# Using Neural Networks to Differentiate Newly Discovered BL Lacs and FSRQs
among the 4FGL Unassociated Sources Employing Gamma-ray, X-ray, UV/Optical and
IR Data

Amanpreet Kaur Department of Astronomy and Astrophysics
Pennsylvania State University University Park, PA 16802, USA  Stephen Kerby
Department of Astronomy and Astrophysics
Pennsylvania State University University Park, PA 16802, USA  Abraham D.
Falcone Department of Astronomy and Astrophysics
Pennsylvania State University University Park, PA 16802, USA

###### Abstract

Among the $\sim$ 2157 unassociated sources in the third data release (DR3) of
the fourth $Fermi$ catalog, $\sim$ 1200 were observed with the Neil Gehrels
$Swift$ Observatory pointed instruments. These observations yielded 238 high
S/N X-ray sources within the 95% $Fermi$ uncertainty regions. Recently, Kerby
et al. (2021) employed neural networks to find blazar candidates among these
238 X-ray counterparts to the 4FGL unassociated sources and found 112 likely
blazar counterpart sources. A complete sample of blazars, along with their sub
classification, is a necessary step to help understand the puzzle of the
blazar sequence and for the overall completeness of the gamma-ray emitting
blazar class in the $Fermi$ catalog. We employed a multi-perceptron neural
network classifier to identify FSRQs and BL Lacs among these 112 blazar
candidates using the gamma-ray, X-ray, UV/optical and IR properties. This
classifier provided probability estimates for each source to be associated
with one or the other category, such that Pfsrq represents the probability for
a source to be associated with the FSRQ subclass. Using this approach, 4 FSRQs
and 50 BL Lacs are classified as such with $>99\%$ confidence, while the
remaining 58 blazars could not be unambiguously classified as either BL Lac or
FSRQ.

††facilities: Fermi, Swift(XRT and UVOT), WISE††software: Astropy (Astropy
Collaboration et al., 2013), numpy (Harris et al., 2020), scikitlearn
(Pedregosa et al., 2011), Topcat (Taylor, 2005)

##  1 Introduction

The third release (DR3) of the fourth catalog (4FGL, Abdollahi et al., 2022))
of $Fermi$ Large Area Telescope (LAT) catalog with 6658 sources contains
approximately 2157 unidentified/unassociated sources (i.e. approximately one-
third are unassociated). The lack of identification for so many sources
represents a major gap in our understanding of the high energy universe.
Therefore, exploring the nature of these sources remains fundamental to
understanding the gamma-ray universe. Most of the identified objects in the
catalog are blazars ($\sim$75%), and the others are pulsars, X-ray binaries,
supernova remnants, novae, GRBs etc. The brighter of these blazars offer the
opportunity to study the more extreme gamma-ray emitters on an individual
basis, while the lower-significance and dimmer new blazars offer the
opportunity to explore the population in a more complete manner by extending
the discovery space to lower fluxes. It is likely that the unassociated source
population contains a significant number of blazars, which are missing
associations for various reasons such as being on the fainter side or extreme
nature etc. In general, blazars are defined as a powerful subclass of the
Active Galactic Nuclei which have their jets pointing along our line of sight
(Blandford & Rees, 1978). The overall spectral energy distribution of these
sources display a double-bump structure, such that the synchrotron emission
process is responsible for the lower energy bump (Radio to X-ray) and the
higher one (X-ray rays to gamma-rays) is attributed to either synchrotron self
Compton mechanism and/or external inverse Compton processes, and/or hadronic
processes such as proton synchrotron (e.g., see Böttcher et al., 2013; van den
Berg et al., 2019). Blazars are further classified into two subclasses based
on their optical spectra; Flat Spectrum Radio Quasars (FSRQs) and BL Lacertae
Objects (BL Lacs). The former exhibit broad emission lines, whereas the BL
Lacs show no lines or narrow lines (equivalent width $<$ 5 Å) (Stickel et al.,
1991). Understanding the origin of the differences between the two subclasses
of blazars has been one of the open questions in the field. The idea of the
blazar sequence, first described by Fossati et al. (1998) and re-visited by
Ghisellini & Tavecchio (2008); Ghisellini et al. (2017), revealed that the
most luminous blazars possess lower synchrotron frequencies, which often is
the case in FSRQs, and vice versa for BL Lacs. Based on this principle, Abdo
et al. (2010) divided blazars into three categories based on their synchrotron
peak frequencies ($\nu^{pk}_{syn}<$) as follows: low-synchrotron-peaked
blazars; LSP: $\nu^{pk}_{syn}<$ 14, ISP: $14>\nu^{pk}_{syn}>$ 15 and HSP:
$\nu^{pk}_{syn}>$ 15 such that most of the FSRQs belong to the LSP category
and BL Lacs contribute to the ISP and HSP. However, Giommi et al. (2012) argue
that the blazar sequence can be an effect of selection bias and also this
sequence has been challenged by finding highly-luminous, high-synchrotron-
peaked blazars, e.g. Padovani et al. (2012). Moreover, Ghisellini et al.
(1998) suggested a unified scheme for blazars in which FSRQs eventually evolve
into BL Lacs once their accretion disk is exhausted. The observational
evidence of finding FSRQs at typically higher redshifts than that of BL Lacs
supports this scenario. In the past few years, several ($\sim$30) BL Lacs have
been found at high redshifts e.g., (Rau et al., 2012; Kaur et al., 2017b, a;
Rajagopal et al., 2020; Paliya et al., 2020; Koptelova & Hwang, 2022). The
blazar parameter space and the theories regarding their evolution need to be
further explored by obtaining a more complete sample of both types of blazars.
As an example, also see Paliya et al. (2021) to see bimodality in blazars
based on the disk luminosity. Therefore, the rather large unassociated 4FGL
source list needs to be probed to find additional blazars, which then need to
be classified as FSRQs or BL Lacs using spectroscopic observations. Ideally
one would also obtain and analyze broadband multiwavelength data for these
gamma-ray sources to identify and evaluate possible counterparts, which would
be take multiple years for completion.
The Neil Gehrels Swift observatory ($Swift$) has completed X-ray and
UV/optical observations for $\sim$ 1000 unassociated sources through a fill-in
program (Falcone et al., 2020) based on the following criteria: (i) the 95%
$Fermi$ uncertainty region associated with the source is less than the Swift-
XRT field of view, which is 23 arcmin across, (ii) the source was not on the
galactic ridge where diffuse background could lead to false associations. With
a typical exposure time of $\sim$4 ksec, these observations resulted in a
total of 238 X-ray counterparts found (with S/N $\geq$ 4) within the 95%
uncertainty regions of 208 $Fermi$ 4FGL-DR3 sources. The photometric data
including X-ray images, detected sources, count rates, SNR etc. for all of
these unassociated sources are available on the public web page
http://www.swift.psu.edu/unassociated/.

In the past few years, various authors explored using machine learning to
classify blazars such as Doert & Errando (2014); Salvetti et al. (2017); Kang
et al. (2019); Kaur et al. (2019, 2019); Kovačević et al. (2020); Chiaro et
al. (2021). Most recently, (Kerby et al., 2021) (K21 from now on) has found
blazar as well as pulsar candidates among these 238 X-ray sources employing
the gamma-ray, X-ray and UV/Optical properties using a method of neural
networks. The objective of this letter is to classify these blazar candidates
further into their subclasses; FSRQs and BL Lacs using a neural network
classifier employing the data from gamma-ray, X-ray, UV/Opt, and IR regimes.
This letter is organized as follows: Section 2 describes the multi-wavelength
sample selection criteria for this work, Section 3 explains the analysis
procedure for classification, and Section 4 describes the results. The
concluding remarks, as well as discussion in regard to the results obtained,
are provided in Section 5.

##  2 Observations and Data Selection

###  2.1 Sample Selection - Blazar Candidates

The source sample for this work is derived from the work of K21, therefore the
basic analysis steps are only briefly described in this section. The thorough
details of each step for analysis are already explained in K21.

From the list of $\sim$ 2157 4FGL unassociated sources, the Neil Gehrels Swift
Observatory ($Swift$) had completed observations for $\sim$ 500 sources by
February 1, 2021 with an average exposure time of 4 ksec per source to find
potential X-ray counterparts. A total of 238 X-ray sources with SNR$\geq$4
were found among the 208 4FGL unassociated fields within their 95% uncertainty
regions. Out of these, more than one X-ray source was found within the 95%
regions of the 14 4FGL fields, whereas the rest have exactly one X-ray source
within this region. The basic photometric results such as the X-ray Right
Ascension, X-ray Declination, Count Rate and SNR are made available to the
community on the webpage111https://www.swift.psu.edu/unassociated. K21
collected these data for 238 X-ray sources and conducted X-ray spectral
analysis fitting `powerlaw` models using `XSpec v12.10`(Arnaud, 1996) to
obtain spectral parameters such as spectral indices and X-ray fluxes in the
0.3-10 keV band. A thorough description of the analysis procedure is provided
in Section 3.1 in K21. Whenever $Swift$ observes using the X-ray telescope,
observations are also conducted with at least one out of the six UV-optical
filters (v, b, u, uvw1, uvm2, uvw2; ranging from 5468Åto 1928Å) mounted on the
UltraViolet Optical Telescope (UVOT)(Roming et al., 2005). For any UV/optical
source(s) found within the X-ray positional uncertainty regions, a photometric
analysis was conducted using `uvotsource` task in the $Swift$ data analysis
pipeline which provides the magnitudes in the AB system. Whenever no source
was found, an upper limit was calculated. In a few cases, there were
indistinguishable multiple sources within the X-ray positional uncertainty
regions, these sources were removed from our final list of uassociated
sources. All the details of this analysis are provided in Section 2.2 in K21.
Finally, these magnitudes were then converted into equivalent of the Johnson V
magnitudes for uniformity across the source list, the details of this
conversion as well as all the assumptions are clearly laid out in section 3.2
in K21. In the end, the final sample comprised 205 sources corresponding to
188 4FGL unassociated fields for which X-ray as well as UV-opt data were
available. Out of these, 174 had single X-ray and UV sources in their
respective 4FGL uncertainty regions and 14 had multiple X-ray/UV sources.
For these 205 sources, K21 conducted a neural network analysis to find that
132 were likely blazars with probabilities, Pbzr, $\geq$99%, where Pbzr is the
probability for a source to be associated with a blazar class as provided by
the underlying neural network method. The two subclasses of the gamma-ray
emitting blazars display distinct colors when compared in a 2-dimensional
color-color plot using the publicly available data, AllWISE(Cutri & al., 2013)
obtained with the Wide-field Infrared Survey Explorer (WISE) (Wright et al.,
2010). These authors plotted color indices, `w1-w2` vs `w2-w3`, (`w1, w2, w3`
correspond to 3.4, 4.6, 12 $\mu$m, respectively) for various known gamma-ray
emitting BL Lacs and FSRQs and found that these two sublcasses occupy
different parameter space (Massaro et al., 2011, 2012; D’Abrusco et al.,
2014). Since the objective of the work presented here is to classify the
blazar candidates into BL Lacs and FSRQs, we employ the infrared properties
along with existing gamma-ray, X-ray and UV/opt data for these sources. In
order to do so, we conducted WISE positional matches for the $Swift$-UVOT
positions within 5” (maximum XRT positional uncertainty for a given source in
our sample) for the 132 blazar candidates and found 112 matches. We note that
it is possible that a few of these WISE counterparts could be spatially
coincident with the XRT and UVOT position by a random chance, but the
probability of this is low. In order to confirm this, we used the $Swift$-XRT
blazar catalog with 2831 blazars using 15 years of data (Giommi et al., 2019).
When searched for WISE counterparts within 5” positional uncertainities, it
was found that only 22 secondary sources were found in addition to the actual
WISE counterparts for these blazars. This suggests a $\sim$ 0.7% probability
for a WISE source which can be found via chance coincidence at a random
position in the sky within a 5” uncertainty region. We, therefore, finalize
our source sample size of blazar candidates among the 4FGL unassociated source
list to 112 such that the required gamma-ray, X-ray, UV-opt and IR properties
are known for these sources. The relevant eight properties for this
classification work are as itemized below. The parameters for each training or
research source include:

  * •

Gamma-ray photon index, $\Gamma_{\gamma}$ (`PL_Index` in the 4FGL catalog)

  * •

The logarithm of gamma-ray flux, $\log{F_{\gamma}}$, in $\rm{erg/s/cm^{2}}$
(`Energy_Flux` in the 4FGL catalog)

  * •

The logarithm of X-ray to gamma-ray flux ratio, $\log{F_{X}/F_{\gamma}}$

  * •

The logarithm of V-band to gamma-ray flux ratio, $\log{F_{V}/F_{\gamma}}$.

  * •

The significance of the curvature in the gamma-ray spectrum, henceforth simply
curvature (`PLEC_SigCurv` in the 4FGL catalog)

  * •

The year-over-year gamma-ray variability index (`Variability_Index` in the
4FGL catalog)

  * •

WISE color index 1, `w1-w2` and

  * •

WISE color index 2, `w2-w3`

Normalized histograms of all parameters for both the known FSRQs and BL Lacs
and the research sample are shown in Figure 1.

Figure 1: Normalized histograms for the known BL Lacs (blue), known FSRQs
(red), and unassocicated (black line) samples.

###  2.2 Training Data: Known BL Lacs and FSRQs

In order to classify our sample of blazar candidates into the two subclasses;
BL Lacs and FSRQs, we would require a large sample of these two categories for
which the exact same gamma-ray to IR properties can be established. The neural
network described later would use the information from this known sample of
two classes to train itself to be able to distinguish between them. For this
step, we selected a sample of 427 FSRQs and 671 BL Lacs for which the relevant
multiwavelength data, i.e., the above mentioned eight properties were
available. For these blazars, all the gamma-ray properties were obtained from
the 4FGL catalog, X-ray fluxes were provided in the BZCAT (Massaro et al.,
2015), which were obtained from the ROSAT X-ray source catalog(Voges et al.,
1999). These X-ray fluxes were provided in the 0.1-2.5 keV band, but these
were converted to 0.3-10 keV for consistency using the Portable, Interactive
Multi-Mission Simulator `PIMMS`(Mukai, 1993). The photon indices were assumed
to be 2.0 and the hydrogen column densities were obtained using the LAB
survey(Kalberla et al., 2005) for the conversion process. The WISE data were
also obtained from the BZCAT catalog. The optical fluxes were obtained from
various resources such as SIMBAD Astronomical
Database222http://simbad.u-strasbg.fr/simbad/, the Sloan Digital Sky
Survey333https://www.sdss.org as well as Gaia
archive444https://gea.esac.esa.int/archive/. All the magnitudes obtained were
converted to V band using the same principles as outlined in section 3.2 in
K21, which were then converted to the respective optical flux values. Once the
training data as well as the unknown data (blazar candidates without their
subclassification) are finalized, the next step was to develop a neural
network classifier which is explained below. The eight properties for all the
sources in the source sample (112) as well as the training sample (1098) are
provided in Table 2 and Table 1, respectively. It should be noted that
variability in blazars is witnessed in both the subclasses but it is more
pronounced in the FSRQs as compared to BL Lacs possibly due to the brightness
factor (FSRQs are brighter and easily detectable). This effect is also seen in
our training sample which therefore is an efficient parameter for the
classification. Even though the Fermi data used for this work are taken and
averaged over multiple years as compared to the X-ray, UV and WISE data which
were obtained within a few hours, the signal-to-noise ratio or data quality
for all these lower energy regimes taken over a few hours is comparable to
Fermi data taken over years. Therefore, using multiwavelength data for this
classification is justified.

##  3 Analysis-Neutral Network Classification

To classify the research sample of new likely blazars into likely FSRQ and
likely BL Lacs, we applied a multi-layer perceptron (MLP) neural network
classifier (NNC) approach. Because the number of known FSRQs and BL Lacs in
our catalogs were slightly unbalanced (427 known FSRQs and 671 known BL Lacs),
we first applied Synthetic Minority Over-sampling Technique (SMOTE) (Chawla et
al., 2002) to generate additional FSRQs to create a balanced dataset made up
of real FSRQs and BL Lacs plus additional FSRQs created with a k-nearest
neighbors approach to match the distribution of real FSRQs. It is essential to
have a larger training sample for better accuracies for the classification,
therefore a technique like SMOTE is used to increase the overall sample size
instead of decreasing it. The resulting post-SMOTE distributions for all the
parameters are similar to the pre-SMOTE distributions, see Figure 2.

Figure 2: A comparison of the distributions of BL Lacs and FSRQs for each
parameter before and after applying SMOTE. It is clearly seem that the change
in distributions are minimal. The label pre corresponds to data before using
SMOTE to artificially add more data and post after the application to balance
both the classes.

To build the NNC for this research, we split the catalog of known FSRQs and BL
Lacs (plus SMOTE-generated FSRQs) into a training subsample and a validation
subsample in an 80/20 split with proportional amounts of FSRQs and BL Lacs in
each subsample. Building the NNC method, we constructed an approach where the
unassociated sources are assigned a FSRQ probability $P_{fsrq}$. The NNC has
eight input nodes (one for each parameter of the training dataset), one hidden
layer with three neurons, and one output node returning the predicted FSRQ
probability. In this research we use the `MLPClassifier` function of the
`scikit-learn` Python package for NNC training and validation, training the
NNC with the ‘adam’ optimization approach (Kingma & Ba, 2014).

To determine when to stop iterating while training the NNC, we used the Log-
Loss parameter, an error measure in binary classification approaches that is
similar to a likelihood estimator. For a sample with true classifications
$y_{i}=(0,1)$ and predicted classification $p_{i}\in[0,1]$, the Log-Loss is
given by

$L_{log}=-\sum_{i}\left(y_{i}\log(p_{i})+(1-y_{i})\log(1-p_{i})\right)$

At each iteration step in training the NNC, we calculate $L_{log}$ of both the
training and validation subsamples. As training continues, the training
subsample $L_{log}$ should continuously decrease as the NNC approaches a more
exacting fit. However, at some point the validation $L_{log}$ begins to
increase as the NNC starts to overfit the training sample and lose predictive
capabilities on unknown data points. At this point, training is stopped.

Figure 3: The fraction of the validation FSRQ (red) and BL Lac (blue)
correctly classified as such with various cutoff limits considered a success.
This plot also serve as a CDF-like representation of the validation $P_{fsrq}$
for each subclass. The green dotted line is a 50% cutoff. We interpret the two
slopes in this plot as the ability of the neural network to converge to a
probability value for a given cut off in both the source classes. This plot
shows that more BL Lacs converge to higher probabilities as compared to FSRQs,
which we also see in our results.

To evaluate the accuracy of the NNC, we applied the trained classifier to the
validation dataset of known FSRQ and BL Lac objects. Instead of establishing a
single cutoff for FSRQ/BL Lac classification, we create a cumulative
distribution function to investigate the fraction of known FSRQs and BL Lacs
classified with various confidences. For example, a perfect classification
approach would assign all validation FSRQs $P_{fsrq}=1$ and all validation BL
Lac $P_{fsrq}=0$. The CDF-like plot produced by comparing these ideal scores
to the validation $P_{fsrq}$ assigned by the NNC is shown in Figure 3. The
validation FSRQ and BL Lac are considered correctly classified if
$P_{fsrq}>0.5$ or $<0.5$ respectively, then our NNC achieves a validation
score of over 90% for both subclasses. If we require 90% confidence in our
classifications, the NNC achieves an 80% accuracy for validation BL Lac and
almost 90% accuracy for FSRQ.

##  4 Results

###  4.1 Classification Results

While the sources with $P_{fsrq}>0.5$ are more likely to be FSRQs and
$P_{fsrq}<0.5$ are more likely to be BL Lacs, we adopt a more conservative
approach when classifying; only the sources for which the $P_{fsrq}>0.99$ are
considered to be highly likely FSRQs and only sources with $P_{fsrq}<0.01$ are
classified as highly likely BL Lacs. All the other sources are termed as
ambiguous-type blazar candidates. The validation score for both the subclasses
is shown in Figure 3. This analysis resulted in 50 sources as highly likely BL
Lacs and 4 as highly likely FSRQs. In other words, we found 50 sources for
which $P_{fsrq}<0.01$ and 4 for which $P_{fsrq}>0.99$. The remaining 58
sources are labelled as being blazars whose type is ambiguous. These results
are shown in Table 3. In addition, we conducted literature search to look for
any known blazars or other sources at the UVOT positions for all these
sources. We found 19 additional blazar candidates, 10 BL Lacs and 9
FSRQs(QSOs), 2 Seyferts, one cataclysmic variable, one rationally variable
star as well as a few radio galaxies. Out of the 4 NN identified FSRQs, 2 are
independently confirmed by this literature study. This literature search was
conducted using the SIMBAD Astronomical Database (Wenger et al., 2000) as well
the latest data release (DR16) for the Sloan Digital Sky Survey database
(Ahumada et al., 2020). All these positional coincidences which yielded source
classifications as well redshifts estimates are noted in Table 3.

Figure 4: A comparison of the probabilities for a blazar to be an FSRQ,
$P_{fsrq}$ is shown resulting from the two neural network approaches; MLP and
Keras approach. It is clearly evident that the resulting highly likely FSRQs
and BL Lacs are consistent with both the approaches, thereby proving the
results of this work independent of a NNC approach.

###  4.2 Verification of the results

To verify the stability of our NNC classification scheme, we returned to the
validation step to ensure that our selection of random seed, NNC structure,
and validation subsample did not unexpectedly bias our final classifications.
To examine this possibility, we re-validated our neural network in three ways.

First, we compared our NNC classification of the unassociated sources with
another NNC approach, which employs batch normalization as well as dropping
out layers in order to make the training network more stable and train faster.
The process of batch normalization is analogous to normalization for a
dataset, where the data in a given layer is normalized with respect to its own
mean and standard deviation. This helps in the overall optimization process
since this normalized data would need fewer epochs to complete training the
underlying model (Ioffe & Szegedy, 2015) thereby making the overall training
process efficient. Furthermore, adding dropout reduces the risk of
overfitting, which is generally caused by the network learning spurious
patterns in the training data. By introducing a random dropout for a given
fraction of a layer’s input units, the chance of having these spurious
patterns involved in the overall training decreases significantly (Srivastava
et al., 2014). We applied the `keras` Application Programming Interface (API)
from the `tensorflow ver 2.6.0` library in `python 3.9.7` to construct as well
train this model. This keras NNC consisted of eight neurons (one for each
underlying parameter for providing distinction between the two subclasses)
which were batch normalized, this was followed by one hidden layer with five
neurons and the activation function `relu`. After this initial training, a
dropout layer with a standard/default rate of 30% was introduced followed by
another batch normalization process and finally the output was generated with
one neuron and the activation function `sigmoid`.
The training procedure employed the `adam` optimizer as well as the
$Log$-$Loss$ parameter just in the same way as in the case of the MLP
classifier (see Section 3) to create the final model to be applied to the
source sample. In other words, we used similar optimization as well training
procedure but employing a completely different method to test the
dependability of our results on these different approaches. If the MLP
approach we used provides comparable $P_{fsrq}$ to the Keras approach, we gain
confidence in our classifications. As Figure 4 shows, the unassociated sources
have very similar classifications in the two approaches, suggesting that our
classification results are not overly sensitive to NNC structure. It should be
noted that we emphasize the robustness of classifications in this context,
which is based on only the high confidence probabilities for each class; i.e.,
the $P_{fsrq}$ is either $\geq$ 0.99 or $\leq$ 0.01 for FSRQs or BL Lacs,
respectively. The vast majority of sources that are graded as likely FSRQ or
BL Lacs are so classified in both approaches. We also note that any two neural
network methods would not yield exactly the same results since we are using
probabilities to classify the underlying source class. However, it is
important that the high confidence source classification should be consistent
regardless of the method employed. In this case, both the methods are
consistent with each other when we confidently classify a source to be a BL
Lac or an FSRQ only when their respective probabilities are greater than or
equal to 99%. All the sources classified with $>$99% BL Lac probabilities
using Keras method are also classified as BL Lacs using MLP.
Our work does not classify a source as a BL Lac or an FSRQ with their
respective probabilities below 99% to minimize misclassification of these two
subclasses.

