst by dividing the whole bandpass into multiple 50-MHz sub-bands and
identifying the sub-bands containing burst emission. If the calculations are
performed correctly, the two methods should result in the same results. In
order to check this, we calculate $S_{\nu}$ using two ways. The first is to
assume that the burst energy is spread in the full bandwidth of the telescope
$BW=500\ {\rm MHz}$ for all the bursts. The second is to use the true $BW$ for
each individual burst. When different bandwidths are adopted, the noise level
and the signal-to-noise ratio of a pulse change. Therefore, when using the
observed pulse bandwidth for flux calibration, we recalculated the signal-to-
noise ratio and the $T_{sys}$ and $G$ of the corresponding frequency
bandwidth.

##  3 Results

###  3.1 Rate and Waiting Time

During the 17-day observation campaign, we detected 35, 72, 232, 542 bursts
from FRB 20201124A in the first four days (i.e. from September 25 to September
28), for a total of number of 881 bursts. The bursts are defined as
significant signals separated by dips down to the noise level in this
paper333We note that the definitions of a burst are different among the four
papers in this series, because different groups adopted different criteria for
the different scientific purposes in the respective papers.. The observation
and detection are shown in Figure 1. The cumulative distribution is plotted in
the linear-logarithmic scale. The linear line in the figure suggests that the
accumulated number increases exponentially with time. Interestingly, the
bursts suddenly disappeared in the next day, which is unexpected. The peak
burst rate on the third and fourth day reached $232/\rm hr$ and $542/\rm hr$,
respectively, which exceeded all previously reported burst rates from this and
other repeating FRBs, including $122/\rm hr$ for FRB 20121102A (Li et al.
2021), $4.5/\rm hr$ for FRB 20190520B (Niu et al. 2022), and $45.8/\rm hr$ for
FRB 20201124A itself during the previous active session (Xu et al. 2021).

Figure 1: Observation and Detection of FRB 20201124A. A: the cumulative
distribution of burst detection. B: the burst count in each observation day.
Gray bars are the observation sessions without bursts detection, the red line
shows the exponential fitting of the burst detection. C: the length of each
observation session.

Waiting time is defined as the difference between the arrival time of two
adjacent bursts. All the waiting times were calculated in the same observation
session to avoid the observation gap of about 23 hr. The waiting time
distribution of FRB 20201124A is shown in Figure 2, which can be well-fitted
by two log-normal functions peaking at $10.05$ s and $51.22$ ms, respectively.
Note that the waiting time distribution of FRB 20201124A in the previous
active period was also a bimodal distribution, but the characteristic
timescale of the second (long-duration) peak was $135$ s (Xu et al. 2021). Our
observation suggests that this characteristic waiting time is not universal
within one source, but rather depends on the activity level of the source. The
bimodal form of waiting time has also been found in FRB 20121102A (Li et al.
2021; Hewitt et al. 2022; Aggarwal et al. 2021). The timescale of the second
peak varies also significantly for telescopes with different sensitivities,
with shorter waiting times for more sensitive telescopes (which detect more
bursts).

Figure 2: Waiting time distribution of FRB 20201124A. The blue step and red
line show the distribution of waiting time and two log-normal fitting.

###  3.2 Energy calculation

We calculate the isotropic equivalent burst energy following the Equation:

$E=10^{39}{\rm erg}\frac{4\pi}{1+z}\left(\frac{D_{L}}{10^{28}{\rm
cm}}\right)^{2}\left(\frac{F_{\nu}}{\rm Jy\cdot
ms}\right)\left(\frac{\Delta\nu}{\rm GHz}\right),$ (2)

where $D_{L}=453.3{\rm Mpc}$ is the luminosity distance of FRB 20201124A
corresponding to the redshift $z=0.09795$ acquired in Xu et al. (2021),
$F_{\nu}=S_{\nu}\times W_{\rm eq}$ is the specific fluence, $S_{\nu}$ is the
peak specific flux, $\Delta\nu$ is the bandwidth of each pulse. The adoption
of $\Delta\nu$ is more relevant for narrow-band FRBs, which is typically the
case for the bursts in repeaters. As discussed in § 2.3, we adopt two choices
of $BW$ to calculate $S_{\nu}$ and compare the derived $E$ values.

Figure 3: Specific fluence and energy distribution. Energy is calculated by
Eq. 2. Solid blue lines are distribution for full bandwidth, i.e.
$\Delta\nu=500{\rm MHz}$, red dashed lines are for observed burst bandwidth.

Figure 3A shows the specific fluence ($F_{\nu}$) and the energy distribution
of bursts calculated with $\Delta\nu=500{\rm MHz}$ and the observed bandwidth
for individual bursts, respectively. The specific fluence derived using the
observed narrow bandwidth is greater than that derived assuming the full
bandwidth. This is natural because the definition of $F_{\nu}$ is the average
over frequency channels. Since the energy contained in the observed bandwidth
is similar to that in the full bandwidth but the observed bandwidth is
narrower than the full bandwidth, the average value for the full bandwidth is
smaller. Figure 3B presents the energy distribution of the two methods after
multiplying by the respective bandwidth. It can be seen that the derived
energy distributions between the two methods appear to be similar to each
other, as is expected. The p-value from the K-S test of the energy
distribution calculated with two types of bandwidth is 0.35, which cannot
reject the hypothesis that the two energy distributions are consistent with
each other. Therefore, we conclude that the energy calculation is not
significantly affected by the adoption of the bandwidth, and the normal
methods using the full bandwidth to calculate the energy is reliable.

Li et al. (2021) introduced the detection of 1652 pulses from FRB 20121102A
with FAST and proposes a bimodal energy distribution. The calculation there
following Eq. 9 from Zhang (2018), which differs from Eq. 3 by a constant
$\nu_{c}/\Delta\nu$, if we calibrate the fluence both with the full
bandwidth444The method of Zhang (2018) applies to FRBs with emission bandwidth
much wider than the telescope’s bandwidth, which seems to be the case for at
least some non-repeating FRBs.. Aggarwal (2021) claimed that he recalculated
the energy using the bandwidth in Table 1 of Li et al. (2021), and the
resulting distribution did not show a significant bimodality. As we have shown
in Figure 3A, the specific fluence varies greatly with the bandwidth
selection. The calculation in Aggarwal (2021) simply replaced the $\nu_{c}$
with the apparent observed bandwidth for individual bursts, but still used the
fluence values derived from the full bandwidth to do the calculation.
Therefore the calculations of Aggarwal (2021) resulted in incorrect results.
The bimodal energy distribution for FRB 20121102A as claimed by Li et al.
(2021) remains intact.

###  3.3 Energy Distribution

Energy/luminosity function can provide important hints on the emission
mechanism of the source. As we demonstrated in the previous subsection, the
use of limited bandwidth or full bandwidth does not change the energy
distribution. Therefore, we uniformly use Eq. 2 and the full bandwidth fluence
for energy calculation in the following analysis.

Figure 4: The energy distribution of FRB 20201124A. A: the cumulative energy
distribution of FRB 20201124A (blue) with Band function and single-power-law
function fitting. B: the index of single-power-law fitting as the function of
energy threshold. C: the energy distribution of FRB 20201124A (blue) with two
log-normal fitting.

As shown in Figure 4C, the energy distribution of FRB 20201124A also presents
a clear bimodal distribution, which can be well-fitted by two log-normal
functions peaking at $2.27\times 10^{37}$ erg and $2.28\times 10^{38}$ erg,
respectively. This may indicate the existence of more than one emission
mechanism to generate FRBs. The distribution of FRB 20121102A could be also
fitted by a similar double log-normal distribution (Extended Data Fig. 5 in Li
et al. 2021), but the peak energies is not the same for the two FRB sources.

For a power law energy/luminosity distribution $dN/dE=AE^{\alpha}$, the
cumulative energy distribution can be calculated as

$\displaystyle N(>E)$ $\displaystyle=\int_{E}^{E_{\rm max}}dN=\int_{E}^{E_{\rm
max}}AE^{\alpha}dE$ (3)
$\displaystyle=\frac{A}{-\alpha-1}\left[E^{\alpha+1}-E_{\rm
max}^{\alpha+1}\right]=\frac{A}{-\hat{\alpha}}\left[E^{\hat{\alpha}}-E_{\rm
max}^{\hat{\alpha}}\right],$

where $E_{\rm max}$ is the maximum energy for a certain sample, and
$\hat{\alpha}=\alpha+1$. One can see that in general, the cumulative energy
distribution is also roughly a power law with index $\hat{\alpha}$ is
$\hat{\alpha}<0$. Different types of astrophysical sources have different
$\hat{\alpha}$ values. For example, solar flare events have
$-0.9<\hat{\alpha}<-0.5$ (Maehara et al. 2015) and giant pulses of the Crab
pulsar have $-2.8<\hat{\alpha}<-1.1$ (Mickaliger et al. 2012; Lyu et al.
2021). Different repeating FRBs are observed to have different $\hat{\alpha}$
values: e.g. $-1.8<\hat{\alpha}<-0.7$ for FRB 20121102A (Law et al. 2017;
Cruces et al. 2021; Gourdji et al. 2019), and $\hat{\alpha}\sim-1.3$ for FRB
20180916B (CHIME/FRB Collaboration et al. 2020). For FRB 20201124A,
$\hat{\alpha}\sim-1.2$ was measured for the uGMRT bursts (Marthi et al. 2021)
and $\hat{\alpha}\sim-3.6$ was measured for the CHIME bursts (Lanman et al.
2022). A broken power-law was also used to model the cumulative energy
distribution of FRB 20121102A, the index $\hat{\alpha}=-1.4$ and
$\hat{\beta}=-1.8$ around the turning point $2.3\times 10^{37}$ erg (Hewitt et
al. 2022; Aggarwal et al. 2021). The bursts in our FAST sample also require a
two-segment power law, but the turning point is not obvious. Therefore, we
apply an exponentially connected broken-power-law function (which is called
the Band function proposed by Band et al. (1993) to describe the gamma-ray
spectra of gamma-ray bursts), which reads

$N(>E)=\left\\{\begin{aligned}
&AE^{\hat{\alpha}}\,e^{\left(-E/E_{0}\right)}\quad&E\leq(\hat{\alpha}-\hat{\beta})E_{0}\\\
&AE^{\hat{\beta}}\,\left[\frac{(\hat{\alpha}-\hat{\beta})E_{0}}{e}\right]^{\hat{\alpha}-\hat{\beta}}\quad&E\geq(\hat{\alpha}-\hat{\beta})E_{0}\\\
\end{aligned}\right.$ (4)

where $\hat{\alpha}=\alpha+1$ and $\hat{\beta}=\beta+1$ are the power-law
indices of the lower and higher cumulative energy distributions, and $E_{0}$
is a characteristic energy. Note that strictly speaking the cumulative energy
distribution of two log-normal functions should have a complicated shape. The
simple power law function is insufficient. We therefore adopt the next
simplest function, i.e. a smoothly joint two-segment broken power law function
(the Band function) to fit it. As shown in Figure 4A, this function fits the
data reasonably well. In principle, the turnover in the low-energy end of the
low-energy log-normal component would demand an additional break in the
function to fit the cumulative distribution and indeed there is a deviation at
the low-energy end between the data and fitting function. In any case, when
considering possible selection effect near the sensitivity threshold (which
would compensate the deficit of low-energy bursts from the data), we believe
that the Band function presents a reasonable description of the cumulative
distribution function.

We exclude the bursts that are below the 90% detection threshold ($E_{\rm
th}=3.6\times 10^{36}$ erg), which makes up 1% of the total sample. We then
randomly select 90% of the bursts in the sample to generate a cumulative
energy distribution. We repeat this process 1000 times and fit these 1000
cumulative energy distributions with a power-law function and the Band
function. The central limit theorem makes the fitting parameters converge to a
Gaussian distribution. We use the mean and standard deviation of the Gaussian
distribution as the standard value and error of the fitting parameters. Figure
4A shows the fitting results of the cumulative energy distribution. The power-
law index is $\hat{\alpha}=-0.08\pm 0.01$. The index values in the Band
function are $\hat{\alpha}=-0.22\pm 0.01$ and $\hat{\beta}=-3.27\pm 0.34$,
with the turning point at $(1.1\pm 0.2)\times 10^{39}$ erg. Note that the
power-law indices and the break energy are all different from those derived
from the CHIME bursts. Considering the uncertainties, the index of higher
energy end is consistent with the CHIME result.

We repeat the fitting process with a varying energy threshold. The index
$\hat{\alpha}$ of a single-power-law function does not converge to a single
value in panel B of Figure 4. This is another indication that a single power-
law distribution is inadequate to describe the cumulative energy distribution
of this FRB source.

##  4 Discussion

###  4.1 Comparison with other repeating FRBs

FRB 20121102A, FRB 20190520B and FRB 20201124A are three repeating FRBs which
have been extensively-studied by FAST. FRB 20121102A is the first known
repeating FRB (Spitler et al. 2014, 2016). FRB 20190520B is a repeating FRB
detected by Commensal Radio Astronomy FAST Survey (CRAFTS) (Li et al. 2019;
Niu et al. 2022). Both FRB 20121102A and FRB 20190520B are found to be
associated with a compact persistent radio source (PRS) (Chatterjee et al.
2017; Marcote et al. 2017; Niu et al. 2022). FRB 20201124A is also associated
with persistent radio emission, but it is not a point source and is rather
extended in space (Ravi et al. 2022; Piro et al. 2021b). The FAST-measured
energy distributions of these three FRB sources can be directly compared
against each other to reduce the possible selection biases caused by using
different telescope systems. Figure 5 shows the energy distributions of the
three FRBs in the form of both power density distribution (PDF) and cumulative
density distribution (CDF). Both the PDF and CDF show that the energy
distributions of the three FRB sources are not consistent.

Figure 5: Fluence and energy distribution of FRB 20201124A (green), FRB
20190520B (red) and FRB 20121102A (blue). A is the kernel density estimation
(KDE) of the three FRBs’ fluence. B and C are cumulative distributions and
KDEs of the three FRBs’ energy. The dashed lines are the detection thresholds.

Table 1 shows the observed isotropic radio energy and the inferred burst
energy of the three FRBs. The total observed energy $E_{\rm radio}$ is the sum
of all the observed burst energies in the radio band, which is corrected to
the total energy released during the bursts via Eq.5.

$E_{\rm bursts}=E_{\rm radio}\times F_{b}\times\eta^{-1}\times\zeta^{-1},$ (5)

where $E_{\rm bursts}$ is the total energy emitted by FRB source during
bursts, $F_{b}$ is the beaming factor, $\eta$ is the radio efficiency which is
normalized to $\sim 10^{-5}$ (similar order to FRB 20200428), and $\zeta$ is
the observation duty cycle. For example, the observations of FRB 20201124A
this time were carried out in 4 sessions in 4 days with 1 hour per session.
The duty cycle $\zeta$ is therefore estimated as $(4\times 1\ {\rm
hour})/(4\times 24\ {\rm hours})=1/24$.

Compared with other repeaters, FRB 20201124A has the largest averaged energy,
especially on September 28. Taking the nominal values of $\eta=10^{-5}$ and
$F_{b}=0.1$, the total burst energy released on September 28 has reached
$(2.46\times 10^{46}\ {\rm erg})\eta_{-5}^{-1}F_{b.-1}$. Compared with the
total dipolar magnetic energy of a magnetar $E_{\rm
mag}=(1/6)B_{p}^{2}R^{3}\sim(1.7\times 10^{47}\ {\rm
erg})B_{p,15}^{2}R_{6}^{3}$, the burst energy emitted on this day already
exceeded $14.3\%\ \eta_{-5}^{-1}F_{b,-1}$ of the available magnetar energy.
This raises an even more severe energy budget problem compared with FRB
20121102A (Li et al. 2021). This requires that the radio emission efficiency
should be quite high for the magnetar model or that the magnetar engine does
not apply. For magnetar models, since the synchrotron maser models invoking
relativistic shocks are quite inefficient, the data favors magnetospheric
models for FRBs, which can have a higher efficiency as observed in radio
pulsars (Kumar et al. 2017; Yang & Zhang 2018; Lu et al. 2020; Zhang 2022).
The synchrotron maser model may be still relevant if the central engine is not
a magnetar, but rather an accreting black hole system (e.g. Sridhar et al.
2021), whose total energy budget is not limited by the total magnetic energy
of a magnetar.

Table 1: Energy budget of three repeating FRBs.

Name | ObDays | ObTimes |  Total Observed Energya |  Averaged Energyb |  Total Energyc
---|---|---|---|---|---
| (day) |  $T_{\rm obs}$ (hour) |  $E_{\rm radio}$ (erg) |  $\bar{L}_{\rm radio}$ (erg/s) |  $E_{\rm bursts}$ (erg)
FRB 20201124A | 4 | 4 | $1.60\times 10^{41}$ | $1.11\times 10^{37}$ | $3.85\times 10^{46}$
FRB 20201124A-0928 | 1 | 1 | $1.02\times 10^{41}$ | $2.84\times 10^{37}$ | $2.46\times 10^{46}$
FRB 20121102A | 47 | 59.5 | $3.41\times 10^{41}$ | $1.59\times 10^{36}$ | $6.47\times 10^{46}$
FRB 20190520B | 11 | 18.5 | $1.10\times 10^{40}$ | $1.65\times 10^{35}$ | $1.56\times 10^{45}$

  * a

Sum of the observed isotropic radio energies of all bursts.

  * b

Defined as $\rm E_{\rm radio}/T_{\rm obs}$

  * c

$E_{\rm bursts}=E_{\rm radio}\times\left[(\zeta={\rm
ObTimes/ObDays})^{-1}\times(\eta=10^{-5})^{-1}\times(F_{b}=0.1)\right]$

###  4.2 Comparison of different burst definition schemes

To quantify the specific morphological characteristics of the bursts, we
differentiate two kinds of pulse profile classification schemes. The first
classification scheme is based on a judgment of pulse flux threshold, taking
the pulse profile above the detection threshold as a separated burst. For
conservative considerations, we take the detection threshold using a 3$\sigma$
noise level of the baseline due to the complicated effect on the actual
sensitivity, e.g., the bandwidth limited structure of the bursts and radio
frequency interference (RFI) events. This definition is also the pulse
definition used in previous work, and is the same as the definition used for
FRB 20121102A (Li et al. 2021) and FRB 20190520B (Niu et al. 2022). In the
following text, we call this definition Combined Bursts Definition (CBD).

Figure 6: A burst event example detected on September 26.

For another method, we try to differentiate the bursts by referring to the
morphological clustering characteristics of the pulses in the dynamic
spectrum, which means that pulses that can be distinguished in the time-
frequency diagram are treated as different bursts, like Figure 6. We call this
definition Separated Bursts Definition (SBD). As a result, the event in Figure
6 contains 2 bursts under SBD but 1 burst under CBD. All bursts under SBD are
artificially isolated and flux calibration is performed independently.

Figure 7: A: Waiting time distribution of the bursts from FRB 20201124A with
SBD. The red line shows the log-normal fitting. B: Specific fluence
distribution of bursts with CBD (blue solid line) and SBD (blue dashed line).
C: Energy distribution of bursts with CBD and SBD. D: Cumulative energy
distribution of bursts with CBD and SBD with Band function fitting (red line).

Figure 7A shows the waiting time distribution of bursts with SBD, which is
still a bi-modal distribution and can be modeled with two log-normal functions
peaking at $13.56$ ms and $10.05$ s, respectively. The second peak time around
10 s is consistent with the waiting time distribution of CBD. However, the
first peak time is significantly reduced. The distributions of specific
fluence and energy exhibit distinct distributions under the two burst
definitions. We use the K-S test to check whether the energies calculated from
the two burst definition schemes belong to the same distribution. The p-value
is 0.2%, meaning we could rule out the hypothesis that they were from the same
distribution. We also use the Band function to fit the cumulative energy
distribution of the bursts with SBD. The index values in the Band function are
$\hat{\alpha}=-0.18\pm 0.01$ and $\hat{\beta}=-3.27\pm 0.16$, respectively.
The index in the high energy regime is the same with CBD, while the index in
the lower energy regime is slightly smaller than that of CBD. The turning
point is $(6.4\pm 0.1)\times 10^{38}$ erg, which is smaller than that for CBD.
While we still do not know the true nature of FRBs, different definitions of
bursts may lead to somewhat different analysis results. We caution that when
studying burst energy distributions of FRBs, one needs to specify a burst
definition scheme.

##  5 Conclusions

FRB 20201124A is a repeating FRB discovered by CHIME (CHIME/FRB Collabortion
2021). FAST has monitored source multiple times. Besides an earlier
observational campaign reported by Xu et al. (2021), we study a very active
4-day emitting episode on September 25-28, 2021, in this series of papers. The
main results of this paper are as follows.

  * 1)

Using our CBD definition method, a total of 881 bursts were detected between
September 25 to September 28.

  * 2)

The apparent event rate increased exponentially in 4 days and then dropped to
zero after Sep. 29.

  * 3)

The waiting time of FRB 20201124A shows a bimodal structure, which can be
well-fitted by two log-normal functions. The longer waiting times peak around
10 s and is insensitive to the burst definition criterion. It is much shorter
than that of the previous epoch (Xu et al. 2021), suggesting that it is
related to the active level of the source.

  * 4)

The shorter waiting times peak around either 51 ms or 14 ms, depending on the
definition of burst separation (see Section 3).

