127158 732023

Candidates for Transiting Planets in OGLE-IV Galactic Bulge Fields M. J. M r ó
z1, P. P i e t r u k o w i c z1, R. P o l e s k i1, A. U d a l s k i1,
M. K. S z y m a ń s k i1, M. G r o m a d z k i1, K. U l a c z y k2, S. K o z ł
o w s k i1,
J. S k o w r o n1, D. M. S k o w r o n1, I. S o s z y ń s k i1, P. M r ó z1,
M. R a t a j c z a k1, K. A. R y b i c k i1,3, P. I w a n e k1, M. W r o n a1
1 Astronomical Observatory, University of Warsaw, Al. Ujazdowskie 4, 00-478
Warszawa, Poland
2 Department of Physics, University of Warwick, Coventry CV4 7AL, UK
3 Department of Particle Physics and Astrophysics, Weizmann Institute of
Science, Rehovot 76100, Israel October 9, 2023 We present results of a search
for transiting exoplanets in 10-yr long photometry with thousands of epochs
taken in the direction of the Galactic bulge. This photometry was collected in
the fourth phase of the Optical Gravitational Lensing Experiment (OGLE-IV).
Our search covered $\approx 222000$ stars brighter than
$I=15.5~{}\mathrm{mag}$. Selected transits were verified using a probabilistic
method. The search resulted in 99 high-probability candidates for transiting
exoplanets. The estimated distances to these targets are between
$0.4~{}\mathrm{kpc}$ and $5.5~{}\mathrm{kpc}$, which is a significantly wider
range than for previous transit searches. The planets found are Jupiter-size,
with the exception of one (named OGLE-TR-1003b) located in the hot Neptune
desert. If the candidate is confirmed, it can be important for studies of
highly irradiated intermediate-size planets. The existing long-term, high-
cadence photometry of our candidates increases the chances of detecting
transit timing variations at long timescales. Selected candidates will be
observed by the future NASA flagship mission, the Nancy Grace Roman Space
Telescope, in its search for Galactic bulge microlensing events, which will
further enhance the photometric coverage of these stars. planetary systems –
Planets and satellites: detection – Planets and satellites: fundamental
parameters – Techniques: photometric

##  1 Introduction

Exoplanetary research is one of the most dynamically developing branches of
astronomy. At the end of the twentieth century, advances in observing
techniques enabled the detection of the first extrasolar planets. Currently,
the multitude of exoplanetary discoveries is unprecedented, with the number of
confirmed exoplanets exceeding 5500111exoplanet.eu. This large number of
objects has allowed us to gain a broader understanding of the processes that
govern planetary systems, their evolution, and their characteristics. Many
studies have shown that planetary systems are much more diverse than our own
Solar System (see Zhu and Dong 2021 for a review).

Among the many methods for detecting exoplanets, the transit method plays a
crucial role. It is based on observations of regular dimming of a star’s
brightness due to the presence of a planet blocking part of its light. The
method was first used in 1999 to detect a previously known planet around the
star HD 209458 (Henry et al.2000, Charbonneau et al.2000). The Optical
Gravitational Lensing Experiment (OGLE) was the first survey to successfully
apply the transit technique in discovering exoplanets. In observations of
millions of stars of the Galactic disk, the project has found 219 planetary
transit candidates (Udalski et al.2002abc, 2008, Pont et al.2008), of which
seven were confirmed as planets (Konacki et al.2003ab, Pont et al.2004, 2008,
Bouchy et al.2004, Udalski et al.2008). By announcing the first exoplanet
discovered using the transit technique and confirmed through radial velocity
measurements – OGLE-TR-56b, OGLE paved the way for extremely fruitful ground-
based surveys for transiting exoplanets, such as WASP (Pollacco et al.2006),
HATNet (Bakos et al.2004), NGTS (West et al.2016) and space missions, like
Kepler (Borucki et al.2010) and TESS (Ricker et al.2015). However, the
majority of exoplanetary surveys are limited to bright nearby stars. Only the
Kepler mission was capable of discovering transiting planets around distant
stars, up to 1 kpc away. This ability led to significant differences when
compared to results from surveys with a smaller distance range, such as those
using the radial velocity method (which primarily detects planets at distances
up to 100 pc). In particular, there is a difference in the occurrence rate of
hot Jupiters orbiting nearby stars (Cumming et al.2008, Mayor et al.2011) and
distant stars (Howard et al.2012, Guo et al.2017). Discovering transiting
planets around faint stars in microlensing survey data offers a unique
opportunity to investigate short orbital period planets across a wide range of
galactocentric distances.

Over its more than three decades of operation, the OGLE survey has had a
profound impact on many fields of modern astrophysics. In this study, we
present a large sample of high-probability transiting planet candidates
selected from the OGLE survey database. This database has not been searched
for planetary transits since the early 2000s. The analyzed data were collected
between 2010 and 2019 and consist of between 11 and 17 thousand measurements
per object. Such long, regular, high-quality, and homogeneous observations
have not been matched by any other survey capable of detecting transiting
exoplanets.

In Section 2, we provide a brief description of the OGLE survey and the
analyzed photometric observations. Section 3 introduces the steps taken to
find, verify, and characterize planetary candidates. In Section 4, we present
the final catalog of candidates. The discussion in Section 6 includes our
thoughts on the future of our targets. Finally, in Section 7, we summarize our
work.

##  2 The OGLE survey

The primary objective of the OGLE survey is a continuous monitoring of
billions of stars within the Galactic bulge, disk, and the Magellanic Clouds
to study their photometric variability. For this purpose, the survey employs a
32-detector mosaic camera attached to the 1.3-m Warsaw telescope at the Las
Campanas Observatory, Chile, which is operated by the Carnegie Institution for
Science. The installation of this camera in March 2010 marked the commencement
of the OGLE’s fourth phase (Udalski et al.2015). The camera has a field of
view of 1.4 deg2 and a resolution of 0.26 arcsec/px. The exceptional observing
conditions at Las Campanas allow OGLE to collect photometric data from some of
the most densely populated regions of the sky with very high precision. For
our analysis, we used data from ten observational seasons, between 2010–2019.
Due to the COVID-19 pandemic restrictions, OGLE temporarily stopped its
regular operations in March 2020, resuming observations in August 2022. The
majority of observations were taken through the Cousins $I$ filter, with
additional data collected using the Johnson $V$ filter. For our studies, we
chose four of the most frequently observed fields in the direction of the
Galactic bulge, with up to 16 800 data points per object and a cadence as
short as 19 min (see Table 1). The exposure times of those observations were
100 s in $I$ and 150 s in $V$. The photometric data was reduced using the
Difference Image Analysis (DIA, Woźniak 2000), a technique developed
specifically for dense stellar fields (Alard and Lupton 1998).

T a b l e 1

OGLE-IV fields searched for transiting planets

OGLE field | $N_{\rm{obs}}$ | $N_{*}(I\leq 15.5,~{}(V-I)\leq 2)$
---|---|---
BLG501 | 15 700 | 29 600
BLG504 | 11 100 | 23 200
BLG505 | 16 800 | 52 600
BLG512 | 14 500 | 116 700
SUM |  | 222 100

We focused our search on bright main-sequence stars in the Galactic disk by
employing the following criteria for brightness and color selection:
$I\leqslant$15.5 mag and $(V-I)\leqslant 2~{}$mag. This is illustrated in Fig.
1. In total, approximately 222 100 objects within the analyzed fields met
these criteria (Table 1). After reviewing the light curve of the known
planetary transit OGLE-TR-10 (Udalski et al.2002a) detrended with various
methods, we opted for a straightforward correction method using the median
value from each season. This corrects, in a sufficient way, the decrease in
brightness, caused by the proper motions shifts of targets with respect to the
reference images. To minimize the effects of cosmic rays, weather conditions,
bad CCD columns, satellite and asteroid flybys, and other factors, we
implemented a sigma clipping technique, excluding data points exceeding
$2\sigma$ above the normalized flux.

Color-magnitude diagram for the OGLE sub-field BLG501.15, with the marked
selection cuts.

##  3 Transit Detection

###  3.1 Initial Transits Search

A commonly used technique for transit searches involves the least squares
fitting of transit templates to the light curves, folded according to a grid
of trial periods. In our work, we applied the Transit Least Squares (TLS)
algorithm (Hippke and Heller 2019). This modern method implements a more
realistic transit shape compared to the rectangular template used in the
traditional Box Least Squares (BLS) algorithm (Kovács et al.2002). By
including limb darkening and the planetary ingress and egress effects in the
shape of the light curve, TLS is more sensitive to low signal-to-noise ratio
(SNR) transits. The TLS template is based on the transit model of Mandel and
Agol (2002), with parameters optimized based on a set of previously known
exoplanet transit detections. The use of realistic templates increases the
detection efficiency by 5-10 percent at the expense of computational speed
(Hippke and Heller 2019).

Ground-based observations, such as the ones collected by the OGLE project,
present additional challenges in the detection of periodic signals compared to
continuous data collected by space telescopes. Various natural phenomena, like
the day-night cycle, moonlight contamination, etc., can produce periodic
changes in the structure of observational data (Baluev 2012). To minimize
false positive signals caused by these phenomena, we added an option to TLS to
exclude problematic sections of tested periods from the period grid. We
conducted a trial search to determine which periods should be excluded and
which TLS parameters would be most suitable for our purposes. We initiated the
search by excluding the most prominent multiples of the sidereal day.
Subsequently, throughout this trial run, we extended the excluded period
ranges to minimize recurring false positive signals. This increased the
sensitivity to transit signals and reduced the TLS calculation time (final
excluded period ranges are listed in Table 2). After the preliminary run, we
fixed the following parameters: oversampling factor = 4, transit duration grid
step = 1.1, minimum period = 0.6 d, and maximum period = 500 d. For the
definition of the parameters and other details of the TLS, we refer to Hippke
and Heller (2019).

T a b l e 2

Period ranges excluded from the TLS search grid.

Excluded period range | Comment
---|---
0.6640 – | 0.6665 | 2/3 sidereal day
0.7474 – | 0.7475 | 3/4 sidereal day
0.990 – | 1.010 | 1 sidereal day
1.329 – | 1.331 | 4/3 sidereal day
1.493 – | 1.499 | 3/2 sidereal day
1.661 – | 1.664 | 5/3 sidereal day
1.988 – | 2.001 | 2 sidereal day
2.492 – | 2.497 | 5/2 sidereal day
2.981 – | 3.002 | 3 sidereal day
3.988 – | 3.9905 | 4 sidereal day
3.4895 – | 3.490 | 7/2 sidereal day
4.985 – | 4.9875 | 5 sidereal day
5.9825 – | 5.984 | 6 sidereal day
6.980 – | 6.982 | 7 sidereal day
54.678 – | 55.180 | unknown
58.603 – | 58.604 | unknown
64.929 – | 65.931 | unknown
68.410 – | 68.412 | unknown
100.058 – | 100.062 | unknown
115.205 – | 115.210 | unknown
146.130 – | 146.140 | unknown

Due to residual contamination, we decided to visually inspect the results of
the TLS calculations for almost all the objects. We automatically excluded
only signals caused by breaks in the folded data or no signal detections. True
signals were classified into the following groups: transits, sinusoidal
variations, and other variability. In the next step, we double-checked all the
signals classified as transits to exclude obvious eclipsing binary systems
(based on transit depth and the presence of a secondary eclipse). After this
process, we were left with 4601 potential planetary-like transits.