Figure 5: Keeping the same training and validation subsamples, the resulting
$P_{fsrq}$ values with different random seeds for NNC training are shown here.
It is clearly seen from the figure that the results are stable/consistent
irrespective of the choice of the underlying random seed, in particular, for
the highly likely FSRQs as well as BL Lacs.

Next, we varied the random seed of the training algorithm for the MLP
classifier through a range of values, executing the training step with the
same validation subsample. In this way, we can compare the validation
$P_{fsrq}$ values on a single validation dataset while varying only the random
seed of the NNC training. Figure 5 compares the $P_{fsrq}$ score of the first
of these iterations $i=0$ with nine others up to $i=10$. There are only small
changes in the resultant $P_{fsrq}$ values from one iteration to the next, so
we have confidence that our selection of random seed for NNC training did not
bias our classification results.

Finally, we examine whether our specific division of the collection of known
FSRQs and BL Lacs into specific training and validation subsamples impacted
final classification results. First, we split off 20% of the known blazars
into a ‘super-validation’ subsample. With this list serving as a proxy for the
research sample, we split the remaining known pulsars and blazars into
quintiles, then train five NNCs. Each NNC uses one quintile as a validation
subsample and the remaining as training subsample, akin to a stratified fold
cross-validation approach. After training these five NNCs, we apply each to
the super-validation sample, and compare $P_{fsrq}$ scores between iterations.
Figure 6 shows that changing the validation subsample has little effect on the
$P_{fsrq}$ results for a proxy research sample, and therefore we have little
reason to suspect that our research results are sensitive to randomness in
that way.

Figure 6: With a super-validation sample set aside, we compare $P_{fsrq}$
results for a super-validation sample, a proxy for our research sample, while
varying which fold of the remaining known blazars serves as validation
subsamples.

##  5 Discussion and Conclusions

This work identifies and classifies 4 FSRQs and 50 BL Lacs from the 112 blazar
candidates identified through X-ray counterpart searches among the 4FGL-DR3
unassociated sources by Kerby et al. (2021). In addition, upon using SIMBAD
and SDSS catalogs to conduct further searches for any known sources at the
UV/Opt positions of these sources, we found more BL Lacs, FSRQs, radio
galaxies as well as a CV and two Seyfert type I galaxies. Some of these
identifications are based on the spectroscopic data taken by various studies
as shown in Table 3 and therefore redshift estimates are provided, while the
others employed a photometric method to provide the classification as well as
the redshifts. The latter work was conducted by Chang et al. (2019) which
created a high-synchrotron peaked blazars catalog for various sources which
are coincidentally found in our sample. It should be noted that while our NN
method might not be efficient at finding each and every FSRQ or BL Lac (due to
a smaller training sample size primarily), the accuracy of each identification
is above 99%, as described earlier and is seen in Figure 3. Out of the 15
sources for which spectra were available, Figure 8b, 8e, 9a are identified as
galaxies in the SDSS catalog and these appear to have signatures of lyman
break galaxies.

Figure 7: A histogram of the validation FSRQ (red) and BL Lac (blue)
$P_{FSRQ}$ scores using the fully trained NNC.

In addition, one of the two Seyfert type I sources had an optical spectrum
available in the SDSS catalog. See Figure 9f. Figure 8c, 8f, 9c, 9d and 10a
clearly represent the FSRQ population of the blazar class and the rest are BL
Lacs. Although our source sample would ideally be comprised of only blazar
candidates, a few non-blazar sources were found to be in X-ray and UV
positional coincidence. 4FGL J1513.0-3118 is found to be a positional match
with a rotationally variable star (possibly a new gamma-ray binary); 4FGL
J1910.8+2856 with a cataclysmic variable star; and 4FGL J2351.4-2818 with a
bright Galaxy in a cluster. Further investigations of these sources at both
high and low energy regimes are required before any firm conclusions, which
are out of the scope for this work. Overall, this work yields 48%
classification of blazar candidates into BL Lacs and FSRQs such that the
former represent 45% and the latter 3% of the total classification. The rest
52% are blazars of ambiguous type based on our work, as shown in Table 3. This
work is a substantial step taken towards the completeness of the gamma-ray
emitting blazar class in the Fermi catalog. Furthermore, this work along with
(Kerby et al., 2021) has identified/classified various sources among the
unassociated Fermi catalog using the X-ray, UV/optical, and IR, along with the
gamma-ray data.

Figure 8: The spectra for various sources as obtained from the SDSS-DR16
survey catalog are shown here. Most of our NN results are further confirmed by
these spectroscopic confirmations for each subclass in the blazar category.
See Table 3 for details.  Figure 9: The spectra for various sources as
obtained from the SDSS-DR16 survey catalog are shown here. Most of our NN
results are further confirmed by these spectroscopic confirmations for each
subclass in the blazar category. One of the sources identified as FSRQ
according to NN has been found to be a Seyfert type I (Fig 9f). See Table 3
for more details.  Figure 10:  The spectra for various sources as obtained
from the SDSS-DR16 survey catalog are shown here. Most of our NN results are
further confirmed by these spectroscopic confirmations for each subclass in
the blazar category. See Table 3 for details.

The work presented in this manuscript was made possible due to the NASA
research grants 80NSSC20K0911 and 80NSSC20K1577. This publication made use of
data products from the Wide- field Infrared Survey Explorer, which is a joint
project of the University of California, Los Angeles, and the Jet Propulsion
Laboratory/California Institute of Technology, funded by the National
Aeronautics and Space Administration. The data employed in this research were
extracted from the High Energy Astrophysics Science Archive Research Center
(HEASARC), which is a service of the Astrophysics Science Division at
NASA/GSFC.

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Table 1: The 1098 sources used for training data containing BL Lacs and Flat
Spectrum Radio Quasars