  * 5)

The peak event rate of 542/hr exceeds all the detected FRBs in the past,
including 122/hr of FRB 20121102A (Li et al. 2021), and FRB 20201124A itself,
which was 45.8/hr during the last active period (Xu et al. 2021). The total
burst energy released during this epoch is a significant fraction of magnetar
total energy unless the radio emission frequency is high. This challenges the
synchrotron maser mechanism for FRBs and even the magnetar source model.

  * 6)

The energy distribution cannot be described by a single power-law. The
cumulative distribution of energy can be well modeled by an exponentially
connected broken power law known as the Band function. The slopes at low and
high energy regimes are $\hat{\alpha}=-0.22\pm 0.01$ and $\hat{\beta}=-3.27\pm
0.23$, respectively.

  * 7)

The energy distributions of three active repeating FRBs, namely FRB 20121102A,
FBR 20190520B, and FRB 20201124A, do not appear to be identical. This suggests
that repeating FRBs may have diverse emission properties.

###### Acknowledgements.

This work made use of the data from FAST, a Chinese national mega-science
facility, operated by National Astronomical Observatories, Chinese Academy of
Sciences. This work supported by the Open Project Program of the Key
Laboratory of FAST, Chinese Academy of Sciences. We acknowledge use of the
CHIME/FRB Public Database, provided at https://www.chime-frb.ca/ by the
CHIME/FRB Collaboration. P. W. acknowledges support from the National Natural
Science Foundation of China under grant U2031117, the Youth Innovation
Promotion Association CAS (id. 2021055), CAS Project for Young Scientists in
Basic Reasearch (grant YSBR-006) and the Cultivation Project for FAST
Scientific Payoff and Research Achievement of CAMS-CAS. Y. Feng is supported
by the Key Research Project of Zhejiang Lab no. 2021PE0AC0. J. L. Han is
supported by the National Natural Science Foundation of China (NSFC, Nos.
11988101 and 11833009) and the Key Research Program of the Chinese Academy of
Sciences (Grant No. QYZDJ-SSW-SLH021); D. J. Zhou is supported by the
Cultivation Project for the FAST scientific Payoff and Research Achievement of
CAMS-CAS. K.J. Lee, J.C. Jiang, H. Xu, and J.W. Xu are supported by National
SKA Program of China 2020SKA0120200, National Nature Science Foundation grant
No. 12041303, the CAS-MPG LEGACY project, and funding from the Max-Planck
Partner Group.

## Author Contributions

Y.K.Z., P.W., D.L., and B.Z. developed the concept of the manuscript. B.Z. and
W.W.Z. proposed and chaired the FAST FRB key science project. Y.K.Z. conducted
the data analysis and visualization. Y.K.Z., P.W., and C.H.N. searched the
bursts and analyzed the burst properties. Y.K.Z., Y.F., D.L., B.Z., C.W.T.,
and R.L. led the discussion on the interpretation of the results and writing
of the manuscript. D.J.Z. studied bursts morphology and classification with
the details presented in paper I of this series. J.C.J performed the analysis
of the polarization properties and the results are presented in the Paper III.
J.R.N. performed periodicity search with the results presented in paper IV.
All authors contributed to the analysis or interpretation of the data and to
the final version of the manuscript.

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##  Appendix A Bursts Properties

At 1.5 GHz

Equivalent width

Energy calculated with center frequency.

Energy calculated with band width.