###  3.2 Probabilistic Evaluation

The major disadvantage of the transit method is the need for additional
confirmation of the planetary nature of transiting objects. Firstly, from the
shape of the transit, we can only deduce the radius of the transiting object.
Therefore, we cannot distinguish between hot Jupiters, brown dwarfs, and low-
mass M-type stars, as they can all have similar sizes. Secondly, additional
light blended in the photometric aperture can shallow the transit depth and
lead to underestimated radius measurements. The traditional way of resolving
this degeneracy is to measure the mass through radial velocity (RV)
observations. Nevertheless, there are indirect methods of validation in the
absence of RV measurements. One of them is the Validation of Exoplanet Signals
using a Probabilistic Algorithm (VESPA, Morton 2012). VESPA is a widely used
and well-established publicly available software package that performs
statistical validation. We used it to evaluate 4601 candidates against
astrophysical false positive scenarios. By applying a simple trapezoidal
transit model, known parameters of the host star, and assumptions about the
populations and distribution of field stars, the algorithm calculates the
probability of the analyzed object being a planet given the observed signal
$\rm{Pr(planet|signal)}$. VESPA considers the following false positive
scenarios:

  * •

blended eclipsing binary (BEB), in the case of non-associated eclipsing binary
systems blended within the photometric aperture of the target star,

  * •

hierarchical eclipsing binary (HEB), in case of the target is a hierarchical
triple system in which two components are eclipsing,

  * •

eclipsing binary (EB).

For detailed descriptions, we refer to Morton (2012, 2016).

We prepared normalized flux light curves in the same way as for the TLS. As
initial values required by VESPA (the orbital period $P$, planet-to-star
radius ratio $R_{\rm{p}}/R_{*}$), we used values fitted by the TLS. We derived
the maximum allowed depth of a potential secondary eclipse for each object by
searching the phase-folded light curve for the deepest signal at any phase
outside of the primary transit (Morton 2016). We set the maximum angular
distance (parameter maxrad in VESPA) from the target star where a potential
blending star might be, as $2\zdot\arcs 6$, which is 10 times the pixel size
of the OGLE-IV camera or roughly twice the average seeing of the images.

The obtained values of probability for the planetary origin of transits are
shown in the histogram in Fig. 2. For further analysis, we decided to use only
the cases for which the probability is greater than $80\%.$ Scenarios with the
highest probability for each analyzed transit are shown in Fig. 3. For 1110
transits, VESPA calculation failed, in most cases due to not converging
transit model.

Distribution of $\rm{{Pr}(planet|signal)}$ values for 3491 potential
planetary-like transit. The dashed line marks the minimum value of the
probability for which transit was used in further analyzes.

Most probable scenario for 4601 potential planetary-like transits. Each slide
represents a different scenario simulated with VESPA: BEB – blended eclipsing
binary, HEB – hierarchical triple system with eclipse, EB – eclipsing binary.
PLANETARY – planetary transits, failed – VESPA calculations failed.

###  3.3 Modeling the Candidates

We chose EXOFASTv2 (Eastman et al.2019) for modeling our candidates, which is
Markov Chain Monte Carlo (MCMC) transit modeling code. To properly model the
transit, it is essential to model both the host star and the planet. EXOFASTv2
offers the unique capability of simultaneously constraining host star
parameters using both the transit shape and stellar models, employing
isochrones from stellar evolutionary tracks and spectral energy distribution
(SED). These features of the code are particularly helpful in constraining
system parameters, especially when spectroscopic observations are unavailable.

For modeling, we used OGLE observations in both the $I$\- and $V$-bands, which
were detrended and normalized as in previous steps. When an object was
observed in multiple OGLE fields, we added those observations as separate data
sets. In a few cases, this notably enlarged the number of observations, as for
example for OGLE-TR-1051 (see Fig. 10). We converted the original OGLE time
stamps from Heliocentric Julian Date (HJD) to Barycentric Julian Date
($\rm{BJD_{TDB}}$) using IDL codes written by Eastman (2010). As starting
values for the period $P_{\rm{orb}}$ and the time of conjunction $T_{\rm{C}}$,
we implemented values from the TLS output. Whenever available, we incorporated
parallax $\varpi$ and host effective temperature $T_{\rm{eff}}$ values from
Gaia DR3 (Gaia Collaboration et al.2023a). We applied upper limits for
interstellar extinction toward the Galactic bulge, as calculated by Nataf et
al.(2013). In only a few cases, we utilized Galactic extinction maps by
Gonzalez et al.(2012). SED modeling requires measurements of the star’s
bolometric flux in various bands. We reviewed publicly available photometric
catalogs and their reference images for the Galactic bulge region. As a test
case, we used the well-characterized planetary system OGLE-TR-10 (Udalski et
al.2002a, Konacki et al.2003b, Melo et al.2006), which is located in one of
the analyzed fields, and its transit was detected in the TLS search. For this
object, we prepared a set of modeling inputs in the same manner as for our
candidates. Following SED modeling of OGLE-TR-10, we compared the fitted
parameters to those reported in the literature. Ultimately, we decided to use
measurements from the Dark Energy Camera Plane Survey 2 (DECaPS2, Saydjari et
al.2023), the Pan-STARRS1 Surveys DR2 (Chambers et al.2016), and synthetic
photometry from the Gaia DR3 low-resolution spectra (Gaia Collaboration et
al.2023b), as this set resulted in the best agreement between calculated
parameters and those reported from high-resolution spectroscopy. We assumed
circular orbits for all of our objects since they are on short-period orbits.
For stellar evolution models, we selected the default in EXOFASTv2 \- the MESA
Isochrones and Stellar Tracks (MIST) model (Choi et al.2016). For each object,
we performed a preliminary short modeling with parallel tempering.
Subsequently, using the preliminary results, we recreated priors and conducted
final modeling without parallel tempering and with 50 000 maximum steps.

###  3.4 Final Selection

To further reduce the likelihood of false positive signals in our catalog, we
conducted additional tests on all objects for which we successfully created
models. Our aim was to ensure that the transit signal in the light curve was
not an artifact of a nearby eclipsing binary system. To achieve this, we
cross-matched our candidates with the OGLE collection of eclipsing and
ellipsoidal binary systems (Soszyński et al.2016). Within $1\arcm$ radius
around each candidate, we examined if there was a binary system with an
orbital period or its alias consistent with that of our candidate. If such a
match was found, we excluded the object from further analysis. This was the
case for 138 out of 1243 transits at this stage of the vetting process. In the
same manner as for the binary systems catalog, we cross-matched our final
candidates with all the results from the TLS search. This additional step was
designed to help eliminate false positive signals of instrumental origin and
resulted in the exclusion of additional 110 detections. Furthermore, we
analyzed the histogram of periods detected by the TLS in each observed field
and removed candidates with orbital periods close to the peaks of this
histogram. An example section of the histogram from filed BLG501 is shown in
Fig. 4. Those peaks vary between observation fields and can be associated with
multiple astrophysical or instrumental signals, such as remaining aliases of
the sidereal day, diffraction spikes from nearby bright stars, lunar cycle, or
bad columns in the CCD detector. We checked previously reported planetary-like
transits from the third phase of the OGLE project (Udalski et al.2002abc,
2008, Pont et al.2008), and we did not find any matches with our detections
beside the mentioned OGLE-TR-10. OGLE-TR-10b is the only confirmed planet,
which was regularly observed during OGLE-IV. The absence of matches with
previously unconfirmed candidates can be attributed to the more rigorous
selection process.

To conclude the selection process, we chose the 99 most promising candidates
for transiting planets, which will be presented in detail in Section 4. This
final step considered various factors, including the number of observations,
how well the created model fits the observational data, and whether the
transit exhibits the V-shape, which could indicate a grazing binary system
eclipse.

Example section of the orbital periods distribution resulting from the TLS
search in the field BLG501. Each bin represents 2000 values from the TLS
period grid. The red fields indicate the excluded periods from Table 2.

##  4 The Planetary Candidates

Here, we present the selected planetary candidates. Table 3 displays their
observational parameters, including celestial coordinates, orbital period of
the companion ($P_{\rm{orb}}$), time of conjunction ($T_{\rm{c}}$), total
transit duration ($T_{\rm{14}}$), fractional transit depth ($\delta$),
brightness in $I$\- and $V$-band, signal-to-noise ratio (SNR), and the
probability that the transit is of planetary origin given the signal
($\rm{{Pr}(planet|signal)}$). Table 4 presents the selected physical
parameters of the systems, including parameters of the host such as mass
($M_{*}$), radius ($R_{*}$), surface gravity ($\rm{log}g$), effective
temperature ($T_{\rm{eff}}$), metalicity ($\rm{[Fe/H]}$), and distance ($d$);
parameters of the companion such as orbital radius ($a$), inclination ($i$),
and equilibrium temperature ($T_{\rm{eq}}$). For the detailed definitions of
the parameters, we refer to Eastman et al.(2019). Figs. 7-13 show
observational data of transits with fitted models. The identifiers of our
planetary candidates follow the format OGLE-TR-NNNN, where NNNN represents a
four-digit consecutive number starting from 1001 to distinguish from previous
findings of the OGLE project (Udalski et al.2002abc, 2008, Pont et al.2008).
The SNR is defined as:

${\rm SNR}=\frac{\delta}{\sigma_{o}}n^{1/2}$ (1)

where $\delta$ represents the transit depth, $\sigma$ is the standard
deviation of the out-of-transit points, and $n$ is the number of in-transit
points (Pont et al.2006), Calculations of SNR values are based on EXOFASTv2
models. All the selected candidates have SNR greater than 6, with median value
$\rm{med}(\rm{SNR})=20.46$. The values of probability that the transit is of
planetary origin $\rm{Pr(planet|signal)}$ were obtained with VESPA. As
mentioned above, $\rm{Pr(planet|signal)}$ ranges between $0.8$ and $1.0$, with
$\rm{Pr(planet|signal)}\geq 0.99$ for 63 objects . The remaining parameters
are median values resulting from the MCMC modeling (for detailed definitions
of the parameters see Eastman et al.2019). The majority of our candidates
belong to the hot Jupiters family. The orbital periods range from $0.67$ d
(slightly above the minimal period search by the TLS algorithm, $0.60$ d) to
$63.22$ d. The radii of companions are typical for Jupiter-like gas giants,
with a median value of $\rm{med}(R_{\rm{p}})=1.385~{}R_{\rm{J}}$, with an
exception of OGLE-TR-1003b. This candidate has the size corresponding to
Neptune-like planets ($R_{\rm{p}}=0.529~{}R_{\rm{J}}$). The proximity to its
host star places OGLE-TR-1003b in the parameter space of the so-called hot
Neptune desert, which is an observed dearth of Neptune-size planets on orbits
with periods shorter than $\approx 5-10$ d (Mazeh et al.2016). In Fig. 5 we
present how the radii of candidates are distributed depending on the orbital
period or equilibrium temperature, with the Neptune desert area marked. The
distance distributions of the candidates span between 0.4 kpc and 5.5 kpc,
which translates to $2.8-7.9$ kpc from the Galactic center, as shown in Fig.
6. Additionally, Fig. 6 illustrates the uniqueness of our findings in
comparison to other known exoplanets in the Galaxy. To date, only observations
from the Hubble Space Telescope have enabled the detection of sixteen
transiting planetary candidates (two confirmed through RV measurements) close
to the Galactic center (Sahu et al.2006, 2008). The only detection method that
efficiently probes this region of the Galaxy is the microlensing method.
Nevertheless, this method is sensitive to planets on wider orbits compared to
transit detections and, due to its transient nature, limits follow-up in-depth
characterization of systems.

The full list of determined parameters of the systems with photometric data is
available on the OGLE website 222ogledb.astrouw.edu.pl/~ogle/OCVS/.

Parameters of detected planetary candidates. The Jovian-size objects are
indicated by red points with error bars. Blue diamond mark the sub-Jovian
object – OGLE-TR-1003. Gray dots – currently known confirmed planets
(exoplanets.eu, as for September 2023). The hot Neptune desert from Mazeh et
al.(2016) shown with dashed lines in the left panel.

Galactic distribution of our planetary candidates and known confirmed
exoplanets (exoplanets.eu, as for September 2023).

##  5 Future Prospects

We confirmed that observations of the Galactic bulge regions offer
opportunities for planetary transit research. These regions are often
overlooked by typical transit surveys due to the challenges associated with
crowding. Nevertheless, they are and will continue to be monitored by surveys
with a specific focus on detecting microlensing events. The large number of
photometric measurements collected this way can be used for planetary transit
studies.