Fermi | log Fγ | $\Gamma_{\gamma}$ | Variability | Curvature | log FX/F$\gamma$ | log FV/F$\gamma$ | w1-w2 | w2-w3
---|---|---|---|---|---|---|---|---
4FGL |  |  | log | log |  |  |  |
|  |  | BL Lacs |  |  |  |  |
J0001.2$-$0747 | -11.04 | 2.1 | 0.27 | 1.52 | -1.08 | -4.96 | 0.95 | 2.59
J0006.3$-$0620 | -11.81 | 2.13 | -0.06 | 1.31 | 0.06 | -4.18 | 1.14 | 2.99
J0008.0+4711 | -10.74 | 2.05 | 0.66 | 0.81 | -1.2 | -5.4 | 0.94 | 2.42
J0008.4$-$2339 | -11.63 | 1.66 | 0.47 | 1.14 | 0.35 | -4.37 | 0.55 | 1.93
J0009.1+0628 | -11.27 | 2.1 | 0.08 | 1.12 | -0.64 | -4.82 | 0.94 | 2.76
J0009.3+5030 | -10.61 | 1.99 | 0.67 | 2.17 | -1.67 | -4.72 | 0.63 | 2.21
J0013.9$-$1854 | -11.48 | 2.0 | 0.07 | 0.64 | 0.63 | -4.04 | 0.23 | 1.32
J0014.1$-$5022 | -11.54 | 2.02 | -0.14 | 0.32 | 0.72 | -4.7 | 0.4 | 1.66
J0014.2+0854 | -11.63 | 2.47 | -0.45 | 0.98 | -0.2 | -4.21 | 0.32 | 1.85
J0014.7+5801 | -11.53 | 1.72 | 0.27 | 1.17 | -0.01 | -4.72 | 0.6 | 2.45
J0015.2+3537 | -11.93 | 1.93 | -4.0 | 0.87 | 0.42 | -4.57 | 0.8 | 2.5
J0018.4+2946 | -11.45 | 1.7 | 0.32 | 0.68 | 0.56 | -5.15 | 0.6 | 2.3
J0019.3$-$8152 | -11.17 | 2.11 | 0.23 | 1.29 | -0.79 | -4.49 | 0.89 | 2.25
J0019.6+2022 | -11.45 | 2.16 | 0.16 | 1.2 | -0.98 | -5.63 | 1.04 | 3.12
J0021.5$-$2552 | -11.14 | 2.12 | 0.22 | 1.47 | -1.27 | -4.88 | 0.8 | 2.33
J0021.9$-$5140 | -11.18 | 2.07 | 0.03 | 1.49 | 0.02 | -4.92 | 0.81 | 2.35
J0022.0+0006 | -11.76 | 1.53 | -0.45 | 0.97 | 0.11 | -4.93 | 0.34 | 1.97
J0022.1$-$1854 | -11.13 | 1.94 | 0.52 | 1.2 | -0.69 | -4.5 | 0.85 | 2.33
J0022.5+0608 | -10.69 | 2.15 | 0.51 | 1.77 | -1.57 | -5.65 | 1.02 | 3.18
J0026.6$-$4600 | -11.64 | 1.95 | -0.12 | 1.14 | 0.89 | -4.32 | 0.68 | 2.17
J0032.4$-$2849 | -11.68 | 2.36 | -0.24 | 1.15 | -0.75 | -4.68 | 0.74 | 2.45
J0033.5$-$1921 | -10.53 | 1.76 | 0.76 | 1.87 | -0.21 | -4.83 | 0.8 | 2.29
J0035.2+1514 | -10.94 | 1.85 | 0.52 | 1.46 | -0.24 | -4.69 | 0.78 | 2.36
J0035.9+5950 | -10.4 | 1.76 | 0.56 | 2.3 | -0.51 | -6.24 | 0.6 | 1.81
J0037.8+1239 | -11.07 | 2.22 | -0.29 | 1.79 | -1.07 | -4.25 | 0.63 | 2.21
J0040.3+4050 | -11.6 | 1.93 | 0.02 | 1.22 | -0.03 | -4.96 | 0.39 | 2.14
J0040.4$-$2340 | -11.64 | 2.35 | -0.04 | 1.26 | -1.07 | -4.14 | 0.68 | 2.49
J0042.0+3640 | -11.73 | 2.1 | -1.34 | 0.86 | 0.26 | -4.11 | 0.59 | 1.91
J0045.3+2128 | -10.8 | 1.81 | 0.58 | 2.35 | -0.59 | -4.85 | 0.72 | 2.28
J0045.7+1217 | -11.0 | 1.98 | 0.21 | 1.57 | -0.92 | -5.0 | 0.81 | 2.16
J0047.9+3947 | -11.06 | 1.98 | 0.23 | 1.72 | -1.26 | -4.54 | 0.6 | 1.9
J0049.7+0237 | -10.83 | 2.21 | 0.5 | 2.06 | -1.37 | -5.67 | 1.36 | 1.65
J0050.7$-$0929 | -10.44 | 2.02 | 0.73 | 2.2 | -0.86 | -4.89 | 0.89 | 0.7
J0051.2$-$6242 | -10.71 | 1.76 | 0.76 | 2.22 | -0.49 | -5.08 | 0.71 | 2.18
J0054.7$-$2455 | -11.04 | 1.77 | 0.5 | 1.23 | -0.36 | -5.0 | 0.75 | 1.96
J0056.3$-$0935 | -11.07 | 1.87 | -0.2 | 1.36 | 0.03 | -4.66 | 0.38 | 1.66
J0056.4$-$2118 | -11.1 | 1.91 | 0.67 | 1.4 | -0.9 | -4.77 | 0.95 | 2.51
J0058.0$-$3233 | -10.97 | 2.11 | 0.75 | 1.82 | -1.74 | -4.91 | 0.96 | 2.58
J0059.3$-$0152 | -11.56 | 1.81 | 0.22 | 0.95 | -0.09 | -4.18 | 0.39 | 1.9
J0109.1+1815 | -11.11 | 2.11 | 0.35 | 0.94 | 0.1 | -4.37 | 0.83 | 2.35
J0110.1+6805 | -10.62 | 2.0 | 0.07 | 1.11 | -1.58 | -4.85 | 0.84 | 2.44
J0110.7$-$1254 | -11.62 | 2.03 | -0.43 | 0.88 | 0.84 | -4.38 | 0.44 | 1.96
J0111.4+0534 | -11.92 | 1.92 | -0.03 | 1.16 | 0.58 | -4.88 | 0.4 | 1.98
J0112.1+2245 | -10.12 | 2.09 | 0.87 | 2.63 | -1.25 | -4.98 | 0.95 | 2.49
J0113.7+0225 | -11.47 | 2.48 | -0.15 | 1.15 | -0.45 | -3.77 | 0.44 | 2.38
J0114.8+1326 | -10.91 | 2.11 | 0.07 | 1.68 | -1.07 | -4.68 | 0.81 | 2.3
J0114.9$-$3400 | -11.76 | 1.72 | -0.87 | 1.22 | 0.16 | -4.69 | 0.37 | 1.93
J0115.6+0356 | -10.85 | 2.08 | 0.36 | 1.25 | -1.06 | -5.12 | 0.95 | 2.4
J0115.8+2519 | -10.7 | 1.92 | 0.2 | 2.49 | -0.64 | -5.54 | 0.72 | 2.15
J0117.5$-$2442 | -12.05 | 1.83 | 0.0 | 0.79 | 0.69 | -3.97 | 0.34 | 1.2
J0120.4$-$2701 | -10.47 | 1.91 | 0.68 | 1.56 | -1.34 | -4.6 | 0.93 | 2.62
J0123.1+3421 | -11.52 | 1.7 | 0.02 | 1.17 | 1.26 | -3.4 | 0.64 | 1.92
J0123.7$-$2311 | -11.2 | 1.86 | -0.11 | 1.25 | 0.29 | -5.24 | 0.58 | 2.02
J0127.1+3310 | -11.86 | 1.98 | -0.26 | 0.84 | 0.49 | -4.06 | 0.56 | 2.29
J0127.2$-$0819 | -11.08 | 2.18 | 0.45 | 0.96 | -1.54 | -5.52 | 1.01 | 2.46
J0127.9+4857 | -11.39 | 2.59 | -0.64 | 1.33 | -0.04 | -4.33 | 0.81 | 3.18
J0131.1+6120 | -10.77 | 1.79 | 0.55 | 1.87 | -0.24 | -5.39 | 0.76 | 1.93
J0136.5+3906 | -10.3 | 1.72 | 0.9 | 1.79 | -0.38 | -4.86 | 0.78 | 2.12
J0137.9+5814 | -10.77 | 1.95 | -0.01 | 1.57 | -0.29 | -5.14 | 0.77 | 2.24
J0140.6$-$0758 | -11.76 | 1.86 | 0.19 | 1.1 | 0.84 | -4.8 | 0.49 | 2.02
J0141.4$-$0928 | -10.63 | 2.15 | 0.45 | 2.41 | -1.48 | -4.83 | 1.0 | 2.94
J0143.7$-$5846 | -10.87 | 1.83 | 0.45 | 1.73 | 0.27 | -4.72 | 0.67 | 2.08
J0144.6+2705 | -10.26 | 2.14 | 0.93 | 2.42 | -1.84 | -5.74 | 1.07 | 2.79
J0146.9$-$5202 | -11.46 | 2.08 | 0.33 | 0.89 | -0.51 | -3.93 | 0.35 | 1.8
J0152.6+0147 | -11.04 | 1.98 | -0.14 | 1.36 | -0.12 | -3.85 | 0.39 | 1.76
J0153.0+7517 | -11.28 | 2.0 | 0.17 | 0.88 | -0.21 | -5.12 | 0.79 | 1.78
J0153.9+0823 | -10.83 | 1.95 | 0.66 | 1.64 | -0.77 | -4.59 | 0.9 | 2.39
J0155.0+4433 | -11.46 | 2.19 | 0.58 | 1.23 | -1.2 | -5.58 | 0.94 | 2.28
J0156.9$-$5301 | -11.23 | 1.74 | 0.43 | 1.66 | 0.26 | -4.99 | 0.7 | 2.1
J0158.5$-$3932 | -11.09 | 2.09 | 0.27 | 1.68 | -1.29 | -4.78 | 0.9 | 2.4
J0159.5+1046 | -10.95 | 1.99 | 0.22 | 1.53 | -0.46 | -5.01 | 0.74 | 2.31
J0159.7$-$2740 | -11.35 | 2.06 | 0.2 | 1.13 | -0.73 | -4.46 | 0.85 | 2.43
J0201.1+0036 | -11.94 | 1.88 | -0.18 | 1.01 | 0.83 | -4.27 | 0.49 | 1.92
J0203.6+7233 | -11.23 | 2.26 | 0.06 | 1.48 | -1.47 | -5.29 | 0.66 | 2.47
J0204.0$-$3334 | -11.81 | 1.95 | 0.19 | 1.06 | 0.31 | -4.62 | 0.4 | 2.28
J0208.3$-$6838 | -11.48 | 2.28 | -0.68 | 1.29 | -1.03 | -4.72 | 0.99 | 2.76
J0208.6+3523 | -11.57 | 1.88 | 0.19 | 0.99 | 0.37 | -4.97 | 0.45 | 1.73
J0209.3+4449 | -11.49 | 1.92 | 0.26 | 1.25 | 0.58 | -4.83 | 0.52 | 1.65
J0209.3$-$5228 | -10.68 | 1.85 | 0.37 | 1.86 | -0.08 | -4.84 | 0.63 | 2.01
J0209.9+7229 | -11.3 | 2.28 | 0.63 | 2.18 | -1.14 | -4.99 | 0.91 | 2.72
J0211.2+1051 | -10.29 | 2.12 | 0.69 | 2.49 | -0.78 | -3.91 | 0.92 | 2.28
J0212.4$-$3502 | -11.44 | 2.04 | -0.19 | 1.17 | 0.06 | -4.88 | 0.72 | 2.05
J0212.9+2244 | -11.21 | 2.05 | 0.32 | 1.57 | -0.3 | -4.66 | 0.68 | 2.18
J0214.3+5145 | -11.28 | 1.9 | 0.12 | 1.13 | 0.28 | -4.16 | 0.34 | 1.76
J0216.5+2313 | -11.51 | 1.85 | 0.33 | 1.04 | 0.55 | -4.68 | 0.51 | 1.65
J0216.8$-$6635 | -11.24 | 1.99 | 0.6 | 1.48 | 0.01 | -4.72 | 0.73 | 2.27
J0217.2+0837 | -10.72 | 2.27 | 0.4 | 1.82 | -1.09 | -5.28 | 0.87 | 2.69
J0219.1$-$1724 | -11.53 | 2.1 | -0.09 | 1.24 | -0.27 | -4.21 | 0.47 | 1.64
J0220.8$-$0841 | -11.87 | 1.74 | 0.22 | 1.05 | 0.16 | -4.34 | 0.69 | 2.07
J0222.6+4302 | -9.83 | 1.97 | 0.73 | 3.07 | -1.47 | -5.09 | 0.87 | 2.28
J0223.1$-$1117 | -11.53 | 1.88 | 0.38 | 1.32 | -0.38 | -4.74 | 0.79 | 2.39
J0226.5$-$4441 | -11.45 | 1.95 | 0.24 | 1.48 | 0.18 | -4.72 | 0.66 | 1.74
J0227.3+0201 | -11.15 | 1.96 | 0.08 | 1.04 | 0.75 | -5.21 | 0.6 | 2.15
J0232.8+2018 | -11.43 | 1.79 | -0.26 | 0.83 | 0.53 | -4.61 | 0.34 | 1.45
J0235.6$-$2939 | -11.78 | 2.03 | -0.07 | 1.15 | 0.32 | -4.65 | 0.73 | 1.68
J0237.6$-$3602 | -11.51 | 1.86 | -0.07 | 1.42 | 0.21 | -4.38 | 0.67 | 2.01
J0238.4$-$3116 | -10.94 | 1.82 | -0.37 | 1.56 | -0.01 | -4.49 | 0.65 | 2.02
J0238.6+1637 | -10.0 | 2.16 | 1.07 | 3.72 | -1.56 | -5.04 | 1.13 | 3.32
J0243.4+7119 | -11.13 | 2.13 | 0.51 | 2.08 | -1.26 | -5.47 | 1.02 | 2.53
J0244.6$-$5819 | -11.17 | 1.75 | 0.3 | 1.6 | 0.37 | -4.83 | 0.6 | 1.79
J0250.6+1712 | -11.3 | 1.84 | 0.08 | 1.35 | -0.14 | -4.54 | 0.59 | 2.2
J0253.2$-$0124 | -11.49 | 2.07 | -0.19 | 0.77 | -1.57 | -4.8 | 0.91 | 2.47
J0258.1+2030 | -11.47 | 2.13 | 0.48 | 1.41 | -0.33 | -4.69 | 0.98 | 2.43
J0303.3+0555 | -11.87 | 1.69 | 0.02 | 0.94 | 0.76 | -4.13 | 0.52 | 1.75
J0303.4$-$2407 | -10.27 | 1.91 | 0.52 | 2.56 | -0.63 | -5.04 | 0.85 | 2.34
J0303.6+4716 | -10.62 | 2.2 | 0.6 | 1.85 | -1.48 | -5.0 | 1.07 | 2.67
J0304.4$-$2833 | -11.71 | 1.73 | 0.44 | 1.0 | 0.54 | -4.94 | 0.6 | 2.01
J0304.5$-$0054 | -11.68 | 2.05 | -0.79 | 1.14 | -0.11 | -4.75 | 0.55 | 2.36
J0312.9+3614 | -11.34 | 1.88 | -0.02 | 1.01 | -0.08 | -4.54 | 0.05 | 1.66
J0314.3+0620 | -11.45 | 1.9 | 0.13 | 0.65 | 0.64 | -4.55 | 0.66 | 2.02
J0316.2+0905 | -10.74 | 1.93 | 0.37 | 1.76 | -0.64 | -5.38 | 0.82 | 2.24
J0316.2$-$2608 | -11.2 | 1.87 | 0.44 | 1.05 | 0.02 | -4.64 | 0.74 | 2.25
J0316.2$-$6437 | -11.25 | 1.79 | 0.47 | 1.11 | 0.09 | -4.72 | 0.7 | 2.61
J0319.8+1845 | -11.24 | 1.66 | 0.03 | 1.64 | 0.5 | -4.85 | 0.65 | 2.26
J0322.0+2335 | -10.8 | 1.99 | 0.21 | 1.25 | -1.04 | -4.76 | 0.78 | 2.12
J0323.7$-$0111 | -11.06 | 1.9 | 0.46 | 1.08 | -0.82 | -4.56 | 0.85 | 2.19
J0325.6$-$1646 | -10.92 | 1.86 | 0.42 | 1.58 | 0.7 | -4.6 | 0.68 | 2.01
J0326.2+0225 | -11.07 | 1.88 | 0.17 | 1.26 | 0.49 | -4.39 | 0.61 | 2.12
J0333.7+2916 | -10.87 | 1.97 | 0.6 | 1.34 | -2.31 | -4.72 | 0.81 | 1.96
J0333.9+6537 | -10.85 | 1.98 | 0.43 | 1.81 | -1.37 | -5.04 | 0.89 | 2.4
J0334.2$-$3725 | -10.57 | 2.03 | 0.64 | 2.0 | -2.14 | -4.89 | 0.96 | 2.75
J0334.2$-$4008 | -10.51 | 2.18 | 0.74 | 2.68 | -1.29 | -5.48 | 1.07 | 2.95
J0336.5$-$0348 | -11.84 | 1.63 | -0.21 | 0.86 | 0.42 | -3.96 | 0.38 | 1.47
J0338.1$-$2443 | -11.92 | 1.73 | -0.04 | 1.0 | 0.28 | -4.35 | 0.41 | 2.03
J0340.5$-$2118 | -10.97 | 2.26 | 0.23 | 1.62 | -1.01 | -4.71 | 0.98 | 2.65
J0348.6$-$1609 | -11.12 | 2.37 | 0.25 | 1.55 | -0.74 | -4.72 | 1.02 | 2.72
J0349.4$-$1159 | -11.41 | 1.76 | 0.04 | 1.1 | 0.9 | -4.71 | 0.47 | 1.69
J0352.9$-$3623 | -11.71 | 1.63 | 0.5 | 1.07 | 0.41 | -4.52 | 0.65 | 2.16
J0354.7+8009 | -11.45 | 2.27 | 0.26 | 2.44 | -1.26 | -5.1 | 1.02 | 2.82
J0357.0$-$4955 | -11.33 | 2.17 | 0.31 | 1.05 | -0.88 | -4.53 | 0.92 | 2.7
J0359.0$-$3053 | -11.66 | 1.93 | 0.15 | 1.25 | 0.34 | -4.42 | 0.45 | 2.36
J0402.0$-$2616 | -11.36 | 2.13 | 0.52 | 1.49 | -1.16 | -4.95 | 1.07 | 2.85
J0407.5+0741 | -11.0 | 2.31 | 0.01 | 1.51 | -1.29 | -4.87 | 0.99 | 3.07
J0409.8$-$0359 | -11.37 | 2.06 | 0.61 | 1.57 | -0.78 | -4.8 | 0.93 | 2.38
J0416.9+0105 | -11.14 | 1.88 | -0.66 | 1.36 | 0.84 | -4.25 | 0.68 | 1.98
J0422.3+1951 | -11.27 | 2.06 | -0.3 | 1.31 | -0.06 | -4.72 | 0.66 | 2.0
J0424.7+0036 | -10.71 | 2.21 | 0.3 | 1.7 | -1.11 | -4.92 | 0.97 | 2.59
J0424.9$-$5331 | -11.15 | 2.26 | 0.57 | 1.94 | -0.83 | -4.57 | 0.97 | 2.59
J0428.6$-$3756 | -9.67 | 2.1 | 1.12 | 3.54 | -2.37 | -6.77 | 1.09 | 3.05
J0429.3$-$3238 | -11.85 | 2.01 | 0.08 | 0.87 | 0.7 | -4.59 | 0.7 | 1.46
J0430.3$-$2507 | -11.37 | 2.18 | 0.09 | 0.96 | -1.33 | -4.53 | 0.83 | 2.16
J0433.6+2905 | -10.58 | 2.08 | 0.67 | 2.25 | -1.29 | -5.38 | 1.02 | 1.09
J0434.1$-$2014 | -11.4 | 2.27 | 0.33 | 1.41 | -0.73 | -4.71 | 0.99 | 2.58
J0438.9$-$4521 | -10.99 | 2.42 | 0.23 | 1.48 | -0.91 | -6.09 | 1.14 | 3.24
J0440.2$-$2458 | -11.58 | 1.63 | 0.36 | 0.92 | 0.24 | -4.7 | 0.41 | 2.12
J0440.8+2749 | -11.06 | 2.04 | 0.43 | 0.93 | -1.34 | -5.08 | 0.78 | 2.0
J0441.5+1505 | -11.43 | 2.03 | -0.82 | 0.81 | 0.78 | -4.84 | 0.62 | 1.71
J0448.6$-$1632 | -11.04 | 1.9 | 0.38 | 1.27 | -0.11 | -4.83 | 0.79 | 2.2
J0449.4$-$4350 | -9.94 | 1.86 | 0.84 | 2.53 | -0.81 | -4.99 | 0.83 | 2.39
J0502.5+1340 | -11.36 | 2.23 | 0.05 | 1.34 | -1.09 | -5.68 | 0.98 | 2.63
J0502.9+6533 | -11.84 | 1.73 | 0.11 | 0.27 | 0.89 | -4.54 | 0.43 | 1.75
J0503.5$-$1116 | -11.55 | 1.9 | 0.06 | 1.06 | 0.56 | -5.1 | 0.4 | 2.25
J0505.6+0415 | -11.2 | 1.94 | 0.18 | 0.99 | 0.03 | -4.66 | 0.59 | 2.02
J0506.0+6113 | -11.15 | 2.03 | -0.22 | 1.27 | -0.65 | -5.71 | 0.72 | 2.07
J0506.7$-$0857 | -11.38 | 2.19 | -0.46 | 1.26 | -0.87 | -5.02 | 0.84 | 2.39
J0506.9$-$5435 | -11.17 | 1.66 | 0.61 | 1.2 | 0.24 | -4.53 | 0.73 | 1.97
J0507.9+6737 | -10.62 | 1.58 | 0.54 | 1.75 | 0.08 | -5.02 | 0.7 | 2.17
J0509.4+0542 | -10.12 | 2.08 | 0.7 | 3.06 | -1.79 | -4.64 | 0.89 | 2.42
J0509.6+8425 | -11.71 | 2.82 | -4.0 | 0.97 | -0.36 | -3.73 | 1.15 | 2.66
J0509.6$-$0402 | -11.53 | 2.03 | -0.57 | 1.03 | 0.83 | -4.91 | 0.51 | 2.11
J0515.8+1527 | -10.81 | 1.94 | 0.47 | 1.61 | -1.69 | -5.4 | 0.93 | 2.33
J0516.4+7350 | -11.34 | 1.88 | 0.06 | 0.68 | -0.45 | -4.77 | 0.73 | 1.83
J0516.7$-$6207 | -10.69 | 2.18 | 0.53 | 2.32 | -0.48 | -5.29 | 1.07 | 2.93
J0521.7+2112 | -9.93 | 1.94 | 0.64 | 2.91 | -1.57 | -5.5 | 0.84 | 2.25
J0536.4$-$3343 | -10.99 | 1.77 | 0.49 | 1.28 | 0.01 | -4.63 | 0.7 | 2.05
J0537.7$-$5717 | -11.37 | 2.01 | 0.42 | 1.11 | -0.63 | -4.4 | 0.84 | 2.3
J0538.2$-$3910 | -11.7 | 1.96 | -0.1 | 1.49 | -0.15 | -4.66 | 0.58 | 2.07
J0538.8$-$4405 | -9.78 | 2.11 | 1.02 | 3.99 | -1.56 | -5.65 | 1.08 | 2.92
J0540.5+5823 | -11.17 | 1.94 | -0.76 | 1.19 | 0.25 | -4.72 | 0.67 | 2.1
J0543.9$-$5531 | -10.73 | 1.76 | 0.59 | 1.75 | 0.03 | -4.95 | 0.71 | 2.05
J0550.5$-$3216 | -11.41 | 1.89 | -2.56 | 0.95 | 1.17 | -3.63 | 0.26 | 1.66
J0553.5$-$2034 | -11.23 | 1.94 | 0.54 | 1.29 | -0.59 | -4.72 | 0.85 | 2.1
J0558.0$-$3837 | -11.13 | 1.91 | 0.32 | 1.15 | 0.32 | -4.55 | 0.67 | 2.09
J0558.8$-$7459 | -11.21 | 2.05 | 0.33 | 1.3 | -1.21 | -4.53 | 0.98 | 2.56
J0601.0+3838 | -11.07 | 2.01 | 0.19 | 0.96 | -1.8 | -4.72 | 0.97 | 2.42
J0607.2$-$2518 | -11.7 | 1.95 | 0.4 | 1.08 | 0.32 | -4.43 | 0.45 | 2.33
J0607.4+4739 | -10.55 | 2.04 | 0.71 | 2.01 | -1.51 | -5.1 | 0.93 | 2.54
J0609.2$-$0247 | -11.09 | 1.88 | 0.62 | 1.01 | -1.07 | -4.72 | 0.84 | 2.28
J0610.1$-$1848 | -11.23 | 2.34 | 0.29 | 1.46 | -0.85 | -4.84 | 1.05 | 2.8
J0612.8+4122 | -10.4 | 1.99 | 0.93 | 1.92 | -1.86 | -5.22 | 1.0 | 2.51
J0615.3$-$3117 | -11.44 | 2.12 | -0.66 | 1.34 | -1.02 | -4.2 | 0.89 | 2.06
J0617.2+5701 | -10.89 | 2.09 | 0.42 | 1.62 | -1.28 | -5.03 | 0.97 | 2.56
J0617.7$-$1715 | -11.11 | 1.93 | 0.56 | 1.17 | -1.51 | -4.35 | 0.29 | 1.64
J0621.7$-$3411 | -11.78 | 2.07 | -0.03 | 0.86 | 0.38 | -4.94 | 0.6 | 2.14
J0621.8+1746 | -11.58 | 1.89 | -0.09 | 1.21 | 0.06 | -4.72 | 0.46 | 2.3
J0623.9$-$5259 | -11.69 | 2.07 | -0.41 | 0.93 | -0.35 | -4.95 | 0.53 | 1.76
J0625.3+4439 | -11.05 | 2.09 | 0.27 | 1.44 | -0.54 | -4.51 | 0.96 | 2.52
J0629.3$-$1959 | -10.7 | 2.23 | 0.55 | 2.57 | -1.72 | -5.58 | 1.24 | 3.01
J0630.9$-$2406 | -10.32 | 1.81 | 0.89 | 2.07 | -1.28 | -4.93 | 0.86 | 2.28
J0648.7+1516 | -10.79 | 1.71 | -0.08 | 1.47 | -0.06 | -4.88 | 0.62 | 2.03
J0650.7+2503 | -10.33 | 1.74 | 0.53 | 2.44 | -0.21 | -4.82 | 0.73 | 1.98
J0654.7+4246 | -11.44 | 2.01 | 0.0 | 1.27 | -0.67 | -4.2 | 0.55 | 2.14
J0656.3+4235 | -11.6 | 1.99 | 0.06 | 1.12 | 0.07 | -4.0 | 0.16 | 1.48
J0656.3$-$2404 | -11.75 | 2.07 | -1.33 | 0.88 | -0.86 | -4.89 | 0.45 | 1.76
J0700.5$-$6610 | -10.37 | 2.08 | 0.81 | 2.42 | -1.63 | -4.83 | 0.92 | 2.39
J0706.5+3744 | -10.92 | 1.88 | 0.5 | 0.88 | -0.99 | -4.72 | 0.85 | 2.12
J0706.8+7742 | -11.04 | 2.04 | 0.71 | 2.24 | -1.37 | -4.72 | 0.88 | 2.45
J0709.1+2241 | -10.98 | 2.06 | 0.28 | 1.96 | -0.84 | -4.72 | 0.81 | 2.09
J0710.4+5908 | -11.17 | 1.69 | 0.36 | 1.44 | 0.64 | -4.27 | 0.5 | 1.89
J0710.9+4733 | -11.29 | 2.67 | 0.42 | 1.79 | -0.54 | -4.83 | 0.2 | 1.98
J0712.7+5033 | -10.9 | 2.2 | -0.14 | 2.03 | -1.4 | -5.4 | 1.06 | 2.79
J0718.6$-$4319 | -10.69 | 1.93 | 0.75 | 1.18 | -1.4 | -4.98 | 0.86 | 2.25
J0721.9+7120 | -9.67 | 2.08 | 0.96 | 3.44 | -1.64 | -4.84 | 1.0 | 2.27
J0723.0$-$0732 | -11.25 | 2.12 | -0.09 | 1.02 | 0.1 | -4.71 | 0.72 | 2.14
J0723.4+5841 | -12.12 | 1.62 | 0.31 | 1.0 | 0.27 | -4.72 | 0.43 | 1.66
J0727.1+3734 | -12.05 | 1.83 | 0.29 | 0.95 | -0.26 | -4.47 | 0.36 | 1.86
J0730.4+3308 | -11.41 | 1.95 | 0.3 | 0.77 | -0.1 | -4.38 | 0.84 | 2.5
J0731.9+2805 | -11.81 | 2.02 | 0.03 | 1.0 | 0.56 | -4.07 | 0.51 | 1.81
J0738.1+1742 | -10.23 | 2.03 | 0.78 | 2.15 | -1.44 | -5.1 | 0.94 | 2.52
J0740.9+3203 | -11.59 | 2.44 | -1.17 | 0.65 | -0.87 | -4.64 | 0.4 | 1.5
J0744.1+7434 | -11.31 | 1.91 | -4.0 | 1.04 | 0.45 | -4.28 | 0.63 | 1.92
J0747.5+0905 | -11.5 | 2.03 | -0.09 | 0.56 | 0.21 | -4.81 | 0.48 | 1.87
J0749.2+2314 | -11.74 | 1.94 | -0.91 | 0.73 | -0.52 | -4.42 | 0.37 | 1.56
J0749.7+7450 | -11.7 | 2.09 | -0.42 | 1.14 | 0.72 | -4.7 | 0.6 | 1.96
J0753.0+5353 | -10.88 | 2.14 | 0.37 | 1.16 | -1.16 | -5.09 | 1.08 | 2.73
J0754.7+4823 | -10.86 | 2.1 | 0.66 | 1.97 | -1.11 | -5.0 | 1.05 | 2.76
J0757.1+0956 | -10.75 | 2.15 | 0.14 | 1.47 | -0.84 | -4.09 | 1.1 | 2.64