Table 2: The properties of the FRB 20201124A bursts Burst ID | ObsDate |  MJDa | DM |  Widthb | PeakFlux | Fluence |  Energycc |  Energywd | BandWidth |  Widthb | PeakFlux | Fluence |  Energywc
---|---|---|---|---|---|---|---|---|---|---|---|---|---
|  | Barycentric |  | Full Band | Full Band | Full Band | Full Band | Full Band |  | Limited Band | Limited Band | Limited Band | Limited Band
|  |  |  (pc cm-3) | (ms) | (mJy) | (Jy ms) | (erg) | (erg) | (MHz) | (ms) | (mJy) | (Jy ms) | (erg)
|  |  |  |  |  |  |  |  |  |  |  |  |
B001 | 20210925 | 59482.944514719 | 412.97 | 3.31 |  12.39$\pm$0.26 |  0.04$\pm$0.86 | 1.148(1)e+37 | 4.590(1)e+36 | 200 | 3.81 |  22.50$\pm$0.74 |  0.09$\pm$0.01 | 4.210(45)e+36
B002 | 20210925 | 59482.946731974 | 412.97 | 3.78 |  28.61$\pm$0.05 |  0.11$\pm$0.2 | 3.023(28)e+37 | 1.209(11)e+37 | 150 | 3.55 |  79.38$\pm$0.36 |  0.28$\pm$0.01 | 1.038(10)e+37
B003 | 20210925 | 59482.947007613 | 412.97 | 4.34 |  5.99$\pm$0.07 |  0.03$\pm$0.29 | 7.278(1)e+36 | 2.911(1)e+36 | 50 | 5.18 |  32.52$\pm$0.22 |  0.17$\pm$0.01 | 2.071(22)e+36
B004 | 20210925 | 59482.947121260 | 412.97 | 2.70 |  7.41$\pm$0.09 |  0.02$\pm$0.24 | 5.598(1)e+36 | 2.239(1)e+36 | 100 | 3.54 |  20.05$\pm$0.42 |  0.07$\pm$0.01 | 1.747(22)e+36
B005 | 20210925 | 59482.947355910 | 412.97 | 4.47 |  9.61$\pm$0.1 |  0.04$\pm$0.45 | 1.204(1)e+37 | 4.814(1)e+36 | 100 | 4.00 |  38.02$\pm$0.22 |  0.15$\pm$0.01 | 3.740(45)e+36
B006 | 20210925 | 59482.947576756 | 412.97 | 2.85 |  10.89$\pm$1.93 |  0.03$\pm$5.49 | 8.677(1)e+36 | 3.471(1)e+36 | 150 | 3.17 |  22.96$\pm$4.26 |  0.07$\pm$0.01 | 2.687(34)e+36
B007 | 20210925 | 59482.947690227 | 412.97 | 8.46 |  211.11$\pm$1.1 |  1.79$\pm$9.33 | 5.002(45)e+38 | 2.001(18)e+38 | 300 | 7.82 |  462.35$\pm$2.39 |  3.62$\pm$0.03 | 2.668(25)e+38
B008 | 20210925 | 59482.950048429 | 412.97 | 5.77 |  68.47$\pm$0.64 |  0.40$\pm$3.7 | 1.106(11)e+38 | 4.422(45)e+37 | 450 | 5.26 |  75.19$\pm$0.71 |  0.40$\pm$0.01 | 4.373(40)e+37
B009 | 20210925 | 59482.952261654 | 412.97 | 4.83 |  29.58$\pm$0.28 |  0.14$\pm$1.37 | 4.003(28)e+37 | 1.601(11)e+37 | 200 | 4.79 |  67.06$\pm$0.66 |  0.32$\pm$0.01 | 1.581(13)e+37
B010 | 20210925 | 59482.953261568 | 412.97 | 5.96 |  38.59$\pm$0.37 |  0.23$\pm$2.22 | 6.438(56)e+37 | 2.575(22)e+37 | 150 | 5.30 |  104.79$\pm$1.05 |  0.56$\pm$0.01 | 2.049(20)e+37
B011 | 20210925 | 59482.953261777 | 412.97 | 5.88 |  62.74$\pm$0.56 |  0.37$\pm$3.29 | 1.033(8)e+38 | 4.131(34)e+37 | 350 | 4.09 |  123.75$\pm$1.18 |  0.51$\pm$0.01 | 4.360(40)e+37
B012 | 20210925 | 59482.953545641 | 412.97 | 4.81 |  6.24$\pm$0.61 |  0.03$\pm$2.92 | 8.397(1)e+36 | 3.359(1)e+36 | 100 | 2.97 |  31.24$\pm$0.87 |  0.09$\pm$0.01 | 2.284(22)e+36
B013 | 20210925 | 59482.953787567 | 412.97 | 3.12 |  6.40$\pm$0.06 |  0.02$\pm$0.19 | 5.598(1)e+36 | 2.239(1)e+36 | 100 | 1.73 |  26.89$\pm$0.37 |  0.05$\pm$0.01 | 1.142(22)e+36
B014 | 20210925 | 59482.955691648 | 412.97 | 3.71 |  30.70$\pm$0.06 |  0.11$\pm$0.23 | 3.191(28)e+37 | 1.276(11)e+37 | 300 | 3.42 |  49.57$\pm$0.32 |  0.17$\pm$0.01 | 1.249(13)e+37
B015 | 20210925 | 59482.959269256 | 412.97 | 6.77 |  227.02$\pm$0.3 |  1.54$\pm$2.06 | 4.302(45)e+38 | 1.721(18)e+38 | 400 | 6.10 |  290.64$\pm$0.5 |  1.77$\pm$0.02 | 1.744(18)e+38
B016 | 20210925 | 59482.961554168 | 412.97 | 14.39 |  375.59$\pm$2.33 |  5.40$\pm$33.52 | 1.512(16)e+39 | 6.049(64)e+38 | 350 | 12.42 |  584.60$\pm$2.99 |  7.26$\pm$0.08 | 6.249(66)e+38
B017 | 20210925 | 59482.961568878 | 412.97 | 2.70 |  8.13$\pm$3.83 |  0.02$\pm$10.35 | 6.158(1)e+36 | 2.463(1)e+36 | 150 | 2.82 |  22.93$\pm$6.0 |  0.06$\pm$0.01 | 2.385(34)e+36
B018 | 20210925 | 59482.962379029 | 412.97 | 8.69 |  14.73$\pm$3.94 |  0.13$\pm$34.27 | 3.583(28)e+37 | 1.433(11)e+37 | 250 | 7.76 |  28.63$\pm$5.76 |  0.22$\pm$0.01 | 1.366(17)e+37
B019 | 20210925 | 59482.963114767 | 412.97 | 6.23 |  10.11$\pm$2.38 |  0.06$\pm$14.81 | 1.763(28)e+37 | 7.054(112)e+36 | 150 | 5.42 |  26.20$\pm$3.85 |  0.14$\pm$0.01 | 5.240(67)e+36
B020 | 20210925 | 59482.965566529 | 412.97 | 3.83 |  113.65$\pm$0.08 |  0.44$\pm$0.33 | 1.218(14)e+38 | 4.870(56)e+37 | 200 | 3.40 |  269.33$\pm$0.25 |  0.92$\pm$0.01 | 4.501(49)e+37
B021 | 20210925 | 59482.965939315 | 412.97 | 6.92 |  8.82$\pm$0.16 |  0.06$\pm$1.07 | 1.707(28)e+37 | 6.830(112)e+36 | 200 | 7.26 |  15.43$\pm$0.31 |  0.11$\pm$0.01 | 5.508(45)e+36
B022 | 20210925 | 59482.965939574 | 412.97 | 9.44 |  193.32$\pm$0.11 |  1.82$\pm$1.01 | 5.108(56)e+38 | 2.043(22)e+38 | 400 | 8.71 |  248.37$\pm$0.29 |  2.16$\pm$0.02 | 2.126(23)e+38
B023 | 20210925 | 59482.966453859 | 412.97 | 3.25 |  6.47$\pm$1.23 |  0.02$\pm$4.0 | 5.878(1)e+36 | 2.351(1)e+36 | 150 | 2.82 |  19.06$\pm$3.01 |  0.05$\pm$0.01 | 1.982(34)e+36
B024 | 20210925 | 59482.966454059 | 412.97 | 3.48 |  8.34$\pm$0.1 |  0.03$\pm$0.33 | 8.117(1)e+36 | 3.247(1)e+36 | 150 | 4.70 |  17.84$\pm$0.16 |  0.08$\pm$0.01 | 3.090(34)e+36
B025 | 20210925 | 59482.967833165 | 412.97 | 6.66 |  10.06$\pm$2.11 |  0.07$\pm$14.04 | 1.875(28)e+37 | 7.501(112)e+36 | 150 | 5.00 |  25.15$\pm$2.72 |  0.13$\pm$0.01 | 4.635(67)e+36
B026 | 20210925 | 59482.973830260 | 412.97 | 5.60 |  189.00$\pm$0.07 |  1.06$\pm$0.4 | 2.961(34)e+38 | 1.184(13)e+38 | 400 | 5.11 |  238.46$\pm$0.21 |  1.22$\pm$0.01 | 1.198(14)e+38
B027 | 20210925 | 59482.974318269 | 412.97 | 6.53 |  112.95$\pm$0.09 |  0.74$\pm$0.59 | 2.066(25)e+38 | 8.263(101)e+37 | 450 | 3.83 |  191.88$\pm$0.2 |  0.73$\pm$0.01 | 8.125(87)e+37
B028 | 20210925 | 59482.974319569 | 412.97 | 4.60 |  15.01$\pm$0.11 |  0.07$\pm$0.51 | 1.931(28)e+37 | 7.725(112)e+36 | 350 | 4.26 |  20.31$\pm$0.29 |  0.09$\pm$0.01 | 7.445(78)e+36
B029 | 20210925 | 59482.978616609 | 412.97 | 3.44 |  9.60$\pm$2.2 |  0.03$\pm$7.58 | 9.237(1)e+36 | 3.695(1)e+36 | 250 | 2.57 |  17.71$\pm$2.78 |  0.05$\pm$0.01 | 2.799(56)e+36
B030 | 20210925 | 59482.978819236 | 412.97 | 3.79 |  7.13$\pm$1.32 |  0.03$\pm$4.99 | 7.557(1)e+36 | 3.023(1)e+36 | 100 | 7.42 |  24.32$\pm$2.19 |  0.18$\pm$0.01 | 4.434(67)e+36
B031 | 20210925 | 59482.980459129 | 412.97 | 9.60 |  382.98$\pm$0.99 |  3.68$\pm$9.54 | 1.029(13)e+39 | 4.118(50)e+38 | 350 | 8.41 |  648.75$\pm$1.05 |  5.45$\pm$0.07 | 4.694(57)e+38
B032 | 20210925 | 59482.980459629 | 412.97 | 7.48 |  41.30$\pm$0.18 |  0.31$\pm$1.31 | 8.649(112)e+37 | 3.460(45)e+37 | 200 | 6.33 |  81.25$\pm$0.24 |  0.51$\pm$0.01 | 2.530(31)e+37
B033 | 20210925 | 59482.981124866 | 412.97 | 4.42 |  12.67$\pm$0.12 |  0.06$\pm$0.51 | 1.567(28)e+37 | 6.270(112)e+36 | 200 | 4.92 |  27.04$\pm$0.22 |  0.13$\pm$0.01 | 6.538(90)e+36
B034 | 20210925 | 59482.981353739 | 412.97 | 5.51 |  33.00$\pm$0.09 |  0.18$\pm$0.47 | 5.094(56)e+37 | 2.038(22)e+37 | 400 | 5.23 |  39.85$\pm$0.36 |  0.21$\pm$0.01 | 2.051(27)e+37
B035 | 20210925 | 59482.982836085 | 412.97 | 5.53 |  11.04$\pm$0.86 |  0.06$\pm$4.77 | 1.707(28)e+37 | 6.830(112)e+36 | 100 | 5.30 |  43.64$\pm$1.44 |  0.23$\pm$0.01 | 5.688(90)e+36
B036 | 20210926 | 59483.864686554 | 412.18 | 8.68 |  43.66$\pm$4.69 |  0.38$\pm$40.72 | 1.061(8)e+38 | 4.243(34)e+37 | 300 | 4.25 |  126.74$\pm$7.79 |  0.54$\pm$0.01 | 3.974(34)e+37
B037 | 20210926 | 59483.865235197 | 412.18 | 3.18 |  7.24$\pm$0.89 |  0.02$\pm$2.83 | 6.438(1)e+36 | 2.575(1)e+36 | 50 | 3.48 |  29.35$\pm$1.18 |  0.10$\pm$0.01 | 1.254(11)e+36
B038 | 20210926 | 59483.866094138 | 412.18 | 5.09 |  42.79$\pm$0.51 |  0.22$\pm$2.58 | 6.102(56)e+37 | 2.441(22)e+37 | 300 | 4.30 |  74.26$\pm$1.02 |  0.32$\pm$0.01 | 2.358(20)e+37
B039 | 20210926 | 59483.866095148 | 412.18 | 3.39 |  10.62$\pm$0.16 |  0.04$\pm$0.53 | 1.008(1)e+37 | 4.031(1)e+36 | 100 | 3.16 |  42.64$\pm$0.34 |  0.13$\pm$0.01 | 3.314(45)e+36
B040 | 20210926 | 59483.866310688 | 412.18 | 7.29 |  103.89$\pm$0.41 |  0.76$\pm$2.97 | 2.119(20)e+38 | 8.476(78)e+37 | 250 | 6.75 |  209.03$\pm$0.49 |  1.41$\pm$0.01 | 8.671(73)e+37
B041 | 20210926 | 59483.866348127 | 412.18 | 6.89 |  311.66$\pm$0.14 |  2.15$\pm$0.95 | 6.010(53)e+38 | 2.404(21)e+38 | 350 | 4.03 |  660.19$\pm$0.66 |  2.66$\pm$0.02 | 2.290(19)e+38
B042 | 20210926 | 59483.866349010 | 412.18 | 3.94 |  8.63$\pm$0.38 |  0.03$\pm$1.5 | 9.517(1)e+36 | 3.807(1)e+36 | 100 | 3.67 |  23.33$\pm$1.14 |  0.09$\pm$0.01 | 2.105(22)e+36
B043 | 20210926 | 59483.866349538 | 412.18 | 11.01 |  153.91$\pm$0.14 |  1.69$\pm$1.5 | 4.742(39)e+38 | 1.897(16)e+38 | 300 | 9.72 |  290.28$\pm$0.26 |  2.82$\pm$0.02 | 2.081(18)e+38
B044 | 20210926 | 59483.867032708 | 412.18 | 5.18 |  81.11$\pm$0.06 |  0.42$\pm$0.33 | 1.176(11)e+38 | 4.702(45)e+37 | 400 | 4.62 |  99.88$\pm$0.31 |  0.46$\pm$0.01 | 4.541(36)e+37
B045 | 20210926 | 59483.867435873 | 412.18 | 4.14 |  32.59$\pm$0.37 |  0.14$\pm$1.52 | 3.779(28)e+37 | 1.511(11)e+37 | 400 | 3.56 |  36.80$\pm$0.64 |  0.13$\pm$0.01 | 1.290(9)e+37
B046 | 20210926 | 59483.869077769 | 412.18 | 3.26 |  57.72$\pm$0.09 |  0.19$\pm$0.3 | 5.262(56)e+37 | 2.105(22)e+37 | 200 | 2.87 |  144.04$\pm$0.45 |  0.41$\pm$0.01 | 2.033(18)e+37
B047 | 20210926 | 59483.869521302 | 412.18 | 1.27 |  9.46$\pm$0.89 |  0.01$\pm$1.13 | 3.359(1)e+36 | 1.344(1)e+36 | 100 | 2.27 |  26.86$\pm$1.82 |  0.06$\pm$0.01 | 1.500(22)e+36
B048 | 20210926 | 59483.870084040 | 412.18 | 6.93 |  35.50$\pm$2.68 |  0.25$\pm$18.58 | 6.886(56)e+37 | 2.754(22)e+37 | 450 | 6.10 |  38.53$\pm$5.54 |  0.23$\pm$0.01 | 2.600(20)e+37
B049 | 20210926 | 59483.870098317 | 412.18 | 7.09 |  207.31$\pm$1.91 |  1.47$\pm$13.52 | 4.114(34)e+38 | 1.646(13)e+38 | 450 | 6.40 |  225.77$\pm$2.8 |  1.45$\pm$0.01 | 1.599(13)e+38
B050 | 20210926 | 59483.870919457 | 412.18 | 7.81 |  119.66$\pm$0.19 |  0.93$\pm$1.46 | 2.614(22)e+38 | 1.046(9)e+38 | 200 | 7.45 |  286.00$\pm$0.36 |  2.13$\pm$0.02 | 1.047(9)e+38
B051 | 20210926 | 59483.870941448 | 412.18 | 4.15 |  55.48$\pm$0.07 |  0.23$\pm$0.31 | 6.438(56)e+37 | 2.575(22)e+37 | 200 | 4.02 |  125.82$\pm$0.25 |  0.51$\pm$0.01 | 2.490(22)e+37
B052 | 20210926 | 59483.871067702 | 412.18 | 3.35 |  4.48$\pm$0.24 |  0.02$\pm$0.79 | 4.198(1)e+36 | 1.679(1)e+36 | 50 | 5.92 |  27.06$\pm$0.57 |  0.16$\pm$0.01 | 1.970(22)e+36
B053 | 20210926 | 59483.871607732 | 412.18 | 5.16 |  6.78$\pm$1.32 |  0.04$\pm$6.84 | 9.797(1)e+36 | 3.919(1)e+36 | 100 | 3.97 |  18.36$\pm$2.52 |  0.07$\pm$0.01 | 1.791(22)e+36
B054 | 20210926 | 59483.871783389 | 412.18 | 3.17 |  41.90$\pm$1.0 |  0.13$\pm$3.17 | 3.723(28)e+37 | 1.489(11)e+37 | 250 | 3.06 |  78.38$\pm$2.07 |  0.24$\pm$0.01 | 1.472(11)e+37
B055 | 20210926 | 59483.871783684 | 412.18 | 5.18 |  11.39$\pm$0.69 |  0.06$\pm$3.59 | 1.651(1)e+37 | 6.606(1)e+36 | 200 | 4.18 |  27.69$\pm$0.85 |  0.12$\pm$0.01 | 5.688(45)e+36
B056 | 20210926 | 59483.872236820 | 412.18 | 5.57 |  120.14$\pm$0.21 |  0.67$\pm$1.16 | 1.872(14)e+38 | 7.490(56)e+37 | 350 | 5.16 |  180.32$\pm$0.52 |  0.93$\pm$0.01 | 8.002(63)e+37
B057 | 20210926 | 59483.872543849 | 412.18 | 4.14 |  11.58$\pm$0.28 |  0.05$\pm$1.14 | 1.344(1)e+37 | 5.374(1)e+36 | 100 | 4.64 |  47.73$\pm$0.31 |  0.22$\pm$0.01 | 5.441(45)e+36
B058 | 20210926 | 59483.872931633 | 412.18 | 4.13 |  36.57$\pm$0.48 |  0.15$\pm$1.98 | 4.226(28)e+37 | 1.691(11)e+37 | 300 | 3.74 |  71.89$\pm$1.23 |  0.27$\pm$0.01 | 1.982(13)e+37
B059 | 20210926 | 59483.874111422 | 412.18 | 4.18 |  9.80$\pm$0.08 |  0.04$\pm$0.33 | 1.148(1)e+37 | 4.590(1)e+36 | 150 | 2.80 |  26.66$\pm$0.27 |  0.07$\pm$0.01 | 2.754(34)e+36
B060 | 20210926 | 59483.874111868 | 412.18 | 4.91 |  21.39$\pm$0.29 |  0.10$\pm$1.44 | 2.939(28)e+37 | 1.176(11)e+37 | 100 | 4.17 |  87.31$\pm$0.32 |  0.36$\pm$0.01 | 8.957(90)e+36
B061 | 20210926 | 59483.874349238 | 412.18 | 5.42 |  10.52$\pm$1.71 |  0.06$\pm$9.26 | 1.595(1)e+37 | 6.382(1)e+36 | 250 | 4.03 |  14.93$\pm$1.86 |  0.06$\pm$0.01 | 3.695(56)e+36
B062 | 20210926 | 59483.874349725 | 412.18 | 3.34 |  20.06$\pm$0.97 |  0.07$\pm$3.25 | 1.875(28)e+37 | 7.501(112)e+36 | 250 | 3.49 |  37.10$\pm$2.4 |  0.13$\pm$0.01 | 7.949(56)e+36
B063 | 20210926 | 59483.875056675 | 412.18 | 4.91 |  64.17$\pm$0.35 |  0.32$\pm$1.7 | 8.817(56)e+37 | 3.527(22)e+37 | 200 | 4.54 |  151.23$\pm$2.23 |  0.69$\pm$0.01 | 3.372(27)e+37
B064 | 20210926 | 59483.875057431 | 412.18 | 3.66 |  9.83$\pm$0.09 |  0.04$\pm$0.31 | 1.008(1)e+37 | 4.031(1)e+36 | 100 | 4.07 |  40.94$\pm$0.37 |  0.17$\pm$0.01 | 4.098(45)e+36
B065 | 20210926 | 59483.875402715 | 412.18 | 3.16 |  67.82$\pm$0.45 |  0.21$\pm$1.42 | 5.990(56)e+37 | 2.396(22)e+37 | 200 | 3.03 |  153.88$\pm$1.05 |  0.47$\pm$0.01 | 2.293(18)e+37
B066 | 20210926 | 59483.876300725 | 412.18 | 4.84 |  71.42$\pm$0.04 |  0.35$\pm$0.17 | 9.685(84)e+37 | 3.874(34)e+37 | 200 | 4.30 |  168.89$\pm$0.27 |  0.73$\pm$0.01 | 3.569(27)e+37
B067 | 20210926 | 59483.876301212 | 412.18 | 3.75 |  6.94$\pm$0.06 |  0.03$\pm$0.21 | 7.278(1)e+36 | 2.911(1)e+36 | 50 | 5.33 |  34.70$\pm$0.18 |  0.18$\pm$0.01 | 2.273(22)e+36
B068 | 20210926 | 59483.878282943 | 412.18 | 23.10 |  153.41$\pm$0.34 |  3.54$\pm$7.81 | 9.920(73)e+38 | 3.968(29)e+38 | 450 | 21.11 |  170.38$\pm$0.62 |  3.60$\pm$0.03 | 3.978(29)e+38
B069 | 20210926 | 59483.878603455 | 412.18 | 3.77 |  282.69$\pm$0.09 |  1.06$\pm$0.35 | 2.981(22)e+38 | 1.192(9)e+38 | 350 | 2.42 |  520.17$\pm$0.23 |  1.26$\pm$0.01 | 1.083(8)e+38
B070 | 20210926 | 59483.878676878 | 412.18 | 9.11 |  75.18$\pm$0.96 |  0.68$\pm$8.76 | 1.917(14)e+38 | 7.669(56)e+37 | 200 | 8.39 |  181.13$\pm$1.41 |  1.52$\pm$0.01 | 7.470(58)e+37
B071 | 20210926 | 59483.879074091 | 412.18 | 7.23 |  14.39$\pm$0.09 |  0.10$\pm$0.67 | 2.911(28)e+37 | 1.164(11)e+37 | 150 | 2.59 |  48.35$\pm$0.47 |  0.13$\pm$0.01 | 4.613(56)e+36
B072 | 20210926 | 59483.879856241 | 412.18 | 8.89 |  212.05$\pm$0.29 |  1.89$\pm$2.58 | 5.279(36)e+38 | 2.112(15)e+38 | 500 | 6.56 |  212.18$\pm$0.58 |  1.39$\pm$0.01 | 1.712(13)e+38
B073 | 20210926 | 59483.880226783 | 412.18 | 5.47 |  93.26$\pm$0.08 |  0.51$\pm$0.42 | 1.428(11)e+38 | 5.710(45)e+37 | 200 | 4.92 |  219.97$\pm$0.22 |  1.08$\pm$0.01 | 5.320(40)e+37