One of the notable advantages of our catalog is the extended time span of
available observations. For many of our candidates, we can expand the time
coverage to an exceptional 23-year period by incorporating observations from
the previous phase of the OGLE project (OGLE-III, 2001-2009). This long time
span of regular observations has not been achieved by any other survey capable
of detecting exoplanets. Consequently, our planetary candidates become
valuable objects for studies of long-term orbital evolution (Hagey et
al.2022).

Furthermore, the upcoming Nancy Grace Roman Space Telescope (Spergel et
al.2015, Montet et al.2017) is expected to provide an additional 40 000
precise photometric and astrometric measurements of our targets. While our
objects are brighter than the planned saturation limit of Roman ($14.8$ mag in
filter $W149$, Penny et al.2019), the expected relative precision will still
be of order of 1 part per thousand (Montet et al.2017). Using noise estimation
for a single epoch in the Roman $W149$ filter from Gould et al.(2015):

$\sigma=1.0\times 10^{(2/15)(H-15)}~{}\textrm{mmag}\quad\textrm{for}\quad
8\lesssim H\lesssim 15~{}\rm{mag}$ (2)

where $H$ stands for the near-infrared $H-$band, using values determined from
created SED models, we find that for our targets, $\sigma$ would be around
$0.001$ mag.

As we mentioned in Subsection 3.2, the time-series observations alone are not
enough to confirm the planetary nature of the objects. Given the relative
faintness of our targets and the accessibility of telescopes, performing
follow-up RV observations for all our candidates may not be achievable.
Nevertheless, this challenge exists since transit detections have increased in
numbers, and various alternative validation methods have been developed, such
as the probabilistic validation method used by us. Conducting additional
photometric observations, including multi-band transit observations or high-
resolution adaptive optics observations, will further help in establishing the
level of blended light. Additionally, obtaining low-resolution spectroscopic
observations of the host stars can help narrow down their parameters and,
indirectly, the parameters of the companions.

It is important to acknowledge that many of the selection steps for candidates
presented in this work were subjective. Therefore, we advise exercising
caution when using this catalog beyond a collection of individual cases for
further analyses.

##  6 Conclusions

We conducted a planetary transit search using photometric observations
collected during the fourth phase of the OGLE project. We used observations of
main sequence stars within four fields covering a total area of
$5.6~{}\rm{deg^{2}}$ in the direction of the Galactic bulge. To identify
potential candidates, we employed a method that fits realistic transit shapes
to data folded according to the grid of trial periods. After the vetting
process, which included the evaluation of the probability of false positive
signals, we selected the most promising objects. Using all available data,
sourced both from the OGLE project and the public domain, we developed
comprehensive models of planetary systems. We presented selected 99 highly-
probable planetary candidates. The majority of these candidates fall within
the category of hot and warm Jupiters, with the exception of one object
exhibiting a sub-Jovian size. Notably, this companion in OGLE-TR-1003 is
located in the hot Neptune desert. Our candidates are distributed across a
wide range of distances, extending up to 5.5 kpc, dovetailing with planets
discovered with the microlensing method. This synergy offers an extraordinary
opportunity for the study of planetary systems, encompassing those with the
shortest to the longest orbital periods as a function of Galactic distance.
Furthermore, finding transiting planets in fields monitored by microlensing
surveys is extremely beneficial in terms of time coverage of observations. In
the case of our candidates, the OGLE database can provide regular and
consistent observations since 2001, with the potential for further extensions
as the project continues. Additionally, the upcoming Nancy Grace Roman Space
Telescope mission is expected to provide additional observations of our
targets with improved precision.

We thank all the OGLE observers for their contribution to the collection of
the photometric data over the decades.

This work has been funded by the National Science Centre, Poland, grant no.
2022/45/B/ST9/00243. For the purpose of Open Access, the author has applied a
CC-BY public copyright license to any Author Accepted Manuscript (AAM) version
arising from this submission.

We used data from the European Space Agency (ESA) mission Gaia, processed by
the Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC
has been provided by national institutions, in particular the institutions
participating in the Gaia Multilateral Agreement.

This project used public archival data from the Dark Energy Survey (DES).
Funding for the DES Projects has been provided by the U.S. Department of
Energy, the U.S. National Science Foundation, the Ministry of Science and
Education of Spain, the Science and Technology Facilities Council of the
United Kingdom, the Higher Education Funding Council for England, the National
Center for Supercomputing Applications at the University of Illinois at
Urbana-Champaign, the Kavli Institute of Cosmological Physics at the
University of Chicago, the Center for Cosmology and Astro-Particle Physics at
the Ohio State University, the Mitchell Institute for Fundamental Physics and
Astronomy at Texas A&M University, Financiadora de Estudos e Projetos,
Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro,
Conselho Nacional de Desenvolvimento Científico e Tecnológico and the
Ministério da Ciência, Tecnologia e Inovação, the Deutsche
Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy
Survey. The Collaborating Institutions are Argonne National Laboratory, the
University of California at Santa Cruz, the University of Cambridge, Centro de
Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the
University of Chicago, University College London, the DES-Brazil Consortium,
the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH)
Zürich, Fermi National Accelerator Laboratory, the University of Illinois at
Urbana-Champaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the
Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory,
the Ludwig-Maximilians Universität München and the associated Excellence
Cluster Universe, the University of Michigan, the National Optical Astronomy
Observatory, the University of Nottingham, The Ohio State University, the
OzDES Membership Consortium, the University of Pennsylvania, the University of
Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the
University of Sussex, and Texas A&M University. Based in part on observations
at Cerro Tololo Inter-American Observatory, National Optical Astronomy
Observatory, which is operated by the Association of Universities for Research
in Astronomy (AURA) under a cooperative agreement with the National Science
Foundation.

The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been
made possible through contributions by the Institute for Astronomy, the
University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society
and its participating institutes, the Max Planck Institute for Astronomy,
Heidelberg and the Max Planck Institute for Extraterrestrial Physics,
Garching, The Johns Hopkins University, Durham University, the University of
Edinburgh, the Queen’s University Belfast, the Harvard-Smithsonian Center for
Astrophysics, the Las Cumbres Observatory Global Telescope Network
Incorporated, the National Central University of Taiwan, the Space Telescope
Science Institute, the National Aeronautics and Space Administration under
Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA
Science Mission Directorate, the National Science Foundation Grant No.
AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the
Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation.

Light curves of planetary transit candidates: OGLE-TR-1001–OGLE-TR-1015. Gray
points – folded observational data, red points – binned observational data,
green line – fitted MCMC model with minima $\chi^{2}$.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1016–OGLE-TR-1030.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1031–OGLE-TR-1045.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1046–OGLE-TR-1060.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1061–OGLE-TR-1075.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1076–OGLE-TR-1090.

Same as Fig. 7, planetary transit candidates: OGLE-TR-1091–OGLE-TR-1099.

T a b l e 3

Observational parameters of systems with planetary candidates.