J0801.1+6444 | -11.67 | 2.06 | -0.23 | 1.5 | -0.17 | -4.68 | 0.39 | 1.31
J0805.4+7534 | -10.81 | 1.85 | 0.32 | 1.48 | -0.29 | -3.79 | 0.53 | 2.16
J0806.5+5930 | -11.51 | 2.0 | -0.2 | 1.28 | 0.2 | -4.02 | 0.68 | 2.12
J0807.1$-$0541 | -10.9 | 2.18 | 0.55 | 2.07 | -1.26 | -5.74 | 0.93 | 2.63
J0809.6+3455 | -11.55 | 1.8 | -1.32 | 1.19 | 0.5 | -4.26 | 0.3 | 1.84
J0809.8+5218 | -10.37 | 1.88 | 0.49 | 2.52 | -0.38 | -4.71 | 0.72 | 1.87
J0811.0$-$7529 | -10.64 | 1.93 | 0.68 | 1.37 | -1.39 | -5.19 | 0.83 | 2.34
J0811.4+0146 | -10.46 | 2.09 | 0.74 | 2.68 | -1.8 | -5.26 | 1.05 | 2.25
J0812.8+6507 | -11.56 | 2.07 | -0.58 | 0.94 | 0.06 | -4.72 | 0.56 | 1.5
J0812.9+5555 | -11.72 | 2.18 | -0.14 | 1.25 | -0.1 | -4.56 | 0.71 | 2.04
J0814.2$-$1013 | -10.95 | 2.11 | 0.26 | 1.4 | -0.28 | -4.7 | 0.85 | 2.55
J0814.6+6430 | -10.71 | 2.24 | 0.35 | 1.97 | -1.49 | -5.09 | 0.91 | 2.7
J0816.3+5739 | -10.87 | 2.09 | 0.45 | 1.56 | -0.61 | -4.92 | 0.85 | 2.39
J0816.4$-$1311 | -10.69 | 1.85 | 0.52 | 1.93 | -0.03 | -4.95 | 0.76 | 2.06
J0817.8+3243 | -11.59 | 2.04 | 0.31 | 0.74 | -0.4 | -4.73 | 0.73 | 2.64
J0818.2+4222 | -10.3 | 2.11 | 0.94 | 2.43 | -1.86 | -5.82 | 1.08 | 2.97
J0818.4+2816 | -11.58 | 2.06 | 0.19 | 1.31 | -0.97 | -4.36 | 0.7 | 2.12
J0819.4$-$0756 | -11.6 | 1.85 | -0.13 | 0.4 | 0.09 | -4.64 | 0.53 | 2.11
J0820.9+2353 | -11.56 | 2.19 | -0.8 | 1.15 | -0.29 | -4.6 | 0.63 | 2.09
J0820.9$-$1258 | -11.5 | 2.23 | -0.16 | 0.76 | -0.18 | -3.34 | 1.06 | 2.83
J0823.3+2224 | -11.48 | 2.34 | 0.12 | 1.06 | -0.95 | -5.18 | 1.05 | 2.74
J0825.8+0309 | -11.09 | 2.2 | -0.27 | 0.74 | -0.37 | -4.64 | 0.99 | 3.31
J0825.9$-$2230 | -10.37 | 2.01 | 0.78 | 2.37 | -1.17 | -4.95 | 0.95 | 2.61
J0828.3+4152 | -11.99 | 1.89 | -0.23 | 0.72 | 0.38 | -4.33 | 0.4 | 0.96
J0829.0+1755 | -11.48 | 2.1 | 0.21 | 1.06 | 0.0 | -2.92 | 0.35 | 1.89
J0831.8+0429 | -10.5 | 2.27 | 0.73 | 2.63 | -1.38 | -4.9 | 0.99 | 2.55
J0832.4+4912 | -11.4 | 2.38 | -1.64 | 0.65 | -1.08 | -5.29 | 1.03 | 2.76
J0837.3+1458 | -11.8 | 1.85 | 0.14 | 0.79 | 1.2 | -3.81 | 0.39 | 1.62
J0839.4+1803 | -11.46 | 2.18 | -0.56 | 1.29 | -0.71 | -4.31 | 0.87 | 2.57
J0841.3$-$3554 | -10.87 | 1.82 | 0.8 | 1.57 | -0.23 | -4.72 | 0.8 | 2.3
J0842.5+0251 | -11.79 | 2.03 | -0.1 | 1.1 | -0.3 | -4.76 | 0.34 | 2.12
J0844.2+5312 | -11.06 | 2.03 | 0.23 | 1.7 | -1.4 | -5.17 | 0.88 | 2.53
J0847.2+1134 | -11.26 | 1.72 | 0.2 | 1.24 | 0.64 | -4.34 | 0.58 | 2.04
J0847.9$-$0702 | -11.31 | 2.24 | -0.51 | 1.07 | -0.02 | -4.09 | 1.02 | 2.95
J0850.5+3455 | -11.43 | 2.01 | -0.47 | 1.16 | -0.42 | -4.55 | 0.38 | 1.72
J0854.0+2753 | -12.16 | 1.48 | 0.29 | 1.08 | -0.04 | -4.7 | 0.42 | 2.26
J0854.3+4408 | -11.64 | 1.8 | 0.52 | 1.18 | 0.23 | -4.05 | 0.62 | 2.06
J0854.8+2006 | -10.24 | 2.22 | 0.69 | 2.89 | -1.17 | -4.77 | 1.05 | 2.6
J0856.6$-$1105 | -10.65 | 2.05 | 0.64 | 1.61 | -1.46 | -5.1 | 0.98 | 2.85
J0859.4+6218 | -11.62 | 2.29 | -1.26 | 1.33 | -0.23 | -4.72 | 0.74 | 1.85
J0902.4+2051 | -10.82 | 2.15 | 0.35 | 1.89 | -1.33 | -4.69 | 0.89 | 2.44
J0905.6+1358 | -10.99 | 1.79 | 0.64 | 1.46 | -0.99 | -4.57 | 0.84 | 2.48
J0906.3$-$0905 | -11.27 | 2.11 | 0.29 | 1.9 | -0.97 | -4.52 | 1.06 | 2.34
J0908.9+2311 | -11.23 | 1.82 | 0.4 | 1.21 | -0.75 | -4.42 | 0.74 | 2.27
J0909.7+3104 | -11.86 | 1.95 | -0.15 | 0.8 | 0.76 | -4.17 | 0.44 | 1.82
J0910.6+3329 | -10.8 | 1.95 | 0.38 | 1.31 | -0.76 | -4.33 | 0.86 | 2.34
J0912.2+2800 | -11.87 | 1.68 | 0.39 | 1.18 | -0.02 | -4.54 | 0.76 | 2.49
J0912.9$-$2102 | -10.94 | 1.87 | -0.03 | 1.17 | 0.37 | -4.82 | 0.6 | 2.13
J0915.9+2933 | -10.7 | 1.89 | 0.69 | 1.38 | -0.16 | -4.69 | 0.73 | 2.28
J0916.7+5238 | -11.82 | 1.84 | 0.27 | 1.01 | 0.75 | -4.26 | 0.45 | 1.55
J0921.7+2336 | -11.39 | 2.06 | -0.12 | 1.32 | -1.06 | -4.83 | 0.8 | 2.57
J0924.0+0534 | -11.71 | 2.06 | -1.27 | 0.98 | 0.42 | -4.59 | 0.54 | 2.46
J0925.7+5959 | -11.73 | 1.96 | -0.03 | 1.11 | -0.16 | -4.81 | 0.77 | 1.71
J0928.5+4048 | -11.67 | 2.08 | 0.16 | 1.04 | -0.6 | -4.64 | 0.79 | 1.41
J0929.3+5014 | -10.9 | 2.13 | 0.27 | 1.84 | -1.0 | -4.66 | 0.98 | 2.9
J0930.3+8612 | -11.03 | 2.22 | 0.48 | 1.9 | -1.48 | -5.57 | 1.01 | 2.46
J0930.5+4951 | -11.64 | 1.82 | -0.31 | 1.19 | 1.2 | -4.5 | 0.54 | 1.38
J0930.7+3502 | -11.81 | 2.2 | -0.04 | 0.87 | -0.17 | -5.17 | 1.0 | 3.0
J0932.7+1041 | -11.7 | 1.95 | 0.32 | 0.99 | -0.22 | -4.59 | 0.53 | 2.37
J0934.5$-$1720 | -11.68 | 1.94 | -0.11 | 0.91 | 0.51 | -4.4 | 0.45 | 2.14
J0940.4+6148 | -11.56 | 1.83 | 0.1 | 1.27 | 0.01 | -4.76 | 0.48 | 1.92
J0942.3+2842 | -11.84 | 1.9 | -0.36 | 1.16 | -0.52 | -5.07 | 0.64 | 1.97
J0944.2+5557 | -11.92 | 2.24 | 0.4 | 0.49 | -1.44 | -4.97 | 0.54 | 2.39
J0945.7+5759 | -11.62 | 2.09 | 0.49 | 1.6 | -0.81 | -4.43 | 0.75 | 2.42
J0946.0+4735 | -11.96 | 2.14 | -0.2 | 0.53 | -0.66 | -4.9 | 0.76 | 2.3
J0946.2+0104 | -11.6 | 1.89 | 0.23 | 1.01 | 0.2 | -5.31 | 0.3 | 2.24
J0950.2+4553 | -11.34 | 1.99 | 0.06 | 1.04 | -1.24 | -5.1 | 0.9 | 2.69
J0952.1+3932 | -11.92 | 1.72 | 0.27 | 0.55 | 0.31 | -5.01 | 0.32 | 3.81
J0952.2+7503 | -11.94 | 1.49 | 0.37 | 1.1 | 0.67 | -4.86 | 0.35 | 1.34
J0953.0$-$0840 | -10.59 | 1.89 | 0.58 | 1.6 | -0.8 | -4.92 | 0.84 | 2.51
J0954.2+4913 | -11.6 | 1.59 | 0.58 | 0.82 | 0.06 | -4.88 | 0.64 | 2.13
J0955.1+3551 | -12.0 | 1.89 | -2.0 | 0.78 | 0.26 | -4.99 | 0.5 | 2.33
J0958.0$-$0319 | -11.99 | 1.64 | 0.26 | 1.09 | 0.42 | -4.44 | 0.56 | 1.7
J0958.7+6534 | -10.43 | 2.22 | 0.56 | 3.33 | -1.51 | -5.21 | 1.03 | 3.18
J0959.4+2120 | -11.58 | 2.18 | -0.6 | 1.16 | 0.53 | -4.22 | 0.65 | 2.01
J1001.1+2911 | -11.07 | 2.27 | 0.12 | 2.33 | -1.27 | -5.11 | 1.08 | 2.23
J1002.5+2215 | -11.53 | 1.91 | -0.04 | 0.46 | -0.49 | -4.82 | 0.61 | 1.72
J1006.5+6440 | -11.8 | 1.87 | -0.52 | 0.87 | -0.07 | -4.64 | 0.71 | 2.29
J1007.0+3455 | -11.55 | 1.82 | 0.34 | 1.0 | -0.0 | -4.9 | 0.84 | 2.18
J1008.0+0620 | -10.93 | 2.19 | 0.27 | 1.92 | -1.05 | -5.05 | 0.99 | 2.74
J1010.2$-$3119 | -11.11 | 1.76 | -0.38 | 1.58 | 0.46 | -4.54 | 0.51 | 1.66
J1012.3+0629 | -11.06 | 2.09 | 0.45 | 1.32 | -1.1 | -4.74 | 0.96 | 2.68
J1015.0+4926 | -10.05 | 1.84 | 0.7 | 2.43 | -0.49 | -5.25 | 0.81 | 2.32
J1018.8+5913 | -11.55 | 2.07 | 0.33 | 1.06 | -1.11 | -4.45 | 0.73 | 2.48
J1021.1+1626 | -11.9 | 1.93 | -0.32 | 0.95 | 1.07 | -4.31 | 0.71 | 2.13
J1022.7$-$0112 | -11.12 | 1.95 | 0.19 | 1.08 | 0.19 | -4.78 | 0.65 | 2.12
J1023.8+3002 | -11.8 | 1.86 | -0.33 | 1.22 | 0.0 | -4.55 | 0.65 | 1.88
J1023.8$-$4335 | -10.92 | 1.77 | 0.69 | 1.56 | 0.39 | -4.43 | 0.73 | 2.01
J1024.8+2332 | -11.42 | 2.44 | -0.25 | 1.2 | -0.88 | -4.39 | 0.98 | 2.77
J1026.9+0608 | -11.73 | 1.69 | -0.06 | 0.81 | -0.19 | -4.84 | 0.5 | 2.27
J1026.9$-$1749 | -10.85 | 1.95 | 0.27 | 2.02 | -0.48 | -4.63 | 0.65 | 2.01
J1027.0$-$8542 | -11.0 | 1.87 | 0.51 | 0.37 | -1.24 | -4.5 | 0.89 | 2.4
J1027.6+6317 | -11.39 | 1.96 | 0.26 | 0.95 | -0.41 | -4.95 | 0.82 | 2.28
J1031.1+7442 | -11.22 | 2.16 | 0.19 | 1.52 | -0.41 | -4.5 | 0.79 | 2.56
J1031.3+5053 | -10.92 | 1.74 | 0.44 | 1.11 | 0.8 | -4.71 | 0.63 | 1.91
J1033.5+4221 | -12.09 | 1.76 | 0.05 | 1.12 | -0.14 | -4.21 | 0.37 | 1.88
J1037.7+5711 | -10.46 | 1.88 | 0.82 | 2.19 | -1.04 | -5.0 | 0.89 | 2.18
J1041.7+3902 | -11.79 | 1.85 | 0.3 | 1.19 | 0.03 | -4.56 | 0.45 | 1.7
J1046.8$-$2534 | -11.56 | 1.74 | 0.32 | 0.99 | 0.18 | -4.68 | 0.48 | 2.0
J1049.7+5011 | -11.7 | 2.25 | 0.25 | 1.3 | -0.17 | -5.08 | 0.36 | 1.93
J1051.4+3942 | -11.65 | 1.73 | 0.28 | 1.26 | 0.49 | -4.7 | 0.52 | 2.26
J1051.9+0103 | -11.58 | 1.93 | 0.23 | 1.2 | -1.13 | -4.98 | 0.76 | 1.85
J1053.7+4930 | -11.3 | 1.92 | 0.05 | 1.26 | -0.45 | -4.64 | 0.43 | 1.86
J1054.5+2211 | -10.88 | 2.14 | 0.29 | 1.55 | -1.19 | -4.84 | 0.78 | 2.13
J1055.5$-$0125 | -11.41 | 1.93 | -0.56 | 0.99 | -0.4 | -4.84 | 0.7 | 2.4
J1057.8$-$2754 | -11.28 | 1.91 | 0.23 | 1.26 | -0.1 | -4.68 | 0.49 | 1.94
J1058.4+0133 | -10.21 | 2.23 | 0.71 | 2.58 | -1.42 | -5.95 | 1.1 | 2.72
J1058.6+2817 | -11.29 | 2.23 | -0.22 | 1.65 | -0.97 | -5.0 | 1.01 | 2.73
J1058.6+5627 | -10.5 | 1.94 | 0.6 | 2.24 | -0.67 | -4.87 | 0.79 | 2.31
J1058.6$-$8003 | -10.78 | 2.26 | 0.8 | 2.69 | -1.25 | -5.37 | 1.07 | 3.18
J1059.2$-$1134 | -10.5 | 2.16 | 0.59 | 2.08 | -1.3 | -5.34 | 0.96 | 2.67
J1100.3+4020 | -11.39 | 1.85 | 0.42 | 1.05 | 0.46 | -4.36 | 0.74 | 2.0
J1101.4+4108 | -11.5 | 1.79 | 0.39 | 1.17 | -0.48 | -4.92 | 0.72 | 1.93
J1103.6$-$2329 | -11.26 | 1.77 | -0.17 | 1.1 | 0.92 | -4.2 | 0.55 | 1.87
J1103.9$-$5357 | -10.51 | 2.16 | 0.78 | 2.74 | -1.71 | -5.49 | 1.01 | 2.82
J1104.4+3812 | -9.37 | 1.78 | 0.55 | 3.13 | -0.03 | -4.63 | 0.65 | 1.76
J1107.8+1501 | -11.18 | 1.95 | 0.42 | 0.93 | 0.15 | -4.94 | 0.67 | 1.87
J1110.2+7135 | -11.48 | 1.91 | 0.29 | 1.13 | -0.22 | -4.56 | 0.82 | 2.33
J1110.5$-$1836 | -11.27 | 1.95 | 0.43 | 1.55 | -1.31 | -5.21 | 0.91 | 2.66
J1111.0+3542 | -11.86 | 2.0 | 0.39 | 1.02 | -0.25 | -4.62 | 0.8 | 2.67
J1112.4+1751 | -11.73 | 2.3 | -0.01 | 0.82 | 0.24 | -4.53 | 0.63 | 1.53
J1117.0+2013 | -10.85 | 1.96 | -0.18 | 2.14 | 0.71 | -4.07 | 0.61 | 2.0
J1117.6+2550 | -11.49 | 2.23 | -1.54 | 1.05 | -0.39 | -4.06 | 0.7 | 1.74
J1118.0+5356 | -11.08 | 1.9 | 0.53 | 1.11 | -0.92 | -4.85 | 0.78 | 2.13
J1119.6$-$3047 | -11.89 | 1.73 | -0.25 | 1.04 | 0.42 | -4.75 | 0.4 | 2.66
J1120.8+4212 | -10.75 | 1.62 | 0.6 | 0.95 | -0.02 | -4.93 | 0.72 | 1.99
J1123.8+7230 | -11.99 | 1.66 | 0.26 | 0.57 | 0.89 | -4.37 | 0.55 | 2.13
J1124.0+2045 | -11.73 | 1.98 | 0.09 | 1.06 | -0.4 | -4.67 | 0.87 | 2.4
J1124.9+4934 | -11.29 | 1.75 | 0.62 | 1.58 | -0.14 | -5.0 | 0.66 | 2.1
J1125.5$-$3557 | -11.23 | 2.01 | -0.34 | 1.64 | -1.05 | -4.55 | 0.88 | 2.21
J1125.9$-$0742 | -11.51 | 2.11 | -0.42 | 0.62 | 0.25 | -4.93 | 0.59 | 1.79
J1131.4+5809 | -11.5 | 2.07 | 0.09 | 1.25 | -0.9 | -4.09 | 0.82 | 2.36
J1132.7+0034 | -10.6 | 2.14 | 0.37 | 1.4 | -1.76 | -5.47 | 0.93 | 2.56
J1134.8$-$1729 | -11.87 | 1.66 | 0.33 | 0.72 | 0.44 | -4.61 | 0.38 | 2.64
J1136.4+6736 | -11.2 | 1.75 | 0.2 | 1.44 | 0.71 | -4.62 | 0.44 | 2.04
J1136.4+7009 | -10.88 | 1.81 | 0.07 | 1.45 | 0.76 | -3.76 | 0.39 | 2.02
J1136.8+2550 | -11.59 | 1.94 | -0.92 | 1.11 | -0.4 | -4.24 | 0.37 | 2.5
J1137.9$-$1708 | -11.55 | 1.71 | 0.49 | 1.26 | 0.22 | -4.77 | 0.41 | 2.48
J1140.5+1528 | -11.72 | 1.76 | -0.14 | 0.91 | 0.74 | -4.21 | 0.51 | 2.15
J1143.1+6122 | -11.46 | 2.04 | 0.68 | 1.9 | -0.99 | -4.63 | 0.83 | 2.37
J1147.0$-$3812 | -10.62 | 2.23 | 0.5 | 2.03 | -1.08 | -4.7 | 1.12 | 2.92
J1149.4+2441 | -11.7 | 1.96 | 0.18 | 0.71 | 0.78 | -4.48 | 0.57 | 1.88
J1150.4+2418 | -10.8 | 2.23 | 0.5 | 1.43 | -1.39 | -4.34 | 1.01 | 2.7
J1150.6+4154 | -10.73 | 1.8 | 0.79 | 1.81 | -0.61 | -4.97 | 0.79 | 2.32
J1151.5+5859 | -11.13 | 1.88 | 0.52 | 1.14 | -0.62 | -4.14 | 0.8 | 2.21
J1153.7+3822 | -11.91 | 1.93 | -0.25 | 0.98 | -0.16 | -4.52 | 0.71 | 2.39
J1154.0$-$0010 | -11.34 | 1.81 | 0.32 | 1.29 | 0.08 | -4.94 | 0.59 | 1.56
J1202.4+4442 | -11.77 | 2.6 | -0.28 | 0.99 | -0.48 | -4.36 | 0.68 | 2.33
J1202.5+3852 | -11.47 | 2.45 | -0.12 | 1.12 | -0.81 | -4.92 | 0.9 | 2.6
J1203.1+6031 | -11.07 | 2.12 | 0.31 | 1.37 | -0.72 | -4.19 | 0.65 | 2.49
J1204.0+1146 | -11.49 | 1.89 | 0.33 | 1.09 | -0.09 | -4.57 | 0.55 | 1.75
J1204.2$-$0709 | -11.04 | 1.89 | 0.48 | 1.5 | -0.62 | -5.0 | 0.59 | 2.03
J1208.4+6121 | -11.76 | 2.07 | -0.28 | 1.36 | -0.32 | -4.48 | 0.61 | 2.0
J1209.4+4118 | -11.19 | 1.93 | 0.4 | 1.16 | -0.63 | -4.78 | 0.93 | 2.56
J1211.6+3901 | -11.88 | 2.05 | -0.43 | 1.17 | -0.46 | -4.96 | 0.26 | 2.8
J1212.0+2242 | -11.77 | 2.02 | -0.71 | 0.87 | 0.73 | -4.54 | 0.48 | 2.1
J1213.0+5129 | -11.47 | 2.11 | -0.46 | 1.03 | -0.2 | -4.81 | 0.69 | 2.25
J1213.3$-$2618 | -11.47 | 1.81 | 0.42 | 1.19 | 0.39 | -4.97 | 0.57 | 1.91
J1215.1+0731 | -11.56 | 1.72 | -0.61 | 1.04 | 0.41 | -3.68 | 0.42 | 1.8
J1216.1+0930 | -11.46 | 2.06 | -0.15 | 0.86 | -0.19 | -2.66 | 0.31 | 1.78
J1216.1$-$0242 | -11.78 | 1.94 | 0.03 | 1.05 | 0.18 | -3.96 | 0.62 | 2.03
J1217.9+3007 | -10.0 | 1.93 | 0.76 | 2.8 | -0.26 | -5.08 | 0.83 | 2.24
J1219.7$-$0313 | -11.27 | 1.94 | 0.16 | 1.26 | -0.15 | -4.75 | 0.64 | 1.97
J1220.1+3432 | -11.24 | 2.11 | 0.23 | 1.4 | -0.94 | -4.44 | 0.88 | 2.48
J1221.3+3010 | -10.36 | 1.71 | 0.45 | 1.78 | -0.09 | -4.82 | 0.66 | 1.92
J1221.5+2814 | -10.43 | 2.15 | 0.36 | 2.49 | -1.11 | -4.85 | 0.87 | 2.31
J1223.8+8039 | -11.03 | 2.27 | 0.67 | 1.42 | -1.35 | -5.41 | 1.1 | 2.78
J1224.1+2239 | -11.89 | 1.85 | 0.29 | 0.79 | -0.33 | -4.55 | 0.65 | 2.48
J1224.4+2436 | -10.85 | 1.93 | 0.28 | 2.25 | -0.62 | -4.94 | 0.73 | 2.08
J1226.7+0637 | -11.63 | 1.74 | 0.27 | 1.31 | -0.05 | -4.1 | 0.64 | 1.75
J1230.2+2517 | -10.44 | 2.09 | 0.7 | 3.24 | -0.88 | -4.2 | 0.96 | 2.4
J1231.5+1421 | -11.44 | 1.88 | -0.22 | 1.12 | 0.06 | -4.48 | 0.68 | 2.23
J1231.6+6415 | -11.52 | 1.91 | -0.02 | 0.95 | 0.25 | -4.37 | 0.39 | 1.74
J1231.7+2847 | -10.68 | 2.0 | 0.48 | 2.37 | -0.8 | -5.11 | 0.83 | 2.22
J1233.6+5027 | -11.61 | 2.46 | 0.22 | 0.96 | -0.97 | -4.37 | 0.72 | 2.22
J1236.3+3858 | -11.63 | 1.99 | -0.8 | 1.2 | -0.54 | -4.67 | 0.56 | 2.11
J1237.8+6256 | -12.0 | 1.89 | -0.25 | 1.26 | 0.7 | -4.14 | 0.55 | 1.8
J1238.3$-$1959 | -11.14 | 2.15 | 0.2 | 1.59 | -0.96 | -4.88 | 0.9 | 2.46
J1239.4+0728 | -11.39 | 2.23 | 0.02 | 1.09 | -0.63 | -5.49 | 1.09 | 3.01
J1241.5+3439 | -11.79 | 1.92 | -1.23 | 1.22 | 0.26 | -4.93 | 0.5 | 2.36
J1241.8$-$1456 | -11.35 | 1.87 | 0.41 | 1.15 | 0.62 | -4.65 | 0.72 | 2.11
J1241.9+0636 | -11.89 | 1.85 | 0.4 | 1.22 | 0.22 | -4.36 | 0.64 | 2.01
J1243.2+3627 | -10.59 | 1.77 | 0.69 | 1.11 | -0.07 | -5.09 | 0.78 | 2.25
J1244.5+1616 | -11.56 | 2.17 | -0.69 | 0.87 | -0.31 | -4.96 | 0.28 | 1.94
J1245.1+5709 | -11.4 | 2.13 | 0.32 | 1.34 | -0.75 | -4.63 | 0.9 | 2.56
J1245.8+0232 | -11.65 | 2.25 | 0.62 | 1.26 | -1.01 | -4.92 | 0.84 | 2.12
J1247.0+4421 | -11.47 | 1.82 | 0.42 | 1.23 | 0.12 | -4.98 | 0.52 | 1.7
J1248.3+5820 | -10.29 | 1.9 | 0.74 | 1.97 | -0.77 | -4.86 | 0.87 | 2.32
J1248.7+5127 | -11.68 | 2.07 | -0.71 | 1.14 | -0.47 | -4.35 | 0.9 | 2.39
J1249.8+3707 | -11.38 | 1.78 | 0.21 | 1.55 | -0.86 | -4.98 | 0.84 | 2.28
J1251.2+1039 | -11.63 | 2.13 | 0.05 | 1.33 | -0.08 | -4.3 | 0.76 | 2.27
J1253.2+5301 | -10.47 | 2.04 | 0.84 | 2.06 | -1.76 | -5.37 | 0.91 | 2.46
J1253.5$-$3934 | -11.86 | 1.66 | 0.46 | 1.22 | 1.05 | -4.1 | 0.42 | 1.47
J1253.8+0327 | -11.06 | 1.99 | 0.36 | 1.24 | -0.38 | -4.34 | 0.21 | 1.5
J1253.8+6242 | -11.34 | 1.99 | 0.07 | 1.67 | -0.82 | -5.11 | 0.85 | 2.4
J1256.2$-$1146 | -11.05 | 1.92 | -0.18 | 1.0 | -0.74 | -4.27 | 0.34 | 1.86
J1257.2+3646 | -11.24 | 2.03 | 0.43 | 1.63 | -0.76 | -4.74 | 0.78 | 2.41
J1257.6+2413 | -12.07 | 1.65 | -0.21 | 0.75 | 1.27 | -2.93 | 0.34 | 1.22
J1258.7$-$0452 | -11.66 | 1.78 | 0.24 | 1.22 | 0.65 | -5.34 | 0.52 | 2.04
J1301.6+4056 | -11.8 | 1.93 | 0.15 | 1.23 | 0.17 | -4.33 | 0.68 | 2.06
J1302.8+5748 | -11.44 | 2.27 | -0.42 | 1.54 | -0.88 | -5.3 | 1.07 | 2.79
J1304.3$-$4353 | -10.63 | 1.89 | 0.67 | 2.01 | -0.68 | -4.49 | 0.86 | 2.34
J1307.6$-$4259 | -10.71 | 1.94 | 0.35 | 1.36 | -0.58 | -4.5 | 0.73 | 2.1
J1309.4+4305 | -10.82 | 1.9 | 0.66 | 1.49 | -1.24 | -4.87 | 0.89 | 2.41
J1309.7+1153 | -11.2 | 2.19 | 0.22 | 0.84 | -0.78 | -4.95 | 1.07 | 2.73
J1310.2$-$1158 | -11.32 | 2.04 | -0.17 | 0.83 | -0.26 | -4.12 | 0.48 | 1.82
J1311.0+0034 | -11.36 | 2.1 | -2.0 | 1.04 | -0.33 | -4.69 | 0.79 | 2.27
J1311.8+3954 | -11.96 | 1.94 | -0.06 | 0.79 | -0.66 | -4.88 | 0.75 | 2.27
J1314.7+2348 | -10.96 | 2.04 | 0.64 | 1.55 | -0.66 | -4.51 | 0.86 | 2.46
J1315.0$-$4236 | -11.36 | 1.69 | 0.15 | 0.91 | 0.65 | -4.12 | 0.31 | 1.39
J1319.5+1404 | -11.65 | 2.0 | 0.35 | 1.17 | 0.73 | -4.33 | 0.6 | 1.91
J1322.9+0437 | -11.7 | 1.92 | 0.41 | 1.18 | 0.44 | -4.66 | 0.52 | 1.73
J1323.9+1405 | -11.25 | 1.88 | 0.5 | 1.47 | -0.4 | -5.05 | 0.7 | 2.27
J1325.6$-$0227 | -11.79 | 1.88 | 0.45 | 1.04 | 0.29 | -5.05 | 0.35 | 2.58
J1326.1+1232 | -11.92 | 1.94 | 0.23 | 0.94 | 0.79 | -4.38 | 0.44 | 1.89
J1326.8$-$5256 | -10.67 | 2.32 | 0.71 | 2.59 | -1.57 | -4.98 | 1.12 | 2.92
J1329.0$-$5607 | -10.36 | 2.45 | 0.84 | 3.01 | -1.49 | -5.72 | 1.12 | 2.81
J1330.2+7002 | -11.43 | 1.97 | 0.27 | 1.45 | -0.34 | -4.57 | 0.82 | 2.37
J1330.3+4441 | -11.48 | 2.07 | 0.35 | 1.0 | -0.3 | -4.83 | 0.82 | 2.2
J1331.0+5653 | -11.88 | 1.87 | 0.2 | 0.66 | -0.11 | -4.74 | 0.38 | 2.22
J1331.6+1711 | -11.4 | 2.35 | -0.44 | 1.1 | -0.92 | -5.49 | 0.92 | 2.53
J1335.3$-$2949 | -11.45 | 1.97 | -4.0 | 1.19 | 0.32 | -5.03 | 0.5 | 1.86