B074 | 20210926 | 59483.880466827 | 412.18 | 6.46 |  10.38$\pm$0.17 |  0.07$\pm$1.08 | 1.875(1)e+37 | 7.501(1)e+36 | 200 | 4.84 |  26.54$\pm$0.84 |  0.13$\pm$0.01 | 6.315(45)e+36
B075 | 20210926 | 59483.880813045 | 412.18 | 2.29 |  8.73$\pm$0.08 |  0.02$\pm$0.19 | 5.598(1)e+36 | 2.239(1)e+36 | 100 | 2.61 |  21.61$\pm$0.11 |  0.06$\pm$0.01 | 1.388(22)e+36
B076 | 20210926 | 59483.881119121 | 412.18 | 5.97 |  16.93$\pm$0.16 |  0.10$\pm$0.94 | 2.827(28)e+37 | 1.131(11)e+37 | 150 | 4.84 |  47.96$\pm$0.29 |  0.23$\pm$0.01 | 8.565(67)e+36
B077 | 20210926 | 59483.883632446 | 412.18 | 8.38 |  108.88$\pm$0.5 |  0.91$\pm$4.17 | 2.553(20)e+38 | 1.021(8)e+38 | 250 | 6.97 |  256.06$\pm$1.21 |  1.78$\pm$0.01 | 1.097(8)e+38
B078 | 20210926 | 59483.883836521 | 412.18 | 6.73 |  176.73$\pm$0.08 |  1.19$\pm$0.51 | 3.331(22)e+38 | 1.332(9)e+38 | 350 | 5.23 |  298.80$\pm$0.39 |  1.56$\pm$0.01 | 1.346(9)e+38
B079 | 20210926 | 59483.884844752 | 412.18 | 4.92 |  85.71$\pm$0.52 |  0.42$\pm$2.57 | 1.181(6)e+38 | 4.725(22)e+37 | 300 | 4.15 |  164.33$\pm$1.22 |  0.68$\pm$0.01 | 5.032(32)e+37
B080 | 20210926 | 59483.885707702 | 412.18 | 5.45 |  18.34$\pm$0.55 |  0.10$\pm$2.98 | 2.799(28)e+37 | 1.120(11)e+37 | 100 | 4.54 |  72.58$\pm$1.33 |  0.33$\pm$0.01 | 8.106(67)e+36
B081 | 20210926 | 59483.887452049 | 412.18 | 6.46 |  57.28$\pm$0.05 |  0.37$\pm$0.34 | 1.036(6)e+38 | 4.142(22)e+37 | 150 | 6.02 |  151.31$\pm$0.33 |  0.91$\pm$0.01 | 3.359(24)e+37
B082 | 20210926 | 59483.887664102 | 412.18 | 4.22 |  11.86$\pm$1.14 |  0.05$\pm$4.79 | 1.400(1)e+37 | 5.598(1)e+36 | 100 | 5.83 |  30.29$\pm$1.27 |  0.18$\pm$0.01 | 4.344(45)e+36
B083 | 20210926 | 59483.891226358 | 412.18 | 2.12 |  11.80$\pm$2.09 |  0.02$\pm$4.43 | 6.998(1)e+36 | 2.799(1)e+36 | 100 | 4.05 |  25.64$\pm$3.76 |  0.10$\pm$0.01 | 2.553(22)e+36
B084 | 20210926 | 59483.891699437 | 412.18 | 4.32 |  9.49$\pm$0.92 |  0.04$\pm$3.96 | 1.148(1)e+37 | 4.590(1)e+36 | 100 | 4.82 |  29.64$\pm$1.31 |  0.14$\pm$0.01 | 3.516(22)e+36
B085 | 20210926 | 59483.892220131 | 412.18 | 10.89 |  78.68$\pm$0.56 |  0.86$\pm$6.06 | 2.399(17)e+38 | 9.595(67)e+37 | 300 | 7.94 |  189.69$\pm$1.39 |  1.51$\pm$0.01 | 1.111(7)e+38
B086 | 20210926 | 59483.892808160 | 412.18 | 5.79 |  80.98$\pm$0.09 |  0.47$\pm$0.53 | 1.313(6)e+38 | 5.251(22)e+37 | 400 | 4.83 |  114.35$\pm$0.35 |  0.55$\pm$0.01 | 5.435(34)e+37
B087 | 20210926 | 59483.892808675 | 412.18 | 4.86 |  8.64$\pm$0.11 |  0.04$\pm$0.52 | 1.176(1)e+37 | 4.702(1)e+36 | 100 | 4.75 |  22.42$\pm$0.16 |  0.11$\pm$0.01 | 2.620(22)e+36
B088 | 20210926 | 59483.894640599 | 412.18 | 5.73 |  12.56$\pm$0.27 |  0.07$\pm$1.56 | 2.015(1)e+37 | 8.061(1)e+36 | 150 | 2.25 |  32.38$\pm$0.74 |  0.07$\pm$0.01 | 2.687(1)e+36
B089 | 20210926 | 59483.895078090 | 412.18 | 2.84 |  9.49$\pm$0.95 |  0.03$\pm$2.7 | 7.557(1)e+36 | 3.023(1)e+36 | 250 | 3.58 |  10.68$\pm$1.36 |  0.04$\pm$0.01 | 2.351(1)e+36
B090 | 20210926 | 59483.895658199 | 412.18 | 4.90 |  279.21$\pm$1.54 |  1.37$\pm$7.56 | 3.829(22)e+38 | 1.532(9)e+38 | 500 | 4.44 |  279.13$\pm$1.54 |  1.24$\pm$0.01 | 1.525(9)e+38
B091 | 20210926 | 59483.895700046 | 412.18 | 4.55 |  23.06$\pm$0.67 |  0.10$\pm$3.06 | 2.939(28)e+37 | 1.176(11)e+37 | 100 | 3.47 |  97.56$\pm$1.64 |  0.34$\pm$0.01 | 8.330(67)e+36
B092 | 20210926 | 59483.895881803 | 412.18 | 5.06 |  22.54$\pm$0.08 |  0.11$\pm$0.38 | 3.191(28)e+37 | 1.276(11)e+37 | 150 | 4.85 |  57.24$\pm$0.2 |  0.28$\pm$0.01 | 1.024(7)e+37
B093 | 20210926 | 59483.896042101 | 412.18 | 2.71 |  14.05$\pm$0.06 |  0.04$\pm$0.17 | 1.064(1)e+37 | 4.254(1)e+36 | 200 | 2.71 |  31.27$\pm$0.19 |  0.08$\pm$0.01 | 4.165(45)e+36
B094 | 20210926 | 59483.896265661 | 412.18 | 8.68 |  30.19$\pm$0.12 |  0.26$\pm$1.05 | 7.333(56)e+37 | 2.933(22)e+37 | 150 | 8.12 |  75.13$\pm$0.36 |  0.61$\pm$0.01 | 2.250(13)e+37
B095 | 20210926 | 59483.896633672 | 412.18 | 5.31 |  10.36$\pm$0.75 |  0.06$\pm$4.0 | 1.539(1)e+37 | 6.158(1)e+36 | 100 | 5.28 |  34.47$\pm$1.8 |  0.18$\pm$0.01 | 4.478(22)e+36
B096 | 20210926 | 59483.896764390 | 412.18 | 4.79 |  9.18$\pm$0.65 |  0.04$\pm$3.14 | 1.232(1)e+37 | 4.926(1)e+36 | 250 | 5.03 |  16.87$\pm$1.64 |  0.08$\pm$0.01 | 5.217(1)e+36
B097 | 20210926 | 59483.897673601 | 412.18 | 4.70 |  10.86$\pm$1.21 |  0.05$\pm$5.69 | 1.428(1)e+37 | 5.710(1)e+36 | 200 | 4.16 |  23.87$\pm$2.0 |  0.10$\pm$0.01 | 4.882(45)e+36
B098 | 20210926 | 59483.898236478 | 412.18 | 4.04 |  52.54$\pm$0.36 |  0.21$\pm$1.45 | 5.934(28)e+37 | 2.374(11)e+37 | 300 | 3.58 |  84.11$\pm$0.56 |  0.30$\pm$0.01 | 2.224(13)e+37
B099 | 20210926 | 59483.898804482 | 412.18 | 3.70 |  10.54$\pm$0.58 |  0.04$\pm$2.15 | 1.092(1)e+37 | 4.366(1)e+36 | 200 | 2.35 |  29.48$\pm$1.09 |  0.07$\pm$0.01 | 3.404(1)e+36
B100 | 20210926 | 59483.899297459 | 412.18 | 4.73 |  20.74$\pm$0.18 |  0.10$\pm$0.86 | 2.743(28)e+37 | 1.097(11)e+37 | 250 | 5.01 |  43.27$\pm$0.32 |  0.22$\pm$0.01 | 1.332(6)e+37
B101 | 20210926 | 59483.899536772 | 412.18 | 5.23 |  10.71$\pm$0.42 |  0.06$\pm$2.19 | 1.567(1)e+37 | 6.270(1)e+36 | 100 | 5.53 |  29.98$\pm$1.0 |  0.17$\pm$0.01 | 4.075(22)e+36
B102 | 20210926 | 59483.901420449 | 412.18 | 14.94 |  159.46$\pm$0.12 |  2.38$\pm$1.82 | 6.667(36)e+38 | 2.667(15)e+38 | 300 | 11.52 |  507.65$\pm$0.61 |  5.85$\pm$0.03 | 4.315(23)e+38
B103 | 20210926 | 59483.901566710 | 412.18 | 1.94 |  6.19$\pm$0.37 |  0.01$\pm$0.72 | 3.359(1)e+36 | 1.344(1)e+36 | 50 | 4.51 |  36.35$\pm$1.02 |  0.16$\pm$0.01 | 2.015(11)e+36
B104 | 20210926 | 59483.902023911 | 412.18 | 6.29 |  10.01$\pm$0.08 |  0.06$\pm$0.48 | 1.763(1)e+37 | 7.054(1)e+36 | 100 | 8.52 |  25.97$\pm$0.25 |  0.22$\pm$0.01 | 5.441(45)e+36
B105 | 20210926 | 59483.902347678 | 412.18 | 7.20 |  177.62$\pm$0.07 |  1.28$\pm$0.52 | 3.580(20)e+38 | 1.432(8)e+38 | 350 | 6.58 |  314.84$\pm$0.2 |  2.07$\pm$0.01 | 1.781(9)e+38
B106 | 20210926 | 59483.902445444 | 412.18 | 5.50 |  114.38$\pm$0.05 |  0.63$\pm$0.27 | 1.760(8)e+38 | 7.042(34)e+37 | 350 | 4.80 |  200.03$\pm$0.12 |  0.96$\pm$0.01 | 8.265(40)e+37
B107 | 20210926 | 59483.902446090 | 412.18 | 8.10 |  9.13$\pm$0.06 |  0.07$\pm$0.47 | 2.071(1)e+37 | 8.285(1)e+36 | 100 | 7.83 |  28.63$\pm$0.23 |  0.22$\pm$0.01 | 5.508(45)e+36
B108 | 20210927 | 59484.815064813 | 411.51 | 2.79 |  12.88$\pm$0.31 |  0.04$\pm$0.86 | 1.008(1)e+37 | 4.031(1)e+36 | 300 | 2.18 |  18.38$\pm$0.47 |  0.04$\pm$0.01 | 2.956(1)e+36
B109 | 20210927 | 59484.815066874 | 411.51 | 6.97 |  13.20$\pm$0.48 |  0.09$\pm$3.33 | 2.575(28)e+37 | 1.030(11)e+37 | 200 | 6.39 |  31.52$\pm$1.16 |  0.20$\pm$0.01 | 9.897(90)e+36
B110 | 20210927 | 59484.815083222 | 411.51 | 5.33 |  6.38$\pm$0.49 |  0.03$\pm$2.59 | 9.517(1)e+36 | 3.807(1)e+36 | 100 | 5.15 |  19.82$\pm$0.68 |  0.10$\pm$0.01 | 2.508(45)e+36
B111 | 20210927 | 59484.815192614 | 411.51 | 2.04 |  10.79$\pm$0.25 |  0.02$\pm$0.51 | 6.158(1)e+36 | 2.463(1)e+36 | 100 | 2.58 |  56.11$\pm$0.32 |  0.14$\pm$0.01 | 3.560(67)e+36
B112 | 20210927 | 59484.815539225 | 411.51 | 5.29 |  8.12$\pm$0.05 |  0.04$\pm$0.28 | 1.204(1)e+37 | 4.814(1)e+36 | 200 | 3.58 |  20.11$\pm$0.17 |  0.07$\pm$0.01 | 3.538(45)e+36
B113 | 20210927 | 59484.815633103 | 411.51 | 10.61 |  65.59$\pm$0.07 |  0.70$\pm$0.77 | 1.948(20)e+38 | 7.792(78)e+37 | 250 | 8.35 |  149.99$\pm$0.2 |  1.25$\pm$0.01 | 7.701(71)e+37
B114 | 20210927 | 59484.815717973 | 411.51 | 6.33 |  109.44$\pm$0.06 |  0.69$\pm$0.35 | 1.940(20)e+38 | 7.759(78)e+37 | 500 | 5.67 |  109.47$\pm$0.06 |  0.62$\pm$0.01 | 7.636(73)e+37
B115 | 20210927 | 59484.816079467 | 411.51 | 10.00 |  41.40$\pm$1.59 |  0.41$\pm$15.91 | 1.159(14)e+38 | 4.635(56)e+37 | 250 | 8.37 |  83.38$\pm$1.59 |  0.70$\pm$0.01 | 4.288(45)e+37
B116 | 20210927 | 59484.816079808 | 411.51 | 12.21 |  171.17$\pm$0.13 |  2.09$\pm$1.6 | 5.850(59)e+38 | 2.340(24)e+38 | 450 | 11.07 |  188.74$\pm$0.71 |  2.09$\pm$0.02 | 2.312(22)e+38
B117 | 20210927 | 59484.816203397 | 411.51 | 4.42 |  14.93$\pm$0.13 |  0.07$\pm$0.57 | 1.847(28)e+37 | 7.389(112)e+36 | 200 | 4.20 |  33.63$\pm$0.34 |  0.14$\pm$0.01 | 6.942(45)e+36
B118 | 20210927 | 59484.816484609 | 411.51 | 5.72 |  66.95$\pm$0.08 |  0.38$\pm$0.46 | 1.072(11)e+38 | 4.288(45)e+37 | 200 | 5.11 |  166.25$\pm$0.18 |  0.85$\pm$0.01 | 4.178(40)e+37
B119 | 20210927 | 59484.816555900 | 411.51 | 6.19 |  157.40$\pm$0.04 |  0.98$\pm$0.22 | 2.729(28)e+38 | 1.092(11)e+38 | 350 | 5.32 |  225.18$\pm$0.14 |  1.20$\pm$0.01 | 1.031(9)e+38
B120 | 20210927 | 59484.816556524 | 411.51 | 5.07 |  10.06$\pm$0.17 |  0.05$\pm$0.86 | 1.428(28)e+37 | 5.710(112)e+36 | 100 | 4.46 |  40.27$\pm$0.44 |  0.18$\pm$0.01 | 4.411(67)e+36
B121 | 20210927 | 59484.817061129 | 411.51 | 6.90 |  117.29$\pm$0.09 |  0.81$\pm$0.64 | 2.264(22)e+38 | 9.058(90)e+37 | 250 | 6.35 |  257.01$\pm$0.23 |  1.63$\pm$0.01 | 1.003(8)e+38
B122 | 20210927 | 59484.817111779 | 411.51 | 5.49 |  298.76$\pm$0.06 |  1.64$\pm$0.32 | 4.590(45)e+38 | 1.836(18)e+38 | 350 | 4.97 |  397.86$\pm$0.25 |  1.98$\pm$0.02 | 1.702(16)e+38
B123 | 20210927 | 59484.817112134 | 411.51 | 4.52 |  10.63$\pm$0.05 |  0.05$\pm$0.21 | 1.344(1)e+37 | 5.374(1)e+36 | 150 | 4.19 |  43.88$\pm$0.09 |  0.18$\pm$0.01 | 6.785(67)e+36
B124 | 20210927 | 59484.817112541 | 411.51 | 17.91 |  237.31$\pm$0.05 |  4.25$\pm$0.91 | 1.190(12)e+39 | 4.758(47)e+38 | 450 | 17.54 |  263.04$\pm$0.09 |  4.61$\pm$0.04 | 5.105(47)e+38
B125 | 20210927 | 59484.817556805 | 411.51 | 6.20 |  193.85$\pm$0.06 |  1.20$\pm$0.37 | 3.362(34)e+38 | 1.345(13)e+38 | 450 | 5.15 |  208.08$\pm$0.14 |  1.07$\pm$0.01 | 1.185(12)e+38
B126 | 20210927 | 59484.817557288 | 411.51 | 9.94 |  265.82$\pm$0.29 |  2.64$\pm$2.85 | 7.398(73)e+38 | 2.959(29)e+38 | 250 | 8.39 |  547.94$\pm$0.44 |  4.60$\pm$0.05 | 2.825(32)e+38
B127 | 20210927 | 59484.817776928 | 411.51 | 5.67 |  9.16$\pm$0.06 |  0.05$\pm$0.32 | 1.456(1)e+37 | 5.822(1)e+36 | 100 | 4.15 |  39.07$\pm$0.17 |  0.16$\pm$0.01 | 3.986(67)e+36
B128 | 20210927 | 59484.817795359 | 411.51 | 3.24 |  21.27$\pm$0.11 |  0.07$\pm$0.36 | 1.931(28)e+37 | 7.725(112)e+36 | 200 | 3.52 |  50.21$\pm$0.24 |  0.18$\pm$0.01 | 8.688(90)e+36
B129 | 20210927 | 59484.817978132 | 411.51 | 3.28 |  274.28$\pm$0.06 |  0.90$\pm$0.19 | 2.522(25)e+38 | 1.009(10)e+38 | 500 | 3.27 |  274.43$\pm$0.2 |  0.90$\pm$0.01 | 1.102(11)e+38
B130 | 20210927 | 59484.818559283 | 411.51 | 6.10 |  28.54$\pm$0.83 |  0.17$\pm$5.07 | 4.870(56)e+37 | 1.948(22)e+37 | 400 | 5.64 |  33.62$\pm$2.36 |  0.19$\pm$0.01 | 1.863(27)e+37
B131 | 20210927 | 59484.819455676 | 411.51 | 3.98 |  33.39$\pm$0.75 |  0.13$\pm$2.99 | 3.723(56)e+37 | 1.489(22)e+37 | 350 | 3.76 |  52.38$\pm$2.75 |  0.20$\pm$0.01 | 1.693(24)e+37
B132 | 20210927 | 59484.819456077 | 411.51 | 7.11 |  245.40$\pm$0.03 |  1.74$\pm$0.23 | 4.884(62)e+38 | 1.954(25)e+38 | 500 | 6.48 |  245.66$\pm$0.24 |  1.59$\pm$0.02 | 1.958(25)e+38
B133 | 20210927 | 59484.819457073 | 411.51 | 5.85 |  83.06$\pm$0.05 |  0.49$\pm$0.3 | 1.360(17)e+38 | 5.441(67)e+37 | 300 | 5.45 |  165.00$\pm$0.17 |  0.90$\pm$0.01 | 6.630(87)e+37
B134 | 20210927 | 59484.819993471 | 411.51 | 9.81 |  34.34$\pm$0.91 |  0.34$\pm$8.97 | 9.433(140)e+37 | 3.773(56)e+37 | 400 | 8.80 |  43.82$\pm$1.63 |  0.39$\pm$0.01 | 3.793(49)e+37
B135 | 20210927 | 59484.820093607 | 411.51 | 4.11 |  9.01$\pm$0.05 |  0.04$\pm$0.19 | 1.036(1)e+37 | 4.142(1)e+36 | 150 | 3.58 |  24.67$\pm$0.25 |  0.09$\pm$0.01 | 3.258(34)e+36
B136 | 20210927 | 59484.820194444 | 411.51 | 5.25 |  7.99$\pm$0.59 |  0.04$\pm$3.09 | 1.176(28)e+37 | 4.702(112)e+36 | 300 | 2.77 |  11.20$\pm$1.03 |  0.03$\pm$0.01 | 2.284(1)e+36
B137 | 20210927 | 59484.820254376 | 411.51 | 1.68 |  7.13$\pm$0.04 |  0.01$\pm$0.07 | 3.359(1)e+36 | 1.344(1)e+36 | 50 | 4.50 |  51.66$\pm$0.14 |  0.23$\pm$0.01 | 2.855(45)e+36
B138 | 20210927 | 59484.821266385 | 411.51 | 2.43 |  11.13$\pm$0.05 |  0.03$\pm$0.11 | 7.557(1)e+36 | 3.023(1)e+36 | 200 | 2.46 |  17.39$\pm$0.19 |  0.04$\pm$0.01 | 2.105(45)e+36
B139 | 20210927 | 59484.821306547 | 411.51 | 9.13 |  35.81$\pm$0.13 |  0.33$\pm$1.19 | 9.153(112)e+37 | 3.661(45)e+37 | 300 | 7.87 |  61.00$\pm$0.17 |  0.48$\pm$0.01 | 3.540(47)e+37
B140 | 20210927 | 59484.821308755 | 411.51 | 7.02 |  56.11$\pm$0.13 |  0.39$\pm$0.94 | 1.103(11)e+38 | 4.411(45)e+37 | 250 | 6.53 |  118.08$\pm$0.3 |  0.77$\pm$0.01 | 4.742(62)e+37
B141 | 20210927 | 59484.821356845 | 411.51 | 3.59 |  228.18$\pm$0.06 |  0.82$\pm$0.23 | 2.295(31)e+38 | 9.181(123)e+37 | 400 | 3.28 |  316.01$\pm$0.34 |  1.04$\pm$0.01 | 1.020(13)e+38
B142 | 20210927 | 59484.821781065 | 411.51 | 4.78 |  87.65$\pm$0.11 |  0.42$\pm$0.52 | 1.173(17)e+38 | 4.691(67)e+37 | 400 | 4.42 |  104.15$\pm$0.97 |  0.46$\pm$0.01 | 4.528(52)e+37
B143 | 20210927 | 59484.821860545 | 411.51 | 8.04 |  29.36$\pm$0.08 |  0.24$\pm$0.65 | 6.606(84)e+37 | 2.642(34)e+37 | 200 | 7.87 |  65.87$\pm$0.19 |  0.52$\pm$0.01 | 2.548(31)e+37
B144 | 20210927 | 59484.822123683 | 411.51 | 4.10 |  12.92$\pm$0.45 |  0.05$\pm$1.84 | 1.483(1)e+37 | 5.934(1)e+36 | 150 | 3.00 |  45.27$\pm$0.66 |  0.14$\pm$0.01 | 5.005(56)e+36
B145 | 20210927 | 59484.822191905 | 411.51 | 4.62 |  297.30$\pm$0.66 |  1.37$\pm$3.04 | 3.846(48)e+38 | 1.538(19)e+38 | 450 | 4.20 |  324.93$\pm$1.44 |  1.36$\pm$0.02 | 1.509(19)e+38
B146 | 20210927 | 59484.822192898 | 411.51 | 4.39 |  54.47$\pm$0.2 |  0.24$\pm$0.87 | 6.690(84)e+37 | 2.676(34)e+37 | 200 | 4.05 |  138.67$\pm$0.34 |  0.56$\pm$0.01 | 2.759(36)e+37
B147 | 20210927 | 59484.822555006 | 411.51 | 3.13 |  6.71$\pm$1.1 |  0.02$\pm$3.43 | 5.878(1)e+36 | 2.351(1)e+36 | 100 | 3.59 |  23.56$\pm$1.1 |  0.08$\pm$0.01 | 2.082(22)e+36
B148 | 20210927 | 59484.822651454 | 411.51 | 7.27 |  55.55$\pm$0.41 |  0.40$\pm$2.96 | 1.131(14)e+38 | 4.523(56)e+37 | 300 | 6.43 |  107.01$\pm$0.76 |  0.69$\pm$0.01 | 5.072(60)e+37
B149 | 20210927 | 59484.822725490 | 411.51 | 4.17 |  28.32$\pm$0.41 |  0.12$\pm$1.71 | 3.303(28)e+37 | 1.321(11)e+37 | 350 | 3.56 |  39.67$\pm$0.72 |  0.14$\pm$0.01 | 1.215(16)e+37
B150 | 20210927 | 59484.822725772 | 411.51 | 9.09 |  206.60$\pm$1.7 |  1.88$\pm$15.45 | 5.259(64)e+38 | 2.104(26)e+38 | 500 | 5.66 |  314.84$\pm$1.81 |  1.78$\pm$0.02 | 2.192(26)e+38