Name | RA | DEC | $P_{\rm{orb}}$ | $T_{\rm{c}}$ | $T_{\rm{14}}$ | $\delta$ | $I$ | $V$ | $\rm{SNR}$ | $\rm{{Pr}(planet|signal)}$
---|---|---|---|---|---|---|---|---|---|---
| (J2000) | (J2000) | [d] |  [$\rm{BJD_{TDB}}-2450000$] | [d] |  | [mag] | [mag] |  |
OGLE-TR-1001 | $17:49:43.17$ | $-29:23:41.9$ | $2.1093174$ | $5378.18379$ | $0.1043$ | $0.00823$ | 13.923 | 14.815 | 58.05 | 1.00
OGLE-TR-1002 | $17:49:51.28$ | $-29:18:01.1$ | $13.197893$ | $5379.7864$ | $0.1740$ | $0.0142$ | 15.419 | 17.021 | 32.86 | 0.93
OGLE-TR-1003 | $17:50:22.77$ | $-29:23:19.4$ | $2.7762253$ | $5379.3403$ | $0.1123$ | $0.00285$ | 15.382 | 16.872 | 12.60 | 1.00
OGLE-TR-1004 | $17:50:23.35$ | $-30:15:01.4$ | $10.186892$ | $5379.8420$ | $0.1964$ | $0.00635$ | 14.168 | 15.348 | 29.93 | 1.00
OGLE-TR-1005 | $17:50:28.70$ | $-29:54:23.9$ | $4.5659828$ | $5380.5474$ | $0.2317$ | $0.00655$ | 14.824 | 15.931 | 35.43 | 1.00
OGLE-TR-1006 | $17:50:38.40$ | $-29:22:06.8$ | $1.8082001$ | $5377.0093$ | $0.0970$ | $0.00287$ | 14.902 | 16.640 | 16.33 | 0.99
OGLE-TR-1007 | $17:50:47.56$ | $-30:11:59.7$ | $3.5659243$ | $5379.2049$ | $0.1960$ | $0.01082$ | 12.855 | 13.626 | 56.25 | 1.00
OGLE-TR-1008 | $17:50:48.36$ | $-29:40:49.1$ | $63.2215$ | $5416.535$ | $0.552$ | $0.00331$ | 15.056 | 16.583 | 6.39 | 1.00
OGLE-TR-1009 | $17:50:56.70$ | $-29:40:49.1$ | $29.549047$ | $5398.1766$ | $0.3472$ | $0.01088$ | 14.155 | 15.146 | 36.99 | 1.00
OGLE-TR-1010 | $17:51:30.88$ | $-29:55:45.2$ | $2.2063895$ | $5377.4247$ | $0.1826$ | $0.00699$ | 14.519 | 15.718 | 51.76 | 1.00
OGLE-TR-1011 | $17:51:53.22$ | $-30:01:15.7$ | $16.854160$ | $5389.1759$ | $0.313$ | $0.00654$ | 15.463 | 17.080 | 15.91 | 0.99
OGLE-TR-1012 | $17:52:14.08$ | $-29:14:41.8$ | $3.576539$ | $5379.8131$ | $0.1629$ | $0.00396$ | 15.365 | 16.549 | 14.31 | 1.00
OGLE-TR-1013 | $17:52:27.45$ | $-29:53:02.5$ | $23.89398$ | $5390.170$ | $0.240$ | $0.00538$ | 15.031 | 16.035 | 9.03 | 0.99
OGLE-TR-1014 | $17:52:29.08$ | $-29:25:30.7$ | $12.06657$ | $5379.955$ | $0.321$ | $0.00254$ | 14.280 | 15.423 | 7.05 | 0.98
OGLE-TR-1015 | $17:52:32.93$ | $-30:03:59.9$ | $16.47033$ | $5377.320$ | $0.433$ | $0.00241$ | 15.432 | 16.491 | 7.33 | 1.00
OGLE-TR-1016 | $17:52:47.03$ | $-29:53:32.2$ | $3.918334$ | $5377.401$ | $0.186$ | $0.00184$ | 15.122 | 16.191 | 8.98 | 0.88
OGLE-TR-1017 | $17:53:03.85$ | $-30:06:36.0$ | $8.293105$ | $5378.3103$ | $0.1452$ | $0.0121$ | 15.172 | 16.462 | 23.69 | 1.00
OGLE-TR-1018 | $17:54:28.67$ | $-30:04:39.9$ | $3.795212$ | $5376.7046$ | $0.1650$ | $0.00446$ | 15.380 | 16.568 | 15.26 | 1.00
OGLE-TR-1019 | $17:54:35.45$ | $-27:43:17.3$ | $23.07172$ | $5377.6698$ | $0.358$ | $0.0215$ | 15.306 | 17.194 | 17.85 | 0.92
OGLE-TR-1020 | $17:55:01.28$ | $-29:27:10.0$ | $37.78747$ | $5388.5955$ | $0.313$ | $0.0202$ | 15.348 | 17.030 | 38.64 | 1.00
OGLE-TR-1021 | $17:55:17.82$ | $-27:37:51.7$ | $50.24001$ | $5394.4031$ | $0.3439$ | $0.02392$ | 14.680 | 15.917 | 36.94 | 0.98
OGLE-TR-1022 | $17:55:17.87$ | $-27:52:33.5$ | $8.102826$ | $5383.7016$ | $0.335$ | $0.00336$ | 14.119 | 15.414 | 21.31 | 0.99
OGLE-TR-1023 | $17:55:18.63$ | $-28:22:08.5$ | $6.598261$ | $5378.3482$ | $0.1358$ | $0.0161$ | 15.220 | 16.799 | 36.96 | 1.00
OGLE-TR-1024 | $17:55:28.73$ | $-27:26:23.4$ | $1.4272776$ | $5377.3506$ | $0.1400$ | $0.00269$ | 15.145 | 16.774 | 9.66 | 0.94
OGLE-TR-1025 | $17:55:41.38$ | $-27:29:06.8$ | $6.949874$ | $5377.984$ | $0.368$ | $0.00138$ | 14.727 | 16.192 | 7.64 | 0.84
OGLE-TR-1026 | $17:55:43.01$ | $-27:55:57.9$ | $4.119552$ | $5376.948$ | $0.357$ | $0.00208$ | 14.528 | 15.635 | 10.82 | 0.97
OGLE-TR-1027 | $17:55:49.63$ | $-29:11:39.3$ | $2.624793$ | $5261.407$ | $0.144$ | $0.00203$ | 14.785 | 16.199 | 12.84 | 0.82
OGLE-TR-1028 | $17:55:56.66$ | $-29:17:03.8$ | $0.74714108$ | $5376.7574$ | $0.1027$ | $0.00489$ | 13.753 | 15.111 | 43.03 | 0.90
OGLE-TR-1029 | $17:56:00.49$ | $-28:49:24.8$ | $2.5308880$ | $5261.7539$ | $0.1081$ | $0.01217$ | 15.194 | 16.400 | 44.07 | 1.00
OGLE-TR-1030 | $17:56:05.22$ | $-27:56:09.0$ | $18.187463$ | $5388.3494$ | $0.280$ | $0.00841$ | 15.276 | 16.945 | 18.11 | 0.99
OGLE-TR-1031 | $17:56:11.67$ | $-27:40:02.7$ | $2.420147$ | $5376.749$ | $0.186$ | $0.00280$ | 14.337 | 15.605 | 7.38 | 1.00
OGLE-TR-1032 | $17:56:16.96$ | $-28:24:39.9$ | $14.165438$ | $5383.9723$ | $0.3117$ | $0.01825$ | 15.242 | 16.913 | 50.46 | 1.00
OGLE-TR-1033 | $17:56:22.42$ | $-29:10:17.1$ | $17.909180$ | $5381.5566$ | $0.3724$ | $0.00680$ | 15.296 | 16.933 | 25.54 | 1.00
OGLE-TR-1034 | $17:56:39.10$ | $-27:36:45.3$ | $5.4047713$ | $5377.5239$ | $0.1843$ | $0.02099$ | 15.194 | 16.986 | 62.69 | 0.98
OGLE-TR-1035 | $17:56:42.84$ | $-28:19:34.9$ | $55.27448$ | $5379.163$ | $0.292$ | $0.0124$ | 13.646 | 14.566 | 15.59 | 0.98
OGLE-TR-1036 | $17:56:47.29$ | $-28:37:15.7$ | $0.93942100$ | $5261.03860$ | $0.0782$ | $0.01648$ | 14.029 | 14.911 | 96.27 | 0.92
OGLE-TR-1037 | $17:57:00.17$ | $-28:20:07.3$ | $6.535826$ | $5381.591$ | $0.232$ | $0.00162$ | 14.706 | 15.982 | 7.21 | 0.86
OGLE-TR-1038 | $17:57:12.92$ | $-27:29:09.3$ | $3.769846$ | $5379.148$ | $0.436$ | $0.00477$ | 13.630 | 14.904 | 6.95 | 1.00
OGLE-TR-1039 | $17:57:19.05$ | $-29:49:41.8$ | $9.158188$ | $5380.9316$ | $0.1984$ | $0.00325$ | 14.900 | 16.115 | 13.59 | 0.94
OGLE-TR-1040 | $17:57:21.04$ | $-28:49:13.1$ | $19.496967$ | $5277.9227$ | $0.1955$ | $0.01203$ | 15.394 | 16.719 | 18.42 | 1.00
OGLE-TR-1041 | $17:57:27.61$ | $-29:30:00.4$ | $3.0470709$ | $5377.2418$ | $0.1426$ | $0.00881$ | 14.996 | 16.394 | 45.77 | 1.00
OGLE-TR-1042 | $17:57:29.88$ | $-28:42:17.1$ | $7.675599$ | $5267.8518$ | $0.2646$ | $0.01221$ | 15.492 | 17.101 | 39.99 | 1.00
OGLE-TR-1043 | $17:57:44.37$ | $-27:58:28.5$ | $2.196576$ | $5378.07$ | $0.091$ | $0.0031$ | 15.359 | 17.073 | 7.24 | 0.98
OGLE-TR-1044 | $17:57:54.98$ | $-27:48:40.8$ | $5.1944381$ | $5380.3002$ | $0.1583$ | $0.0417$ | 13.836 | 14.852 | 21.54 | 1.00
OGLE-TR-1045 | $17:57:55.52$ | $-29:13:04.2$ | $2.1355658$ | $5262.4665$ | $0.1623$ | $0.0302$ | 14.730 | 15.750 | 26.05 | 1.00
OGLE-TR-1046 | $17:57:56.84$ | $-27:36:50.5$ | $10.619790$ | $5381.1543$ | $0.2896$ | $0.01414$ | 15.245 | 16.751 | 34.92 | 0.96
OGLE-TR-1047 | $17:58:06.08$ | $-27:46:06.7$ | $10.295061$ | $5378.3788$ | $0.2506$ | $0.01349$ | 15.476 | 16.759 | 33.56 | 1.00
OGLE-TR-1048 | $17:58:07.33$ | $-29:27:32.2$ | $5.2472019$ | $5378.6899$ | $0.1735$ | $0.01730$ | 15.431 | 16.736 | 32.92 | 1.00