J1336.2+2320 | -11.74 | 2.0 | 0.24 | 1.24 | -0.08 | -4.46 | 0.56 | 1.92
J1338.9+1153 | -11.3 | 2.04 | -0.74 | 1.57 | -0.77 | -4.74 | 0.89 | 2.22
J1340.5+4409 | -11.76 | 1.66 | -0.2 | 1.08 | 0.46 | -4.69 | 0.37 | 1.01
J1341.2+3958 | -11.6 | 1.86 | -0.24 | 0.98 | 0.65 | -4.54 | 0.38 | 1.65
J1341.6+5515 | -12.02 | 2.09 | 0.04 | 1.02 | 0.22 | -4.21 | 0.54 | 1.83
J1351.3+1115 | -11.06 | 1.88 | 0.43 | 1.35 | -0.58 | -4.93 | 0.67 | 2.13
J1353.2+3740 | -11.71 | 2.13 | 0.2 | 1.16 | -0.17 | -4.18 | 0.49 | 1.55
J1353.3+1434 | -11.25 | 2.25 | -0.24 | 1.61 | -1.01 | -4.54 | 1.0 | 2.83
J1353.4+5600 | -11.84 | 2.18 | -1.35 | 1.15 | 0.49 | -4.57 | 0.54 | 2.16
J1357.5+0127 | -11.37 | 2.2 | 0.31 | 0.87 | -0.1 | -4.67 | 0.82 | 2.41
J1359.8$-$3746 | -11.08 | 2.04 | -0.35 | 1.54 | -1.0 | -4.63 | 0.86 | 2.46
J1402.6+1600 | -11.8 | 1.96 | -0.56 | 1.25 | -0.41 | -3.73 | 0.85 | 2.53
J1404.8+0402 | -11.25 | 2.06 | -0.23 | 1.21 | -0.05 | -4.23 | 0.75 | 2.09
J1404.8+6554 | -11.31 | 1.93 | 0.18 | 1.6 | -0.14 | -5.08 | 0.53 | 2.17
J1406.6$-$3934 | -11.81 | 1.55 | 0.39 | 1.43 | 0.37 | -4.79 | 0.47 | 2.11
J1406.9+1643 | -11.6 | 1.79 | 0.41 | 1.23 | 0.43 | -4.54 | 0.54 | 2.01
J1410.4+2820 | -11.55 | 2.1 | 0.25 | 1.2 | -0.06 | -4.3 | 0.7 | 1.99
J1415.5+4830 | -11.14 | 1.94 | 0.26 | 2.23 | -0.88 | -5.29 | 0.72 | 2.26
J1416.1$-$2417 | -11.55 | 1.83 | 0.26 | 1.41 | -0.27 | -4.16 | 0.48 | 1.88
J1417.9+2543 | -11.48 | 1.45 | 0.3 | 0.91 | 1.0 | -4.24 | 0.58 | 2.11
J1418.4$-$0233 | -10.53 | 1.79 | 0.76 | 1.94 | -0.44 | -4.56 | 0.86 | 2.38
J1418.9+7731 | -11.45 | 1.77 | 0.55 | 1.24 | -0.11 | -4.72 | 0.72 | 1.46
J1419.3+0444 | -11.61 | 1.91 | 0.3 | 0.61 | -0.82 | -4.56 | 0.91 | 2.23
J1419.8+5423 | -10.83 | 2.36 | 0.18 | 2.42 | -0.93 | -4.27 | 0.93 | 2.87
J1420.3+0612 | -11.55 | 2.53 | 0.02 | 1.31 | -1.33 | -5.13 | 0.77 | 2.11
J1422.6+5801 | -11.67 | 1.68 | 0.52 | 0.88 | 1.2 | -4.43 | 0.48 | 1.72
J1423.1+3738 | -11.32 | 2.11 | 0.44 | 2.37 | -1.3 | -4.98 | 0.89 | 2.76
J1425.0+3615 | -11.22 | 1.87 | 0.49 | 0.89 | -1.11 | -4.74 | 0.92 | 2.45
J1426.1+3403 | -11.42 | 2.09 | 0.31 | 1.21 | -0.78 | -4.42 | 0.91 | 2.59
J1427.0+2348 | -9.91 | 1.82 | 0.86 | 2.4 | -1.19 | -4.91 | 0.83 | 2.24
J1427.6$-$3305 | -10.76 | 2.29 | 0.65 | 2.42 | -0.95 | -5.1 | 1.14 | 2.98
J1428.5+4240 | -11.06 | 1.63 | 0.09 | 1.22 | 0.94 | -4.36 | 0.51 | 1.88
J1435.5+2021 | -11.35 | 2.22 | 0.45 | 0.96 | -0.97 | -5.01 | 0.84 | 2.47
J1436.9+5638 | -11.18 | 1.9 | 0.16 | 1.41 | -0.26 | -5.06 | 0.57 | 2.1
J1439.3+3932 | -11.25 | 1.97 | -0.32 | 1.29 | 0.63 | -4.43 | 0.72 | 2.14
J1439.7+4958 | -11.16 | 2.3 | 0.22 | 1.66 | -1.3 | -4.81 | 1.11 | 2.97
J1440.9+0609 | -11.14 | 2.12 | 0.16 | 1.42 | -0.8 | -4.64 | 0.81 | 2.04
J1442.7+1200 | -11.25 | 1.8 | 0.33 | 1.19 | 0.48 | -4.64 | 0.52 | 1.83
J1443.9$-$3908 | -10.39 | 1.83 | 0.65 | 1.5 | -0.45 | -4.99 | 0.72 | 2.04
J1445.0$-$0326 | -11.09 | 1.75 | 0.49 | 1.01 | -0.07 | -4.63 | 0.69 | 1.97
J1448.0+3608 | -10.82 | 1.79 | 0.74 | 1.4 | -0.18 | -4.77 | 0.77 | 2.24
J1451.4+6355 | -11.51 | 1.82 | -0.13 | 1.47 | 0.06 | -5.17 | 0.58 | 1.82
J1454.4+5124 | -10.44 | 2.02 | 0.74 | 2.6 | -1.64 | -5.74 | 0.91 | 2.48
J1501.0+2238 | -10.88 | 2.0 | 0.36 | 1.82 | -0.28 | -4.27 | 0.83 | 2.51
J1503.7$-$1540 | -10.98 | 1.82 | 0.44 | 1.16 | 0.25 | -5.1 | 0.65 | 2.11
J1505.0$-$3433 | -11.35 | 2.28 | 0.31 | 1.6 | -1.47 | -5.04 | 1.23 | 2.83
J1506.4$-$0540 | -11.94 | 1.59 | 0.06 | 1.04 | 0.53 | -4.9 | 0.26 | 2.19
J1506.6+0813 | -11.02 | 1.79 | 0.56 | 1.51 | -0.46 | -4.82 | 0.73 | 2.27
J1508.8+2708 | -11.56 | 2.05 | -4.0 | 0.88 | 0.5 | -4.68 | 0.48 | 1.91
J1509.7+5556 | -11.4 | 1.88 | 0.42 | 0.79 | -0.56 | -4.6 | 0.79 | 2.31
J1516.8+2918 | -11.65 | 2.36 | 0.03 | 1.15 | 0.09 | -4.47 | 0.29 | 1.57
J1516.9+1934 | -11.48 | 2.58 | -1.3 | 1.49 | -0.75 | -4.84 | 1.06 | 2.94
J1517.7+6525 | -11.03 | 1.82 | 0.58 | 1.41 | 0.44 | -4.17 | 0.71 | 2.14
J1517.7$-$2422 | -10.18 | 2.12 | 0.41 | 2.11 | -1.46 | -4.26 | 0.89 | 2.71
J1518.6+4044 | -11.57 | 1.88 | 0.13 | 0.92 | -0.36 | -2.95 | 0.18 | 1.66
J1520.4+5546 | -11.53 | 2.22 | -0.18 | 1.09 | -0.57 | -4.89 | 0.84 | 2.7
J1520.8$-$0348 | -11.03 | 1.81 | 0.74 | 0.89 | -0.78 | -5.19 | 0.84 | 2.24
J1522.6$-$2730 | -10.72 | 2.2 | 0.75 | 2.17 | -1.12 | -5.52 | 1.03 | 3.06
J1529.2+3812 | -11.77 | 2.05 | 0.26 | 0.92 | -0.08 | -4.58 | 0.77 | 1.87
J1532.0+3016 | -11.3 | 1.92 | -0.06 | 1.37 | 0.23 | -3.78 | 0.23 | 1.94
J1533.2+1855 | -11.44 | 1.82 | -0.59 | 0.49 | 0.6 | -4.24 | 0.54 | 1.79
J1533.2+3416 | -11.38 | 1.89 | 0.33 | 1.13 | 0.19 | -4.78 | 0.77 | 2.04
J1534.8+3716 | -11.52 | 2.06 | -0.28 | 1.29 | -0.78 | -4.35 | 0.57 | 1.96
J1535.0+5320 | -11.66 | 1.83 | 0.23 | 0.71 | 1.04 | -4.68 | 0.52 | 1.93
J1535.4+3919 | -11.64 | 2.2 | 0.19 | 1.14 | 0.15 | -4.58 | 0.76 | 2.55
J1540.1+8155 | -11.13 | 1.71 | 0.52 | 0.86 | 0.23 | -4.75 | 0.68 | 2.09
J1540.7+1449 | -11.41 | 2.15 | -0.2 | 1.19 | -0.33 | -4.35 | 1.06 | 2.83
J1543.0+6130 | -10.23 | 1.99 | 0.88 | 2.61 | -1.72 | -5.11 | 0.88 | 2.49
J1546.0+0819 | -11.17 | 1.9 | 0.47 | 1.11 | -0.49 | -4.75 | 0.82 | 2.11
J1548.8$-$2250 | -10.9 | 1.79 | 0.15 | 1.47 | 0.03 | -4.85 | 0.69 | 2.13
J1553.5$-$3118 | -10.91 | 1.95 | 0.52 | 1.77 | -0.6 | -4.78 | 0.76 | 2.22
J1555.7+1111 | -9.76 | 1.69 | 0.94 | 2.03 | -0.64 | -4.9 | 0.82 | 1.9
J1558.8+5625 | -10.96 | 2.12 | 0.46 | 1.74 | -1.59 | -4.9 | 0.98 | 2.7
J1602.2+3051 | -11.75 | 2.25 | -4.0 | 0.79 | -0.04 | -4.33 | 0.85 | 2.24
J1603.8$-$4903 | -10.3 | 2.01 | 0.59 | 2.6 | -1.76 | -6.21 | 0.75 | 1.77
J1604.5$-$4441 | -10.69 | 2.41 | 0.27 | 2.39 | -1.31 | -6.2 | 1.06 | 2.98
J1605.5+5423 | -11.83 | 1.85 | 0.21 | 0.97 | 0.75 | -4.65 | 0.27 | 1.54
J1606.3+5629 | -11.78 | 1.79 | 0.02 | 1.17 | 0.45 | -4.82 | 0.48 | 2.29
J1607.0+1550 | -10.68 | 2.26 | 0.74 | 0.89 | -1.73 | -5.96 | 0.98 | 3.1
J1610.7$-$6648 | -10.51 | 1.76 | 0.86 | 1.82 | -0.98 | -5.17 | 0.73 | 2.07
J1616.7+4107 | -11.75 | 2.25 | 0.25 | 1.05 | 0.26 | -4.37 | 0.71 | 2.45
J1626.3+3514 | -11.72 | 1.75 | 0.42 | 0.83 | -0.02 | -4.53 | 0.64 | 2.05
J1630.7+5221 | -10.95 | 2.04 | 0.51 | 1.38 | -1.19 | -5.16 | 0.83 | 2.17
J1637.1+1316 | -11.72 | 2.26 | 0.06 | 0.78 | -0.3 | -4.76 | 0.78 | 2.28
J1637.6+4548 | -12.01 | 1.92 | -0.29 | 1.06 | 0.17 | -4.28 | 0.38 | 2.23
J1637.7+7326 | -12.04 | 1.88 | 0.1 | 1.49 | 0.08 | -4.62 | 0.71 | 1.77
J1641.9$-$0621 | -10.92 | 2.35 | 0.43 | 1.62 | -1.27 | -6.28 | 1.15 | 2.81
J1642.4+2211 | -11.92 | 2.02 | -0.07 | 0.96 | 0.42 | -4.46 | 0.48 | 1.42
J1643.5$-$0646 | -11.37 | 2.14 | -0.84 | 1.51 | -0.31 | -4.24 | 0.43 | 1.91
J1644.2+4546 | -11.9 | 1.89 | -0.24 | 0.93 | 0.45 | -4.34 | 0.45 | 1.77
J1647.5+2911 | -11.63 | 2.27 | -1.55 | 1.19 | -0.39 | -3.73 | 0.38 | 1.6
J1647.5+4950 | -10.85 | 2.39 | -0.02 | 1.98 | -0.87 | -4.79 | 0.92 | 2.77
J1651.6+7219 | -11.49 | 1.88 | -0.13 | 1.16 | -0.02 | -4.06 | 0.73 | 1.4
J1652.7+4024 | -11.55 | 1.93 | 0.17 | 1.23 | -0.68 | -4.69 | 0.77 | 2.03
J1653.8+3945 | -9.89 | 1.76 | 0.5 | 2.73 | -0.21 | -4.27 | 0.48 | 1.97
J1702.6+3114 | -11.43 | 1.87 | 0.24 | 1.11 | -0.6 | -5.02 | 0.71 | 2.31
J1705.0+7134 | -11.73 | 2.34 | 0.2 | 1.21 | 0.13 | -4.42 | 0.78 | 2.27
J1712.7+2932 | -11.41 | 1.84 | 0.2 | 0.58 | -0.68 | -4.67 | 0.74 | 2.37
J1719.2+1745 | -10.72 | 2.06 | 0.74 | 3.1 | -1.39 | -5.76 | 1.1 | 2.7
J1725.0+1152 | -10.39 | 1.87 | 0.61 | 1.52 | -0.21 | -4.76 | 0.79 | 2.06
J1728.3+5013 | -10.67 | 1.78 | 0.25 | 2.25 | 0.32 | -4.56 | 0.64 | 2.18
J1730.8+3715 | -11.42 | 2.05 | 0.4 | 1.31 | -0.54 | -4.29 | 0.72 | 2.14
J1736.0+2033 | -11.35 | 1.91 | 0.49 | 1.7 | -1.08 | -4.93 | 0.75 | 2.11
J1742.5+5944 | -11.36 | 2.19 | 0.1 | 1.23 | -1.1 | -4.34 | 0.95 | 2.61
J1744.0+1935 | -11.05 | 1.95 | 0.26 | 1.11 | 0.02 | -4.51 | 0.45 | 1.92
J1745.4$-$0753 | -10.79 | 2.08 | -0.66 | 0.92 | -1.41 | -5.4 | 1.03 | 2.71
J1745.6+3950 | -11.71 | 2.18 | -0.61 | 0.8 | -0.08 | -4.45 | 0.53 | 1.89
J1747.2+4937 | -11.93 | 1.88 | -0.28 | 1.21 | 0.38 | -4.71 | 0.36 | 1.92
J1747.9+4704 | -11.87 | 2.39 | 0.5 | 0.86 | -0.56 | -5.49 | 1.15 | 2.78
J1748.6+7005 | -10.35 | 2.03 | 0.71 | 2.73 | -1.45 | -5.29 | 1.01 | 2.71
J1749.0+4321 | -10.96 | 2.09 | 0.3 | 1.5 | -1.45 | -5.17 | 1.06 | 2.92
J1751.5+0938 | -10.32 | 2.26 | 0.84 | 2.96 | -1.26 | -5.23 | 1.14 | 3.01
J1754.2+3212 | -10.63 | 1.92 | 0.77 | 2.57 | -1.16 | -5.33 | 0.86 | 2.17
J1756.3+5522 | -11.3 | 1.85 | 0.36 | 1.3 | 0.47 | -4.29 | 0.64 | 1.77
J1757.0+7032 | -11.76 | 1.83 | -0.02 | 1.22 | 0.7 | -4.39 | 0.65 | 1.99
J1800.1+7037 | -11.63 | 2.12 | 0.14 | 1.25 | 0.07 | -4.73 | 0.8 | 2.49
J1800.6+7828 | -10.27 | 2.21 | 0.69 | 2.45 | -1.5 | -5.13 | 1.09 | 2.8
J1806.8+6949 | -10.45 | 2.3 | 0.66 | 2.04 | -0.94 | -4.08 | 0.86 | 2.47
J1807.9+4650 | -11.8 | 1.89 | -0.32 | 1.05 | -0.32 | -4.4 | 0.74 | 2.44
J1809.3+2042 | -11.4 | 2.08 | -0.29 | 0.99 | -0.44 | -4.27 | 0.78 | 2.25
J1811.3+0340 | -10.94 | 1.87 | 0.53 | 1.55 | -0.95 | -5.11 | 0.74 | 1.94
J1813.5+3144 | -10.95 | 2.17 | 0.17 | 1.59 | -0.94 | -4.85 | 0.81 | 2.13
J1823.5+6858 | -11.36 | 2.21 | 0.68 | 0.75 | -1.52 | -5.07 | 0.86 | 2.57
J1824.1+5651 | -10.63 | 2.38 | 0.57 | 2.33 | -0.97 | -5.57 | 1.01 | 2.55
J1829.3+5402 | -11.28 | 1.86 | 0.44 | 1.32 | -0.41 | -4.6 | 0.81 | 2.22
J1836.4+3137 | -11.19 | 2.37 | -0.41 | 1.37 | -0.99 | -4.75 | 0.8 | 2.46
J1838.8+4802 | -10.57 | 1.85 | 0.62 | 2.4 | -0.97 | -5.31 | 0.73 | 2.22
J1841.8+3218 | -11.36 | 1.9 | 0.62 | 1.61 | 0.16 | -4.68 | 0.71 | 2.12
J1848.5+6537 | -11.81 | 1.75 | 0.29 | 1.36 | 0.4 | -4.48 | 0.44 | 1.88
J1848.9+4247 | -11.54 | 2.03 | -0.48 | 1.19 | 0.55 | -4.86 | 0.55 | 1.89
J1853.8+6714 | -11.83 | 2.22 | 0.07 | 0.95 | 0.11 | -3.57 | 0.49 | 1.91
J1903.2+5540 | -10.4 | 1.95 | 0.87 | 1.85 | -1.29 | -5.42 | 0.91 | 2.32
J1917.7$-$1921 | -10.41 | 1.94 | 0.31 | 1.76 | -0.8 | -4.55 | 0.76 | 2.45
J1921.8$-$1607 | -10.99 | 1.83 | 0.44 | 1.63 | -1.0 | -4.63 | 0.74 | 3.6
J1926.8+6154 | -10.9 | 1.91 | 0.63 | 1.76 | -0.48 | -4.72 | 0.78 | 2.15
J1927.5+6117 | -11.03 | 2.17 | 0.41 | 1.58 | -1.2 | -4.81 | 1.03 | 2.82
J1931.1+0937 | -10.53 | 1.86 | 0.67 | 1.95 | -0.25 | -4.72 | 0.54 | 1.66
J1933.3+0726 | -10.91 | 1.84 | 0.33 | 1.24 | -0.62 | -4.72 | 0.66 | 2.14
J1936.9$-$4720 | -11.1 | 1.78 | 0.22 | 1.66 | -0.15 | -4.97 | 0.64 | 2.08
J1942.7+1033 | -10.49 | 1.87 | 0.4 | 1.73 | -0.71 | -4.96 | 0.86 | 2.24
J1954.6$-$1122 | -10.82 | 2.44 | 0.18 | 2.24 | -1.31 | -5.62 | 1.17 | 2.84
J1958.3$-$3010 | -10.95 | 1.85 | 0.07 | 1.58 | 0.09 | -4.71 | 0.44 | 1.87
J2000.0+6508 | -9.96 | 1.82 | 0.41 | 3.17 | -0.19 | -4.0 | 0.64 | 1.92
J2001.2+4353 | -10.44 | 1.95 | 0.72 | 3.1 | -1.21 | -5.04 | 0.84 | 1.84
J2001.7+7040 | -11.3 | 2.16 | 0.17 | 1.2 | -1.24 | -4.72 | 0.86 | 2.51
J2005.1+7003 | -11.26 | 1.85 | 0.56 | 1.57 | -0.62 | -4.72 | 0.74 | 1.89
J2005.5+7752 | -10.59 | 2.21 | 0.55 | 2.58 | -1.43 | -4.85 | 1.03 | 2.97
J2009.4$-$4849 | -10.5 | 1.83 | 0.45 | 2.19 | 0.36 | -3.46 | 0.74 | 2.17
J2010.0+7229 | -10.79 | 2.3 | 0.7 | 1.88 | -1.76 | -5.61 | 1.11 | 3.05
J2012.0+4629 | -10.41 | 2.06 | 0.75 | 2.68 | -0.64 | -5.23 | 1.0 | 2.9
J2014.3$-$0047 | -11.27 | 1.98 | -0.45 | 1.41 | -0.5 | -4.72 | 0.7 | 2.39
J2014.5+0648 | -11.31 | 1.85 | 0.12 | 0.78 | -0.72 | -4.72 | 0.63 | 1.66
J2015.2$-$0137 | -10.93 | 2.23 | 0.5 | 1.09 | -1.3 | -4.95 | 0.96 | 2.62
J2016.3$-$0903 | -10.95 | 1.98 | 0.5 | 1.53 | -1.23 | -4.72 | 0.88 | 2.39
J2025.3+3341 | -10.53 | 2.63 | 0.66 | 2.06 | -2.02 | -4.72 | 1.26 | 3.58
J2032.0+1219 | -11.19 | 2.41 | 0.25 | 1.56 | -1.19 | -5.05 | 1.11 | 3.33
J2039.0$-$1046 | -10.74 | 2.08 | 0.68 | 1.51 | -1.2 | -4.78 | 0.95 | 2.59
J2039.5+5218 | -11.25 | 1.84 | 0.05 | 0.82 | -0.37 | -5.19 | 0.12 | 1.67
J2042.1+2427 | -11.25 | 1.91 | -0.82 | 1.16 | 0.47 | -3.95 | 0.25 | 1.55
J2049.7$-$0036 | -12.06 | 1.54 | -0.33 | 0.92 | 0.7 | -4.55 | 0.4 | 2.7
J2050.0+0408 | -11.05 | 2.29 | -0.35 | 1.16 | -1.16 | -5.35 | 1.02 | 2.96
J2052.5+0810 | -12.08 | 1.49 | 0.41 | 1.02 | 0.73 | -4.55 | 0.49 | 2.35
J2054.8+0015 | -11.54 | 1.82 | -1.41 | 1.05 | 0.03 | -4.65 | 0.52 | 1.98
J2055.4$-$0020 | -11.41 | 1.84 | 0.24 | 1.1 | 0.45 | -4.66 | 0.65 | 2.62
J2108.7$-$0250 | -11.42 | 2.04 | -0.58 | 0.95 | -0.1 | -4.23 | 0.54 | 2.0
J2108.9$-$6638 | -11.09 | 2.12 | -0.1 | 0.99 | -0.36 | -5.07 | 0.95 | 2.26
J2116.2+3339 | -10.51 | 1.9 | 0.8 | 2.14 | -1.75 | -4.72 | 0.77 | 1.95
J2127.7+3612 | -10.99 | 1.99 | 0.63 | 1.69 | -1.09 | -4.72 | 0.83 | 2.42
J2131.0$-$2746 | -11.09 | 1.79 | 0.61 | 1.45 | -0.17 | -5.07 | 0.7 | 1.76
J2131.5$-$0916 | -11.14 | 1.99 | -0.17 | 1.42 | 0.34 | -4.9 | 0.68 | 2.17
J2131.7$-$2515 | -11.44 | 1.84 | 0.31 | 1.05 | 0.23 | -4.82 | 0.58 | 2.05
J2134.2$-$0154 | -10.88 | 2.3 | 0.36 | 2.01 | -1.27 | -5.56 | 1.15 | 3.36
J2138.8$-$2055 | -11.76 | 1.76 | 0.24 | 1.01 | 0.88 | -4.76 | 0.53 | 2.24
J2139.4$-$4235 | -10.27 | 2.01 | 0.75 | 2.91 | -1.53 | -5.05 | 0.93 | 2.3
J2145.7+0718 | -11.6 | 2.08 | -0.41 | 0.5 | 0.62 | -4.46 | 0.63 | 2.13
J2146.5$-$1344 | -10.82 | 1.72 | 0.75 | 1.54 | -0.79 | -4.72 | 0.73 | 2.12
J2149.6+0323 | -11.23 | 2.16 | 0.1 | 1.64 | -1.52 | -4.53 | 0.93 | 2.5
J2150.1$-$1410 | -11.34 | 1.78 | 0.32 | 1.09 | 0.52 | -4.9 | 0.58 | 1.71
J2152.0$-$1205 | -11.64 | 2.07 | 0.32 | 0.84 | 0.37 | -4.76 | 0.75 | 1.9
J2152.5+1737 | -11.74 | 2.27 | -0.36 | 1.12 | -0.88 | -4.26 | 1.06 | 2.94
J2153.1$-$0041 | -11.69 | 1.79 | -0.58 | 1.2 | 0.51 | -4.54 | 0.6 | 1.88
J2158.8$-$3013 | -9.67 | 1.85 | 0.73 | 2.82 | 0.51 | -4.41 | 0.75 | 1.82
J2159.1$-$2840 | -11.33 | 1.88 | 0.46 | 1.22 | -0.75 | -4.81 | 0.64 | 1.52
J2202.7+4216 | -9.64 | 2.2 | 0.98 | 3.55 | -1.0 | -5.09 | 0.99 | 2.82
J2204.3+0438 | -11.31 | 2.38 | 0.2 | 1.29 | -0.49 | -3.61 | 0.45 | 2.24
J2206.8$-$0032 | -10.99 | 2.25 | 0.42 | 2.0 | -1.37 | -5.57 | 0.98 | 3.08
J2211.0$-$0003 | -11.63 | 1.95 | 0.12 | 0.91 | 0.17 | -4.81 | 0.68 | 2.12
J2216.9+2421 | -11.09 | 2.28 | 0.26 | 1.62 | -1.02 | -5.03 | 1.04 | 2.82
J2221.5$-$5225 | -11.06 | 1.77 | 0.54 | 1.57 | 0.13 | -4.54 | 0.72 | 2.14
J2223.3+0102 | -11.73 | 1.9 | 0.11 | 1.09 | -0.93 | -4.72 | 0.82 | 2.26
J2224.0$-$1127 | -11.73 | 2.11 | 0.33 | 1.14 | -0.81 | -4.59 | 0.89 | 2.58
J2232.8+1334 | -11.94 | 1.78 | -0.0 | 1.07 | 0.45 | -4.46 | 0.57 | 1.82
J2236.5$-$1433 | -10.25 | 2.17 | 0.84 | 3.25 | -1.79 | -6.05 | 1.08 | 2.96
J2243.4$-$2544 | -10.84 | 2.13 | 0.63 | 1.54 | -0.99 | -5.11 | 0.97 | 2.51
J2243.9+2021 | -10.39 | 1.86 | 0.84 | 2.08 | -1.28 | -4.85 | 0.83 | 2.34
J2244.9$-$0007 | -11.69 | 2.31 | -0.38 | 0.86 | -0.29 | -4.86 | 0.58 | 2.41
J2247.4$-$0001 | -11.21 | 2.06 | 0.25 | 1.16 | -1.11 | -5.34 | 1.01 | 3.06
J2247.8+4413 | -11.19 | 1.79 | -0.04 | 1.11 | -0.17 | -4.87 | 0.66 | 2.18
J2249.4$-$1300 | -10.96 | 2.41 | -0.22 | 2.39 | -0.05 | -5.32 | 0.33 | 2.34
J2250.0+3825 | -11.06 | 1.73 | -0.49 | 1.44 | -0.21 | -4.18 | 0.6 | 1.93
J2250.7$-$2806 | -10.63 | 2.18 | 0.69 | 2.79 | -1.5 | -6.24 | 1.03 | 2.35
J2252.0+4031 | -10.96 | 2.05 | 0.25 | 1.38 | -1.13 | -4.76 | 0.82 | 2.56
J2253.7+1405 | -11.64 | 1.96 | 0.1 | 1.28 | -0.44 | -4.69 | 0.52 | 1.81
J2255.2+2411 | -10.95 | 2.11 | -0.18 | 1.29 | -1.01 | -4.79 | 0.92 | 2.55
J2256.6$-$2011 | -11.03 | 2.12 | 0.19 | 0.94 | -0.81 | -5.21 | 1.06 | 2.86
J2257.5+0748 | -11.66 | 2.41 | -0.2 | 1.12 | -0.61 | -3.73 | 0.89 | 2.6
J2258.3$-$3643 | -11.55 | 2.12 | -0.08 | 1.3 | -1.11 | -4.72 | 0.58 | 2.35
J2258.4$-$5524 | -11.46 | 2.21 | -0.47 | 0.86 | 0.26 | -4.54 | 0.68 | 1.98
J2304.6+3704 | -11.11 | 1.85 | 0.14 | 1.58 | 0.21 | -4.73 | 0.67 | 2.02
J2307.4$-$1206 | -11.85 | 1.94 | -0.79 | 1.01 | 0.32 | -4.54 | 0.59 | 2.12
J2314.0+1445 | -11.17 | 1.85 | 0.29 | 1.09 | -0.33 | -4.53 | 0.43 | 1.63
J2315.6$-$5018 | -11.38 | 2.4 | -0.62 | 1.64 | -0.64 | -5.04 | 1.06 | 3.0
J2319.1$-$4207 | -11.49 | 2.01 | -0.48 | 0.79 | -0.14 | -3.53 | 0.17 | 1.42
J2319.7+1609 | -11.81 | 1.88 | 0.31 | 0.89 | 0.62 | -4.23 | 0.66 | 1.8
J2322.7+3436 | -11.34 | 1.96 | -0.31 | 1.09 | -0.28 | -3.85 | 0.29 | 1.71
J2322.8$-$4916 | -11.2 | 1.87 | 0.56 | 1.51 | -0.26 | -4.72 | 0.72 | 2.19
J2323.8+4210 | -10.71 | 1.89 | 0.65 | 1.58 | -0.51 | -4.93 | 0.77 | 2.12
J2324.7$-$4041 | -10.93 | 1.79 | 0.53 | 1.7 | 0.44 | -4.12 | 0.75 | 2.04
J2325.2+3957 | -10.87 | 2.12 | 0.71 | 1.88 | -1.53 | -5.09 | 1.02 | 2.92
J2325.4$-$4800 | -10.93 | 2.11 | 0.32 | 1.69 | -0.59 | -4.99 | 0.91 | 2.58