B151 | 20210927 | 59484.822781633 | 411.51 | 8.09 |  156.21$\pm$0.15 |  1.26$\pm$1.2 | 3.538(45)e+38 | 1.415(18)e+38 | 400 | 7.30 |  201.26$\pm$0.32 |  1.47$\pm$0.02 | 1.446(18)e+38
B152 | 20210927 | 59484.822816484 | 411.51 | 13.03 |  740.65$\pm$0.66 |  9.65$\pm$8.59 | 2.702(34)e+39 | 1.081(14)e+39 | 500 | 11.71 |  740.98$\pm$1.56 |  8.68$\pm$0.11 | 1.067(13)e+39
B153 | 20210927 | 59484.822949804 | 411.51 | 2.96 |  133.06$\pm$1.55 |  0.39$\pm$4.58 | 1.103(14)e+38 | 4.411(56)e+37 | 200 | 2.69 |  334.96$\pm$2.06 |  0.90$\pm$0.01 | 4.438(58)e+37
B154 | 20210927 | 59484.822997882 | 411.51 | 6.48 |  6.63$\pm$0.8 |  0.04$\pm$5.21 | 1.204(28)e+37 | 4.814(112)e+36 | 100 | 2.45 |  24.89$\pm$1.1 |  0.06$\pm$0.01 | 1.500(22)e+36
B155 | 20210927 | 59484.823628987 | 411.51 | 7.27 |  78.68$\pm$0.1 |  0.57$\pm$0.72 | 1.601(20)e+38 | 6.404(78)e+37 | 400 | 6.57 |  101.27$\pm$0.68 |  0.67$\pm$0.01 | 6.548(81)e+37
B156 | 20210927 | 59484.823629206 | 411.51 | 14.32 |  175.33$\pm$1.14 |  2.51$\pm$16.36 | 7.028(90)e+38 | 2.811(36)e+38 | 300 | 13.88 |  274.66$\pm$2.17 |  3.81$\pm$0.05 | 2.812(35)e+38
B157 | 20210927 | 59484.823630066 | 411.51 | 9.17 |  23.98$\pm$2.91 |  0.22$\pm$26.67 | 6.158(84)e+37 | 2.463(34)e+37 | 100 | 9.47 |  103.67$\pm$3.6 |  0.98$\pm$0.01 | 2.414(36)e+37
B158 | 20210927 | 59484.823654783 | 411.51 | 3.06 |  71.20$\pm$0.1 |  0.22$\pm$0.32 | 6.102(84)e+37 | 2.441(34)e+37 | 450 | 2.75 |  75.42$\pm$0.41 |  0.21$\pm$0.01 | 2.297(30)e+37
B159 | 20210927 | 59484.823781511 | 411.51 | 4.29 |  27.53$\pm$2.31 |  0.12$\pm$9.9 | 3.303(28)e+37 | 1.321(11)e+37 | 150 | 3.84 |  89.80$\pm$2.48 |  0.35$\pm$0.01 | 1.273(17)e+37
B160 | 20210927 | 59484.823866837 | 411.51 | 4.69 |  8.96$\pm$0.82 |  0.04$\pm$3.85 | 1.176(28)e+37 | 4.702(112)e+36 | 100 | 5.69 |  28.01$\pm$1.15 |  0.16$\pm$0.01 | 3.919(67)e+36
B161 | 20210927 | 59484.823896871 | 411.51 | 8.38 |  17.91$\pm$0.72 |  0.15$\pm$6.0 | 4.198(56)e+37 | 1.679(22)e+37 | 200 | 7.77 |  48.20$\pm$2.1 |  0.37$\pm$0.01 | 1.841(22)e+37
B162 | 20210927 | 59484.824066464 | 411.51 | 2.85 |  8.79$\pm$0.49 |  0.02$\pm$1.39 | 6.998(1)e+36 | 2.799(1)e+36 | 150 | 4.16 |  27.34$\pm$2.9 |  0.11$\pm$0.01 | 4.198(67)e+36
B163 | 20210927 | 59484.824629002 | 411.51 | 3.38 |  11.23$\pm$0.85 |  0.04$\pm$2.89 | 1.064(1)e+37 | 4.254(1)e+36 | 100 | 3.05 |  60.63$\pm$0.98 |  0.18$\pm$0.01 | 4.546(67)e+36
B164 | 20210927 | 59484.824656846 | 411.51 | 3.94 |  47.25$\pm$1.88 |  0.19$\pm$7.4 | 5.206(56)e+37 | 2.082(22)e+37 | 300 | 3.35 |  86.94$\pm$1.94 |  0.29$\pm$0.01 | 2.150(27)e+37
B165 | 20210927 | 59484.824658221 | 411.51 | 6.47 |  30.45$\pm$0.18 |  0.20$\pm$1.15 | 5.514(56)e+37 | 2.206(22)e+37 | 200 | 6.34 |  71.95$\pm$1.08 |  0.46$\pm$0.01 | 2.244(27)e+37
B166 | 20210927 | 59484.824661556 | 411.51 | 16.61 |  323.06$\pm$0.2 |  5.37$\pm$3.39 | 1.502(18)e+39 | 6.008(74)e+38 | 500 | 8.95 |  435.05$\pm$1.02 |  3.89$\pm$0.05 | 4.787(58)e+38
B167 | 20210927 | 59484.824959354 | 411.51 | 2.54 |  25.21$\pm$2.58 |  0.06$\pm$6.55 | 1.791(28)e+37 | 7.166(112)e+36 | 200 | 2.54 |  54.96$\pm$5.96 |  0.14$\pm$0.01 | 6.852(90)e+36
B168 | 20210927 | 59484.825119162 | 411.51 | 3.40 |  24.40$\pm$1.91 |  0.08$\pm$6.49 | 2.323(28)e+37 | 9.293(112)e+36 | 100 | 3.55 |  103.29$\pm$5.36 |  0.37$\pm$0.01 | 9.024(134)e+36
B169 | 20210927 | 59484.825121426 | 411.51 | 10.71 |  84.81$\pm$1.01 |  0.91$\pm$10.82 | 2.542(31)e+38 | 1.017(12)e+38 | 250 | 10.10 |  179.78$\pm$2.69 |  1.82$\pm$0.02 | 1.116(14)e+38
B170 | 20210927 | 59484.825174523 | 411.51 | 0.91 |  5.51$\pm$0.09 |  0.00$\pm$0.08 | 1.400(1)e+36 | 5.598(1)e+35 | 100 | 2.13 |  23.06$\pm$0.65 |  0.05$\pm$0.01 | 1.209(22)e+36
B171 | 20210927 | 59484.825174810 | 411.51 | 2.96 |  9.81$\pm$0.2 |  0.03$\pm$0.61 | 8.117(1)e+36 | 3.247(1)e+36 | 200 | 3.97 |  19.29$\pm$0.46 |  0.08$\pm$0.01 | 3.762(45)e+36
B172 | 20210927 | 59484.825308762 | 411.51 | 4.17 |  28.27$\pm$2.64 |  0.12$\pm$11.0 | 3.303(28)e+37 | 1.321(11)e+37 | 300 | 3.91 |  48.40$\pm$2.64 |  0.19$\pm$0.01 | 1.397(20)e+37
B173 | 20210927 | 59484.825310690 | 411.51 | 5.24 |  12.22$\pm$1.08 |  0.06$\pm$5.67 | 1.791(28)e+37 | 7.166(112)e+36 | 100 | 5.22 |  56.39$\pm$1.08 |  0.29$\pm$0.01 | 7.233(112)e+36
B174 | 20210927 | 59484.825311568 | 411.51 | 5.41 |  14.97$\pm$0.37 |  0.08$\pm$1.99 | 2.267(28)e+37 | 9.069(112)e+36 | 150 | 5.48 |  38.70$\pm$0.43 |  0.21$\pm$0.01 | 7.826(101)e+36
B175 | 20210927 | 59484.825312014 | 411.51 | 1.73 |  8.07$\pm$0.43 |  0.01$\pm$0.74 | 3.919(1)e+36 | 1.567(1)e+36 | 50 | 7.01 |  36.74$\pm$0.68 |  0.26$\pm$0.01 | 3.168(45)e+36
B176 | 20210927 | 59484.827075500 | 411.51 | 4.79 |  164.96$\pm$3.13 |  0.79$\pm$15.0 | 2.211(28)e+38 | 8.845(112)e+37 | 450 | 4.39 |  175.01$\pm$3.14 |  0.77$\pm$0.01 | 8.505(101)e+37
B177 | 20210927 | 59484.827075732 | 411.51 | 4.53 |  46.81$\pm$1.06 |  0.21$\pm$4.81 | 5.934(84)e+37 | 2.374(34)e+37 | 250 | 4.42 |  94.87$\pm$2.13 |  0.42$\pm$0.01 | 2.575(34)e+37
B178 | 20210927 | 59484.827379212 | 411.51 | 6.17 |  37.13$\pm$0.16 |  0.23$\pm$0.98 | 6.410(84)e+37 | 2.564(34)e+37 | 300 | 5.21 |  57.56$\pm$0.32 |  0.30$\pm$0.01 | 2.210(27)e+37
B179 | 20210927 | 59484.827380008 | 411.51 | 13.91 |  147.82$\pm$0.44 |  2.06$\pm$6.06 | 5.755(67)e+38 | 2.302(27)e+38 | 300 | 13.68 |  312.10$\pm$0.56 |  4.27$\pm$0.05 | 3.150(39)e+38
B180 | 20210927 | 59484.827712022 | 411.51 | 5.96 |  13.77$\pm$0.11 |  0.08$\pm$0.68 | 2.295(28)e+37 | 9.181(112)e+36 | 350 | 5.39 |  20.79$\pm$0.32 |  0.11$\pm$0.01 | 9.640(78)e+36
B181 | 20210927 | 59484.827713498 | 411.51 | 6.65 |  33.99$\pm$0.1 |  0.23$\pm$0.68 | 6.326(84)e+37 | 2.530(34)e+37 | 200 | 6.22 |  83.21$\pm$0.14 |  0.52$\pm$0.01 | 2.544(31)e+37
B182 | 20210927 | 59484.828076558 | 411.51 | 2.91 |  23.68$\pm$0.09 |  0.07$\pm$0.27 | 1.931(28)e+37 | 7.725(112)e+36 | 200 | 2.87 |  51.09$\pm$0.79 |  0.15$\pm$0.01 | 7.210(90)e+36
B183 | 20210927 | 59484.828834912 | 411.51 | 4.87 |  55.42$\pm$0.14 |  0.27$\pm$0.68 | 7.557(84)e+37 | 3.023(34)e+37 | 250 | 4.17 |  118.71$\pm$0.22 |  0.50$\pm$0.01 | 3.045(39)e+37
B184 | 20210927 | 59484.828908828 | 411.51 | 5.86 |  42.32$\pm$0.45 |  0.25$\pm$2.64 | 6.942(84)e+37 | 2.777(34)e+37 | 150 | 5.36 |  135.02$\pm$0.74 |  0.72$\pm$0.01 | 2.667(34)e+37
B185 | 20210927 | 59484.829635469 | 411.51 | 5.92 |  85.97$\pm$0.39 |  0.51$\pm$2.3 | 1.425(17)e+38 | 5.699(67)e+37 | 350 | 5.48 |  131.19$\pm$0.62 |  0.72$\pm$0.01 | 6.191(71)e+37
B186 | 20210927 | 59484.830431677 | 411.51 | 3.25 |  21.52$\pm$0.38 |  0.07$\pm$1.25 | 1.959(28)e+37 | 7.837(112)e+36 | 150 | 3.25 |  69.13$\pm$0.78 |  0.22$\pm$0.01 | 8.296(101)e+36
B187 | 20210927 | 59484.830432187 | 411.51 | 10.80 |  24.73$\pm$0.23 |  0.27$\pm$2.45 | 7.473(84)e+37 | 2.989(34)e+37 | 200 | 9.46 |  58.90$\pm$0.4 |  0.56$\pm$0.01 | 2.741(31)e+37
B188 | 20210927 | 59484.830432579 | 411.51 | 4.45 |  26.95$\pm$0.71 |  0.12$\pm$3.15 | 3.359(28)e+37 | 1.344(11)e+37 | 100 | 4.36 |  124.62$\pm$1.52 |  0.54$\pm$0.01 | 1.337(18)e+37
B189 | 20210927 | 59484.830594912 | 411.51 | 6.30 |  75.84$\pm$2.87 |  0.48$\pm$18.11 | 1.338(17)e+38 | 5.352(67)e+37 | 300 | 5.57 |  150.03$\pm$3.7 |  0.84$\pm$0.01 | 6.160(74)e+37
B190 | 20210927 | 59484.830595235 | 411.51 | 4.89 |  244.72$\pm$1.1 |  1.20$\pm$5.4 | 3.350(39)e+38 | 1.340(16)e+38 | 450 | 4.51 |  266.84$\pm$4.06 |  1.20$\pm$0.01 | 1.331(16)e+38
B191 | 20210927 | 59484.830595799 | 411.51 | 3.57 |  15.70$\pm$0.64 |  0.06$\pm$2.27 | 1.567(28)e+37 | 6.270(112)e+36 | 200 | 3.65 |  36.72$\pm$3.22 |  0.13$\pm$0.01 | 6.583(90)e+36
B192 | 20210927 | 59484.830662870 | 411.51 | 7.67 |  25.93$\pm$1.1 |  0.20$\pm$8.43 | 5.570(56)e+37 | 2.228(22)e+37 | 100 | 7.78 |  114.77$\pm$1.31 |  0.89$\pm$0.01 | 2.194(31)e+37
B193 | 20210927 | 59484.830722229 | 411.51 | 4.07 |  5.90$\pm$0.32 |  0.02$\pm$1.28 | 6.718(1)e+36 | 2.687(1)e+36 | 200 | 2.61 |  17.10$\pm$0.9 |  0.04$\pm$0.01 | 2.194(45)e+36
B194 | 20210927 | 59484.830741528 | 411.51 | 4.68 |  22.20$\pm$0.37 |  0.10$\pm$1.72 | 2.911(28)e+37 | 1.164(11)e+37 | 300 | 4.49 |  39.98$\pm$0.85 |  0.18$\pm$0.01 | 1.323(13)e+37
B195 | 20210927 | 59484.830741992 | 411.51 | 5.58 |  51.80$\pm$0.11 |  0.29$\pm$0.59 | 8.089(84)e+37 | 3.236(34)e+37 | 200 | 5.10 |  132.06$\pm$0.53 |  0.67$\pm$0.01 | 3.314(40)e+37
B196 | 20210927 | 59484.830837877 | 411.51 | 6.76 |  76.51$\pm$0.16 |  0.52$\pm$1.09 | 1.447(17)e+38 | 5.788(67)e+37 | 450 | 5.87 |  83.51$\pm$0.58 |  0.49$\pm$0.01 | 5.426(64)e+37
B197 | 20210927 | 59484.831353639 | 411.51 | 2.55 |  27.04$\pm$3.73 |  0.07$\pm$9.51 | 1.931(28)e+37 | 7.725(112)e+36 | 200 | 2.13 |  63.65$\pm$4.09 |  0.14$\pm$0.01 | 6.673(90)e+36
B198 | 20210927 | 59484.831904204 | 411.51 | 9.63 |  352.86$\pm$0.68 |  3.40$\pm$6.58 | 9.508(112)e+38 | 3.803(45)e+38 | 500 | 8.65 |  353.02$\pm$1.78 |  3.05$\pm$0.04 | 3.755(44)e+38
B199 | 20210927 | 59484.832022331 | 411.51 | 8.46 |  184.56$\pm$0.08 |  1.56$\pm$0.71 | 4.369(50)e+38 | 1.748(20)e+38 | 400 | 7.62 |  224.40$\pm$0.36 |  1.71$\pm$0.02 | 1.682(20)e+38
B200 | 20210927 | 59484.832041199 | 411.51 | 4.63 |  134.94$\pm$0.69 |  0.62$\pm$3.21 | 1.749(20)e+38 | 6.998(78)e+37 | 250 | 4.24 |  281.44$\pm$1.34 |  1.19$\pm$0.01 | 7.328(84)e+37
B201 | 20210927 | 59484.832087389 | 411.51 | 3.26 |  11.95$\pm$0.35 |  0.04$\pm$1.15 | 1.092(1)e+37 | 4.366(1)e+36 | 200 | 3.62 |  21.64$\pm$0.48 |  0.08$\pm$0.01 | 3.851(45)e+36
B202 | 20210927 | 59484.832492855 | 411.51 | 7.55 |  14.84$\pm$2.58 |  0.11$\pm$19.46 | 3.135(56)e+37 | 1.254(22)e+37 | 300 | 6.51 |  28.11$\pm$2.58 |  0.18$\pm$0.01 | 1.350(20)e+37
B203 | 20210927 | 59484.832736324 | 411.51 | 3.50 |  17.41$\pm$2.11 |  0.06$\pm$7.41 | 1.707(28)e+37 | 6.830(112)e+36 | 100 | 4.85 |  57.12$\pm$3.85 |  0.28$\pm$0.01 | 6.807(90)e+36
B204 | 20210927 | 59484.832867013 | 411.51 | 8.91 |  25.71$\pm$1.95 |  0.23$\pm$17.37 | 6.410(84)e+37 | 2.564(34)e+37 | 400 | 8.53 |  30.31$\pm$2.52 |  0.26$\pm$0.01 | 2.544(27)e+37
B205 | 20210927 | 59484.832867923 | 411.51 | 4.52 |  17.24$\pm$1.14 |  0.08$\pm$5.15 | 2.183(28)e+37 | 8.733(112)e+36 | 200 | 3.78 |  47.76$\pm$2.1 |  0.18$\pm$0.01 | 8.867(90)e+36
B206 | 20210927 | 59484.833054538 | 411.51 | 5.68 |  13.57$\pm$9.24 |  0.08$\pm$52.46 | 2.155(28)e+37 | 8.621(112)e+36 | 200 | 4.95 |  34.96$\pm$9.25 |  0.17$\pm$0.01 | 8.509(90)e+36
B207 | 20210927 | 59484.833076579 | 411.51 | 4.40 |  18.66$\pm$1.38 |  0.08$\pm$6.04 | 2.295(28)e+37 | 9.181(112)e+36 | 300 | 3.98 |  32.53$\pm$2.33 |  0.13$\pm$0.01 | 9.539(134)e+36
B208 | 20210927 | 59484.833080540 | 411.51 | 5.72 |  527.52$\pm$3.72 |  3.02$\pm$21.26 | 8.445(95)e+38 | 3.378(38)e+38 | 450 | 5.27 |  558.63$\pm$5.22 |  2.94$\pm$0.03 | 3.255(37)e+38
B209 | 20210927 | 59484.833231156 | 411.51 | 4.48 |  333.91$\pm$1.66 |  1.50$\pm$7.44 | 4.184(48)e+38 | 1.674(19)e+38 | 450 | 3.67 |  429.70$\pm$4.28 |  1.58$\pm$0.02 | 1.744(19)e+38
B210 | 20210927 | 59484.833312992 | 411.51 | 3.72 |  10.22$\pm$0.08 |  0.04$\pm$0.3 | 1.064(1)e+37 | 4.254(1)e+36 | 300 | 4.38 |  14.36$\pm$0.37 |  0.06$\pm$0.01 | 4.635(67)e+36
B211 | 20210927 | 59484.833314185 | 411.51 | 5.64 |  32.64$\pm$0.97 |  0.18$\pm$5.48 | 5.150(56)e+37 | 2.060(22)e+37 | 200 | 5.67 |  71.78$\pm$1.26 |  0.41$\pm$0.01 | 2.002(22)e+37
B212 | 20210927 | 59484.834155240 | 411.51 | 5.23 |  77.32$\pm$2.17 |  0.40$\pm$11.33 | 1.131(14)e+38 | 4.523(56)e+37 | 500 | 4.75 |  77.31$\pm$3.33 |  0.37$\pm$0.01 | 4.512(56)e+37
B213 | 20210927 | 59484.834763741 | 411.51 | 7.98 |  114.72$\pm$1.97 |  0.92$\pm$15.74 | 2.564(28)e+38 | 1.026(11)e+38 | 300 | 7.25 |  215.51$\pm$2.02 |  1.56$\pm$0.02 | 1.152(13)e+38
B214 | 20210927 | 59484.834893955 | 411.51 | 14.78 |  166.52$\pm$1.24 |  2.46$\pm$18.26 | 6.891(78)e+38 | 2.756(31)e+38 | 400 | 7.64 |  352.41$\pm$2.72 |  2.69$\pm$0.03 | 2.649(30)e+38
B215 | 20210927 | 59484.835245092 | 411.51 | 10.68 |  211.82$\pm$0.3 |  2.26$\pm$3.16 | 6.334(73)e+38 | 2.534(29)e+38 | 500 | 5.47 |  387.41$\pm$1.55 |  2.12$\pm$0.02 | 2.603(30)e+38
B216 | 20210927 | 59484.835246085 | 411.51 | 3.95 |  29.60$\pm$0.88 |  0.12$\pm$3.48 | 3.275(28)e+37 | 1.310(11)e+37 | 200 | 3.56 |  81.94$\pm$0.93 |  0.29$\pm$0.01 | 1.433(18)e+37
B217 | 20210927 | 59484.835359072 | 411.51 | 4.42 |  680.57$\pm$0.34 |  3.01$\pm$1.5 | 8.420(95)e+38 | 3.368(38)e+38 | 450 | 4.02 |  721.88$\pm$1.14 |  2.90$\pm$0.03 | 3.208(36)e+38
B218 | 20210927 | 59484.835615052 | 411.51 | 3.75 |  6.66$\pm$0.11 |  0.02$\pm$0.42 | 6.998(1)e+36 | 2.799(1)e+36 | 50 | 2.49 |  44.32$\pm$0.42 |  0.11$\pm$0.01 | 1.355(22)e+36
B219 | 20210927 | 59484.835615517 | 411.51 | 6.69 |  18.98$\pm$0.2 |  0.13$\pm$1.35 | 3.555(28)e+37 | 1.422(11)e+37 | 100 | 6.54 |  84.14$\pm$0.48 |  0.55$\pm$0.01 | 1.352(18)e+37
B220 | 20210927 | 59484.835615785 | 411.51 | 8.13 |  33.93$\pm$0.22 |  0.28$\pm$1.8 | 7.725(84)e+37 | 3.090(34)e+37 | 150 | 7.70 |  106.23$\pm$0.61 |  0.82$\pm$0.01 | 3.016(34)e+37
B221 | 20210927 | 59484.835940687 | 411.51 | 4.13 |  124.38$\pm$0.11 |  0.51$\pm$0.45 | 1.439(17)e+38 | 5.755(67)e+37 | 500 | 3.57 |  124.59$\pm$0.35 |  0.44$\pm$0.01 | 5.468(65)e+37
B222 | 20210927 | 59484.835941515 | 411.51 | 5.52 |  71.56$\pm$0.14 |  0.39$\pm$0.76 | 1.106(11)e+38 | 4.422(45)e+37 | 300 | 4.64 |  143.93$\pm$0.9 |  0.67$\pm$0.01 | 4.925(54)e+37
B223 | 20210927 | 59484.836025131 | 411.51 | 3.11 |  10.62$\pm$0.58 |  0.03$\pm$1.81 | 9.237(1)e+36 | 3.695(1)e+36 | 150 | 2.80 |  26.01$\pm$1.08 |  0.07$\pm$0.01 | 2.687(34)e+36
B224 | 20210927 | 59484.836201831 | 411.51 | 7.09 |  189.71$\pm$0.38 |  1.34$\pm$2.66 | 3.765(42)e+38 | 1.506(17)e+38 | 400 | 6.46 |  242.76$\pm$0.91 |  1.57$\pm$0.02 | 1.541(17)e+38
B225 | 20210927 | 59484.836285079 | 411.51 | 5.22 |  43.49$\pm$0.39 |  0.23$\pm$2.03 | 6.354(84)e+37 | 2.542(34)e+37 | 300 | 4.52 |  87.33$\pm$1.06 |  0.39$\pm$0.01 | 2.909(34)e+37
B226 | 20210927 | 59484.836334881 | 411.51 | 8.27 |  50.54$\pm$3.28 |  0.42$\pm$27.11 | 1.170(14)e+38 | 4.680(56)e+37 | 300 | 8.01 |  75.95$\pm$5.22 |  0.61$\pm$0.01 | 4.488(49)e+37