OGLE-TR-1049 | $17:58:17.11$ | $-27:34:26.1$ | $19.15773$ | $5384.334$ | $0.737$ | $0.00122$ | 14.629 | 16.007 | 6.33 | 1.00
OGLE-TR-1050 | $17:58:27.67$ | $-29:49:32.0$ | $1.6114682$ | $5377.8440$ | $0.1208$ | $0.0152$ | 15.269 | 16.204 | 41.03 | 0.97
OGLE-TR-1051 | $17:58:31.55$ | $-29:16:55.4$ | $1.0213727$ | $5376.673$ | $0.465$ | $0.001312$ | 15.324 | 17.065 | 17.85 | 0.97
OGLE-TR-1052 | $17:58:33.17$ | $-29:23:01.1$ | $6.921614$ | $5377.348$ | $0.534$ | $0.00169$ | 14.876 | 16.149 | 12.62 | 0.96
OGLE-TR-1053 | $17:58:34.08$ | $-28:48:24.9$ | $3.6519106$ | $5273.7362$ | $0.1135$ | $0.0109$ | 14.915 | 15.829 | 47.88 | 1.00
OGLE-TR-1054 | $17:58:39.75$ | $-27:22:32.0$ | $8.58268$ | $5378.537$ | $0.342$ | $0.00272$ | 15.066 | 16.220 | 6.25 | 0.98
OGLE-TR-1055 | $17:58:41.82$ | $-29:11:27.7$ | $2.104221$ | $5503.963$ | $0.236$ | $0.00135$ | 14.919 | 16.800 | 7.99 | 0.95
OGLE-TR-1056 | $17:58:55.74$ | $-28:53:03.8$ | $7.7213$ | $5263.3$ | $0.195$ | $0.00181$ | 14.913 | 16.686 | 7.03 | 0.94
OGLE-TR-1057 | $17:59:05.12$ | $-28:29:51.9$ | $5.854539$ | $5378.9814$ | $0.586$ | $0.00491$ | 15.245 | 17.114 | 18.57 | 1.00
OGLE-TR-1058 | $17:59:14.69$ | $-27:44:55.6$ | $17.41082$ | $5382.036$ | $0.403$ | $0.00217$ | 14.806 | 16.222 | 8.02 | 0.94
OGLE-TR-1059 | $17:59:24.87$ | $-28:01:37.4$ | $7.208224$ | $5377.8502$ | $0.2321$ | $0.00646$ | 15.412 | 16.726 | 19.09 | 0.97
OGLE-TR-1060 | $17:59:27.20$ | $-28:00:26.8$ | $12.831750$ | $5386.0147$ | $0.2709$ | $0.01508$ | 15.307 | 16.677 | 34.86 | 1.00
OGLE-TR-1061 | $17:59:30.54$ | $-27:23:20.3$ | $2.6528610$ | $5376.6303$ | $0.1696$ | $0.00915$ | 14.119 | 14.767 | 55.65 | 1.00
OGLE-TR-1062 | $17:59:44.10$ | $-28:05:53.7$ | $16.52749$ | $5383.916$ | $0.327$ | $0.00445$ | 15.152 | 16.495 | 7.76 | 1.00
OGLE-TR-1063 | $17:59:51.37$ | $-29:17:22.5$ | $3.5835181$ | $5261.3897$ | $0.1596$ | $0.01070$ | 14.703 | 15.560 | 51.49 | 1.00
OGLE-TR-1064 | $18:00:00.26$ | $-29:15:02.6$ | $0.6700153$ | $5286.4298$ | $0.0945$ | $0.00320$ | 15.472 | 16.582 | 20.52 | 0.99
OGLE-TR-1065 | $18:00:17.82$ | $-28:49:53.7$ | $4.967119$ | $5380.6973$ | $0.194$ | $0.00310$ | 15.463 | 17.413 | 11.33 | 1.00
OGLE-TR-1066 | $18:00:24.34$ | $-28:20:56.8$ | $10.03302$ | $5386.199$ | $0.588$ | $0.00219$ | 15.257 | 16.412 | 11.24 | 0.84
OGLE-TR-1067 | $18:01:02.46$ | $-29:09:54.7$ | $2.573161$ | $5376.738$ | $0.325$ | $0.00217$ | 14.744 | 16.651 | 23.79 | 0.94
OGLE-TR-1068 | $18:01:11.74$ | $-28:53:43.1$ | $0.68587341$ | $5376.9436$ | $0.0858$ | $0.00619$ | 12.800 | 13.359 | 41.69 | 1.00
OGLE-TR-1069 | $18:01:16.03$ | $-28:25:46.1$ | $10.605366$ | $5383.6787$ | $0.5106$ | $0.01568$ | 15.339 | 16.611 | 54.25 | 1.00
OGLE-TR-1070 | $18:01:17.40$ | $-28:30:28.0$ | $1.7293835$ | $5380.2336$ | $0.1135$ | $0.01428$ | 15.400 | 16.324 | 34.25 | 0.81
OGLE-TR-1071 | $18:01:17.69$ | $-28:48:23.4$ | $4.26703$ | $5383.137$ | $0.458$ | $0.0049$ | 15.424 | 17.366 | 15.87 | 1.00
OGLE-TR-1072 | $18:01:20.90$ | $-28:26:24.4$ | $1.6133903$ | $5377.4958$ | $0.0986$ | $0.00808$ | 15.112 | 16.169 | 33.32 | 1.00
OGLE-TR-1073 | $18:01:28.64$ | $-28:25:28.0$ | $6.92344$ | $5380.819$ | $0.400$ | $0.00130$ | 15.283 | 17.176 | 6.60 | 1.00
OGLE-TR-1074 | $18:01:46.42$ | $-28:00:52.9$ | $0.7182068$ | $5376.8768$ | $0.0807$ | $0.00344$ | 15.167 | 16.364 | 24.77 | 0.92
OGLE-TR-1075 | $18:01:47.87$ | $-28:01:19.6$ | $30.55566$ | $5390.5423$ | $0.441$ | $0.01590$ | 15.297 | 16.490 | 39.16 | 1.00
OGLE-TR-1076 | $18:01:59.91$ | $-28:46:32.9$ | $5.785527$ | $5380.2351$ | $0.2844$ | $0.01468$ | 15.057 | 16.128 | 25.86 | 1.00
OGLE-TR-1077 | $18:02:01.98$ | $-28:43:15.8$ | $14.40827$ | $5381.544$ | $0.255$ | $0.00397$ | 14.606 | 15.541 | 6.52 | 0.99
OGLE-TR-1078 | $18:02:16.54$ | $-29:05:43.6$ | $4.3297076$ | $5377.6280$ | $0.2245$ | $0.00740$ | 14.700 | 15.665 | 45.05 | 1.00
OGLE-TR-1079 | $18:02:44.77$ | $-28:48:25.6$ | $13.45047$ | $5381.447$ | $0.554$ | $0.00294$ | 15.351 | 17.201 | 7.58 | 1.00
OGLE-TR-1080 | $18:02:50.21$ | $-28:21:44.1$ | $4.7576944$ | $5377.9397$ | $0.2339$ | $0.00446$ | 14.871 | 16.122 | 25.76 | 1.00
OGLE-TR-1081 | $18:03:14.00$ | $-28:27:14.8$ | $6.406942$ | $5377.5162$ | $0.1741$ | $0.00608$ | 14.978 | 15.934 | 23.62 | 1.00
OGLE-TR-1082 | $18:03:15.26$ | $-28:45:00.7$ | $3.403645$ | $5379.0038$ | $0.379$ | $0.00377$ | 15.398 | 17.377 | 18.94 | 1.00
OGLE-TR-1083 | $18:03:15.36$ | $-28:24:25.6$ | $5.410081$ | $5380.6355$ | $0.1406$ | $0.01005$ | 15.057 | 16.084 | 20.41 | 1.00
OGLE-TR-1084 | $18:03:18.58$ | $-28:24:45.1$ | $39.79726$ | $5402.3122$ | $0.2763$ | $0.01558$ | 14.141 | 14.969 | 39.18 | 0.94
OGLE-TR-1085 | $18:03:21.39$ | $-28:12:40.2$ | $3.636724$ | $5377.8549$ | $0.129$ | $0.00316$ | 15.362 | 17.017 | 12.74 | 1.00
OGLE-TR-1086 | $18:03:39.15$ | $-28:47:04.6$ | $6.703196$ | $5383.100$ | $0.237$ | $0.00510$ | 15.324 | 16.785 | 17.18 | 0.94
OGLE-TR-1087 | $18:03:46.16$ | $-28:07:56.2$ | $4.243165$ | $5378.3633$ | $0.206$ | $0.00654$ | 15.148 | 16.438 | 30.74 | 1.00
OGLE-TR-1088 | $18:03:47.49$ | $-28:05:03.0$ | $5.0748842$ | $5378.05549$ | $0.1469$ | $0.01584$ | 14.438 | 15.373 | 66.06 | 1.00
OGLE-TR-1089 | $18:04:07.51$ | $-28:41:30.5$ | $51.09021$ | $5384.643$ | $0.346$ | $0.0186$ | 14.961 | 16.088 | 15.94 | 1.00
OGLE-TR-1090 | $18:04:14.72$ | $-28:20:22.9$ | $6.555184$ | $5376.6412$ | $0.2352$ | $0.00525$ | 14.240 | 14.918 | 18.22 | 1.00
OGLE-TR-1091 | $18:04:18.26$ | $-28:24:30.5$ | $55.74533$ | $5427.429$ | $0.429$ | $0.0129$ | 15.249 | 17.054 | 21.54 | 0.99
OGLE-TR-1092 | $18:04:23.84$ | $-28:48:50.7$ | $3.660176$ | $5380.164$ | $0.212$ | $0.00188$ | 15.294 | 16.873 | 7.65 | 1.00
OGLE-TR-1093 | $18:04:46.65$ | $-28:57:20.9$ | $1.4751354$ | $5377.1974$ | $0.134$ | $0.0113$ | 14.756 | 16.523 | 80.19 | 0.98
OGLE-TR-1094 | $18:04:49.42$ | $-28:00:44.0$ | $13.20038$ | $5388.402$ | $0.312$ | $0.0102$ | 15.497 | 17.402 | 9.66 | 1.00
OGLE-TR-1095 | $18:04:53.49$ | $-28:13:33.0$ | $0.7848204$ | $5377.2801$ | $0.0864$ | $0.00282$ | 15.239 | 17.210 | 15.83 | 0.90
OGLE-TR-1096 | $18:05:07.41$ | $-28:15:56.6$ | $3.437753$ | $5377.2231$ | $0.446$ | $0.00514$ | 15.446 | 17.249 | 27.43 | 1.00
OGLE-TR-1097 | $18:05:15.35$ | $-28:08:47.3$ | $10.756626$ | $5385.3247$ | $0.1199$ | $0.01424$ | 15.128 | 16.745 | 29.74 | 0.90
OGLE-TR-1098 | $18:05:29.39$ | $-28:15:28.8$ | $5.880841$ | $5379.1189$ | $0.1454$ | $0.0203$ | 15.372 | 16.404 | 40.22 | 0.93
OGLE-TR-1099 | $18:05:36.98$ | $-28:28:27.6$ | $10.46173$ | $5376.945$ | $0.630$ | $0.00279$ | 15.369 | 17.213 | 14.37 | 1.00