J2325.6+1644 | -11.61 | 1.96 | 0.0 | 1.22 | -0.64 | -4.72 | 0.74 | 2.39
J2329.2+3755 | -11.12 | 1.9 | -0.01 | 1.17 | -0.41 | -4.86 | 0.74 | 2.31
J2330.6$-$3726 | -11.42 | 2.46 | -0.14 | 1.1 | -0.72 | -4.06 | 0.97 | 2.55
J2338.9+2124 | -11.33 | 2.01 | -0.41 | 1.26 | 0.21 | -4.31 | 0.82 | 2.46
J2340.8+8015 | -10.74 | 1.94 | 0.62 | 1.11 | -0.38 | -5.66 | 0.77 | 2.06
J2343.6+3438 | -11.37 | 1.77 | 0.15 | 1.32 | 0.44 | -4.81 | 0.54 | 1.71
J2346.7+8008 | -11.17 | 2.41 | 0.43 | 1.19 | -1.34 | -5.18 | 1.05 | 2.27
J2347.0+5141 | -10.49 | 1.81 | 0.16 | 1.78 | -0.27 | -4.55 | 0.33 | 1.72
J2353.5$-$1457 | -11.84 | 2.08 | -1.41 | 0.92 | 0.41 | -4.88 | 0.52 | 2.48
J2353.7$-$3037 | -11.39 | 2.16 | 0.21 | 1.01 | -0.93 | -4.65 | 0.98 | 2.96
J2357.4$-$1718 | -11.39 | 1.76 | 0.17 | 0.68 | 0.86 | -4.41 | 0.67 | 1.95
J2359.0$-$3038 | -11.27 | 1.82 | -0.32 | 1.06 | 1.22 | -4.14 | 0.68 | 2.14
|  |  | FSRQ |  |  |  |  |
J0004.4-4737 | -11.25 | 2.37 | 0.38 | 2.14 | -0.48 | -5.19 | 1.09 | 3.33
J0005.9+3824 | -11.12 | 2.67 | 0.49 | 1.43 | -0.66 | -4.96 | 1.11 | 3.29
J0010.6+2043 | -11.67 | 2.32 | -0.19 | 1.43 | -0.28 | -4.29 | 1.0 | 2.65
J0010.6$-$3025 | -11.31 | 2.46 | 0.27 | 1.96 | -1.12 | -5.15 | 1.02 | 3.03
J0011.4+0057 | -11.27 | 2.33 | 0.2 | 1.86 | -0.94 | -4.83 | 1.07 | 3.17
J0013.6$-$0424 | -11.7 | 2.31 | -0.14 | 1.0 | -0.49 | -4.91 | 1.02 | 3.58
J0016.2$-$0016 | -11.05 | 2.74 | 0.62 | 1.91 | -1.25 | -5.78 | 1.21 | 2.93
J0017.5$-$0514 | -10.95 | 2.56 | 0.41 | 2.36 | -0.81 | -5.21 | 1.08 | 2.71
J0019.6+7327 | -10.72 | 2.62 | 0.45 | 2.5 | -1.9 | -5.72 | 1.08 | 2.6
J0030.3$-$4224 | -10.81 | 2.52 | 0.31 | 1.9 | -1.19 | -5.63 | 1.16 | 2.86
J0038.2$-$2459 | -10.85 | 2.26 | 0.61 | 3.22 | -0.68 | -5.04 | 1.09 | 3.06
J0047.9+2233 | -11.24 | 2.51 | -0.22 | 2.1 | -1.72 | -5.13 | 1.01 | 2.84
J0049.6$-$4500 | -11.66 | 2.63 | 0.03 | 0.97 | 0.36 | -3.94 | 0.88 | 3.04
J0050.0$-$5736 | -11.18 | 2.62 | -0.7 | 1.82 | -0.81 | -5.06 | 0.99 | 2.81
J0051.1$-$0648 | -11.05 | 2.35 | 0.6 | 2.18 | -1.18 | -5.59 | 1.11 | 2.18
J0051.5$-$4220 | -11.42 | 2.8 | 0.51 | 1.38 | -0.88 | -4.94 | 1.16 | 3.43
J0059.2+0006 | -11.65 | 2.38 | -0.4 | 1.07 | -0.34 | -4.34 | 1.17 | 2.82
J0101.8$-$7543 | -11.71 | 2.79 | -0.33 | 0.79 | -0.5 | -4.29 | 1.25 | 2.85
J0102.8+5824 | -10.36 | 2.29 | 0.64 | 3.12 | -1.39 | -6.17 | 1.11 | 2.54
J0108.6+0134 | -9.9 | 2.36 | 1.18 | 3.81 | -2.42 | -6.3 | 1.16 | 3.23
J0109.7+6133 | -10.5 | 2.62 | 0.81 | 2.98 | -1.62 | -4.72 | 1.05 | 3.08
J0112.8+3208 | -10.51 | 2.34 | 0.7 | 3.02 | -0.51 | -5.53 | 1.03 | 2.87
J0113.4+4948 | -10.79 | 2.22 | 0.52 | 2.67 | -0.98 | -5.41 | 1.1 | 3.03
J0115.1$-$0129 | -11.31 | 2.72 | -0.87 | 1.69 | -0.6 | -4.42 | 1.41 | 3.07
J0116.0$-$1136 | -10.97 | 2.36 | 0.26 | 2.47 | -0.74 | -5.27 | 1.13 | 2.86
J0118.9$-$2141 | -10.52 | 2.26 | 0.81 | 2.31 | -1.99 | -5.92 | 1.15 | 2.77
J0125.7$-$0015 | -11.4 | 2.96 | 0.01 | 0.78 | -0.3 | -4.88 | 0.86 | 3.17
J0126.0$-$2221 | -11.28 | 2.59 | 0.31 | 2.06 | -1.02 | -4.96 | 1.03 | 2.64
J0132.7$-$1654 | -10.62 | 2.34 | 0.63 | 2.41 | -1.61 | -5.6 | 1.15 | 3.05
J0133.1$-$5201 | -10.74 | 2.32 | 0.69 | 3.15 | -0.98 | -6.22 | 1.14 | 2.96
J0134.3$-$3842 | -11.69 | 2.49 | 0.09 | 1.53 | -0.17 | -4.35 | 1.11 | 2.75
J0134.5+2637 | -11.0 | 1.99 | 0.23 | 1.04 | -0.7 | -4.7 | 0.81 | 2.14
J0137.0+4751 | -10.44 | 2.3 | 0.89 | 3.15 | -1.2 | -5.6 | 1.07 | 2.7
J0137.6$-$2430 | -10.87 | 2.54 | 0.62 | 2.54 | -0.69 | -4.91 | 1.18 | 3.09
J0145.0$-$2732 | -11.01 | 2.6 | 0.48 | 2.91 | -0.95 | -5.43 | 1.21 | 3.31
J0152.2+2206 | -11.16 | 2.68 | 0.38 | 1.54 | -0.89 | -4.88 | 1.19 | 3.07
J0157.7$-$4614 | -11.31 | 2.45 | 0.59 | 2.09 | -1.51 | -5.7 | 1.14 | 3.18
J0202.4+0849 | -11.65 | 1.83 | 0.37 | 1.13 | 0.05 | -4.79 | 0.48 | 2.13
J0205.0$-$1700 | -10.84 | 2.63 | 0.54 | 2.37 | -1.07 | -5.2 | 1.11 | 2.98
J0205.2+3212 | -10.89 | 2.66 | 0.35 | 2.41 | -1.07 | -5.15 | 1.51 | 3.35
J0206.4$-$1151 | -10.85 | 2.4 | 0.34 | 2.31 | -1.53 | -5.69 | 1.1 | 2.69
J0210.7$-$5101 | -10.23 | 2.34 | 1.0 | 3.17 | -1.55 | -5.38 | 1.14 | 2.86
J0217.0$-$0821 | -11.35 | 2.34 | 0.37 | 0.83 | -0.48 | -5.59 | 1.08 | 3.1
J0217.4+7352 | -10.87 | 2.94 | 0.37 | 1.61 | -1.05 | -5.57 | 1.04 | 3.42
J0217.8+0144 | -10.54 | 2.24 | 0.72 | 2.66 | -1.37 | -4.74 | 1.11 | 3.19
J0221.1+3556 | -10.07 | 2.29 | 0.72 | 3.54 | -2.02 | -4.72 | 1.14 | 2.71
J0222.0$-$1616 | -11.36 | 2.4 | -0.42 | 1.6 | -0.9 | -3.48 | 1.02 | 2.98
J0224.2+0700 | -11.49 | 2.5 | -0.35 | 1.34 | -0.22 | -5.35 | 1.06 | 2.79
J0224.9+1843 | -11.3 | 2.95 | 0.44 | 1.72 | 0.13 | -5.54 | 1.09 | 3.62
J0228.7+6718 | -11.16 | 2.58 | 0.49 | 1.17 | -0.89 | -5.11 | 1.16 | 3.28
J0229.5$-$3644 | -10.94 | 2.6 | 0.61 | 2.43 | -0.97 | -5.5 | 1.1 | 3.43
J0230.8+4032 | -11.02 | 2.45 | 0.54 | 2.47 | -0.5 | -5.42 | 1.14 | 3.16
J0231.2$-$4745 | -11.18 | 2.76 | -0.13 | 1.73 | -0.99 | -4.86 | 1.13 | 2.6
J0231.8+1322 | -10.97 | 2.68 | 0.14 | 2.37 | -1.15 | -4.96 | 0.96 | 3.05
J0236.8$-$6136 | -10.92 | 2.35 | 0.13 | 2.9 | -0.87 | -5.32 | 1.03 | 3.46
J0237.8+2848 | -9.94 | 2.32 | 1.07 | 3.72 | -1.96 | -6.3 | 1.19 | 2.81
J0239.7+0415 | -11.08 | 2.78 | 0.14 | 2.21 | -0.91 | -5.16 | 1.22 | 2.67
J0245.4+2408 | -11.15 | 2.68 | 0.04 | 2.03 | -1.43 | -5.27 | 1.09 | 3.28
J0245.9$-$4650 | -10.51 | 2.42 | 0.87 | 3.06 | -1.53 | -5.73 | 1.07 | 2.62
J0252.8$-$2219 | -10.34 | 2.36 | 0.85 | 3.08 | -1.75 | -6.29 | 1.13 | 2.98
J0253.2$-$5441 | -11.15 | 2.53 | 0.16 | 2.25 | -0.58 | -5.41 | 1.16 | 3.02
J0259.4+0746 | -10.71 | 2.2 | 0.52 | 2.41 | -1.87 | -5.33 | 1.05 | 3.04
J0259.5+1924 | -11.5 | 2.37 | -0.93 | 0.77 | -0.82 | -4.93 | 1.05 | 2.49
J0301.6$-$7155 | -11.35 | 2.54 | 0.18 | 1.63 | -1.01 | -4.72 | 0.92 | 3.19
J0303.6$-$6211 | -11.0 | 2.45 | 0.47 | 2.18 | -0.96 | -5.32 | 1.22 | 3.18
J0309.0+1029 | -10.8 | 2.35 | 0.58 | 2.7 | -1.27 | -5.58 | 1.13 | 3.15
J0309.9$-$6058 | -10.59 | 2.49 | 0.77 | 2.89 | -1.61 | -5.65 | 1.13 | 3.65
J0310.9+3815 | -11.31 | 2.4 | 0.29 | 1.24 | -0.5 | -5.41 | 1.05 | 1.99
J0314.6$-$6549 | -11.64 | 2.44 | -0.38 | 0.78 | -0.07 | -4.8 | 1.01 | 2.91
J0315.9$-$1033 | -11.09 | 2.48 | 0.33 | 2.09 | -1.49 | -5.15 | 1.19 | 3.25
J0325.7+2225 | -10.7 | 2.65 | 0.8 | 2.25 | -0.98 | -5.7 | 1.22 | 3.56
J0332.1$-$1123 | -11.65 | 2.39 | 0.3 | 1.55 | -0.38 | -4.45 | 0.91 | 3.44
J0336.4+3224 | -10.89 | 2.8 | 0.81 | 1.66 | -0.32 | -4.95 | 1.3 | 2.61
J0336.8$-$3612 | -11.41 | 2.81 | 0.05 | 1.1 | -0.76 | -4.63 | 1.23 | 3.12
J0339.5$-$0146 | -10.18 | 2.32 | 0.89 | 3.18 | -1.6 | -6.02 | 1.18 | 2.82
J0343.2$-$2529 | -11.2 | 2.54 | 0.48 | 2.29 | -1.28 | -5.24 | 0.99 | 3.03
J0348.5$-$2749 | -10.48 | 2.18 | 0.71 | 3.57 | -1.17 | -5.81 | 1.13 | 3.23
J0349.8$-$2103 | -10.86 | 2.48 | 0.79 | 2.55 | -1.2 | -6.42 | 1.19 | 3.0
J0359.6+5057 | -10.48 | 2.66 | 0.67 | 2.89 | -1.26 | -5.7 | 1.33 | 3.45
J0403.3+2601 | -11.49 | 2.59 | 0.39 | 1.07 | -1.02 | -4.55 | 1.0 | 3.33
J0403.9$-$3605 | -10.13 | 2.53 | 1.12 | 3.78 | -1.35 | -5.58 | 1.2 | 3.74
J0405.6$-$1308 | -11.06 | 2.55 | -0.15 | 1.9 | -0.61 | -4.62 | 1.11 | 2.43
J0407.0$-$3826 | -10.67 | 2.36 | 0.78 | 2.54 | -1.5 | -5.37 | 1.17 | 2.57
J0416.5$-$1852 | -11.06 | 2.39 | 0.03 | 2.2 | -1.19 | -4.98 | 1.23 | 2.41
J0422.1$-$0644 | -10.77 | 2.49 | 0.46 | 2.68 | -1.34 | -5.23 | 0.98 | 2.86
J0422.8+0225 | -11.4 | 2.83 | 0.58 | 1.29 | -0.64 | -5.24 | 1.2 | 3.19
J0423.3$-$0120 | -10.45 | 2.33 | 0.77 | 3.09 | -1.07 | -5.19 | 1.14 | 3.7
J0429.3$-$4326 | -11.74 | 2.41 | -0.33 | 1.15 | -0.78 | -4.3 | 1.27 | 3.04
J0433.6$-$6030 | -10.97 | 2.44 | 0.62 | 2.24 | -1.57 | -5.07 | 0.4 | 2.84
J0440.3$-$4333 | -11.14 | 2.64 | 0.82 | 2.8 | -0.92 | -4.72 | 0.89 | 2.98
J0442.6$-$0017 | -10.38 | 2.44 | 0.73 | 3.0 | -1.05 | -6.15 | 1.07 | 3.35
J0449.1+1121 | -10.5 | 2.51 | 0.81 | 2.25 | -1.74 | -6.34 | 1.18 | 3.2
J0449.6$-$8100 | -12.05 | 2.11 | -0.3 | 1.04 | 0.05 | -4.47 | 1.08 | 2.4
J0451.8$-$4651 | -11.24 | 2.45 | 0.36 | 2.24 | -0.85 | -5.2 | 0.99 | 2.74
J0453.1$-$2806 | -10.67 | 2.65 | 0.67 | 2.5 | -1.65 | -5.45 | 1.05 | 3.08
J0455.7$-$4617 | -10.88 | 2.52 | 0.48 | 2.22 | -0.89 | -4.92 | 1.17 | 2.83
J0456.6$-$3136 | -11.22 | 2.52 | 0.26 | 1.32 | -0.96 | -5.38 | 1.07 | 2.63
J0457.0+0646 | -11.31 | 2.54 | 0.02 | 1.84 | -0.63 | -4.97 | 1.07 | 2.82
J0457.0$-$2324 | -9.75 | 2.21 | 1.11 | 3.64 | -2.14 | -6.49 | 1.13 | 3.12
J0501.2$-$0158 | -10.28 | 2.37 | 0.93 | 3.16 | -1.41 | -5.92 | 1.11 | 2.74
J0503.1$-$6045 | -11.65 | 2.71 | 0.29 | 1.17 | -0.71 | -4.99 | 0.84 | 2.85
J0505.3+0459 | -10.17 | 2.37 | 1.01 | 3.46 | -1.76 | -6.27 | 1.17 | 3.59
J0505.8$-$0419 | -11.17 | 2.4 | -0.3 | 1.79 | -1.54 | -4.87 | 1.03 | 3.61
J0507.7$-$6104 | -11.0 | 2.52 | 0.29 | 1.84 | -0.99 | -5.12 | 1.07 | 2.89
J0509.4+1012 | -11.01 | 2.41 | 0.28 | 1.9 | -1.01 | -5.26 | 1.06 | 2.24
J0510.0+1800 | -10.41 | 2.2 | 0.81 | 3.26 | -1.66 | -6.03 | 1.12 | 3.23
J0515.6$-$4556 | -10.76 | 2.42 | 0.39 | 2.91 | -0.85 | -5.08 | 0.95 | 2.86
J0521.3$-$1734 | -11.46 | 2.37 | 0.52 | 0.63 | -0.88 | -4.64 | 0.88 | 2.59
J0525.4$-$4600 | -11.46 | 2.38 | -0.03 | 0.86 | -0.58 | -4.3 | 1.19 | 3.05
J0526.2$-$4830 | -10.56 | 2.3 | 0.66 | 2.86 | -1.52 | -6.28 | 1.11 | 3.25
J0530.9+1332 | -10.66 | 2.56 | 0.83 | 2.67 | -1.09 | -6.18 | 1.0 | 2.96
J0532.6+0732 | -10.24 | 2.36 | 0.89 | 2.76 | -1.92 | -5.93 | 1.15 | 2.83
J0533.3+4823 | -10.47 | 2.41 | 0.75 | 2.37 | -1.82 | -6.33 | 1.24 | 3.32
J0533.8$-$3749 | -11.58 | 2.34 | -4.0 | 1.5 | -0.78 | -5.29 | 1.14 | 3.13
J0536.4$-$3401 | -10.7 | 2.62 | 0.58 | 2.63 | -1.12 | -5.46 | 1.11 | 2.72
J0539.9$-$2839 | -10.8 | 2.73 | 0.57 | 2.03 | -0.95 | -6.04 | 1.17 | 2.38
J0540.8$-$5415 | -11.22 | 2.63 | -0.06 | 2.06 | -1.14 | -4.87 | 1.1 | 3.03
J0541.6$-$0541 | -11.15 | 2.55 | 0.19 | 1.16 | -1.2 | -5.85 | 1.2 | 2.58
J0550.3$-$5733 | -11.75 | 2.22 | -1.34 | 1.21 | -0.11 | -4.89 | 1.17 | 3.19
J0555.6+3947 | -10.76 | 2.76 | 0.7 | 2.19 | -1.08 | -5.28 | 0.89 | 3.35
J0600.6$-$3939 | -11.2 | 2.86 | 0.45 | 0.95 | -0.17 | -5.08 | 1.28 | 3.14
J0601.1$-$7035 | -10.74 | 2.42 | 0.69 | 2.76 | -1.88 | -5.51 | 1.15 | 2.48
J0608.0+6721 | -11.3 | 2.49 | 0.34 | 1.91 | -0.84 | -5.78 | 1.06 | 2.87
J0608.0$-$0835 | -10.63 | 2.43 | 0.5 | 2.46 | -1.64 | -5.61 | 0.47 | 2.25
J0608.1$-$1521 | -10.87 | 2.58 | 0.26 | 2.49 | -1.61 | -4.72 | 1.16 | 2.9
J0609.0$-$2219 | -11.68 | 2.24 | 0.33 | 1.36 | -0.9 | -5.16 | 1.18 | 3.39
J0610.9$-$6054 | -11.44 | 2.58 | 0.07 | 1.42 | -0.9 | -4.8 | 1.14 | 2.93
J0612.5$-$3138 | -11.25 | 2.5 | -0.38 | 1.56 | -1.03 | -4.99 | 1.11 | 2.93
J0622.4$-$6433 | -11.61 | 3.04 | -0.61 | 0.9 | 0.68 | -3.15 | 0.9 | 2.38
J0625.8$-$5441 | -11.38 | 2.73 | 0.12 | 1.36 | -1.2 | -5.04 | 1.47 | 3.69
J0635.6$-$7518 | -10.9 | 2.7 | -0.37 | 2.65 | -0.3 | -4.24 | 1.09 | 2.93
J0638.6+7320 | -11.29 | 3.03 | -0.36 | 1.71 | -0.67 | -4.47 | 1.23 | 3.21
J0648.0$-$3045 | -10.86 | 2.49 | 0.59 | 2.63 | -1.51 | -6.14 | 1.19 | 2.74
J0654.3+5042 | -10.89 | 2.23 | 0.62 | 2.38 | -1.49 | -4.64 | 0.72 | 3.09
J0654.4+4514 | -10.82 | 2.27 | 0.49 | 2.84 | -0.93 | -6.42 | 1.11 | 3.63
J0701.5$-$4634 | -10.85 | 2.44 | 0.78 | 2.58 | -1.25 | -5.79 | 1.19 | 3.47
J0713.8+1935 | -10.8 | 2.4 | 0.64 | 2.9 | -1.75 | -5.4 | 0.98 | 3.24
J0718.0+4536 | -11.19 | 2.43 | 0.66 | 2.19 | -0.96 | -4.91 | 1.17 | 2.79
J0719.3+3307 | -10.47 | 2.2 | 0.9 | 2.97 | -1.79 | -5.19 | 1.06 | 3.18
J0721.3+0405 | -10.83 | 2.56 | 0.63 | 1.94 | -1.28 | -5.39 | 1.09 | 2.76
J0725.2+1425 | -10.36 | 2.29 | 0.75 | 3.33 | -1.68 | -5.75 | 1.11 | 2.83
J0726.4$-$4727 | -10.92 | 2.48 | 0.59 | 2.1 | -1.53 | -5.56 | 1.17 | 3.31
J0729.1+5703 | -11.6 | 2.51 | 0.03 | 1.57 | -0.21 | -4.04 | 0.86 | 2.67
J0730.3$-$1141 | -9.89 | 2.3 | 1.06 | 3.36 | -2.12 | -7.07 | 1.06 | 3.41
J0734.0+5021 | -11.24 | 2.47 | 0.39 | 1.82 | -0.7 | -5.32 | 1.04 | 2.75
J0739.2+0137 | -10.24 | 2.41 | 0.89 | 3.29 | -1.07 | -5.19 | 1.01 | 2.8
J0741.4$-$4709 | -11.31 | 2.59 | -0.19 | 1.43 | -0.88 | -5.05 | 1.01 | 2.47
J0742.6+5443 | -10.62 | 2.32 | 0.77 | 3.36 | -1.46 | -4.98 | 1.04 | 2.08
J0746.4+2546 | -11.17 | 2.86 | 0.5 | 1.94 | -0.91 | -5.54 | 0.94 | 3.82
J0748.6+2400 | -11.07 | 2.34 | 0.25 | 2.14 | -0.49 | -5.32 | 1.08 | 3.0
J0749.9+1823 | -11.46 | 2.52 | -0.05 | 1.37 | -1.05 | -5.44 | 1.19 | 3.2
J0750.8+1229 | -11.03 | 2.52 | 0.27 | 2.19 | -0.39 | -4.72 | 1.08 | 2.84
J0805.4+6147 | -11.17 | 2.8 | 0.52 | 2.34 | -0.58 | -5.41 | 1.2 | 3.59
J0808.2$-$0751 | -10.22 | 2.22 | 0.92 | 3.23 | -1.49 | -6.42 | 1.0 | 3.08
J0809.3+4053 | -11.45 | 2.59 | 0.25 | 1.59 | -0.47 | -5.16 | 1.19 | 2.94
J0818.8+3229 | -11.8 | 2.23 | 0.08 | 1.23 | 0.12 | -5.3 | 1.07 | 2.65
J0824.7+5552 | -11.06 | 2.61 | 0.07 | 2.04 | -0.79 | -5.05 | 1.26 | 3.07
J0824.9+3915 | -11.08 | 2.43 | 0.42 | 1.55 | -0.56 | -5.05 | 1.22 | 3.05
J0830.8+2410 | -10.73 | 2.52 | 0.78 | 3.21 | -0.8 | -5.01 | 1.24 | 2.72
J0833.9+4223 | -11.23 | 2.43 | 0.23 | 1.42 | -0.55 | -4.5 | 1.02 | 2.88
J0836.5$-$2026 | -11.24 | 2.91 | 0.49 | 1.4 | -0.75 | -5.36 | 0.97 | 3.64
J0839.8+0105 | -11.12 | 2.42 | 0.69 | 2.01 | -0.85 | -5.36 | 1.15 | 3.34
J0841.3+7053 | -10.32 | 2.82 | 1.16 | 3.53 | -0.6 | -5.12 | 1.14 | 3.46
J0850.1$-$1212 | -10.67 | 2.3 | 0.67 | 2.81 | -1.3 | -4.89 | 1.08 | 3.28
J0852.2+2834 | -11.53 | 2.49 | 0.29 | 1.03 | -0.76 | -5.1 | 0.86 | 2.74
J0857.9$-$1949 | -11.02 | 2.52 | 0.05 | 1.87 | -0.95 | -5.3 | 1.21 | 3.05
J0903.1+4652 | -11.2 | 2.47 | -0.31 | 1.3 | -1.07 | -5.42 | 1.23 | 3.28
J0909.1+0121 | -10.57 | 2.47 | 0.69 | 2.92 | -1.26 | -5.19 | 1.09 | 2.36
J0909.7$-$0230 | -10.67 | 2.29 | 0.71 | 2.18 | -1.84 | -5.59 | 0.86 | 2.5
J0910.6+2247 | -11.3 | 2.34 | 0.52 | 2.18 | -1.41 | -5.9 | 0.94 | 3.73
J0914.4+0249 | -11.68 | 2.45 | -0.07 | 1.18 | -0.42 | -5.05 | 1.06 | 3.22
J0916.7+3856 | -11.2 | 2.46 | 0.26 | 1.82 | -1.19 | -5.4 | 1.12 | 3.16
J0920.9+4441 | -10.33 | 2.35 | 1.06 | 3.33 | -1.31 | -5.77 | 1.21 | 3.21
J0922.4$-$0528 | -11.27 | 2.14 | 0.36 | 1.09 | -0.74 | -4.83 | 0.84 | 2.61
J0928.1$-$2035 | -11.29 | 2.45 | 0.2 | 2.03 | 0.0 | -4.11 | 1.04 | 2.93
J0937.1+5008 | -11.4 | 2.4 | 0.42 | 1.61 | -0.34 | -5.02 | 1.17 | 3.02
J0949.0+4038 | -11.5 | 2.61 | -0.58 | 1.5 | -0.76 | -4.55 | 1.27 | 3.12
J0949.2+1749 | -11.62 | 2.52 | -0.23 | 1.52 | -0.61 | -4.02 | 1.1 | 3.06
J0956.7+2516 | -10.98 | 2.55 | 0.52 | 1.96 | -0.98 | -4.75 | 1.16 | 2.89
J0957.3$-$1348 | -11.14 | 2.47 | 0.57 | 2.06 | -1.18 | -4.9 | 1.13 | 3.28
J0957.6+5523 | -10.04 | 2.01 | 1.04 | 1.58 | -1.91 | -5.96 | 1.02 | 2.94
J0958.0+4728 | -11.12 | 2.59 | 0.67 | 2.39 | -0.88 | -5.17 | 1.11 | 3.12
J1006.7$-$2159 | -10.59 | 2.35 | 0.42 | 3.12 | -1.43 | -5.01 | 0.96 | 2.67
J1007.6$-$3332 | -10.9 | 2.44 | 0.75 | 2.49 | -1.58 | -5.14 | 1.04 | 2.23
J1010.8$-$0158 | -11.35 | 2.54 | 0.01 | 1.39 | -0.47 | -4.94 | 1.31 | 1.47
J1011.3$-$0427 | -11.77 | 2.56 | 0.27 | 1.44 | -0.94 | -4.47 | 1.1 | 2.59
J1012.7+2439 | -10.7 | 2.31 | 0.87 | 2.86 | -1.81 | -5.97 | 1.1 | 2.86
J1014.8+2257 | -11.29 | 2.79 | -0.18 | 0.98 | -0.64 | -4.66 | 0.95 | 2.68
J1016.0+0512 | -10.86 | 2.22 | -0.16 | 2.69 | -1.6 | -5.91 | 1.06 | 3.66
J1018.3$-$3124 | -10.87 | 2.54 | 0.6 | 2.32 | -1.41 | -5.31 | 1.18 | 3.13
J1018.4+3540 | -11.2 | 2.59 | 0.34 | 2.14 | -1.04 | -4.86 | 1.31 | 2.85
J1023.1+3949 | -10.8 | 2.37 | 0.71 | 3.26 | -1.19 | -5.04 | 1.22 | 3.24
J1028.4$-$0234 | -11.35 | 2.61 | 0.17 | 1.62 | -0.95 | -5.11 | 1.03 | 3.23
J1031.6+6019 | -11.05 | 2.61 | 0.1 | 2.08 | -1.04 | -5.11 | 1.19 | 2.72
J1033.1+4115 | -10.88 | 2.41 | 0.35 | 2.05 | -1.03 | -5.82 | 1.21 | 3.24
J1033.9+6050 | -10.38 | 2.22 | 0.93 | 2.92 | -1.32 | -6.01 | 1.01 | 2.73
J1036.2+2202 | -11.24 | 2.61 | -0.0 | 1.99 | -0.84 | -5.26 | 1.15 | 2.07
J1037.4$-$2933 | -11.17 | 2.41 | -0.01 | 1.73 | -0.57 | -4.25 | 1.11 | 2.88
J1037.7$-$2822 | -10.75 | 2.42 | 0.56 | 2.57 | -1.68 | -5.71 | 1.04 | 3.19
J1043.2+2408 | -11.03 | 2.32 | 0.14 | 1.67 | -0.74 | -4.74 | 0.96 | 1.68
J1044.6+8053 | -11.04 | 2.78 | 0.72 | 1.67 | -0.76 | -4.4 | 1.06 | 2.74
J1048.4+7143 | -10.05 | 2.29 | 1.05 | 3.88 | -1.67 | -6.39 | 1.13 | 3.01
J1051.6+2109 | -11.53 | 2.77 | 0.44 | 1.72 | -0.63 | -4.71 | 1.21 | 2.93
J1056.8+7012 | -10.93 | 2.68 | 0.57 | 2.37 | -1.02 | -5.31 | 1.21 | 3.53
J1058.5+8115 | -11.19 | 2.51 | 0.24 | 1.98 | -1.06 | -5.65 | 1.16 | 3.1
J1102.9+3014 | -11.57 | 2.96 | 0.06 | 0.95 | -0.35 | -4.65 | 1.09 | 2.64
J1106.0+2813 | -11.0 | 2.37 | 0.37 | 2.11 | -1.09 | -5.34 | 1.16 | 3.56