B227 | 20210927 | 59484.836341526 | 411.51 | 4.39 |  30.78$\pm$2.85 |  0.14$\pm$12.51 | 3.779(56)e+37 | 1.511(22)e+37 | 200 | 4.18 |  75.44$\pm$2.86 |  0.32$\pm$0.01 | 1.550(18)e+37
B228 | 20210927 | 59484.836524844 | 411.51 | 10.83 |  10.71$\pm$3.98 |  0.12$\pm$43.05 | 3.247(28)e+37 | 1.299(11)e+37 | 200 | 7.57 |  33.45$\pm$3.98 |  0.25$\pm$0.01 | 1.245(13)e+37
B229 | 20210927 | 59484.836530494 | 411.51 | 8.89 |  197.66$\pm$0.31 |  1.76$\pm$2.75 | 4.918(53)e+38 | 1.967(21)e+38 | 250 | 8.06 |  468.96$\pm$0.66 |  3.78$\pm$0.04 | 2.323(27)e+38
B230 | 20210927 | 59484.836651585 | 411.51 | 2.46 |  8.95$\pm$0.3 |  0.02$\pm$0.73 | 6.158(1)e+36 | 2.463(1)e+36 | 200 | 3.55 |  20.26$\pm$1.53 |  0.07$\pm$0.01 | 3.538(45)e+36
B231 | 20210927 | 59484.836820724 | 411.51 | 11.52 |  67.71$\pm$0.79 |  0.78$\pm$9.09 | 2.183(25)e+38 | 8.733(101)e+37 | 250 | 10.29 |  144.84$\pm$1.75 |  1.49$\pm$0.02 | 9.164(106)e+37
B232 | 20210927 | 59484.836906709 | 411.51 | 7.32 |  52.60$\pm$1.04 |  0.38$\pm$7.61 | 1.078(11)e+38 | 4.310(45)e+37 | 450 | 6.77 |  56.73$\pm$2.25 |  0.38$\pm$0.01 | 4.252(50)e+37
B233 | 20210927 | 59484.836972623 | 411.51 | 3.40 |  19.39$\pm$0.74 |  0.07$\pm$2.52 | 1.847(28)e+37 | 7.389(112)e+36 | 150 | 3.70 |  47.24$\pm$1.92 |  0.17$\pm$0.01 | 6.449(67)e+36
B234 | 20210927 | 59484.837056097 | 411.51 | 5.16 |  30.02$\pm$0.33 |  0.16$\pm$1.71 | 4.338(56)e+37 | 1.735(22)e+37 | 150 | 4.82 |  92.20$\pm$2.14 |  0.44$\pm$0.01 | 1.639(20)e+37
B235 | 20210927 | 59484.837062285 | 411.51 | 6.51 |  33.31$\pm$0.07 |  0.22$\pm$0.44 | 6.074(56)e+37 | 2.430(22)e+37 | 200 | 6.57 |  77.79$\pm$0.34 |  0.51$\pm$0.01 | 2.512(27)e+37
B236 | 20210927 | 59484.837288293 | 411.51 | 6.76 |  276.35$\pm$0.12 |  1.87$\pm$0.81 | 5.229(59)e+38 | 2.091(24)e+38 | 350 | 6.23 |  444.45$\pm$0.24 |  2.77$\pm$0.03 | 2.382(27)e+38
B237 | 20210927 | 59484.837542013 | 411.51 | 7.05 |  14.19$\pm$0.35 |  0.10$\pm$2.44 | 2.799(28)e+37 | 1.120(11)e+37 | 200 | 6.78 |  34.11$\pm$0.6 |  0.23$\pm$0.01 | 1.138(13)e+37
B238 | 20210927 | 59484.838798528 | 411.51 | 3.78 |  198.79$\pm$0.15 |  0.75$\pm$0.57 | 2.102(22)e+38 | 8.408(90)e+37 | 450 | 3.37 |  218.25$\pm$0.83 |  0.74$\pm$0.01 | 8.142(91)e+37
B239 | 20210927 | 59484.838830119 | 411.51 | 2.03 |  6.39$\pm$0.18 |  0.01$\pm$0.37 | 3.639(1)e+36 | 1.456(1)e+36 | 100 | 1.70 |  29.98$\pm$0.49 |  0.05$\pm$0.01 | 1.254(22)e+36
B240 | 20210927 | 59484.838830452 | 411.51 | 2.78 |  7.20$\pm$0.1 |  0.02$\pm$0.28 | 5.598(1)e+36 | 2.239(1)e+36 | 100 | 4.90 |  34.94$\pm$0.54 |  0.17$\pm$0.01 | 4.210(67)e+36
B241 | 20210927 | 59484.838830757 | 411.51 | 2.56 |  14.83$\pm$1.99 |  0.04$\pm$5.1 | 1.064(1)e+37 | 4.254(1)e+36 | 200 | 2.42 |  36.14$\pm$2.11 |  0.09$\pm$0.01 | 4.299(45)e+36
B242 | 20210927 | 59484.838831093 | 411.51 | 8.47 |  126.30$\pm$0.56 |  1.07$\pm$4.79 | 2.995(34)e+38 | 1.198(13)e+38 | 300 | 6.24 |  272.49$\pm$1.16 |  1.70$\pm$0.02 | 1.254(14)e+38
B243 | 20210927 | 59484.839152182 | 411.51 | 2.55 |  40.41$\pm$0.45 |  0.10$\pm$1.14 | 2.883(28)e+37 | 1.153(11)e+37 | 200 | 2.36 |  92.02$\pm$0.68 |  0.22$\pm$0.01 | 1.066(13)e+37
B244 | 20210927 | 59484.839264577 | 411.51 | 4.06 |  10.84$\pm$0.28 |  0.04$\pm$1.13 | 1.232(1)e+37 | 4.926(1)e+36 | 100 | 4.86 |  37.12$\pm$0.57 |  0.18$\pm$0.01 | 4.434(67)e+36
B245 | 20210927 | 59484.839269867 | 411.51 | 2.60 |  9.22$\pm$0.65 |  0.02$\pm$1.68 | 6.718(1)e+36 | 2.687(1)e+36 | 200 | 3.41 |  17.88$\pm$1.99 |  0.06$\pm$0.01 | 3.000(45)e+36
B246 | 20210927 | 59484.839553036 | 411.51 | 8.28 |  312.52$\pm$1.36 |  2.59$\pm$11.22 | 7.244(78)e+38 | 2.898(31)e+38 | 500 | 7.51 |  312.39$\pm$2.98 |  2.35$\pm$0.03 | 2.885(31)e+38
B247 | 20210927 | 59484.839903310 | 411.51 | 5.80 |  60.00$\pm$1.78 |  0.35$\pm$10.3 | 9.741(112)e+37 | 3.896(45)e+37 | 350 | 5.47 |  83.10$\pm$3.8 |  0.45$\pm$0.01 | 3.911(39)e+37
B248 | 20210927 | 59484.840349946 | 411.51 | 3.53 |  37.93$\pm$0.16 |  0.13$\pm$0.58 | 3.751(28)e+37 | 1.500(11)e+37 | 200 | 3.32 |  101.26$\pm$0.25 |  0.34$\pm$0.01 | 1.652(18)e+37
B249 | 20210927 | 59484.840704911 | 411.51 | 4.25 |  72.98$\pm$0.41 |  0.31$\pm$1.73 | 8.677(84)e+37 | 3.471(34)e+37 | 300 | 4.28 |  112.27$\pm$1.02 |  0.48$\pm$0.01 | 3.547(40)e+37
B250 | 20210927 | 59484.840739605 | 411.51 | 3.36 |  12.21$\pm$0.28 |  0.04$\pm$0.95 | 1.148(1)e+37 | 4.590(1)e+36 | 150 | 2.55 |  31.39$\pm$0.63 |  0.08$\pm$0.01 | 2.956(34)e+36
B251 | 20210927 | 59484.840740342 | 411.51 | 4.10 |  12.67$\pm$0.66 |  0.05$\pm$2.7 | 1.456(28)e+37 | 5.822(112)e+36 | 250 | 3.79 |  24.76$\pm$1.44 |  0.09$\pm$0.01 | 5.766(56)e+36
B252 | 20210927 | 59484.840740652 | 411.51 | 2.40 |  19.60$\pm$0.5 |  0.05$\pm$1.21 | 1.316(28)e+37 | 5.262(112)e+36 | 200 | 2.16 |  50.27$\pm$1.65 |  0.11$\pm$0.01 | 5.329(45)e+36
B253 | 20210927 | 59484.840763967 | 411.51 | 4.95 |  111.39$\pm$1.02 |  0.55$\pm$5.04 | 1.542(17)e+38 | 6.169(67)e+37 | 200 | 4.49 |  279.20$\pm$1.56 |  1.25$\pm$0.01 | 6.162(67)e+37
B254 | 20210927 | 59484.840849563 | 411.51 | 5.08 |  21.67$\pm$0.25 |  0.11$\pm$1.28 | 3.079(28)e+37 | 1.232(11)e+37 | 400 | 4.51 |  25.86$\pm$0.84 |  0.12$\pm$0.01 | 1.146(9)e+37
B255 | 20210927 | 59484.840998978 | 411.51 | 7.47 |  124.83$\pm$0.29 |  0.93$\pm$2.17 | 2.612(28)e+38 | 1.045(11)e+38 | 200 | 6.49 |  324.44$\pm$0.71 |  2.11$\pm$0.02 | 1.035(12)e+38
B256 | 20210927 | 59484.841275031 | 411.51 | 5.41 |  22.75$\pm$0.18 |  0.12$\pm$0.96 | 3.443(28)e+37 | 1.377(11)e+37 | 100 | 5.98 |  90.35$\pm$0.34 |  0.54$\pm$0.01 | 1.328(18)e+37
B257 | 20210927 | 59484.841681895 | 411.51 | 6.03 |  94.84$\pm$0.32 |  0.57$\pm$1.91 | 1.601(17)e+38 | 6.404(67)e+37 | 250 | 4.63 |  235.81$\pm$1.77 |  1.09$\pm$0.01 | 6.712(72)e+37
B258 | 20210927 | 59484.841683619 | 411.51 | 10.69 |  131.58$\pm$0.89 |  1.41$\pm$9.51 | 3.938(42)e+38 | 1.575(17)e+38 | 200 | 9.75 |  352.20$\pm$1.77 |  3.43$\pm$0.04 | 1.688(18)e+38
B259 | 20210927 | 59484.841697815 | 411.51 | 6.63 |  12.21$\pm$2.87 |  0.08$\pm$19.03 | 2.267(28)e+37 | 9.069(112)e+36 | 350 | 4.46 |  19.19$\pm$3.14 |  0.09$\pm$0.01 | 7.367(78)e+36
B260 | 20210927 | 59484.841727981 | 411.51 | 3.20 |  98.00$\pm$0.18 |  0.31$\pm$0.59 | 8.789(84)e+37 | 3.516(34)e+37 | 400 | 2.87 |  117.25$\pm$0.44 |  0.34$\pm$0.01 | 3.305(36)e+37
B261 | 20210927 | 59484.841800964 | 411.51 | 6.19 |  53.12$\pm$0.3 |  0.33$\pm$1.88 | 9.209(112)e+37 | 3.684(45)e+37 | 450 | 5.58 |  56.96$\pm$1.63 |  0.32$\pm$0.01 | 3.517(40)e+37
B262 | 20210927 | 59484.841994744 | 411.51 | 8.66 |  235.75$\pm$0.07 |  2.04$\pm$0.6 | 5.713(62)e+38 | 2.285(25)e+38 | 350 | 5.99 |  443.85$\pm$0.21 |  2.66$\pm$0.03 | 2.288(24)e+38
B263 | 20210927 | 59484.841995582 | 411.51 | 4.65 |  13.75$\pm$0.26 |  0.06$\pm$1.21 | 1.791(28)e+37 | 7.166(112)e+36 | 200 | 3.95 |  33.68$\pm$0.47 |  0.13$\pm$0.01 | 6.538(90)e+36
B264 | 20210927 | 59484.842052381 | 411.51 | 7.22 |  104.43$\pm$0.61 |  0.75$\pm$4.38 | 2.110(22)e+38 | 8.442(90)e+37 | 300 | 4.50 |  269.57$\pm$1.6 |  1.21$\pm$0.01 | 8.957(94)e+37
B265 | 20210927 | 59484.842107401 | 411.51 | 13.08 |  493.70$\pm$0.43 |  6.46$\pm$5.57 | 1.807(19)e+39 | 7.228(76)e+38 | 350 | 12.38 |  623.84$\pm$0.89 |  7.72$\pm$0.08 | 6.644(70)e+38
B266 | 20210927 | 59484.842108389 | 411.51 | 7.86 |  411.74$\pm$0.9 |  3.24$\pm$7.05 | 9.060(98)e+38 | 3.624(39)e+38 | 350 | 6.51 |  696.73$\pm$0.98 |  4.53$\pm$0.05 | 3.902(42)e+38
B267 | 20210927 | 59484.842322838 | 411.51 | 3.83 |  13.07$\pm$0.32 |  0.05$\pm$1.21 | 1.400(28)e+37 | 5.598(112)e+36 | 100 | 3.05 |  60.70$\pm$0.76 |  0.18$\pm$0.01 | 4.546(67)e+36
B268 | 20210927 | 59484.842342158 | 411.51 | 2.97 |  32.28$\pm$0.72 |  0.10$\pm$2.14 | 2.687(28)e+37 | 1.075(11)e+37 | 200 | 3.55 |  73.15$\pm$1.08 |  0.26$\pm$0.01 | 1.276(13)e+37
B269 | 20210927 | 59484.842342422 | 411.51 | 3.09 |  12.64$\pm$4.1 |  0.04$\pm$12.64 | 1.092(1)e+37 | 4.366(1)e+36 | 100 | 4.90 |  44.99$\pm$4.1 |  0.22$\pm$0.01 | 5.419(67)e+36
B270 | 20210927 | 59484.842351245 | 411.51 | 3.16 |  8.23$\pm$0.99 |  0.03$\pm$3.14 | 7.278(1)e+36 | 2.911(1)e+36 | 200 | 3.43 |  16.46$\pm$1.52 |  0.06$\pm$0.01 | 2.777(45)e+36
B271 | 20210927 | 59484.842632189 | 411.51 | 3.31 |  62.46$\pm$0.75 |  0.21$\pm$2.5 | 5.794(56)e+37 | 2.318(22)e+37 | 300 | 3.00 |  121.92$\pm$1.14 |  0.37$\pm$0.01 | 2.700(27)e+37
B272 | 20210927 | 59484.842886014 | 411.51 | 11.19 |  520.14$\pm$2.14 |  5.82$\pm$23.99 | 1.630(17)e+39 | 6.520(69)e+38 | 300 | 7.62 |  1148.55$\pm$2.6 |  8.75$\pm$0.09 | 6.457(68)e+38
B273 | 20210927 | 59484.843087391 | 411.51 | 4.69 |  17.89$\pm$0.92 |  0.08$\pm$4.3 | 2.351(28)e+37 | 9.405(112)e+36 | 300 | 3.94 |  26.35$\pm$2.35 |  0.10$\pm$0.01 | 7.658(67)e+36
B274 | 20210927 | 59484.843132863 | 411.51 | 3.68 |  14.12$\pm$1.57 |  0.05$\pm$5.77 | 1.456(28)e+37 | 5.822(112)e+36 | 200 | 3.68 |  32.18$\pm$3.32 |  0.12$\pm$0.01 | 5.822(45)e+36
B275 | 20210927 | 59484.843133313 | 411.51 | 6.12 |  143.54$\pm$0.14 |  0.88$\pm$0.85 | 2.458(25)e+38 | 9.830(101)e+37 | 400 | 5.57 |  182.62$\pm$0.26 |  1.02$\pm$0.01 | 9.996(107)e+37
B276 | 20210927 | 59484.843356058 | 411.51 | 3.87 |  18.86$\pm$0.17 |  0.07$\pm$0.65 | 2.043(28)e+37 | 8.173(112)e+36 | 150 | 4.05 |  49.01$\pm$0.27 |  0.20$\pm$0.01 | 7.322(67)e+36
B277 | 20210927 | 59484.843368529 | 411.51 | 3.06 |  8.82$\pm$0.17 |  0.03$\pm$0.52 | 7.557(1)e+36 | 3.023(1)e+36 | 50 | 3.23 |  43.64$\pm$0.33 |  0.14$\pm$0.01 | 1.735(22)e+36
B278 | 20210927 | 59484.843713371 | 411.51 | 7.03 |  13.09$\pm$0.2 |  0.09$\pm$1.41 | 2.575(28)e+37 | 1.030(11)e+37 | 200 | 5.08 |  36.39$\pm$0.8 |  0.18$\pm$0.01 | 9.091(90)e+36
B279 | 20210927 | 59484.843941485 | 411.51 | 10.45 |  183.79$\pm$0.3 |  1.92$\pm$3.1 | 5.374(59)e+38 | 2.150(24)e+38 | 450 | 9.49 |  202.26$\pm$0.35 |  1.92$\pm$0.02 | 2.123(22)e+38
B280 | 20210927 | 59484.843942409 | 411.51 | 6.39 |  57.72$\pm$0.2 |  0.37$\pm$1.27 | 1.033(11)e+38 | 4.131(45)e+37 | 200 | 6.22 |  146.25$\pm$0.56 |  0.91$\pm$0.01 | 4.474(49)e+37
B281 | 20210927 | 59484.844124657 | 411.51 | 4.23 |  15.37$\pm$0.16 |  0.06$\pm$0.66 | 1.819(28)e+37 | 7.278(112)e+36 | 200 | 4.02 |  40.14$\pm$0.41 |  0.16$\pm$0.01 | 7.927(90)e+36
B282 | 20210927 | 59484.844187344 | 411.51 | 5.84 |  429.31$\pm$0.21 |  2.51$\pm$1.25 | 7.014(70)e+38 | 2.806(28)e+38 | 400 | 4.55 |  685.91$\pm$0.38 |  3.12$\pm$0.03 | 3.069(32)e+38
B283 | 20210927 | 59484.844341326 | 411.51 | 7.68 |  172.06$\pm$0.18 |  1.32$\pm$1.39 | 3.698(39)e+38 | 1.479(16)e+38 | 500 | 6.98 |  172.16$\pm$0.66 |  1.20$\pm$0.01 | 1.478(16)e+38
B284 | 20210927 | 59484.844413974 | 411.51 | 5.94 |  271.28$\pm$6.06 |  1.61$\pm$36.0 | 4.509(48)e+38 | 1.804(19)e+38 | 350 | 5.45 |  456.50$\pm$6.42 |  2.49$\pm$0.03 | 2.143(23)e+38
B285 | 20210927 | 59484.844469101 | 411.51 | 6.95 |  314.34$\pm$0.29 |  2.18$\pm$2.04 | 6.116(64)e+38 | 2.446(26)e+38 | 400 | 6.10 |  413.00$\pm$0.62 |  2.52$\pm$0.03 | 2.478(26)e+38
B286 | 20210927 | 59484.844545696 | 411.51 | 2.51 |  67.00$\pm$0.34 |  0.17$\pm$0.85 | 4.702(56)e+37 | 1.881(22)e+37 | 200 | 2.49 |  156.28$\pm$0.38 |  0.39$\pm$0.01 | 1.912(22)e+37
B287 | 20210927 | 59484.844557537 | 411.51 | 11.77 |  360.73$\pm$3.84 |  4.24$\pm$45.16 | 1.188(13)e+39 | 4.753(50)e+38 | 500 | 8.54 |  360.65$\pm$4.95 |  3.08$\pm$0.03 | 3.787(39)e+38
B288 | 20210927 | 59484.844558115 | 411.51 | 11.08 |  10.29$\pm$0.12 |  0.11$\pm$1.3 | 3.191(28)e+37 | 1.276(11)e+37 | 500 | 5.34 |  548.83$\pm$0.17 |  2.93$\pm$0.03 | 3.601(38)e+38
B289 | 20210927 | 59484.844562370 | 411.51 | 5.32 |  25.39$\pm$0.38 |  0.14$\pm$1.99 | 3.779(28)e+37 | 1.511(11)e+37 | 500 | 4.81 |  25.19$\pm$0.85 |  0.12$\pm$0.01 | 1.489(11)e+37
B290 | 20210927 | 59484.844562884 | 411.51 | 4.99 |  24.24$\pm$0.88 |  0.12$\pm$4.39 | 3.387(28)e+37 | 1.355(11)e+37 | 200 | 4.35 |  57.83$\pm$0.88 |  0.25$\pm$0.01 | 1.236(13)e+37
B291 | 20210927 | 59484.844765742 | 411.51 | 4.30 |  10.24$\pm$1.3 |  0.04$\pm$5.58 | 1.232(1)e+37 | 4.926(1)e+36 | 200 | 2.34 |  25.35$\pm$2.47 |  0.06$\pm$0.01 | 2.911(45)e+36
B292 | 20210927 | 59484.845023184 | 411.51 | 5.40 |  49.68$\pm$1.86 |  0.27$\pm$10.03 | 7.501(84)e+37 | 3.000(34)e+37 | 300 | 5.18 |  96.20$\pm$3.91 |  0.50$\pm$0.01 | 3.674(40)e+37
B293 | 20210927 | 59484.845175824 | 411.51 | 7.73 |  89.05$\pm$1.88 |  0.69$\pm$14.56 | 1.926(20)e+38 | 7.703(78)e+37 | 200 | 7.63 |  253.08$\pm$2.26 |  1.93$\pm$0.02 | 9.499(103)e+37
B294 | 20210927 | 59484.845176115 | 411.51 | 14.98 |  649.63$\pm$1.41 |  9.73$\pm$21.13 | 2.724(29)e+39 | 1.090(11)e+39 | 400 | 16.03 |  776.00$\pm$2.59 |  12.44$\pm$0.13 | 1.223(13)e+39
B295 | 20210927 | 59484.845538605 | 411.51 | 4.01 |  43.69$\pm$1.81 |  0.18$\pm$7.25 | 4.898(56)e+37 | 1.959(22)e+37 | 200 | 3.86 |  109.78$\pm$1.81 |  0.42$\pm$0.01 | 2.082(22)e+37
B296 | 20210927 | 59484.845627203 | 411.51 | 4.72 |  124.88$\pm$2.4 |  0.59$\pm$11.33 | 1.651(20)e+38 | 6.606(78)e+37 | 300 | 2.98 |  319.29$\pm$2.62 |  0.95$\pm$0.01 | 7.017(74)e+37
B297 | 20210927 | 59484.846121701 | 411.51 | 6.99 |  301.62$\pm$1.99 |  2.11$\pm$13.9 | 5.900(62)e+38 | 2.360(25)e+38 | 400 | 6.30 |  400.28$\pm$4.46 |  2.52$\pm$0.03 | 2.481(26)e+38
B298 | 20210927 | 59484.846333829 | 411.51 | 6.40 |  26.56$\pm$0.34 |  0.17$\pm$2.14 | 4.758(56)e+37 | 1.903(22)e+37 | 100 | 7.05 |  123.64$\pm$0.95 |  0.87$\pm$0.01 | 2.143(27)e+37
B299 | 20210927 | 59484.846536820 | 411.51 | 2.95 |  24.76$\pm$7.66 |  0.07$\pm$22.59 | 2.043(28)e+37 | 8.173(112)e+36 | 200 | 2.67 |  61.15$\pm$8.13 |  0.16$\pm$0.01 | 8.016(90)e+36
B300 | 20210927 | 59484.847016737 | 411.51 | 5.81 |  168.46$\pm$0.08 |  0.98$\pm$0.44 | 2.740(28)e+38 | 1.096(11)e+38 | 400 | 5.34 |  215.34$\pm$0.61 |  1.15$\pm$0.01 | 1.130(12)e+38
B301 | 20210927 | 59484.847164118 | 411.51 | 5.85 |  69.52$\pm$0.21 |  0.41$\pm$1.25 | 1.139(11)e+38 | 4.557(45)e+37 | 400 | 3.02 |  140.77$\pm$1.15 |  0.43$\pm$0.01 | 4.183(40)e+37
B302 | 20210927 | 59484.847352961 | 411.51 | 5.28 |  64.15$\pm$0.38 |  0.34$\pm$2.02 | 9.489(84)e+37 | 3.796(34)e+37 | 200 | 4.89 |  162.06$\pm$1.23 |  0.79$\pm$0.01 | 3.896(40)e+37