T a b l e 4

Selected physical parameters of systems with planetary candidates.

Name | $M_{*}$ | $R_{*}$ | $\rm{log}g$ | $T_{\rm{eff}}$ | $\rm{[Fe/H]}$ | $d$ | $a$ | $i$ | $T_{\rm{eq}}$ | $R_{\rm{P}}$
---|---|---|---|---|---|---|---|---|---|---
|  [$M_{\odot}$] |  [$R_{\odot}$] | [cgs] | [K] | $[dex]$ | [pc] | [AU] | [deg] | [K] |  [$R_{\rm{J}}$]
OGLE-TR-1001 | $2.44^{+0.42}_{-0.36}$ | $1.57^{+0.23}_{-0.14}$ | $4.42^{+0.13}_{-0.15}$ | $14400^{+2500}_{-3800}$ | $-1.5^{+1.5}_{-1.6}$ | $1810^{+91}_{-79}$ | $0.0437^{+0.0023}_{-0.0024}$ | $84.2^{+2.1}_{-2.3}$ | $4190^{+480}_{-860}$ | $1.39^{+0.22}_{-0.14}$
OGLE-TR-1002 | $1.27^{+0.12}_{-0.14}$ | $1.429^{+0.086}_{-0.099}$ | $4.232^{+0.062}_{-0.059}$ | $6030^{+310}_{-280}$ | $0.38^{+0.11}_{-0.18}$ | $1660^{+130}_{-120}$ | $0.1184^{+0.0036}_{-0.0044}$ | $87.28^{+0.26}_{-0.22}$ | $1007^{+51}_{-46}$ | $1.66^{+0.12}_{-0.15}$
OGLE-TR-1003 | $0.927^{+0.130}_{-0.090}$ | $1.021^{+0.098}_{-0.075}$ | $4.393^{+0.051}_{-0.067}$ | $5770^{+310}_{-250}$ | $-0.11^{+0.23}_{-0.40}$ | $1088^{+120}_{-93}$ | $0.0377^{+0.0017}_{-0.0013}$ | $88.2^{+1.2}_{-1.7}$ | $1452^{+96}_{-78}$ | $0.529^{+0.057}_{-0.042}$
OGLE-TR-1004 | $1.93^{+0.14}_{-0.14}$ | $1.96^{+0.19}_{-0.18}$ | $4.142^{+0.077}_{-0.079}$ | $7780^{+400}_{-400}$ | $0.31^{+0.12}_{-0.19}$ | $1690^{+140}_{-130}$ | $0.1166^{+0.0029}_{-0.0033}$ | $86.64^{+0.46}_{-0.51}$ | $1536^{+76}_{-73}$ | $1.52^{+0.16}_{-0.16}$
OGLE-TR-1005 | $0.965^{+0.330}_{-0.075}$ | $1.763^{+0.210}_{-0.090}$ | $3.949^{+0.052}_{-0.062}$ | $7800^{+830}_{-470}$ | $-3.99^{+1.20}_{-0.31}$ | $2210^{+260}_{-130}$ | $0.0533^{+0.0055}_{-0.0014}$ | $87.9^{+1.5}_{-1.8}$ | $2160^{+230}_{-120}$ | $1.389^{+0.180}_{-0.078}$
OGLE-TR-1006 | $1.74^{+0.14}_{-0.17}$ | $2.19^{+0.20}_{-0.15}$ | $4.003^{+0.044}_{-0.086}$ | $5310^{+300}_{-310}$ | $0.30^{+0.21}_{-0.26}$ | $1520^{+120}_{-97}$ | $0.03521^{+0.00090}_{-0.00110}$ | $75.1^{+1.1}_{-2.0}$ | $2022^{+100}_{-84}$ | $1.131^{+0.150}_{-0.088}$
OGLE-TR-1007 | $1.65^{+0.21}_{-0.12}$ | $2.95^{+0.24}_{-0.23}$ | $3.726^{+0.053}_{-0.053}$ | $6800^{+580}_{-520}$ | $-3.32^{+1.50}_{-0.49}$ | $1690^{+170}_{-160}$ | $0.0569^{+0.0020}_{-0.0015}$ | $78.22^{+0.96}_{-1.00}$ | $2350^{+210}_{-180}$ | $2.98^{+0.29}_{-0.27}$
OGLE-TR-1008 | $0.98^{+0.29}_{-0.35}$ | $2.10^{+0.19}_{-0.16}$ | $3.78^{+0.15}_{-0.20}$ | $5130^{+430}_{-390}$ | $-2.3^{+2.0}_{-1.4}$ | $1770^{+130}_{-120}$ | $0.312^{+0.028}_{-0.041}$ | $88.87^{+0.49}_{-0.44}$ | $652^{+51}_{-56}$ | $1.170^{+0.110}_{-0.087}$
OGLE-TR-1009 | $4.19^{+0.56}_{-0.52}$ | $2.185^{+0.098}_{-0.094}$ | $4.382^{+0.027}_{-0.030}$ | $21600^{+1800}_{-2100}$ | $-3.13^{+1.00}_{-0.57}$ | $3160^{+300}_{-280}$ | $0.302^{+0.013}_{-0.013}$ | $89.80^{+0.14}_{-0.21}$ | $2800^{+230}_{-260}$ | $2.218^{+0.099}_{-0.096}$
OGLE-TR-1010 | $0.826^{+0.039}_{-0.039}$ | $1.711^{+0.140}_{-0.095}$ | $3.888^{+0.056}_{-0.072}$ | $6900^{+260}_{-270}$ | $-4.437^{+0.130}_{-0.076}$ | $1695^{+96}_{-80}$ | $0.03116^{+0.00048}_{-0.00050}$ | $83.9^{+3.0}_{-2.8}$ | $2470^{+88}_{-81}$ | $1.390^{+0.140}_{-0.092}$
OGLE-TR-1011 | $1.56^{+0.22}_{-0.17}$ | $1.94^{+0.42}_{-0.27}$ | $4.070^{+0.086}_{-0.160}$ | $5150^{+380}_{-300}$ | $0.31^{+0.20}_{-0.23}$ | $1870^{+310}_{-210}$ | $0.1525^{+0.0080}_{-0.0075}$ | $88.6^{+1.0}_{-1.3}$ | $896^{+62}_{-51}$ | $1.52^{+0.42}_{-0.25}$
OGLE-TR-1012 | $1.88^{+0.19}_{-0.25}$ | $1.78^{+0.15}_{-0.12}$ | $4.205^{+0.056}_{-0.088}$ | $8170^{+450}_{-400}$ | $0.10^{+0.25}_{-0.49}$ | $2490^{+260}_{-220}$ | $0.0569^{+0.0018}_{-0.0025}$ | $86.4^{+1.8}_{-1.6}$ | $2220^{+140}_{-110}$ | $1.088^{+0.099}_{-0.075}$
OGLE-TR-1013 | $2.00^{+0.60}_{-0.55}$ | $1.47^{+0.13}_{-0.12}$ | $4.40^{+0.13}_{-0.15}$ | $12100^{+3200}_{-2100}$ | $-1.59^{+0.93}_{-1.50}$ | $2670^{+350}_{-260}$ | $0.206^{+0.019}_{-0.021}$ | $89.05^{+0.56}_{-0.48}$ | $1570^{+310}_{-220}$ | $1.049^{+0.085}_{-0.075}$
OGLE-TR-1014 | $0.93^{+0.21}_{-0.11}$ | $1.93^{+0.15}_{-0.14}$ | $3.842^{+0.110}_{-0.086}$ | $6020^{+640}_{-560}$ | $-0.76^{+0.47}_{-1.20}$ | $1100^{+67}_{-60}$ | $0.1023^{+0.0068}_{-0.0040}$ | $88.1^{+1.3}_{-1.2}$ | $1252^{+110}_{-91}$ | $0.944^{+0.070}_{-0.067}$
OGLE-TR-1015 | $0.916^{+0.160}_{-0.094}$ | $2.26^{+0.28}_{-0.21}$ | $3.696^{+0.094}_{-0.100}$ | $5530^{+520}_{-370}$ | $-0.69^{+0.38}_{-0.87}$ | $2690^{+350}_{-270}$ | $0.1250^{+0.0067}_{-0.0044}$ | $88.5^{+1.0}_{-1.2}$ | $1143^{+100}_{-81}$ | $1.071^{+0.098}_{-0.076}$
OGLE-TR-1016 | $1.01^{+0.42}_{-0.18}$ | $2.32^{+0.29}_{-0.31}$ | $3.72^{+0.21}_{-0.14}$ | $5620^{+650}_{-510}$ | $-0.29^{+0.42}_{-1.20}$ | $2680^{+320}_{-290}$ | $0.0495^{+0.0058}_{-0.0029}$ | $79.9^{+2.0}_{-1.9}$ | $1830^{+190}_{-130}$ | $0.983^{+0.088}_{-0.084}$
OGLE-TR-1017 | $1.90^{+0.91}_{-0.50}$ | $1.28^{+0.44}_{-0.16}$ | $4.49^{+0.23}_{-0.29}$ | $12700^{+5200}_{-5100}$ | $-2.6^{+2.7}_{-1.1}$ | $2860^{+630}_{-570}$ | $0.100^{+0.014}_{-0.010}$ | $87.9^{+1.5}_{-1.9}$ | $2200^{+650}_{-690}$ | $1.34^{+0.62}_{-0.18}$
OGLE-TR-1018 | $1.24^{+0.25}_{-0.28}$ | $1.57^{+0.14}_{-0.12}$ | $4.134^{+0.087}_{-0.120}$ | $6360^{+820}_{-630}$ | $0.04^{+0.32}_{-1.20}$ | $1890^{+240}_{-210}$ | $0.0517^{+0.0031}_{-0.0041}$ | $86.2^{+1.9}_{-1.7}$ | $1690^{+240}_{-160}$ | $1.021^{+0.093}_{-0.080}$
OGLE-TR-1019 | $0.820^{+0.078}_{-0.048}$ | $1.385^{+0.079}_{-0.069}$ | $4.076^{+0.049}_{-0.051}$ | $6970^{+410}_{-330}$ | $-4.28^{+1.20}_{-0.24}$ | $1219^{+89}_{-80}$ | $0.1485^{+0.0045}_{-0.0029}$ | $89.65^{+0.24}_{-0.35}$ | $1026^{+58}_{-51}$ | $1.975^{+0.100}_{-0.092}$
OGLE-TR-1020 | $0.57^{+0.17}_{-0.28}$ | $0.865^{+0.055}_{-0.041}$ | $4.29^{+0.12}_{-0.25}$ | $3710^{+190}_{-110}$ | $0.16^{+0.24}_{-1.60}$ | $411^{+29}_{-26}$ | $0.182^{+0.017}_{-0.038}$ | $89.858^{+0.098}_{-0.330}$ | $403^{+34}_{-30}$ | $1.206^{+0.140}_{-0.085}$
OGLE-TR-1021 | $1.504^{+0.100}_{-0.085}$ | $1.459^{+0.062}_{-0.059}$ | $4.288^{+0.029}_{-0.029}$ | $6990^{+360}_{-250}$ | $0.17^{+0.18}_{-0.14}$ | $1586^{+85}_{-77}$ | $0.3053^{+0.0067}_{-0.0058}$ | $89.199^{+0.074}_{-0.072}$ | $737^{+36}_{-28}$ | $2.20^{+0.11}_{-0.10}$
OGLE-TR-1022 | $0.871^{+0.064}_{-0.063}$ | $2.59^{+0.69}_{-0.32}$ | $3.56^{+0.11}_{-0.23}$ | $6490^{+450}_{-790}$ | $-4.16^{+0.96}_{-0.17}$ | $1910^{+210}_{-140}$ | $0.0778^{+0.0025}_{-0.0024}$ | $84.1^{+1.7}_{-2.9}$ | $1801^{+69}_{-74}$ | $1.45^{+0.47}_{-0.22}$
OGLE-TR-1023 | $1.331^{+0.091}_{-0.110}$ | $1.386^{+0.071}_{-0.073}$ | $4.279^{+0.040}_{-0.046}$ | $6290^{+250}_{-240}$ | $0.34^{+0.14}_{-0.21}$ | $1481^{+93}_{-87}$ | $0.0757^{+0.0017}_{-0.0021}$ | $85.92^{+0.29}_{-0.28}$ | $1296^{+56}_{-51}$ | $1.71^{+0.11}_{-0.12}$
OGLE-TR-1024 | $1.44^{+0.27}_{-1.00}$ | $2.03^{+0.17}_{-0.15}$ | $3.96^{+0.10}_{-0.48}$ | $5190^{+430}_{-430}$ | $-0.09^{+0.42}_{-3.20}$ | $1630^{+180}_{-160}$ | $0.0283^{+0.0016}_{-0.0089}$ | $77.0^{+4.6}_{-11.0}$ | $2230^{+210}_{-160}$ | $1.029^{+0.086}_{-0.081}$
OGLE-TR-1025 | $0.42^{+1.10}_{-0.14}$ | $2.85^{+0.23}_{-0.21}$ | $3.16^{+0.50}_{-0.20}$ | $4880^{+260}_{-240}$ | $-3.34^{+3.30}_{-0.48}$ | $1980^{+190}_{-150}$ | $0.0550^{+0.0280}_{-0.0064}$ | $79.2^{+5.8}_{-2.8}$ | $1670^{+110}_{-180}$ | $1.030^{+0.080}_{-0.074}$
OGLE-TR-1026 | $0.857^{+0.140}_{-0.067}$ | $2.73^{+0.32}_{-0.28}$ | $3.503^{+0.100}_{-0.082}$ | $5760^{+480}_{-430}$ | $-1.76^{+0.94}_{-1.20}$ | $1710^{+240}_{-180}$ | $0.0484^{+0.0026}_{-0.0015}$ | $87.4^{+1.8}_{-3.0}$ | $2100^{+170}_{-170}$ | $1.196^{+0.140}_{-0.090}$
OGLE-TR-1027 | $2.06^{+0.47}_{-0.51}$ | $2.95^{+1.10}_{-0.39}$ | $3.80^{+0.11}_{-0.28}$ | $5320^{+370}_{-290}$ | $0.26^{+0.23}_{-0.35}$ | $2570^{+780}_{-340}$ | $0.0477^{+0.0042}_{-0.0037}$ | $75.2^{+2.5}_{-7.7}$ | $2090^{+240}_{-170}$ | $1.21^{+1.20}_{-0.15}$