J1107.0$-$4449 | -10.91 | 2.7 | 0.73 | 2.09 | -0.88 | -5.21 | 1.19 | 3.48
J1107.7$-$3042 | -11.65 | 2.49 | -1.75 | 1.13 | -0.31 | -5.27 | 0.93 | 3.25
J1112.5+3448 | -10.99 | 2.52 | 0.6 | 2.29 | -1.26 | -5.59 | 1.2 | 3.39
J1118.2$-$4634 | -11.51 | 2.42 | 0.47 | 1.69 | -0.17 | -4.13 | 1.2 | 3.01
J1118.6$-$1235 | -11.27 | 2.7 | 0.19 | 1.26 | -0.84 | -5.17 | 1.12 | 3.07
J1119.0+1235 | -11.26 | 2.59 | 0.55 | 1.74 | -0.75 | -5.28 | 1.05 | 3.39
J1121.4$-$0553 | -10.7 | 2.42 | 0.8 | 2.55 | -1.41 | -5.58 | 1.16 | 3.44
J1124.0+2336 | -11.26 | 2.41 | -0.48 | 1.23 | -1.12 | -5.28 | 1.19 | 3.22
J1127.0$-$1857 | -10.18 | 2.2 | 0.91 | 3.59 | -0.75 | -5.93 | 0.98 | 2.58
J1127.4+5648 | -11.42 | 2.72 | 0.12 | 1.69 | -0.9 | -5.02 | 0.87 | 2.96
J1129.8$-$1447 | -11.05 | 2.69 | 0.34 | 2.61 | -0.47 | -4.55 | 1.34 | 2.92
J1131.0+3815 | -10.94 | 2.49 | 0.69 | 2.17 | -1.12 | -5.42 | 1.29 | 2.87
J1145.7+0453 | -11.69 | 3.01 | -0.51 | 1.25 | -0.59 | -4.85 | 1.08 | 2.71
J1145.7$-$6949 | -11.25 | 2.69 | 0.41 | 1.54 | 0.08 | -4.36 | 1.0 | 2.46
J1146.9+3958 | -10.32 | 2.38 | 0.78 | 3.19 | -1.51 | -5.9 | 1.1 | 2.84
J1147.4$-$6758 | -11.42 | 2.55 | 0.61 | 1.03 | -0.54 | -4.73 | 0.93 | 2.66
J1147.8$-$0724 | -11.06 | 2.42 | 0.51 | 2.23 | -1.06 | -5.18 | 1.09 | 2.86
J1148.5+2629 | -11.55 | 2.92 | 0.08 | 1.63 | -0.44 | -4.71 | 1.24 | 2.95
J1152.3$-$0839 | -10.94 | 2.41 | 0.37 | 2.23 | -1.3 | -5.3 | 1.18 | 3.4
J1152.8+3308 | -11.56 | 3.01 | -0.0 | 1.28 | -0.59 | -3.72 | 1.31 | 2.91
J1153.0+8056 | -11.37 | 2.87 | -0.65 | 1.95 | -0.74 | -4.87 | 1.28 | 2.88
J1153.4+4931 | -10.8 | 2.41 | 0.41 | 3.07 | -0.34 | -5.1 | 1.11 | 3.09
J1154.0+6018 | -11.3 | 2.7 | 0.55 | 1.94 | -1.0 | -5.39 | 1.23 | 2.76
J1159.5+2914 | -9.92 | 2.19 | 0.96 | 3.89 | -1.81 | -4.68 | 1.08 | 2.92
J1205.7$-$2635 | -11.04 | 2.53 | 0.03 | 1.6 | -0.82 | -5.6 | 1.15 | 2.37
J1213.6+1306 | -11.17 | 2.47 | 0.56 | 0.74 | -1.45 | -5.08 | 0.95 | 2.89
J1215.0+1656 | -11.06 | 2.41 | -0.21 | 2.34 | -0.99 | -5.78 | 1.18 | 2.0
J1222.5+0414 | -10.71 | 2.79 | 0.5 | 2.21 | -0.99 | -5.32 | 1.17 | 2.73
J1224.9+2122 | -9.71 | 2.34 | 0.86 | 4.31 | -1.66 | -6.13 | 1.06 | 2.77
J1228.7+4858 | -11.27 | 2.56 | 0.3 | 1.94 | -1.14 | -5.12 | 1.16 | 3.47
J1229.0+0202 | -9.94 | 2.7 | 0.96 | 3.85 | 0.08 | -4.83 | 0.97 | 2.28
J1238.5$-$1201 | -11.07 | 2.66 | 0.23 | 2.14 | -0.71 | -4.97 | 0.92 | 2.74
J1239.5+0443 | -10.22 | 2.37 | 1.05 | 3.33 | -2.0 | -6.85 | 1.15 | 3.33
J1246.7$-$2548 | -10.15 | 2.31 | 1.06 | 3.03 | -1.39 | -5.66 | 1.15 | 3.03
J1254.9+1138 | -11.29 | 2.79 | 0.18 | 1.45 | -0.56 | -4.21 | 1.2 | 2.73
J1256.1$-$0547 | -9.35 | 2.29 | 1.22 | 4.48 | -0.99 | -6.59 | 1.36 | 2.47
J1257.8+3228 | -10.95 | 2.32 | 0.62 | 2.56 | -1.22 | -5.55 | 1.05 | 2.73
J1300.4+1416 | -11.06 | 2.74 | 0.2 | 1.55 | -1.07 | -5.45 | 1.21 | 2.81
J1308.5+3547 | -11.26 | 2.37 | 0.69 | 2.1 | -1.04 | -5.67 | 1.05 | 3.1
J1310.5+3221 | -10.55 | 2.34 | 0.56 | 2.64 | -1.38 | -4.38 | 1.13 | 3.08
J1310.9+5514 | -11.45 | 2.51 | 0.02 | 1.25 | -0.96 | -5.19 | 0.88 | 2.59
J1311.0+3233 | -11.23 | 2.4 | 0.49 | 1.99 | -1.29 | -4.33 | 1.11 | 3.21
J1312.8$-$0425 | -10.81 | 2.4 | 0.72 | 2.76 | -1.34 | -5.51 | 1.12 | 2.77
J1316.1$-$3338 | -10.6 | 2.33 | 0.47 | 2.77 | -1.07 | -6.24 | 1.17 | 3.24
J1317.6+3428 | -11.2 | 2.53 | 0.34 | 2.08 | -0.93 | -5.09 | 1.12 | 3.07
J1326.9+2210 | -10.8 | 2.49 | 0.59 | 2.25 | -1.35 | -5.6 | 1.18 | 2.88
J1332.0$-$0509 | -10.46 | 2.51 | 0.91 | 3.34 | -1.74 | -5.78 | 1.28 | 3.45
J1332.2+4722 | -11.45 | 2.64 | 0.07 | 1.58 | -0.8 | -4.57 | 0.92 | 2.91
J1332.6$-$1256 | -10.46 | 2.42 | 0.85 | 2.83 | -2.25 | -5.8 | 1.22 | 3.27
J1334.5+5634 | -11.85 | 2.36 | -0.66 | 1.07 | -0.22 | -4.47 | 1.11 | 2.74
J1337.4+5502 | -11.71 | 2.76 | -1.05 | 1.46 | -0.68 | -4.47 | 1.2 | 2.62
J1337.6$-$1257 | -10.74 | 2.42 | 0.64 | 1.98 | -0.67 | -5.5 | 1.21 | 2.81
J1341.8$-$2053 | -11.2 | 2.73 | 0.2 | 2.03 | -0.78 | -5.04 | 1.42 | 3.31
J1343.6+5755 | -11.84 | 2.72 | -4.0 | 1.3 | -0.68 | -4.72 | 0.94 | 2.98
J1345.5+4453 | -10.05 | 2.27 | 1.06 | 3.63 | -2.31 | -6.7 | 1.1 | 3.02
J1345.8+0706 | -11.04 | 2.44 | 0.17 | 2.32 | -1.16 | -5.87 | 1.09 | 3.13
J1347.6$-$3751 | -11.29 | 2.34 | 0.51 | 1.72 | -0.68 | -5.16 | 1.09 | 3.06
J1349.5$-$1131 | -10.89 | 2.49 | 0.4 | 2.69 | -1.08 | -5.15 | 1.06 | 2.7
J1350.8+3033 | -11.13 | 2.42 | 0.36 | 2.34 | -0.57 | -5.05 | 1.06 | 2.32
J1354.3$-$0206 | -11.46 | 2.73 | 0.58 | 1.07 | -0.52 | -5.34 | 1.01 | 3.16
J1354.8$-$1041 | -11.06 | 2.42 | 0.61 | 2.24 | -0.35 | -5.14 | 0.99 | 3.11
J1357.1+1921 | -11.4 | 2.76 | -0.67 | 1.59 | -0.24 | -3.85 | 1.12 | 2.89
J1358.1+7642 | -11.3 | 2.37 | 0.27 | 1.9 | -1.11 | -5.14 | 1.13 | 3.23
J1359.1+5544 | -11.13 | 2.43 | 0.49 | 1.82 | -1.11 | -5.46 | 1.07 | 2.94
J1359.4+0202 | -11.54 | 2.39 | 0.37 | 1.65 | -0.45 | -4.35 | 1.35 | 2.94
J1359.7+4012 | -11.44 | 2.61 | 0.48 | 1.7 | -1.18 | -5.08 | 0.98 | 3.31
J1401.2$-$0915 | -11.57 | 2.09 | 0.22 | 1.14 | -0.68 | -5.19 | 0.78 | 2.83
J1402.6$-$3330 | -11.55 | 2.76 | 0.48 | 1.26 | -0.37 | -6.49 | 0.97 | 3.96
J1408.9$-$0751 | -10.73 | 2.35 | 0.47 | 2.4 | -1.21 | -5.47 | 1.22 | 2.84
J1419.5+3821 | -11.22 | 2.47 | -0.25 | 1.62 | -1.14 | -5.48 | 1.21 | 3.38
J1422.3+3223 | -11.06 | 2.4 | 0.03 | 2.79 | -0.87 | -5.45 | 1.03 | 3.16
J1423.5$-$7829 | -11.56 | 2.48 | 0.53 | 1.57 | -1.05 | -4.97 | 1.03 | 2.82
J1427.9$-$4206 | -9.43 | 2.2 | 1.24 | 4.13 | -2.32 | -6.49 | 1.12 | 2.96
J1428.9+5406 | -11.61 | 2.57 | 0.14 | 1.5 | -0.87 | -5.38 | 1.06 | 3.23
J1436.9+2321 | -11.3 | 2.49 | 0.06 | 1.24 | -0.69 | -5.25 | 1.24 | 3.32
J1438.9+3710 | -10.93 | 2.41 | 0.64 | 2.52 | -1.62 | -5.87 | 1.11 | 3.11
J1443.9+2501 | -10.34 | 2.09 | 0.96 | 3.47 | -1.31 | -6.19 | 1.02 | 2.89
J1446.7+1719 | -11.6 | 2.5 | -0.12 | 1.63 | -0.59 | -4.97 | 0.99 | 3.1
J1454.4$-$3744 | -11.17 | 2.55 | 0.38 | 1.74 | 0.05 | -4.35 | 1.08 | 2.3
J1457.4$-$3539 | -10.49 | 2.32 | 1.0 | 3.46 | -1.46 | -6.15 | 1.11 | 2.28
J1504.4+1029 | -9.7 | 2.25 | 1.25 | 4.13 | -2.76 | -6.57 | 1.13 | 2.94
J1506.1+3731 | -10.61 | 2.5 | 0.78 | 3.22 | -1.48 | -6.71 | 1.35 | 2.9
J1509.6$-$4334 | -11.34 | 2.68 | 0.58 | 1.05 | -0.98 | -5.18 | 1.07 | 2.54
J1510.8$-$0542 | -10.79 | 2.45 | 0.56 | 1.88 | -1.25 | -4.93 | 1.13 | 2.94
J1512.2+0202 | -10.79 | 2.15 | 0.81 | 1.48 | -0.97 | -5.38 | 0.97 | 2.68
J1512.8$-$0906 | -9.38 | 2.38 | 1.05 | 3.77 | -2.22 | -6.08 | 1.07 | 2.73
J1521.8+4338 | -11.42 | 2.94 | 0.03 | 1.47 | -0.97 | -5.0 | 1.1 | 3.33
J1522.1+3144 | -9.85 | 2.41 | 1.05 | 3.55 | -2.45 | -6.94 | 1.22 | 2.8
J1534.8+0131 | -10.91 | 2.42 | -0.02 | 2.41 | -0.8 | -5.33 | 1.26 | 3.01
J1549.5+0236 | -10.87 | 2.41 | 0.43 | 2.25 | -0.71 | -4.94 | 1.11 | 2.69
J1550.7+0528 | -11.12 | 2.36 | 0.64 | 1.47 | -0.56 | -5.21 | 1.18 | 3.05
J1553.6+1257 | -10.8 | 2.4 | 0.59 | 2.82 | -1.39 | -5.1 | 1.23 | 3.04
J1604.6+5714 | -10.7 | 2.42 | 0.73 | 2.09 | -1.41 | -5.25 | 1.1 | 2.97
J1606.5+2717 | -11.54 | 2.68 | -0.53 | 1.19 | -0.03 | -4.99 | 1.06 | 3.18
J1608.3+4012 | -11.96 | 2.34 | 0.37 | 1.21 | -0.29 | -5.2 | 1.13 | 3.06
J1608.7+1029 | -10.93 | 2.59 | 0.65 | 2.41 | -1.01 | -5.11 | 1.07 | 3.47
J1610.3$-$3958 | -10.85 | 2.58 | 0.18 | 1.49 | -1.42 | -5.4 | 1.12 | 3.47
J1613.6+3411 | -10.93 | 2.44 | 0.16 | 1.83 | -1.13 | -4.89 | 1.12 | 2.93
J1617.9$-$7718 | -10.62 | 2.61 | 0.64 | 2.56 | -1.3 | -5.82 | 1.02 | 3.15
J1623.6+5743 | -11.77 | 2.19 | -0.54 | 0.5 | -1.05 | -4.65 | 0.98 | 2.94
J1625.7+4134 | -11.2 | 2.54 | 0.49 | 1.78 | -1.51 | -6.44 | 1.14 | 3.27
J1625.7$-$2527 | -10.33 | 2.36 | 0.88 | 3.22 | -1.77 | -6.75 | 1.09 | 2.92
J1626.0$-$2950 | -10.41 | 2.56 | 0.73 | 2.64 | -1.48 | -6.63 | 1.2 | 2.9
J1626.8+4337 | -11.64 | 2.91 | -0.26 | 1.14 | -0.19 | -4.65 | 1.37 | 2.99
J1635.2+3808 | -9.79 | 2.41 | 1.32 | 3.82 | -2.64 | -6.23 | 1.17 | 2.98
J1637.7+4717 | -10.8 | 2.43 | 0.46 | 2.79 | -1.5 | -5.42 | 1.21 | 3.35
J1638.1+5721 | -11.21 | 2.68 | 0.27 | 1.92 | -0.44 | -4.43 | 1.01 | 2.8
J1640.4+3945 | -10.57 | 2.42 | 0.5 | 2.61 | -1.92 | -4.87 | 1.14 | 1.54
J1642.9+3948 | -10.52 | 2.4 | 0.25 | 2.31 | -0.74 | -4.96 | 1.18 | 3.14
J1657.0+6010 | -11.51 | 2.45 | -0.09 | 1.41 | -0.95 | -4.93 | 0.97 | 2.65
J1657.7+4808 | -10.67 | 2.41 | 0.77 | 2.55 | -1.91 | -5.93 | 1.19 | 2.69
J1700.0+6830 | -10.52 | 2.38 | 0.86 | 2.97 | -1.96 | -5.12 | 1.04 | 2.82
J1709.7+4318 | -10.59 | 2.33 | 0.74 | 3.2 | -2.07 | -5.95 | 1.14 | 2.73
J1715.8+2151 | -11.78 | 2.26 | -0.06 | 0.9 | -0.21 | -4.66 | 0.91 | 2.81
J1716.1+6836 | -11.16 | 2.38 | -0.32 | 1.99 | -0.35 | -4.95 | 1.02 | 2.8
J1722.6+6104 | -11.38 | 2.84 | 0.16 | 1.76 | -1.2 | -5.09 | 1.12 | 3.3
J1722.7+1014 | -10.85 | 2.21 | -0.01 | 2.07 | -1.1 | -5.68 | 1.04 | 3.47
J1724.1+3304 | -11.77 | 2.05 | -0.08 | 1.09 | -0.51 | -4.27 | 0.73 | 3.26
J1727.4+4530 | -10.62 | 2.49 | 0.7 | 2.77 | -1.61 | -5.82 | 1.08 | 1.7
J1728.4+0427 | -11.09 | 2.59 | 0.6 | 1.8 | -0.93 | -4.55 | 1.01 | 2.77
J1733.0$-$1305 | -10.22 | 2.36 | 0.95 | 2.99 | -1.22 | -6.02 | 1.05 | 2.57
J1734.3+3858 | -10.54 | 2.31 | 0.75 | 3.14 | -2.01 | -5.9 | 1.2 | 3.28
J1739.5+4955 | -10.94 | 2.36 | 0.45 | 2.38 | -1.3 | -5.5 | 1.11 | 2.61
J1740.0+4737 | -11.39 | 2.09 | 0.27 | 1.35 | -1.12 | -5.25 | 1.04 | 3.32
J1740.5+5211 | -10.67 | 2.47 | 0.18 | 2.9 | -1.23 | -5.57 | 1.14 | 2.98
J1744.2$-$0353 | -11.21 | 2.56 | -0.48 | 1.25 | -0.43 | -5.03 | 1.32 | 2.85
J1753.7+2847 | -11.69 | 2.4 | 0.11 | 1.34 | -0.52 | -4.58 | 1.22 | 2.44
J1801.5+4404 | -10.72 | 2.38 | 0.52 | 3.11 | -1.1 | -4.84 | 1.01 | 2.96
J1802.6$-$3940 | -10.32 | 2.37 | 0.92 | 3.5 | -1.61 | -5.71 | 1.38 | 3.52
J1808.1$-$5013 | -11.33 | 2.58 | -0.55 | 1.48 | -1.1 | -5.1 | 1.18 | 2.72
J1829.2$-$5813 | -10.47 | 2.55 | 0.86 | 3.37 | -1.34 | -5.91 | 1.37 | 3.39
J1830.1+0617 | -10.96 | 2.37 | 0.25 | 2.4 | -1.19 | -5.59 | 1.09 | 2.82
J1833.6$-$2103 | -9.72 | 2.53 | 1.04 | 3.39 | -2.1 | -4.72 | 0.98 | 3.15
J1842.3+6810 | -11.38 | 2.57 | -0.1 | 1.35 | -0.46 | -4.62 | 1.02 | 2.06
J1848.4+3217 | -10.67 | 2.41 | 0.75 | 2.73 | -0.99 | -5.53 | 1.14 | 1.05
J1849.2+6705 | -10.35 | 2.29 | 0.94 | 3.27 | -1.69 | -6.49 | 1.09 | 2.94
J1852.4+4856 | -10.81 | 2.29 | 0.42 | 2.62 | -1.9 | -5.52 | 1.05 | 3.45
J1902.9$-$6748 | -10.83 | 2.44 | 0.65 | 2.45 | -1.04 | -5.29 | 1.06 | 2.71
J1911.2$-$2006 | -10.34 | 2.45 | 1.01 | 2.79 | -1.07 | -5.66 | 0.7 | 5.26
J1923.5$-$2104 | -10.7 | 2.29 | 0.81 | 3.28 | -1.08 | -5.14 | 1.05 | 2.84
J1924.8$-$2914 | -10.64 | 2.39 | 0.18 | 2.45 | -0.63 | -5.48 | 1.14 | 3.34
J1933.2$-$4539 | -11.21 | 2.64 | 0.1 | 1.62 | -0.76 | -5.43 | 1.07 | 3.06
J1934.3+6541 | -11.2 | 2.86 | 0.43 | 2.61 | -1.2 | -5.47 | 1.34 | 3.07
J1937.2$-$3958 | -10.96 | 2.66 | 0.26 | 1.75 | -0.82 | -5.48 | 1.22 | 2.67
J1939.5$-$1525 | -11.48 | 2.42 | 0.25 | 1.76 | -0.53 | -5.12 | 1.12 | 2.74
J1951.8$-$0511 | -11.42 | 2.37 | 0.3 | 1.69 | -1.46 | -5.13 | 1.18 | 3.31
J1955.4+5132 | -11.09 | 2.55 | 0.35 | 1.95 | -0.89 | -5.15 | 1.26 | 2.94
J1958.0$-$3845 | -10.56 | 2.34 | 0.97 | 2.4 | -1.04 | -5.11 | 1.14 | 2.5
J1959.1$-$4247 | -11.08 | 2.46 | 0.59 | 2.58 | -1.12 | -5.54 | 1.01 | 3.51
J2000.9$-$1748 | -10.72 | 2.27 | -0.08 | 2.06 | -0.78 | -5.1 | 1.14 | 3.66
J2005.2$-$1822 | -11.44 | 2.48 | -0.25 | 1.31 | -0.59 | -5.0 | 1.12 | 2.92
J2005.8+6424 | -11.47 | 2.37 | 0.53 | 1.73 | -1.11 | -4.97 | 1.35 | 3.62
J2005.9$-$2309 | -10.91 | 2.5 | 0.38 | 2.43 | -1.57 | -5.65 | 1.17 | 3.43
J2011.6$-$1546 | -11.32 | 2.82 | 0.42 | 1.24 | -0.1 | -4.4 | 1.41 | 2.77
J2015.4+6556 | -11.74 | 2.54 | 0.46 | 1.24 | -0.53 | -4.98 | 1.15 | 3.26
J2015.5+3710 | -10.12 | 2.45 | 0.93 | 2.1 | -1.68 | -7.44 | 1.11 | 2.51
J2025.6$-$0735 | -10.05 | 2.29 | 1.04 | 3.53 | -1.8 | -5.99 | 1.17 | 3.1
J2026.0$-$2845 | -11.55 | 2.58 | 0.18 | 1.36 | -0.66 | -4.57 | 0.88 | 1.83
J2030.2$-$0620 | -11.41 | 2.4 | -0.12 | 1.87 | -1.77 | -5.71 | 1.12 | 3.47
J2034.6+1154 | -11.01 | 2.54 | 0.18 | 1.71 | -1.15 | -5.63 | 0.62 | 2.14
J2038.7+5117 | -11.03 | 2.57 | 0.64 | 1.9 | -1.16 | -5.81 | 1.19 | 3.07
J2040.2$-$2506 | -11.54 | 2.46 | 0.1 | 0.88 | -1.17 | -4.7 | 1.26 | 3.18
J2056.2$-$4714 | -10.22 | 2.45 | 0.94 | 3.12 | -1.67 | -6.26 | 1.29 | 3.55
J2115.4+2932 | -10.52 | 2.33 | 0.79 | 2.8 | -1.96 | -6.12 | 1.2 | 3.43
J2118.0+0019 | -11.57 | 2.57 | 0.27 | 1.48 | -0.79 | -4.98 | 1.18 | 2.85
J2121.0+1901 | -10.66 | 2.22 | 0.61 | 1.44 | -2.05 | -6.09 | 1.01 | 2.3
J2123.6+0535 | -11.25 | 2.39 | -0.55 | 1.41 | -0.86 | -4.59 | 1.1 | 2.99
J2126.3$-$4605 | -10.9 | 2.55 | 0.14 | 2.8 | -0.97 | -5.14 | 1.16 | 2.66
J2135.3$-$5006 | -10.93 | 2.43 | 0.29 | 1.78 | -1.5 | -4.72 | 1.16 | 3.63
J2136.2+0032 | -11.29 | 2.88 | 0.43 | 2.05 | -0.38 | -4.38 | 1.0 | 3.24
J2141.8$-$3727 | -11.13 | 2.62 | -0.08 | 1.69 | -1.01 | -4.93 | 1.06 | 2.83
J2142.7$-$0437 | -11.62 | 2.3 | 0.01 | 1.02 | 0.15 | -4.42 | 0.99 | 2.62
J2143.5+1743 | -10.17 | 2.49 | 0.5 | 2.43 | -1.67 | -4.97 | 1.11 | 2.8
J2144.3$-$7802 | -11.47 | 3.06 | 0.22 | 1.42 | -0.15 | -5.15 | 1.16 | 2.7
J2145.0$-$3356 | -10.87 | 2.3 | 0.62 | 2.47 | -1.56 | -5.6 | 1.08 | 3.06
J2146.4$-$1528 | -11.32 | 2.8 | 0.18 | 1.57 | -0.65 | -4.43 | 1.01 | 2.65
J2147.1+0931 | -10.6 | 2.54 | 0.62 | 2.76 | -1.23 | -5.66 | 1.18 | 2.02
J2147.3$-$7536 | -10.25 | 2.44 | 0.8 | 3.44 | -1.61 | -5.51 | 1.23 | 3.49
J2148.6+0652 | -11.27 | 2.8 | 0.5 | 1.59 | -0.23 | -4.16 | 1.32 | 2.76
J2150.7$-$2810 | -11.89 | 2.16 | 0.04 | 1.35 | -0.18 | -4.27 | 1.08 | 2.64
J2151.8$-$3027 | -10.52 | 2.85 | 0.85 | 2.98 | -0.46 | -5.52 | 0.97 | 3.37
J2156.3$-$0036 | -11.25 | 2.25 | -0.07 | 1.81 | -1.02 | -5.9 | 1.1 | 3.01
J2157.5+3127 | -10.55 | 2.31 | 0.93 | 3.2 | -1.7 | -6.15 | 1.1 | 2.99
J2158.1$-$1501 | -10.98 | 2.18 | 0.29 | 1.5 | -0.77 | -4.86 | 1.09 | 2.78
J2201.8+5048 | -10.29 | 2.66 | 0.89 | 3.49 | -1.73 | -6.09 | 1.35 | 3.24
J2203.4+1725 | -10.52 | 2.32 | 0.63 | 2.97 | -1.47 | -4.94 | 1.08 | 2.9
J2207.5$-$5346 | -11.06 | 2.44 | -0.02 | 1.92 | -0.88 | -4.98 | 1.15 | 2.95
J2212.0+2356 | -10.95 | 2.21 | 0.46 | 0.87 | -1.19 | -5.58 | 1.08 | 2.74
J2212.8+0647 | -11.21 | 2.49 | 0.36 | 1.28 | -1.1 | -5.12 | 1.1 | 2.77
J2219.2$-$0342 | -11.2 | 2.68 | 0.27 | 1.95 | -0.58 | -4.19 | 0.83 | 2.87
J2225.6+2120 | -11.32 | 2.81 | 0.46 | 1.4 | -0.15 | -4.8 | 1.21 | 3.38
J2225.7$-$0457 | -10.86 | 2.43 | 0.43 | 2.35 | -0.85 | -5.34 | 1.2 | 3.48
J2229.7$-$0832 | -10.38 | 2.59 | 0.82 | 2.8 | -1.13 | -5.43 | 1.19 | 2.92
J2232.6+1143 | -9.31 | 2.29 | 1.43 | 4.88 | -2.25 | -6.46 | 1.2 | 3.12
J2235.3$-$4836 | -10.95 | 2.51 | -0.74 | 2.02 | -0.58 | -4.77 | 1.08 | 2.86
J2236.3+2828 | -10.33 | 2.27 | 0.89 | 2.74 | -1.54 | -6.11 | 1.05 | 2.85
J2237.0$-$3921 | -11.32 | 2.38 | 0.21 | 2.26 | -0.42 | -4.66 | 1.0 | 2.14
J2239.2$-$5657 | -11.92 | 2.27 | 0.24 | 0.82 | -0.44 | -5.0 | 1.16 | 3.35
J2253.9+1609 | -9.0 | 2.4 | 1.61 | 4.75 | -1.76 | -6.28 | 1.12 | 2.35
J2258.1$-$2759 | -10.46 | 2.41 | 0.99 | 3.12 | -1.2 | -5.09 | 1.12 | 2.98
J2311.0+3425 | -10.35 | 2.35 | 0.9 | 3.3 | -1.84 | -6.29 | 1.08 | 2.66
J2321.9+2734 | -11.11 | 2.15 | 0.43 | 1.08 | -0.86 | -5.33 | 0.97 | 2.55
J2321.9+3204 | -10.52 | 2.26 | 0.89 | 2.97 | -1.94 | -5.52 | 1.06 | 2.69
J2323.5$-$0317 | -10.38 | 2.26 | 0.87 | 2.91 | -1.57 | -5.84 | 1.16 | 3.28
J2327.5+0939 | -10.75 | 2.69 | 0.61 | 2.57 | -1.05 | -5.89 | 1.28 | 3.3
J2329.0+0832 | -11.44 | 2.47 | -0.09 | 1.24 | -1.44 | -5.6 | 0.66 | 2.74
J2329.3$-$4733 | -11.41 | 2.51 | 0.08 | 1.64 | 0.01 | -4.15 | 1.25 | 2.93
J2329.3$-$4955 | -9.92 | 2.28 | 1.17 | 4.12 | -1.8 | -6.52 | 1.18 | 2.91
J2330.5+1102 | -11.28 | 2.79 | 0.45 | 1.58 | -0.86 | -4.8 | 1.33 | 3.14
J2331.0$-$2147 | -10.94 | 2.44 | 0.6 | 2.29 | -1.26 | -5.59 | 1.14 | 2.53
J2331.3$-$1558 | -11.6 | 2.54 | -0.05 | 1.45 | -0.8 | -5.26 | 1.08 | 3.24
J2334.2+0736 | -11.3 | 2.47 | -0.08 | 1.9 | -0.33 | -3.74 | 1.12 | 2.83
J2338.0$-$0230 | -10.94 | 2.49 | 0.19 | 2.11 | -1.11 | -5.61 | 1.15 | 3.08
J2345.2$-$1555 | -10.05 | 2.15 | 1.06 | 3.44 | -1.76 | -6.28 | 0.82 | 2.16
J2348.0$-$1630 | -10.51 | 2.34 | 0.58 | 2.8 | -1.04 | -5.7 | 1.08 | 2.88
J2354.1$-$0958 | -11.78 | 2.44 | 0.04 | 1.13 | -0.84 | -4.91 | 0.81 | 2.94
J2354.6+4554 | -11.57 | 2.31 | 0.35 | 0.41 | -0.67 | -5.51 | 1.19 | 2.89
J2354.9+8151 | -11.36 | 2.54 | 0.01 | 1.12 | -1.12 | -5.6 | 1.05 | 3.02
J2357.8$-$5311 | -11.16 | 2.64 | -0.03 | 2.35 | -0.31 | -4.8 | 1.05 | 1.74
J2359.0+3922 | -11.46 | 2.35 | -0.47 | 1.59 | -0.6 | -5.86 | 1.13 | 3.15