B303 | 20210927 | 59484.847965994 | 411.51 | 4.48 |  17.41$\pm$0.46 |  0.08$\pm$2.06 | 2.183(1)e+37 | 8.733(1)e+36 | 300 | 4.30 |  29.86$\pm$0.78 |  0.13$\pm$0.01 | 9.472(134)e+36
B304 | 20210927 | 59484.848016003 | 411.51 | 6.19 |  74.76$\pm$1.4 |  0.46$\pm$8.68 | 1.296(11)e+38 | 5.184(45)e+37 | 350 | 4.84 |  112.69$\pm$1.4 |  0.55$\pm$0.01 | 4.697(43)e+37
B305 | 20210927 | 59484.848017568 | 411.51 | 8.78 |  72.18$\pm$0.34 |  0.63$\pm$2.98 | 1.774(17)e+38 | 7.098(67)e+37 | 450 | 7.76 |  79.61$\pm$0.54 |  0.62$\pm$0.01 | 6.832(71)e+37
B306 | 20210927 | 59484.848063625 | 411.51 | 6.74 |  28.77$\pm$0.81 |  0.19$\pm$5.43 | 5.430(56)e+37 | 2.172(22)e+37 | 200 | 6.09 |  73.01$\pm$1.65 |  0.44$\pm$0.01 | 2.185(22)e+37
B307 | 20210927 | 59484.848242457 | 411.51 | 5.13 |  545.29$\pm$0.12 |  2.80$\pm$0.61 | 7.826(78)e+38 | 3.130(31)e+38 | 500 | 4.73 |  545.32$\pm$0.3 |  2.58$\pm$0.03 | 3.171(32)e+38
B308 | 20210927 | 59484.848243358 | 411.51 | 10.98 |  218.54$\pm$2.12 |  2.40$\pm$23.34 | 6.718(70)e+38 | 2.687(28)e+38 | 300 | 9.92 |  369.49$\pm$2.73 |  3.67$\pm$0.04 | 2.703(28)e+38
B309 | 20210927 | 59484.848732120 | 411.51 | 3.57 |  13.44$\pm$0.49 |  0.05$\pm$1.74 | 1.344(1)e+37 | 5.374(1)e+36 | 250 | 3.30 |  29.25$\pm$0.98 |  0.10$\pm$0.01 | 5.934(56)e+36
B310 | 20210927 | 59484.849076770 | 411.51 | 7.28 |  14.97$\pm$0.57 |  0.11$\pm$4.12 | 3.051(28)e+37 | 1.220(11)e+37 | 100 | 6.03 |  79.40$\pm$0.83 |  0.48$\pm$0.01 | 1.178(13)e+37
B311 | 20210927 | 59484.849566789 | 411.51 | 3.71 |  27.50$\pm$0.37 |  0.10$\pm$1.39 | 2.855(28)e+37 | 1.142(11)e+37 | 200 | 3.54 |  67.08$\pm$0.77 |  0.24$\pm$0.01 | 1.169(13)e+37
B312 | 20210927 | 59484.849574213 | 411.51 | 2.71 |  481.58$\pm$0.34 |  1.30$\pm$0.93 | 3.653(36)e+38 | 1.461(15)e+38 | 450 | 2.43 |  509.11$\pm$0.87 |  1.24$\pm$0.01 | 1.369(13)e+38
B313 | 20210927 | 59484.849601147 | 411.51 | 4.18 |  44.97$\pm$0.1 |  0.19$\pm$0.43 | 5.262(56)e+37 | 2.105(22)e+37 | 200 | 3.91 |  109.01$\pm$0.45 |  0.43$\pm$0.01 | 2.096(22)e+37
B314 | 20210927 | 59484.849624639 | 411.51 | 7.02 |  295.40$\pm$0.12 |  2.07$\pm$0.84 | 5.805(59)e+38 | 2.322(24)e+38 | 500 | 5.60 |  295.35$\pm$0.28 |  1.65$\pm$0.02 | 2.032(20)e+38
B315 | 20210927 | 59484.849693232 | 411.51 | 3.07 |  340.16$\pm$0.74 |  1.04$\pm$2.27 | 2.922(28)e+38 | 1.169(11)e+38 | 300 | 2.77 |  659.56$\pm$1.75 |  1.83$\pm$0.02 | 1.347(13)e+38
B316 | 20210927 | 59484.850131497 | 411.51 | 2.88 |  570.24$\pm$2.21 |  1.64$\pm$6.38 | 4.596(45)e+38 | 1.838(18)e+38 | 250 | 2.62 |  1388.76$\pm$5.34 |  3.64$\pm$0.04 | 2.239(22)e+38
B317 | 20210927 | 59484.850433479 | 411.51 | 6.34 |  54.12$\pm$0.1 |  0.34$\pm$0.63 | 9.601(84)e+37 | 3.840(34)e+37 | 300 | 5.46 |  123.83$\pm$0.23 |  0.68$\pm$0.01 | 4.991(47)e+37
B318 | 20210927 | 59484.850433797 | 411.51 | 5.04 |  19.43$\pm$0.75 |  0.10$\pm$3.8 | 2.743(28)e+37 | 1.097(11)e+37 | 250 | 5.60 |  46.00$\pm$1.64 |  0.26$\pm$0.01 | 1.584(17)e+37
B319 | 20210927 | 59484.850434221 | 411.51 | 16.21 |  97.26$\pm$0.71 |  1.58$\pm$11.58 | 4.414(45)e+38 | 1.766(18)e+38 | 300 | 15.06 |  231.56$\pm$1.55 |  3.49$\pm$0.03 | 2.573(26)e+38
B320 | 20210927 | 59484.850607072 | 411.51 | 3.04 |  404.14$\pm$0.59 |  1.23$\pm$1.78 | 3.440(34)e+38 | 1.376(13)e+38 | 400 | 2.71 |  487.50$\pm$0.63 |  1.32$\pm$0.01 | 1.297(13)e+38
B321 | 20210927 | 59484.850657895 | 411.51 | 13.19 |  37.08$\pm$0.22 |  0.49$\pm$2.85 | 1.369(14)e+38 | 5.475(56)e+37 | 300 | 12.35 |  69.29$\pm$0.54 |  0.86$\pm$0.01 | 6.310(63)e+37
B322 | 20210927 | 59484.850658350 | 411.51 | 4.14 |  11.60$\pm$0.34 |  0.05$\pm$1.39 | 1.344(1)e+37 | 5.374(1)e+36 | 100 | 6.89 |  45.47$\pm$1.05 |  0.31$\pm$0.01 | 7.703(90)e+36
B323 | 20210927 | 59484.850837928 | 411.51 | 10.11 |  120.62$\pm$0.37 |  1.22$\pm$3.75 | 3.412(34)e+38 | 1.365(13)e+38 | 500 | 9.26 |  120.65$\pm$0.89 |  1.12$\pm$0.01 | 1.374(13)e+38
B324 | 20210927 | 59484.851296707 | 411.51 | 7.20 |  249.16$\pm$3.06 |  1.79$\pm$22.05 | 5.021(50)e+38 | 2.009(20)e+38 | 250 | 6.58 |  587.75$\pm$4.99 |  3.87$\pm$0.04 | 2.379(24)e+38
B325 | 20210927 | 59484.851529432 | 411.51 | 3.17 |  9.47$\pm$0.16 |  0.03$\pm$0.5 | 8.397(1)e+36 | 3.359(1)e+36 | 100 | 3.21 |  24.37$\pm$0.39 |  0.08$\pm$0.01 | 1.926(22)e+36
B326 | 20210927 | 59484.851971473 | 411.51 | 5.62 |  174.13$\pm$2.18 |  0.98$\pm$12.26 | 2.740(28)e+38 | 1.096(11)e+38 | 300 | 5.13 |  331.61$\pm$2.4 |  1.70$\pm$0.02 | 1.254(12)e+38
B327 | 20210927 | 59484.852134510 | 411.51 | 2.00 |  5.00$\pm$0.07 |  0.01$\pm$0.14 | 2.799(1)e+36 | 1.120(1)e+36 | 50 | 2.87 |  77.33$\pm$0.4 |  0.22$\pm$0.01 | 2.732(34)e+36
B328 | 20210927 | 59484.852341880 | 411.51 | 6.08 |  53.46$\pm$0.08 |  0.32$\pm$0.48 | 9.097(84)e+37 | 3.639(34)e+37 | 200 | 5.62 |  134.66$\pm$0.46 |  0.76$\pm$0.01 | 3.722(36)e+37
B329 | 20210927 | 59484.852532819 | 411.51 | 9.86 |  290.45$\pm$0.16 |  2.86$\pm$1.61 | 8.019(76)e+38 | 3.208(30)e+38 | 400 | 7.41 |  458.15$\pm$0.4 |  3.40$\pm$0.03 | 3.340(32)e+38
B330 | 20210927 | 59484.852533552 | 411.51 | 5.17 |  111.56$\pm$1.38 |  0.58$\pm$7.16 | 1.615(17)e+38 | 6.460(67)e+37 | 200 | 4.56 |  305.76$\pm$2.62 |  1.40$\pm$0.01 | 6.861(67)e+37
B331 | 20210927 | 59484.852668167 | 411.51 | 4.41 |  7.71$\pm$1.38 |  0.03$\pm$6.09 | 9.517(1)e+36 | 3.807(1)e+36 | 50 | 5.48 |  41.52$\pm$3.04 |  0.23$\pm$0.01 | 2.799(34)e+36
B332 | 20210927 | 59484.853001168 | 411.51 | 11.70 |  157.49$\pm$0.44 |  1.84$\pm$5.16 | 5.159(50)e+38 | 2.063(20)e+38 | 450 | 10.64 |  173.91$\pm$1.03 |  1.85$\pm$0.02 | 2.046(20)e+38
B333 | 20210927 | 59484.853092443 | 411.51 | 3.54 |  18.36$\pm$0.12 |  0.06$\pm$0.42 | 1.819(28)e+37 | 7.278(112)e+36 | 150 | 3.24 |  62.68$\pm$0.49 |  0.20$\pm$0.01 | 7.490(67)e+36
B334 | 20210927 | 59484.853106057 | 411.51 | 7.89 |  398.52$\pm$0.1 |  3.14$\pm$0.8 | 8.800(84)e+38 | 3.520(34)e+38 | 500 | 7.41 |  398.66$\pm$0.2 |  2.95$\pm$0.03 | 3.632(35)e+38
B335 | 20210927 | 59484.854687262 | 411.51 | 9.47 |  480.26$\pm$3.41 |  4.55$\pm$32.28 | 1.273(12)e+39 | 5.091(48)e+38 | 350 | 7.53 |  720.57$\pm$3.41 |  5.43$\pm$0.05 | 4.670(44)e+38
B336 | 20210927 | 59484.854696278 | 411.51 | 4.62 |  17.73$\pm$0.65 |  0.08$\pm$3.01 | 2.295(28)e+37 | 9.181(112)e+36 | 200 | 5.28 |  34.83$\pm$0.88 |  0.18$\pm$0.01 | 9.046(90)e+36
B337 | 20210927 | 59484.854713653 | 411.51 | 4.22 |  8.76$\pm$0.41 |  0.04$\pm$1.73 | 1.036(1)e+37 | 4.142(1)e+36 | 100 | 3.71 |  36.57$\pm$1.13 |  0.14$\pm$0.01 | 3.336(45)e+36
B338 | 20210927 | 59484.855130997 | 411.51 | 6.28 |  19.43$\pm$0.49 |  0.12$\pm$3.07 | 3.415(28)e+37 | 1.366(11)e+37 | 400 | 6.03 |  24.46$\pm$0.71 |  0.15$\pm$0.01 | 1.451(18)e+37
B339 | 20210927 | 59484.855170377 | 411.51 | 7.13 |  210.35$\pm$0.79 |  1.50$\pm$5.62 | 4.198(39)e+38 | 1.679(16)e+38 | 350 | 6.41 |  344.22$\pm$1.22 |  2.21$\pm$0.02 | 1.899(18)e+38
B340 | 20210928 | 59485.784088726 | 412.55 | 4.14 |  12.79$\pm$0.13 |  0.05$\pm$0.55 | 1.483(28)e+37 | 5.934(112)e+36 | 200 | 4.54 |  28.69$\pm$0.35 |  0.13$\pm$0.01 | 6.404(90)e+36
B341 | 20210928 | 59485.784302145 | 412.55 | 5.67 |  57.70$\pm$0.14 |  0.33$\pm$0.78 | 9.153(140)e+37 | 3.661(56)e+37 | 400 | 5.06 |  76.33$\pm$0.27 |  0.39$\pm$0.01 | 3.798(63)e+37
B342 | 20210928 | 59485.784302732 | 412.55 | 8.18 |  27.88$\pm$0.21 |  0.23$\pm$1.73 | 6.382(112)e+37 | 2.553(45)e+37 | 150 | 7.75 |  77.32$\pm$0.56 |  0.60$\pm$0.01 | 2.210(37)e+37
B343 | 20210928 | 59485.784303356 | 412.55 | 15.91 |  94.41$\pm$1.2 |  1.50$\pm$19.12 | 4.204(67)e+38 | 1.682(27)e+38 | 300 | 12.85 |  205.93$\pm$3.09 |  2.65$\pm$0.04 | 1.951(29)e+38
B344 | 20210928 | 59485.784390425 | 412.55 | 3.21 |  25.83$\pm$0.23 |  0.08$\pm$0.75 | 2.323(28)e+37 | 9.293(112)e+36 | 350 | 2.81 |  39.27$\pm$0.28 |  0.11$\pm$0.01 | 9.483(157)e+36
B345 | 20210928 | 59485.784438434 | 412.55 | 3.69 |  18.95$\pm$0.46 |  0.07$\pm$1.69 | 1.959(28)e+37 | 7.837(112)e+36 | 200 | 2.98 |  40.01$\pm$1.08 |  0.12$\pm$0.01 | 5.867(90)e+36
B346 | 20210928 | 59485.784438707 | 412.55 | 11.64 |  167.25$\pm$1.34 |  1.95$\pm$15.6 | 5.450(90)e+38 | 2.180(36)e+38 | 350 | 7.71 |  316.59$\pm$3.59 |  2.44$\pm$0.04 | 2.102(33)e+38
B347 | 20210928 | 59485.784439317 | 412.55 | 3.46 |  33.22$\pm$0.24 |  0.12$\pm$0.84 | 3.219(56)e+37 | 1.288(22)e+37 | 250 | 3.39 |  75.31$\pm$1.18 |  0.26$\pm$0.01 | 1.567(22)e+37
B348 | 20210928 | 59485.784451845 | 412.55 | 6.01 |  40.95$\pm$1.01 |  0.25$\pm$6.08 | 6.886(112)e+37 | 2.754(45)e+37 | 150 | 6.26 |  107.32$\pm$2.6 |  0.67$\pm$0.01 | 2.479(40)e+37
B349 | 20210928 | 59485.784535762 | 412.55 | 2.52 |  60.25$\pm$0.96 |  0.15$\pm$2.41 | 4.254(56)e+37 | 1.702(22)e+37 | 350 | 2.35 |  86.99$\pm$2.0 |  0.20$\pm$0.01 | 1.756(24)e+37
B350 | 20210928 | 59485.784555518 | 412.55 | 4.04 |  22.53$\pm$1.4 |  0.09$\pm$5.67 | 2.547(28)e+37 | 1.019(11)e+37 | 300 | 3.62 |  29.47$\pm$3.88 |  0.11$\pm$0.01 | 7.860(134)e+36
B351 | 20210928 | 59485.784766559 | 412.55 | 9.31 |  163.98$\pm$0.13 |  1.53$\pm$1.21 | 4.271(67)e+38 | 1.708(27)e+38 | 450 | 6.15 |  240.82$\pm$0.21 |  1.48$\pm$0.02 | 1.639(26)e+38
B352 | 20210928 | 59485.784981334 | 412.55 | 1.13 |  15.88$\pm$1.05 |  0.02$\pm$1.19 | 5.038(1)e+36 | 2.015(1)e+36 | 150 | 2.11 |  27.69$\pm$1.25 |  0.06$\pm$0.01 | 2.150(34)e+36
B353 | 20210928 | 59485.785081872 | 412.55 | 9.70 |  63.42$\pm$0.57 |  0.62$\pm$5.5 | 1.721(28)e+38 | 6.886(112)e+37 | 200 | 9.12 |  154.51$\pm$0.61 |  1.41$\pm$0.02 | 6.928(107)e+37
B354 | 20210928 | 59485.785149768 | 412.55 | 3.51 |  90.60$\pm$2.52 |  0.32$\pm$8.83 | 8.901(140)e+37 | 3.560(56)e+37 | 400 | 3.28 |  110.02$\pm$4.66 |  0.36$\pm$0.01 | 3.547(54)e+37
B355 | 20210928 | 59485.785155330 | 412.55 | 2.89 |  913.29$\pm$1.55 |  2.64$\pm$4.47 | 7.387(118)e+38 | 2.955(47)e+38 | 500 | 2.62 |  913.06$\pm$2.05 |  2.40$\pm$0.04 | 2.944(47)e+38
B356 | 20210928 | 59485.785156845 | 412.55 | 7.70 |  357.69$\pm$1.65 |  2.75$\pm$12.72 | 7.708(123)e+38 | 3.083(49)e+38 | 500 | 7.00 |  357.44$\pm$3.11 |  2.50$\pm$0.04 | 3.078(49)e+38
B357 | 20210928 | 59485.785272185 | 412.55 | 5.99 |  214.90$\pm$0.15 |  1.29$\pm$0.88 | 3.602(56)e+38 | 1.441(22)e+38 | 500 | 5.46 |  214.82$\pm$0.37 |  1.17$\pm$0.02 | 1.441(22)e+38
B358 | 20210928 | 59485.785327226 | 412.55 | 5.73 |  31.27$\pm$0.19 |  0.18$\pm$1.11 | 5.010(84)e+37 | 2.004(34)e+37 | 200 | 5.10 |  78.28$\pm$0.42 |  0.40$\pm$0.01 | 1.962(31)e+37
B359 | 20210928 | 59485.785412350 | 412.55 | 4.83 |  18.00$\pm$0.6 |  0.09$\pm$2.9 | 2.435(28)e+37 | 9.741(112)e+36 | 200 | 3.29 |  32.66$\pm$1.12 |  0.11$\pm$0.01 | 5.284(90)e+36
B360 | 20210928 | 59485.785518550 | 412.55 | 5.12 |  17.56$\pm$1.12 |  0.09$\pm$5.71 | 2.519(28)e+37 | 1.008(11)e+37 | 200 | 4.60 |  45.33$\pm$2.95 |  0.21$\pm$0.01 | 1.026(18)e+37
B361 | 20210928 | 59485.785528816 | 412.55 | 3.27 |  169.33$\pm$0.31 |  0.55$\pm$1.01 | 1.551(25)e+38 | 6.203(101)e+37 | 400 | 2.98 |  219.80$\pm$0.54 |  0.65$\pm$0.01 | 6.440(99)e+37
B362 | 20210928 | 59485.785530186 | 412.55 | 3.96 |  12.12$\pm$0.4 |  0.05$\pm$1.57 | 1.344(28)e+37 | 5.374(112)e+36 | 200 | 2.75 |  41.79$\pm$1.07 |  0.11$\pm$0.01 | 5.643(90)e+36
B363 | 20210928 | 59485.785530500 | 412.55 | 5.55 |  50.82$\pm$0.66 |  0.28$\pm$3.69 | 7.893(112)e+37 | 3.157(45)e+37 | 300 | 5.14 |  107.60$\pm$1.71 |  0.55$\pm$0.01 | 4.078(60)e+37
B364 | 20210928 | 59485.785672412 | 412.55 | 8.14 |  190.17$\pm$2.36 |  1.55$\pm$19.19 | 4.333(70)e+38 | 1.733(28)e+38 | 450 | 7.41 |  202.98$\pm$3.21 |  1.50$\pm$0.02 | 1.665(26)e+38
B365 | 20210928 | 59485.785931764 | 412.55 | 6.12 |  426.61$\pm$2.77 |  2.61$\pm$16.96 | 7.306(115)e+38 | 2.922(46)e+38 | 300 | 5.86 |  670.45$\pm$3.78 |  3.93$\pm$0.06 | 2.900(44)e+38
B366 | 20210928 | 59485.785933305 | 412.55 | 10.20 |  38.54$\pm$5.27 |  0.39$\pm$53.74 | 1.100(17)e+38 | 4.400(67)e+37 | 300 | 6.79 |  83.68$\pm$6.51 |  0.57$\pm$0.01 | 4.190(65)e+37
B367 | 20210928 | 59485.785933911 | 412.55 | 4.52 |  31.17$\pm$1.28 |  0.14$\pm$5.79 | 3.947(56)e+37 | 1.579(22)e+37 | 200 | 4.02 |  76.10$\pm$1.75 |  0.31$\pm$0.01 | 1.505(22)e+37
B368 | 20210928 | 59485.785953735 | 412.55 | 1.64 |  22.53$\pm$0.98 |  0.04$\pm$1.61 | 1.036(28)e+37 | 4.142(112)e+36 | 200 | 1.32 |  39.44$\pm$1.45 |  0.05$\pm$0.01 | 2.553(45)e+36
B369 | 20210928 | 59485.785954058 | 412.55 | 2.86 |  10.82$\pm$0.41 |  0.03$\pm$1.17 | 8.677(1)e+36 | 3.471(1)e+36 | 300 | 2.85 |  20.16$\pm$0.88 |  0.06$\pm$0.01 | 4.232(67)e+36
B370 | 20210928 | 59485.786125663 | 412.55 | 4.39 |  81.78$\pm$1.07 |  0.36$\pm$4.71 | 1.005(17)e+38 | 4.019(67)e+37 | 200 | 4.24 |  208.84$\pm$2.28 |  0.89$\pm$0.01 | 4.358(67)e+37
B371 | 20210928 | 59485.786347303 | 412.55 | 7.12 |  86.56$\pm$1.36 |  0.62$\pm$9.71 | 1.724(28)e+38 | 6.897(112)e+37 | 500 | 6.49 |  86.62$\pm$2.29 |  0.56$\pm$0.01 | 6.908(112)e+37
B372 | 20210928 | 59485.786668691 | 412.55 | 2.30 |  23.50$\pm$2.82 |  0.05$\pm$6.48 | 1.511(28)e+37 | 6.046(112)e+36 | 450 | 1.84 |  25.20$\pm$5.61 |  0.05$\pm$0.01 | 5.139(101)e+36
B373 | 20210928 | 59485.786669387 | 412.55 | 2.50 |  19.60$\pm$4.39 |  0.05$\pm$10.99 | 1.372(28)e+37 | 5.486(112)e+36 | 200 | 2.72 |  31.11$\pm$7.49 |  0.08$\pm$0.01 | 4.165(90)e+36
B374 | 20210928 | 59485.786669870 | 412.55 | 2.40 |  21.65$\pm$0.14 |  0.05$\pm$0.33 | 1.456(28)e+37 | 5.822(112)e+36 | 250 | 2.91 |  38.54$\pm$0.78 |  0.11$\pm$0.01 | 6.886(112)e+36
B375 | 20210928 | 59485.786676397 | 412.55 | 3.70 |  16.21$\pm$0.34 |  0.06$\pm$1.27 | 1.679(28)e+37 | 6.718(112)e+36 | 150 | 4.79 |  36.88$\pm$0.8 |  0.18$\pm$0.01 | 6.516(101)e+36
B376 | 20210928 | 59485.786677166 | 412.55 | 2.77 |  13.70$\pm$0.13 |  0.04$\pm$0.37 | 1.064(28)e+37 | 4.254(112)e+36 | 200 | 2.32 |  31.04$\pm$0.58 |  0.07$\pm$0.01 | 3.538(45)e+36
B377 | 20210928 | 59485.786677543 | 412.55 | 5.14 |  276.75$\pm$0.09 |  1.42$\pm$0.45 | 3.980(62)e+38 | 1.592(25)e+38 | 250 | 4.55 |  663.82$\pm$0.18 |  3.02$\pm$0.04 | 1.858(27)e+38