OGLE-TR-1028 | $1.11^{+0.19}_{-0.14}$ | $2.06^{+0.23}_{-0.16}$ | $3.854^{+0.085}_{-0.095}$ | $5290^{+510}_{-330}$ | $0.22^{+0.23}_{-0.26}$ | $1130^{+130}_{-99}$ | $0.01676^{+0.00090}_{-0.00074}$ | $60.3^{+4.1}_{-5.2}$ | $2830^{+240}_{-160}$ | $1.40^{+0.22}_{-0.14}$
OGLE-TR-1029 | $1.025^{+0.075}_{-0.085}$ | $0.995^{+0.050}_{-0.039}$ | $4.453^{+0.029}_{-0.043}$ | $5650^{+210}_{-200}$ | $0.23^{+0.19}_{-0.19}$ | $1183^{+78}_{-70}$ | $0.03711^{+0.00088}_{-0.00100}$ | $87.9^{+1.2}_{-1.1}$ | $1414^{+62}_{-55}$ | $1.067^{+0.065}_{-0.047}$
OGLE-TR-1030 | $1.40^{+0.11}_{-0.12}$ | $1.556^{+0.160}_{-0.097}$ | $4.204^{+0.058}_{-0.098}$ | $6280^{+330}_{-330}$ | $0.37^{+0.11}_{-0.17}$ | $1536^{+120}_{-99}$ | $0.1517^{+0.0039}_{-0.0045}$ | $88.88^{+0.62}_{-0.65}$ | $974^{+49}_{-41}$ | $1.381^{+0.190}_{-0.099}$
OGLE-TR-1031 | $1.15^{+0.22}_{-0.17}$ | $1.96^{+0.17}_{-0.15}$ | $3.919^{+0.095}_{-0.110}$ | $5490^{+330}_{-420}$ | $0.18^{+0.23}_{-0.24}$ | $1410^{+130}_{-110}$ | $0.0374^{+0.0021}_{-0.0018}$ | $85.5^{+3.0}_{-3.4}$ | $1901^{+92}_{-84}$ | $1.009^{+0.073}_{-0.068}$
OGLE-TR-1032 | $1.417^{+0.084}_{-0.051}$ | $1.699^{+0.050}_{-0.040}$ | $4.131^{+0.014}_{-0.015}$ | $5860^{+290}_{-280}$ | $0.45^{+0.11}_{-0.21}$ | $1598^{+83}_{-74}$ | $0.1287^{+0.0025}_{-0.0016}$ | $89.65^{+0.25}_{-0.36}$ | $1026^{+50}_{-49}$ | $2.232^{+0.067}_{-0.050}$
OGLE-TR-1033 | $0.883^{+0.120}_{-0.083}$ | $1.725^{+0.150}_{-0.082}$ | $3.916^{+0.041}_{-0.062}$ | $7090^{+550}_{-420}$ | $-3.57^{+1.10}_{-0.42}$ | $1880^{+160}_{-130}$ | $0.1286^{+0.0055}_{-0.0041}$ | $89.18^{+0.58}_{-0.82}$ | $1258^{+92}_{-73}$ | $1.381^{+0.130}_{-0.072}$
OGLE-TR-1034 | $0.782^{+0.032}_{-0.022}$ | $1.434^{+0.061}_{-0.061}$ | $4.022^{+0.041}_{-0.037}$ | $6530^{+210}_{-200}$ | $-4.480^{+0.080}_{-0.059}$ | $1409^{+75}_{-72}$ | $0.05554^{+0.00075}_{-0.00052}$ | $85.05^{+0.44}_{-0.41}$ | $1598^{+54}_{-53}$ | $2.02^{+0.11}_{-0.10}$
OGLE-TR-1035 | $1.633^{+0.096}_{-0.092}$ | $1.601^{+0.070}_{-0.067}$ | $4.244^{+0.037}_{-0.042}$ | $7230^{+330}_{-290}$ | $0.15^{+0.16}_{-0.13}$ | $1262^{+42}_{-39}$ | $0.3344^{+0.0064}_{-0.0064}$ | $88.950^{+0.067}_{-0.068}$ | $763^{+29}_{-25}$ | $1.73^{+0.11}_{-0.11}$
OGLE-TR-1036 | $0.794^{+0.083}_{-0.034}$ | $1.329^{+0.050}_{-0.043}$ | $4.099^{+0.028}_{-0.025}$ | $6690^{+320}_{-380}$ | $-3.51^{+2.10}_{-0.86}$ | $1096^{+87}_{-78}$ | $0.01739^{+0.00059}_{-0.00025}$ | $71.70^{+0.71}_{-0.75}$ | $2810^{+140}_{-170}$ | $1.668^{+0.110}_{-0.091}$
OGLE-TR-1037 | $1.42^{+0.32}_{-0.59}$ | $2.56^{+0.26}_{-0.22}$ | $3.78^{+0.13}_{-0.27}$ | $6090^{+440}_{-750}$ | $0.00^{+0.31}_{-2.30}$ | $2280^{+200}_{-170}$ | $0.0778^{+0.0053}_{-0.0120}$ | $83.3^{+1.6}_{-2.3}$ | $1690^{+120}_{-110}$ | $1.001^{+0.085}_{-0.080}$
OGLE-TR-1038 | $0.271^{+0.110}_{-0.073}$ | $2.66^{+0.19}_{-0.18}$ | $3.02^{+0.17}_{-0.15}$ | $4630^{+230}_{-220}$ | $-3.51^{+0.68}_{-0.35}$ | $1187^{+41}_{-40}$ | $0.0352^{+0.0031}_{-0.0028}$ | $84.5^{+3.9}_{-5.0}$ | $1936^{+100}_{-80}$ | $1.79^{+0.22}_{-0.39}$
OGLE-TR-1039 | $1.63^{+0.18}_{-0.24}$ | $2.12^{+0.21}_{-0.15}$ | $3.992^{+0.084}_{-0.130}$ | $6700^{+480}_{-430}$ | $0.08^{+0.22}_{-0.21}$ | $2320^{+220}_{-170}$ | $0.1017^{+0.0037}_{-0.0052}$ | $85.53^{+0.62}_{-0.91}$ | $1485^{+91}_{-78}$ | $1.167^{+0.150}_{-0.096}$
OGLE-TR-1040 | $1.00^{+0.25}_{-0.16}$ | $0.993^{+0.079}_{-0.068}$ | $4.450^{+0.100}_{-0.098}$ | $7370^{+1700}_{-810}$ | $-2.8^{+1.6}_{-1.2}$ | $2010^{+350}_{-270}$ | $0.1438^{+0.0110}_{-0.0081}$ | $89.08^{+0.40}_{-0.33}$ | $940^{+180}_{-110}$ | $1.058^{+0.093}_{-0.078}$
OGLE-TR-1041 | $1.06^{+0.21}_{-0.14}$ | $1.248^{+0.069}_{-0.061}$ | $4.279^{+0.035}_{-0.043}$ | $7190^{+790}_{-1100}$ | $-1.4^{+1.6}_{-2.1}$ | $1370^{+82}_{-76}$ | $0.0423^{+0.0025}_{-0.0018}$ | $88.73^{+0.88}_{-1.30}$ | $1880^{+200}_{-290}$ | $1.140^{+0.060}_{-0.054}$
OGLE-TR-1042 | $0.871^{+0.150}_{-0.092}$ | $1.546^{+0.086}_{-0.071}$ | $4.006^{+0.025}_{-0.026}$ | $5980^{+420}_{-460}$ | $-0.80^{+0.80}_{-1.90}$ | $1390^{+120}_{-100}$ | $0.0727^{+0.0039}_{-0.0027}$ | $89.33^{+0.47}_{-0.73}$ | $1327^{+94}_{-100}$ | $1.662^{+0.087}_{-0.073}$
OGLE-TR-1043 | $1.26^{+0.18}_{-0.17}$ | $1.86^{+0.43}_{-0.26}$ | $3.99^{+0.14}_{-0.16}$ | $5750^{+350}_{-380}$ | $0.24^{+0.17}_{-0.22}$ | $1670^{+320}_{-230}$ | $0.0361^{+0.0017}_{-0.0018}$ | $78.2^{+2.1}_{-1.7}$ | $1990^{+160}_{-130}$ | $1.003^{+0.093}_{-0.084}$
OGLE-TR-1044 | $1.010^{+0.070}_{-0.069}$ | $1.014^{+0.030}_{-0.029}$ | $4.431^{+0.030}_{-0.033}$ | $5580^{+130}_{-120}$ | $0.34^{+0.14}_{-0.16}$ | $804^{+22}_{-21}$ | $0.0589^{+0.0013}_{-0.0014}$ | $89.47^{+0.37}_{-0.53}$ | $1117^{+23}_{-23}$ | $2.015^{+0.066}_{-0.064}$
OGLE-TR-1045 | $0.797^{+0.074}_{-0.038}$ | $1.317^{+0.052}_{-0.041}$ | $4.106^{+0.025}_{-0.026}$ | $7000^{+370}_{-300}$ | $-4.18^{+0.99}_{-0.27}$ | $1810^{+190}_{-190}$ | $0.03010^{+0.00090}_{-0.00048}$ | $88.97^{+0.75}_{-1.10}$ | $2227^{+120}_{-91}$ | $2.228^{+0.082}_{-0.070}$
OGLE-TR-1046 | $0.993^{+0.097}_{-0.079}$ | $1.570^{+0.065}_{-0.064}$ | $4.044^{+0.026}_{-0.029}$ | $5560^{+380}_{-220}$ | $0.05^{+0.23}_{-0.25}$ | $1391^{+99}_{-84}$ | $0.0943^{+0.0030}_{-0.0026}$ | $89.47^{+0.37}_{-0.56}$ | $1094^{+74}_{-43}$ | $1.813^{+0.078}_{-0.071}$
OGLE-TR-1047 | $0.90^{+0.12}_{-0.18}$ | $1.347^{+0.081}_{-0.085}$ | $4.134^{+0.036}_{-0.064}$ | $5530^{+270}_{-250}$ | $-3.45^{+0.84}_{-0.38}$ | $1720^{+140}_{-140}$ | $0.0896^{+0.0038}_{-0.0064}$ | $89.17^{+0.58}_{-0.82}$ | $1039^{+52}_{-48}$ | $1.519^{+0.100}_{-0.099}$
OGLE-TR-1048 | $0.85^{+0.21}_{-0.31}$ | $1.15^{+0.16}_{-0.15}$ | $4.230^{+0.062}_{-0.100}$ | $5400^{+1100}_{-430}$ | $-2.5^{+1.8}_{-1.1}$ | $1530^{+240}_{-190}$ | $0.0573^{+0.0054}_{-0.0084}$ | $88.78^{+0.87}_{-1.40}$ | $1186^{+220}_{-97}$ | $1.47^{+0.22}_{-0.20}$
OGLE-TR-1049 | $0.71^{+0.47}_{-0.19}$ | $3.40^{+0.33}_{-0.25}$ | $3.22^{+0.22}_{-0.13}$ | $5290^{+280}_{-330}$ | $-2.63^{+1.20}_{-0.85}$ | $2440^{+230}_{-180}$ | $0.128^{+0.022}_{-0.012}$ | $88.1^{+1.3}_{-1.9}$ | $1306^{+77}_{-75}$ | $1.144^{+0.120}_{-0.083}$
OGLE-TR-1050 | $0.122^{+0.061}_{-0.017}$ | $0.953^{+0.069}_{-0.052}$ | $3.579^{+0.130}_{-0.059}$ | $4740^{+240}_{-200}$ | $-3.01^{+0.81}_{-0.65}$ | $962^{+100}_{-89}$ | $0.01415^{+0.00170}_{-0.00089}$ | $74.5^{+2.0}_{-1.5}$ | $1860^{+110}_{-110}$ | $1.152^{+0.093}_{-0.080}$
OGLE-TR-1051 | $0.946^{+0.120}_{-0.073}$ | $4.00^{+0.21}_{-0.15}$ | $3.210^{+0.031}_{-0.018}$ | $4770^{+140}_{-150}$ | $-0.20^{+0.23}_{-0.38}$ | $2880^{+220}_{-180}$ | $0.01956^{+0.00098}_{-0.00055}$ | $78.8^{+7.8}_{-12.0}$ | $3280^{+100}_{-110}$ | $1.407^{+0.100}_{-0.069}$
OGLE-TR-1052 | $1.01^{+0.57}_{-0.21}$ | $6.0^{+1.6}_{-1.9}$ | $2.88^{+0.47}_{-0.20}$ | $5360^{+320}_{-280}$ | $-2.5^{+2.3}_{-1.1}$ | $4900^{+1600}_{-1300}$ | $0.0765^{+0.0084}_{-0.0051}$ | $72.0^{+13.0}_{-6.2}$ | $2260^{+290}_{-400}$ | $2.44^{+0.76}_{-0.99}$
OGLE-TR-1053 | $1.11^{+0.41}_{-0.23}$ | $1.53^{+0.27}_{-0.24}$ | $4.128^{+0.110}_{-0.098}$ | $7250^{+650}_{-530}$ | $-1.10^{+0.86}_{-2.20}$ | $2030^{+360}_{-260}$ | $0.0493^{+0.0057}_{-0.0040}$ | $82.8^{+1.2}_{-1.1}$ | $1930^{+170}_{-130}$ | $1.57^{+0.47}_{-0.31}$
OGLE-TR-1054 | $1.55^{+0.34}_{-0.27}$ | $2.51^{+0.49}_{-0.30}$ | $3.80^{+0.16}_{-0.15}$ | $6060^{+940}_{-570}$ | $-1.5^{+1.7}_{-1.7}$ | $2670^{+360}_{-270}$ | $0.0961^{+0.0065}_{-0.0061}$ | $88.2^{+1.3}_{-2.4}$ | $1540^{+140}_{-110}$ | $1.22^{+0.41}_{-0.12}$
OGLE-TR-1055 | $0.97^{+0.21}_{-0.11}$ | $3.00^{+0.33}_{-0.25}$ | $3.477^{+0.093}_{-0.100}$ | $5090^{+230}_{-190}$ | $-0.46^{+0.23}_{-0.48}$ | $1830^{+260}_{-200}$ | $0.0323^{+0.0021}_{-0.0013}$ | $72.5^{+4.0}_{-4.3}$ | $2370^{+180}_{-130}$ | $1.067^{+0.110}_{-0.089}$