Note. — The table parameters are as follows: The logarithm of gamma-ray flux
(log ${F_{\gamma}}$ (erg/s/cm2)), Gamma-ray photon index ($\Gamma_{\gamma}$),
the significance of the curvature in the gamma-ray spectrum (Curvature), the
year-over-year gamma-ray variability index (Variability) are derived from the
4FGL-DR3 catalog. The last four columns correspond to the logarithm of X-ray
to gamma-ray flux ratio ($\log{F_{X}/F_{\gamma}}$), the logarithm of V-band to
gamma-ray flux ratio ($\log{F_{V}/F_{\gamma}}$) , WISE color index 1(w1-w2)
and WISE color index 2 (w2-w3).

Table 2: The Source Sample: the 112 blazar candidates obtained from Kerby et
al. (2021)

Fermi | Swift-XRT | Swift-UVOT | log Fγ | $\Gamma_{\gamma}$ | Variability | Curvature | FX/Fγ | FV/F$\gamma$ | w1-w2 | w2-w3
---|---|---|---|---|---|---|---|---|---|---
4FGL | SwXF4 | SwUVF4 |  |  | log | log | log | log |  |
J0004.4$-$4001 | J000434.1-400036 | J000434.2-400035 | -11.57 | 2.15 | -0.14 | 1.54 | -0.84 | -4.04 | 0.48 | 2.38
J0025.4$-$4838 | J002536.8-483808 | J002536.9-483810 | -11.69 | 2.14 | 0.26 | 1.16 | -0.62 | -4.5 | 0.6 | 1.69
J0026.1$-$0732 | J002611.9-073115 | J002611.6-073115 | -11.77 | 1.94 | 0.03 | 0.95 | 0.42 | -4.44 | 0.55 | 2.22
J0031.5$-$5648 | J003135.1-564640 | J003135.1-564640 | -11.81 | 1.99 | 0.13 | 1.16 | -0.59 | -4.68 | 0.32 | 2.52
J0037.2$-$2653 | J003729.6-265043 | J003729.5-265045 | -12.0 | 2.34 | 0.21 | 0.81 | -0.33 | -4.44 | 0.99 | 3.19
J0057.9+6326 | J005758.1+632642 | J005758.1+632642 | -11.5 | 1.71 | 0.3 | 1.16 | -0.05 | -4.58 | 0.31 | 2.63
J0058.3$-$4603 | J005806.4-460417 | J005806.3-460419 | -12.03 | 2.05 | -0.22 | 1.21 | 0.51 | -4.72 | 0.11 | 2.52
J0118.3$-$6008 | J011824.0-600753 | J011824.0-600753 | -11.73 | 2.18 | 0.3 | 1.49 | -1.01 | -4.45 | 0.68 | 1.94
J0120.2$-$7944 | J011914.7-794510 | J011914.7-794510 | -11.66 | 2.62 | -0.18 | 1.15 | -0.66 | -4.83 | 0.9 | 1.72
J0125.9$-$6303 | J012548.3-630244 | J012548.1-630245 | -11.84 | 2.24 | -0.3 | 0.95 | -0.24 | -4.58 | 0.7 | 1.94
J0156.3$-$2420 | J015624.4-242004 | J015624.6-242003 | -11.56 | 1.94 | 0.19 | 1.6 | -0.42 | -4.15 | 0.82 | 2.19
J0159.0+3313 | J015905.0+331255 | J015905.0+331255 | -11.73 | 1.98 | 0.12 | 1.4 | -0.5 | -4.49 | 0.3 | 0.98
J0209.8+2626 | J020946.5+262528 | J020946.5+262528 | -11.69 | 2.34 | -0.22 | 0.95 | 0.09 | -5.15 | 0.2 | 2.36
J0231.0+3505 | J023112.4+350446 | J023112.2+350445 | -12.01 | 1.71 | 0.4 | 0.95 | 0.42 | -4.59 | 0.23 | 2.08
J0240.2$-$0248 | J024004.6-024505 | J024004.6-024505 | -11.64 | 2.54 | -1.18 | 1.25 | -0.54 | -4.05 | 0.94 | 2.5
J0259.0+0552 | J025857.4+055243 | J025857.6+055244 | -11.21 | 2.04 | 0.55 | 1.37 | -1.04 | -4.72 | 0.81 | 1.92
J0301.6$-$5617 | J030115.2-561648 | J030115.1-561644 | -11.75 | 1.9 | 0.37 | 1.28 | -0.82 | -4.49 | 0.9 | 2.42
J0302.5+3354 | J030226.7+335448 | J030226.7+335448 | -11.78 | 1.89 | -0.27 | 1.21 | -0.32 | -4.8 | 0.4 | 2.03
J0327.6+2620 | J032737.2+262008 | J032737.2+262008 | -11.84 | 1.94 | 0.03 | 0.92 | -0.18 | -4.64 | 0.29 | 2.22
J0406.2+0639 | J040607.7+063919 | J040607.7+063919 | -11.56 | 2.43 | -0.31 | 1.12 | -0.92 | -5.2 | 0.27 | 1.91
J0409.2+2542 | J040921.6+254440 | J040921.6+254440 | -11.62 | 2.04 | -0.18 | 1.0 | -0.57 | -4.54 | 0.65 | 2.02
J0427.8$-$6704 | J042749.5-670435 | J042749.6-670435 | -11.07 | 2.39 | 0.0 | 1.08 | -0.75 | -4.63 | 0.15 | 2.18