B378 | 20210928 | 59485.786758962 | 412.55 | 7.21 |  33.40$\pm$0.66 |  0.24$\pm$4.78 | 6.746(112)e+37 | 2.698(45)e+37 | 350 | 6.61 |  43.43$\pm$1.3 |  0.29$\pm$0.01 | 2.469(39)e+37
B379 | 20210928 | 59485.787137935 | 412.55 | 4.18 |  14.13$\pm$5.49 |  0.06$\pm$22.93 | 1.651(28)e+37 | 6.606(112)e+36 | 100 | 3.17 |  66.04$\pm$11.86 |  0.21$\pm$0.01 | 5.150(134)e+36
B380 | 20210928 | 59485.787373878 | 412.55 | 11.10 |  47.49$\pm$4.49 |  0.53$\pm$49.82 | 1.475(22)e+38 | 5.900(90)e+37 | 200 | 9.16 |  123.40$\pm$8.1 |  1.13$\pm$0.02 | 5.558(78)e+37
B381 | 20210928 | 59485.787374620 | 412.55 | 2.74 |  14.26$\pm$0.19 |  0.04$\pm$0.52 | 1.092(28)e+37 | 4.366(112)e+36 | 100 | 4.87 |  43.61$\pm$0.27 |  0.21$\pm$0.01 | 5.217(134)e+36
B382 | 20210928 | 59485.787503409 | 412.55 | 3.30 |  22.72$\pm$0.15 |  0.08$\pm$0.49 | 2.099(28)e+37 | 8.397(112)e+36 | 150 | 3.86 |  54.76$\pm$0.35 |  0.21$\pm$0.01 | 7.792(101)e+36
B383 | 20210928 | 59485.787584178 | 412.55 | 2.05 |  26.37$\pm$1.52 |  0.05$\pm$3.1 | 1.511(28)e+37 | 6.046(112)e+36 | 250 | 1.91 |  42.39$\pm$1.93 |  0.08$\pm$0.01 | 4.982(56)e+36
B384 | 20210928 | 59485.787584405 | 412.55 | 3.40 |  288.24$\pm$0.2 |  0.98$\pm$0.68 | 2.743(42)e+38 | 1.097(17)e+38 | 500 | 3.05 |  288.06$\pm$0.53 |  0.88$\pm$0.01 | 1.079(16)e+38
B385 | 20210928 | 59485.787585074 | 412.55 | 7.26 |  72.55$\pm$0.09 |  0.53$\pm$0.68 | 1.475(22)e+38 | 5.900(90)e+37 | 300 | 6.64 |  145.22$\pm$0.56 |  0.96$\pm$0.01 | 7.114(101)e+37
B386 | 20210928 | 59485.787641050 | 412.55 | 8.72 |  114.07$\pm$0.14 |  1.00$\pm$1.19 | 2.785(42)e+38 | 1.114(17)e+38 | 350 | 8.11 |  158.41$\pm$0.39 |  1.28$\pm$0.02 | 1.106(16)e+38
B387 | 20210928 | 59485.787641459 | 412.55 | 3.03 |  15.19$\pm$1.93 |  0.05$\pm$5.84 | 1.288(28)e+37 | 5.150(112)e+36 | 200 | 2.41 |  41.98$\pm$2.12 |  0.10$\pm$0.01 | 4.971(90)e+36
B388 | 20210928 | 59485.787641655 | 412.55 | 9.68 |  21.48$\pm$1.18 |  0.21$\pm$11.48 | 5.822(84)e+37 | 2.329(34)e+37 | 250 | 9.13 |  51.75$\pm$1.32 |  0.47$\pm$0.01 | 2.905(39)e+37
B389 | 20210928 | 59485.787870470 | 412.55 | 5.02 |  374.99$\pm$0.61 |  1.88$\pm$3.04 | 5.268(81)e+38 | 2.107(32)e+38 | 400 | 4.53 |  468.15$\pm$1.58 |  2.12$\pm$0.03 | 2.084(31)e+38
B390 | 20210928 | 59485.787931315 | 412.55 | 3.27 |  46.74$\pm$0.16 |  0.15$\pm$0.52 | 4.282(56)e+37 | 1.713(22)e+37 | 200 | 3.18 |  113.53$\pm$0.43 |  0.36$\pm$0.01 | 1.778(27)e+37
B391 | 20210928 | 59485.787940133 | 412.55 | 4.68 |  29.48$\pm$4.48 |  0.14$\pm$20.98 | 3.863(56)e+37 | 1.545(22)e+37 | 150 | 5.25 |  81.59$\pm$7.0 |  0.43$\pm$0.01 | 1.579(24)e+37
B392 | 20210928 | 59485.787940379 | 412.55 | 2.98 |  12.42$\pm$3.04 |  0.04$\pm$9.04 | 1.036(28)e+37 | 4.142(112)e+36 | 100 | 2.09 |  57.53$\pm$3.48 |  0.12$\pm$0.01 | 2.956(67)e+36
B393 | 20210928 | 59485.787966477 | 412.55 | 4.92 |  17.90$\pm$2.0 |  0.09$\pm$9.83 | 2.463(28)e+37 | 9.853(112)e+36 | 250 | 3.50 |  41.32$\pm$5.04 |  0.14$\pm$0.01 | 8.901(112)e+36
B394 | 20210928 | 59485.787967223 | 412.55 | 5.10 |  189.12$\pm$1.8 |  0.96$\pm$9.15 | 2.698(42)e+38 | 1.079(17)e+38 | 350 | 5.12 |  265.72$\pm$1.8 |  1.36$\pm$0.02 | 1.170(17)e+38
B395 | 20210928 | 59485.788034031 | 412.55 | 4.16 |  99.97$\pm$2.83 |  0.42$\pm$11.78 | 1.164(17)e+38 | 4.658(67)e+37 | 200 | 3.84 |  252.16$\pm$4.8 |  0.97$\pm$0.01 | 4.765(72)e+37
B396 | 20210928 | 59485.788222138 | 412.55 | 5.42 |  18.08$\pm$3.28 |  0.10$\pm$17.79 | 2.743(56)e+37 | 1.097(22)e+37 | 200 | 4.95 |  44.72$\pm$4.3 |  0.22$\pm$0.01 | 1.088(18)e+37
B397 | 20210928 | 59485.788432963 | 412.55 | 3.51 |  47.31$\pm$2.14 |  0.17$\pm$7.5 | 4.646(56)e+37 | 1.858(22)e+37 | 200 | 3.07 |  91.37$\pm$2.81 |  0.28$\pm$0.01 | 1.379(22)e+37
B398 | 20210928 | 59485.788433614 | 412.55 | 2.70 |  20.77$\pm$0.7 |  0.06$\pm$1.88 | 1.567(28)e+37 | 6.270(112)e+36 | 300 | 2.83 |  32.46$\pm$1.67 |  0.09$\pm$0.01 | 6.785(67)e+36
B399 | 20210928 | 59485.788466366 | 412.55 | 5.36 |  88.58$\pm$0.32 |  0.48$\pm$1.73 | 1.330(20)e+38 | 5.318(78)e+37 | 500 | 4.91 |  88.36$\pm$0.53 |  0.43$\pm$0.01 | 5.329(78)e+37
B400 | 20210928 | 59485.788541618 | 412.55 | 8.15 |  210.76$\pm$1.21 |  1.72$\pm$9.84 | 4.809(73)e+38 | 1.924(29)e+38 | 500 | 7.41 |  210.48$\pm$2.64 |  1.56$\pm$0.02 | 1.917(29)e+38
B401 | 20210928 | 59485.788636494 | 412.55 | 4.36 |  133.13$\pm$2.86 |  0.58$\pm$12.44 | 1.623(25)e+38 | 6.494(101)e+37 | 300 | 3.95 |  208.21$\pm$1.2 |  0.82$\pm$0.01 | 6.059(87)e+37
B402 | 20210928 | 59485.788637770 | 412.55 | 9.61 |  72.39$\pm$3.77 |  0.70$\pm$36.21 | 1.948(28)e+38 | 7.792(112)e+37 | 250 | 9.07 |  124.48$\pm$3.76 |  1.13$\pm$0.02 | 6.936(106)e+37
B403 | 20210928 | 59485.788792964 | 412.55 | 4.88 |  29.93$\pm$0.69 |  0.15$\pm$3.39 | 4.087(56)e+37 | 1.635(22)e+37 | 350 | 4.42 |  39.96$\pm$1.12 |  0.18$\pm$0.01 | 1.520(24)e+37
B404 | 20210928 | 59485.788927661 | 412.55 | 2.37 |  10.96$\pm$0.39 |  0.03$\pm$0.93 | 7.278(1)e+36 | 2.911(1)e+36 | 200 | 1.89 |  26.05$\pm$0.94 |  0.05$\pm$0.01 | 2.418(45)e+36
B405 | 20210928 | 59485.788953178 | 412.55 | 4.01 |  47.93$\pm$0.11 |  0.19$\pm$0.43 | 5.374(84)e+37 | 2.150(34)e+37 | 200 | 3.62 |  120.16$\pm$5.73 |  0.43$\pm$0.01 | 2.136(31)e+37
B406 | 20210928 | 59485.789051820 | 412.55 | 1.87 |  10.68$\pm$0.26 |  0.02$\pm$0.5 | 5.598(1)e+36 | 2.239(1)e+36 | 200 | 2.67 |  28.97$\pm$0.26 |  0.08$\pm$0.01 | 3.807(45)e+36
B407 | 20210928 | 59485.789052120 | 412.55 | 3.77 |  32.10$\pm$0.25 |  0.12$\pm$0.95 | 3.387(56)e+37 | 1.355(22)e+37 | 400 | 3.05 |  36.70$\pm$0.62 |  0.11$\pm$0.01 | 1.102(18)e+37
B408 | 20210928 | 59485.789112198 | 412.55 | 2.24 |  409.89$\pm$0.11 |  0.92$\pm$0.24 | 2.570(39)e+38 | 1.028(16)e+38 | 400 | 1.99 |  514.27$\pm$0.26 |  1.03$\pm$0.02 | 1.008(15)e+38
B409 | 20210928 | 59485.789288308 | 412.55 | 10.52 |  247.06$\pm$0.52 |  2.60$\pm$5.43 | 7.278(112)e+38 | 2.911(45)e+38 | 450 | 10.40 |  265.17$\pm$1.01 |  2.76$\pm$0.04 | 3.051(43)e+38
B410 | 20210928 | 59485.789422524 | 412.55 | 4.54 |  71.42$\pm$0.92 |  0.32$\pm$4.19 | 9.069(140)e+37 | 3.628(56)e+37 | 300 | 4.31 |  141.62$\pm$2.7 |  0.61$\pm$0.01 | 4.501(60)e+37
B411 | 20210928 | 59485.789519374 | 412.55 | 14.24 |  163.15$\pm$0.06 |  2.32$\pm$0.83 | 6.505(95)e+38 | 2.602(38)e+38 | 450 | 12.15 |  179.72$\pm$0.93 |  2.18$\pm$0.03 | 2.416(35)e+38
B412 | 20210928 | 59485.789595364 | 412.55 | 5.20 |  34.99$\pm$6.74 |  0.18$\pm$35.07 | 5.094(84)e+37 | 2.038(34)e+37 | 250 | 4.28 |  57.66$\pm$8.06 |  0.25$\pm$0.01 | 1.517(22)e+37
B413 | 20210928 | 59485.789597732 | 412.55 | 6.61 |  107.32$\pm$2.78 |  0.71$\pm$18.38 | 1.984(28)e+38 | 7.938(112)e+37 | 450 | 5.99 |  119.46$\pm$4.28 |  0.71$\pm$0.01 | 7.910(111)e+37
B414 | 20210928 | 59485.789876527 | 412.55 | 6.25 |  262.59$\pm$2.48 |  1.64$\pm$15.49 | 4.593(67)e+38 | 1.837(27)e+38 | 450 | 5.73 |  288.63$\pm$4.37 |  1.65$\pm$0.02 | 1.829(26)e+38
B415 | 20210928 | 59485.789908595 | 412.55 | 3.28 |  29.26$\pm$0.47 |  0.10$\pm$1.55 | 2.687(28)e+37 | 1.075(11)e+37 | 250 | 2.96 |  60.85$\pm$1.75 |  0.18$\pm$0.01 | 1.108(17)e+37
B416 | 20210928 | 59485.789992602 | 412.55 | 3.78 |  29.66$\pm$0.45 |  0.11$\pm$1.7 | 3.135(56)e+37 | 1.254(22)e+37 | 200 | 3.42 |  68.09$\pm$1.16 |  0.23$\pm$0.01 | 1.146(18)e+37
B417 | 20210928 | 59485.790000292 | 412.55 | 4.16 |  472.85$\pm$1.29 |  1.97$\pm$5.36 | 5.506(81)e+38 | 2.202(32)e+38 | 450 | 3.85 |  509.89$\pm$2.53 |  1.96$\pm$0.03 | 2.174(31)e+38
B418 | 20210928 | 59485.790169595 | 412.55 | 4.10 |  16.83$\pm$1.06 |  0.07$\pm$4.37 | 1.931(28)e+37 | 7.725(112)e+36 | 250 | 2.55 |  33.92$\pm$3.38 |  0.09$\pm$0.01 | 5.318(56)e+36
B419 | 20210928 | 59485.790171757 | 412.55 | 7.19 |  110.04$\pm$3.1 |  0.79$\pm$22.25 | 2.214(34)e+38 | 8.856(134)e+37 | 500 | 6.55 |  110.47$\pm$4.12 |  0.72$\pm$0.01 | 8.901(134)e+37
B420 | 20210928 | 59485.790174103 | 412.55 | 5.71 |  39.07$\pm$0.27 |  0.22$\pm$1.56 | 6.242(84)e+37 | 2.497(34)e+37 | 200 | 5.73 |  95.00$\pm$1.54 |  0.54$\pm$0.01 | 2.678(40)e+37
B421 | 20210928 | 59485.790194984 | 412.55 | 5.15 |  51.68$\pm$0.25 |  0.27$\pm$1.3 | 7.445(112)e+37 | 2.978(45)e+37 | 400 | 4.67 |  67.32$\pm$0.64 |  0.31$\pm$0.01 | 3.090(45)e+37
B422 | 20210928 | 59485.790199999 | 412.55 | 10.70 |  139.35$\pm$1.72 |  1.49$\pm$18.39 | 4.173(62)e+38 | 1.669(25)e+38 | 500 | 9.79 |  139.43$\pm$2.19 |  1.37$\pm$0.02 | 1.678(25)e+38
B423 | 20210928 | 59485.790201562 | 412.55 | 3.57 |  14.30$\pm$0.7 |  0.05$\pm$2.51 | 1.428(28)e+37 | 5.710(112)e+36 | 150 | 3.49 |  26.38$\pm$1.47 |  0.09$\pm$0.01 | 3.392(34)e+36
B424 | 20210928 | 59485.790201885 | 412.55 | 4.93 |  162.19$\pm$0.66 |  0.80$\pm$3.27 | 2.239(34)e+38 | 8.957(134)e+37 | 350 | 4.62 |  258.75$\pm$0.84 |  1.19$\pm$0.02 | 1.028(13)e+38
B425 | 20210928 | 59485.790382823 | 412.55 | 4.79 |  26.11$\pm$0.65 |  0.12$\pm$3.12 | 3.499(56)e+37 | 1.400(22)e+37 | 150 | 4.63 |  75.47$\pm$1.69 |  0.35$\pm$0.01 | 1.290(17)e+37
B426 | 20210928 | 59485.790383429 | 412.55 | 12.43 |  181.85$\pm$0.18 |  2.26$\pm$2.19 | 6.326(92)e+38 | 2.530(37)e+38 | 400 | 8.54 |  294.06$\pm$0.29 |  2.51$\pm$0.04 | 2.470(36)e+38
B427 | 20210928 | 59485.790383879 | 412.55 | 3.80 |  67.18$\pm$0.11 |  0.26$\pm$0.41 | 7.138(112)e+37 | 2.855(45)e+37 | 200 | 3.52 |  174.63$\pm$0.19 |  0.61$\pm$0.01 | 3.018(40)e+37
B428 | 20210928 | 59485.790386698 | 412.55 | 8.31 |  70.63$\pm$0.21 |  0.59$\pm$1.77 | 1.643(22)e+38 | 6.572(90)e+37 | 250 | 7.77 |  161.19$\pm$0.73 |  1.25$\pm$0.02 | 7.697(101)e+37
B429 | 20210928 | 59485.790407997 | 412.55 | 4.07 |  121.62$\pm$0.31 |  0.50$\pm$1.26 | 1.386(20)e+38 | 5.542(78)e+37 | 300 | 3.56 |  248.16$\pm$0.61 |  0.88$\pm$0.01 | 6.516(87)e+37
B430 | 20210928 | 59485.790691490 | 412.55 | 3.66 |  43.96$\pm$0.75 |  0.16$\pm$2.76 | 4.506(56)e+37 | 1.802(22)e+37 | 300 | 3.95 |  64.86$\pm$1.14 |  0.26$\pm$0.01 | 1.888(27)e+37
B431 | 20210928 | 59485.790771071 | 412.55 | 8.30 |  67.37$\pm$0.73 |  0.56$\pm$6.04 | 1.565(22)e+38 | 6.259(90)e+37 | 500 | 7.58 |  67.40$\pm$0.81 |  0.51$\pm$0.01 | 6.281(90)e+37
B432 | 20210928 | 59485.791275255 | 412.55 | 3.26 |  28.79$\pm$0.29 |  0.09$\pm$0.95 | 2.631(28)e+37 | 1.052(11)e+37 | 300 | 2.57 |  55.90$\pm$0.76 |  0.14$\pm$0.01 | 1.061(13)e+37
B433 | 20210928 | 59485.791286990 | 412.55 | 6.08 |  37.64$\pm$0.94 |  0.23$\pm$5.7 | 6.410(84)e+37 | 2.564(34)e+37 | 250 | 5.59 |  85.12$\pm$1.51 |  0.48$\pm$0.01 | 2.922(39)e+37
B434 | 20210928 | 59485.791437934 | 412.55 | 2.36 |  39.77$\pm$5.5 |  0.09$\pm$13.0 | 2.631(28)e+37 | 1.052(11)e+37 | 200 | 2.01 |  72.85$\pm$5.5 |  0.15$\pm$0.01 | 7.210(134)e+36
B435 | 20210928 | 59485.791439085 | 412.55 | 6.31 |  67.98$\pm$0.91 |  0.43$\pm$5.76 | 1.201(17)e+38 | 4.803(67)e+37 | 250 | 6.01 |  153.72$\pm$1.34 |  0.92$\pm$0.01 | 5.681(69)e+37
B436 | 20210928 | 59485.791471949 | 412.55 | 9.97 |  175.60$\pm$2.2 |  1.75$\pm$21.96 | 4.898(70)e+38 | 1.959(28)e+38 | 400 | 8.56 |  225.89$\pm$3.64 |  1.93$\pm$0.03 | 1.902(28)e+38
B437 | 20210928 | 59485.791520195 | 412.55 | 5.05 |  148.98$\pm$1.23 |  0.75$\pm$6.21 | 2.105(31)e+38 | 8.420(123)e+37 | 500 | 4.61 |  149.18$\pm$2.07 |  0.69$\pm$0.01 | 8.453(123)e+37
B438 | 20210928 | 59485.791520618 | 412.55 | 4.13 |  137.32$\pm$0.14 |  0.57$\pm$0.56 | 1.587(22)e+38 | 6.348(90)e+37 | 500 | 3.75 |  137.31$\pm$0.3 |  0.52$\pm$0.01 | 6.337(90)e+37
B439 | 20210928 | 59485.791725482 | 412.55 | 7.06 |  29.32$\pm$0.15 |  0.21$\pm$1.05 | 5.794(84)e+37 | 2.318(34)e+37 | 150 | 5.63 |  86.39$\pm$0.97 |  0.49$\pm$0.01 | 1.792(26)e+37
B440 | 20210928 | 59485.791736554 | 412.55 | 6.81 |  149.50$\pm$0.27 |  1.02$\pm$1.85 | 2.849(42)e+38 | 1.140(17)e+38 | 500 | 6.18 |  149.69$\pm$0.69 |  0.93$\pm$0.01 | 1.138(17)e+38
B441 | 20210928 | 59485.791736981 | 412.55 | 6.63 |  311.81$\pm$4.77 |  2.07$\pm$31.64 | 5.788(84)e+38 | 2.315(34)e+38 | 500 | 5.88 |  312.03$\pm$5.04 |  1.84$\pm$0.03 | 2.257(34)e+38
B442 | 20210928 | 59485.791800270 | 412.55 | 14.85 |  150.12$\pm$0.45 |  2.23$\pm$6.62 | 6.239(87)e+38 | 2.496(35)e+38 | 300 | 13.93 |  241.27$\pm$1.12 |  3.36$\pm$0.04 | 2.478(33)e+38
B443 | 20210928 | 59485.792142072 | 412.55 | 4.24 |  16.97$\pm$2.93 |  0.07$\pm$12.42 | 2.015(28)e+37 | 8.061(112)e+36 | 200 | 2.01 |  41.65$\pm$2.93 |  0.08$\pm$0.01 | 4.120(45)e+36
B444 | 20210928 | 59485.792142550 | 412.55 | 5.12 |  14.26$\pm$2.34 |  0.07$\pm$11.98 | 2.043(28)e+37 | 8.173(112)e+36 | 250 | 3.95 |  21.00$\pm$1.6 |  0.08$\pm$0.01 | 5.094(56)e+36
B445 | 20210928 | 59485.792398737 | 412.55 | 2.84 |  237.54$\pm$0.83 |  0.68$\pm$2.36 | 1.889(28)e+38 | 7.557(112)e+37 | 450 | 2.53 |  254.76$\pm$1.21 |  0.64$\pm$0.01 | 7.134(101)e+37
B446 | 20210928 | 59485.792398905 | 412.55 | 3.17 |  16.08$\pm$3.37 |  0.05$\pm$10.69 | 1.428(28)e+37 | 5.710(112)e+36 | 200 | 3.49 |  33.66$\pm$6.58 |  0.12$\pm$0.01 | 5.777(90)e+36
B447 | 20210928 | 59485.792535659 | 412.55 | 4.54 |  261.18$\pm$5.65 |  1.19$\pm$25.68 | 3.322(45)e+38 | 1.329(18)e+38 | 400 | 4.08 |  310.57$\pm$13.92 |  1.27$\pm$0.02 | 1.248(17)e+38
B448 | 20210928 | 59485.792585319 | 412.55 | 3.53 |  18.99$\pm$0.53 |  0.07$\pm$1.88 | 1.875(28)e+37 | 7.501(112)e+36 | 200 | 3.92 |  44.10$\pm$1.23 |  0.17$\pm$0.01 | 8.509(134)e+36
B449 | 20210928 | 59485.792585520 | 412.55 | 3.56 |  37.33$\pm$0.19 |  0.13$\pm$0.68 | 3.723(56)e+37 | 1.489(22)e+37 | 200 | 3.39 |  93.96$\pm$0.46 |  0.32$\pm$0.01 | 1.567(22)e+37
B450 | 20210928 | 59485.793049727 | 412.55 | 5.46 |  415.08$\pm$0.96 |  2.27$\pm$5.23 | 6.343(87)e+38 | 2.537(35)e+38 | 400 | 4.89 |  523.57$\pm$2.3 |  2.56$\pm$0.04 | 2.517(35)e+38
B451 | 20210928 | 59485.793122216 | 412.55 | 5.21 |  202.42$\pm$0.69 |  1.06$\pm$3.6 | 2.953(42)e+38 | 1.181(17)e+38 | 250 | 4.67 |  480.82$\pm$1.74 |  2.25$\pm$0.03 | 1.380(18)e+38
B452 | 20210928 | 59485.793126806 | 412.55 | 8.62 |  14.50$\pm$3.98 |  0.12$\pm$34.31 | 3.499(28)e+37 | 1.400(11)e+37 | 200 | 7.66 |  38.01$\pm$4.8 |  0.29$\pm$0.01 | 1.431(21)e+37
B453 | 20210928 | 59485.793213406 | 412.55 | 3.81 |  19.95$\pm$0.35 |  0.08$\pm$1.33 | 2.127(28)e+37 | 8.509(112)e+36 | 200 | 3.17 |  50.62$\pm$0.65 |  0.16$\pm$0.01 | 7.882(90)e+36