OGLE-TR-1056 | $1.071^{+0.110}_{-0.066}$ | $2.55^{+0.48}_{-0.38}$ | $3.66^{+0.15}_{-0.13}$ | $4690^{+160}_{-150}$ | $0.41^{+0.13}_{-0.20}$ | $1690^{+310}_{-220}$ | $0.0791^{+0.0024}_{-0.0018}$ | $82.3^{+1.2}_{-1.3}$ | $1281^{+110}_{-99}$ | $1.048^{+0.085}_{-0.078}$
OGLE-TR-1057 | $0.782^{+0.029}_{-0.014}$ | $3.67^{+0.10}_{-0.10}$ | $3.206^{+0.024}_{-0.023}$ | $5590^{+220}_{-240}$ | $-2.71^{+1.00}_{-0.91}$ | $5400^{+1400}_{-1300}$ | $0.05857^{+0.00071}_{-0.00034}$ | $88.86^{+0.80}_{-1.20}$ | $2130^{+89}_{-95}$ | $2.498^{+0.084}_{-0.084}$
OGLE-TR-1058 | $1.82^{+0.16}_{-0.17}$ | $2.62^{+0.36}_{-0.23}$ | $3.854^{+0.082}_{-0.110}$ | $6640^{+450}_{-360}$ | $0.26^{+0.14}_{-0.20}$ | $2460^{+280}_{-200}$ | $0.1615^{+0.0052}_{-0.0051}$ | $88.5^{+1.0}_{-1.1}$ | $1299^{+81}_{-69}$ | $1.171^{+0.170}_{-0.089}$
OGLE-TR-1059 | $1.02^{+0.31}_{-0.19}$ | $1.48^{+0.13}_{-0.11}$ | $4.11^{+0.12}_{-0.10}$ | $6820^{+850}_{-610}$ | $-1.4^{+1.4}_{-2.0}$ | $1590^{+130}_{-110}$ | $0.0741^{+0.0068}_{-0.0049}$ | $88.3^{+1.1}_{-1.1}$ | $1490.00^{+0.37}_{-0.19}$ | $1.152^{+0.096}_{-0.077}$
OGLE-TR-1060 | $1.116^{+0.200}_{-0.089}$ | $1.532^{+0.096}_{-0.093}$ | $4.127^{+0.070}_{-0.073}$ | $6190^{+560}_{-490}$ | $-3.29^{+3.50}_{-0.53}$ | $1810^{+140}_{-130}$ | $0.1113^{+0.0064}_{-0.0030}$ | $88.52^{+0.85}_{-0.64}$ | $1100^{+91}_{-64}$ | $1.83^{+0.14}_{-0.12}$
OGLE-TR-1061 | $1.79^{+0.24}_{-0.58}$ | $1.805^{+0.086}_{-0.170}$ | $4.173^{+0.031}_{-0.069}$ | $8510^{+1100}_{-520}$ | $-0.15^{+0.44}_{-2.90}$ | $2090^{+140}_{-150}$ | $0.0455^{+0.0020}_{-0.0056}$ | $88.3^{+1.2}_{-1.8}$ | $2600^{+340}_{-160}$ | $1.678^{+0.081}_{-0.160}$
OGLE-TR-1062 | $1.01^{+0.14}_{-0.16}$ | $1.70^{+0.16}_{-0.16}$ | $3.981^{+0.110}_{-0.096}$ | $6870^{+650}_{-900}$ | $-1.6^{+1.5}_{-2.2}$ | $1960^{+550}_{-350}$ | $0.1289^{+0.0052}_{-0.0078}$ | $89.07^{+0.64}_{-0.59}$ | $1220^{+140}_{-180}$ | $1.102^{+0.061}_{-0.068}$
OGLE-TR-1063 | $1.12^{+0.40}_{-0.13}$ | $1.382^{+0.120}_{-0.082}$ | $4.233^{+0.059}_{-0.076}$ | $8290^{+440}_{-490}$ | $-1.9^{+1.4}_{-1.6}$ | $1527^{+89}_{-77}$ | $0.0476^{+0.0051}_{-0.0019}$ | $87.6^{+1.5}_{-1.5}$ | $2137^{+99}_{-110}$ | $1.392^{+0.130}_{-0.090}$
OGLE-TR-1064 | $1.09^{+0.27}_{-0.50}$ | $1.87^{+0.14}_{-0.13}$ | $3.92^{+0.11}_{-0.24}$ | $5240^{+430}_{-310}$ | $-1.22^{+0.76}_{-0.96}$ | $2300^{+220}_{-200}$ | $0.0156^{+0.0012}_{-0.0028}$ | $61.9^{+5.7}_{-11.0}$ | $2850^{+200}_{-200}$ | $1.045^{+0.130}_{-0.097}$
OGLE-TR-1065 | $0.93^{+0.36}_{-0.26}$ | $1.87^{+0.12}_{-0.14}$ | $3.83^{+0.19}_{-0.12}$ | $4270^{+240}_{-220}$ | $0.25^{+0.24}_{-0.38}$ | $1270^{+310}_{-140}$ | $0.0564^{+0.0064}_{-0.0056}$ | $83.8^{+1.4}_{-1.3}$ | $1184^{+62}_{-52}$ | $1.024^{+0.058}_{-0.092}$
OGLE-TR-1066 | $0.881^{+0.220}_{-0.088}$ | $3.70^{+1.40}_{-0.77}$ | $3.28^{+0.15}_{-0.25}$ | $5430^{+370}_{-400}$ | $-1.7^{+1.2}_{-1.6}$ | $4540^{+1600}_{-880}$ | $0.0917^{+0.0075}_{-0.0062}$ | $86.8^{+2.4}_{-6.6}$ | $1670^{+210}_{-150}$ | $1.68^{+0.75}_{-0.39}$
OGLE-TR-1067 | $1.25^{+0.24}_{-0.19}$ | $5.52^{+0.61}_{-0.75}$ | $3.051^{+0.140}_{-0.099}$ | $4620^{+140}_{-140}$ | $0.36^{+0.16}_{-0.20}$ | $2800^{+320}_{-360}$ | $0.0417^{+0.0023}_{-0.0018}$ | $56.0^{+7.1}_{-5.1}$ | $2550^{+130}_{-160}$ | $2.51^{+0.44}_{-0.49}$
OGLE-TR-1068 | $1.67^{+0.14}_{-0.15}$ | $2.27^{+0.27}_{-0.43}$ | $3.944^{+0.160}_{-0.089}$ | $6820^{+360}_{-310}$ | $0.09^{+0.19}_{-0.14}$ | $1430^{+180}_{-200}$ | $0.01856^{+0.00069}_{-0.00074}$ | $58.6^{+7.2}_{-6.1}$ | $3600^{+180}_{-190}$ | $1.74^{+0.86}_{-0.44}$
OGLE-TR-1069 | $0.7726^{+0.0190}_{-0.0089}$ | $2.506^{+0.037}_{-0.034}$ | $3.530^{+0.011}_{-0.011}$ | $5950^{+230}_{-260}$ | $-2.96^{+0.97}_{-0.83}$ | $3010^{+170}_{-160}$ | $0.08670^{+0.00071}_{-0.00033}$ | $89.62^{+0.27}_{-0.42}$ | $1541^{+58}_{-67}$ | $3.053^{+0.044}_{-0.041}$
OGLE-TR-1070 | $0.91^{+0.12}_{-0.15}$ | $1.086^{+0.055}_{-0.060}$ | $4.321^{+0.027}_{-0.027}$ | $5970^{+790}_{-430}$ | $-0.13^{+0.36}_{-3.60}$ | $1680^{+120}_{-100}$ | $0.0274^{+0.0011}_{-0.0015}$ | $88.83^{+0.83}_{-1.30}$ | $1820^{+240}_{-130}$ | $1.259^{+0.063}_{-0.061}$
OGLE-TR-1071 | $1.36^{+0.74}_{-0.49}$ | $7.7^{+1.9}_{-1.8}$ | $2.81^{+0.17}_{-0.17}$ | $4330^{+170}_{-170}$ | $0.42^{+0.13}_{-0.24}$ | $5500^{+1500}_{-1300}$ | $0.0644^{+0.0097}_{-0.0079}$ | $57.8^{+7.6}_{-6.1}$ | $2270^{+180}_{-200}$ | $5.5^{+3.3}_{-2.0}$
OGLE-TR-1072 | $0.97^{+0.16}_{-0.16}$ | $1.140^{+0.068}_{-0.066}$ | $4.311^{+0.075}_{-0.073}$ | $6180^{+530}_{-370}$ | $-0.28^{+0.37}_{-2.00}$ | $1491^{+96}_{-85}$ | $0.0271^{+0.0014}_{-0.0015}$ | $84.4^{+1.8}_{-1.5}$ | $1930^{+180}_{-130}$ | $0.996^{+0.068}_{-0.065}$
OGLE-TR-1073 | $1.34^{+0.54}_{-0.49}$ | $3.26^{+0.82}_{-0.36}$ | $3.51^{+0.16}_{-0.30}$ | $4550^{+170}_{-230}$ | $0.34^{+0.18}_{-0.29}$ | $2240^{+570}_{-300}$ | $0.0795^{+0.0093}_{-0.0110}$ | $84.9^{+3.4}_{-6.3}$ | $1422^{+170}_{-85}$ | $1.110^{+0.310}_{-0.092}$
OGLE-TR-1074 | $1.56^{+0.28}_{-0.25}$ | $2.31^{+0.38}_{-0.24}$ | $3.88^{+0.13}_{-0.12}$ | $6180^{+690}_{-540}$ | $-0.7^{+1.1}_{-2.6}$ | $2860^{+320}_{-290}$ | $0.01868^{+0.00097}_{-0.00130}$ | $56.2^{+5.8}_{-7.8}$ | $3350^{+270}_{-220}$ | $1.29^{+1.10}_{-0.19}$
OGLE-TR-1075 | $0.790^{+0.050}_{-0.026}$ | $1.578^{+0.079}_{-0.058}$ | $3.946^{+0.033}_{-0.043}$ | $6680^{+290}_{-250}$ | $-4.14^{+0.54}_{-0.12}$ | $2250^{+130}_{-120}$ | $0.1768^{+0.0036}_{-0.0020}$ | $89.47^{+0.36}_{-0.42}$ | $962^{+41}_{-37}$ | $1.931^{+0.110}_{-0.073}$
OGLE-TR-1076 | $0.63^{+0.13}_{-0.10}$ | $1.625^{+0.093}_{-0.084}$ | $3.819^{+0.044}_{-0.054}$ | $5380^{+180}_{-230}$ | $-3.45^{+0.80}_{-0.38}$ | $1730^{+120}_{-110}$ | $0.0540^{+0.0035}_{-0.0031}$ | $88.73^{+0.90}_{-1.30}$ | $1420^{+51}_{-60}$ | $1.92^{+0.11}_{-0.10}$
OGLE-TR-1077 | $1.36^{+0.18}_{-0.32}$ | $1.67^{+0.15}_{-0.13}$ | $4.116^{+0.092}_{-0.140}$ | $6370^{+430}_{-420}$ | $0.04^{+0.24}_{-0.21}$ | $1860^{+160}_{-140}$ | $0.1296^{+0.0054}_{-0.0110}$ | $88.13^{+0.90}_{-0.72}$ | $1105^{+74}_{-57}$ | $1.027^{+0.078}_{-0.072}$
OGLE-TR-1078 | $0.94^{+0.48}_{-0.19}$ | $1.67^{+0.20}_{-0.11}$ | $3.973^{+0.060}_{-0.056}$ | $5510^{+250}_{-220}$ | $-3.12^{+3.00}_{-0.64}$ | $1850^{+240}_{-140}$ | $0.0510^{+0.0075}_{-0.0037}$ | $88.73^{+0.88}_{-1.50}$ | $1521^{+67}_{-60}$ | $1.397^{+0.160}_{-0.090}$
OGLE-TR-1079 | $0.46^{+0.36}_{-0.15}$ | $2.95^{+1.10}_{-0.60}$ | $3.17^{+0.25}_{-0.30}$ | $4280^{+250}_{-270}$ | $-0.56^{+0.46}_{-0.90}$ | $2050^{+780}_{-400}$ | $0.093^{+0.017}_{-0.012}$ | $85.1^{+3.4}_{-4.1}$ | $1170^{+150}_{-110}$ | $1.56^{+0.86}_{-0.43}$
OGLE-TR-1080 | $1.599^{+0.130}_{-0.073}$ | $2.057^{+0.120}_{-0.077}$ | $4.018^{+0.025}_{-0.036}$ | $6230^{+320}_{-300}$ | $0.40^{+0.14}_{-0.22}$ | $2340^{+180}_{-140}$ | $0.06480^{+0.00170}_{-0.00098}$ | $88.4^{+1.1}_{-1.5}$ | $1697^{+85}_{-81}$ | $1.334^{+0.083}_{-0.054}$
OGLE-TR-1081 | $1.21^{+0.12}_{-0.15}$ | $1.397^{+0.087}_{-0.081}$ | $4.227^{+0.068}_{-0.075}$ | $5960^{+270}_{-250}$ | $0.25^{+0.18}_{-0.20}$ | $1880^{+130}_{-110}$ | $0.0727^{+0.0024}_{-0.0031}$ | $87.38^{+0.78}_{-0.72}$ | $1261^{+51}_{-46}$ | $1.059^{+0.078}_{-0.071}$
OGLE-TR-1082 | $1.034^{+0.074}_{-0.051}$ | $3.15^{+0.13}_{-0.13}$ | $3.459^{+0.032}_{-0.031}$ | $4550^{+140}_{-110}$ | $0.38^{+0.16}_{-0.30}$ | $2560^{+210}_{-160}$ | $0.04479^{+0.00100}_{-0.00076}$ | $88.0^{+1.4}_{-2.1}$ | $1838^{+63}_{-53}$ | $1.877^{+0.081}_{-0.077}$
OGLE-TR-1083 | $1.067^{+0.090}_{-0.093}$ | $1.112^{+0.062}_{-0.055}$ | $4.375^{+0.051}_{-0.058}$ | $5670^{+190}_{-180}$ | $0.33^{+0.14}_{-0.18}$ | $1468^{+87}_{-78}$ | $0.0624^{+0.0017}_{-0.0019}$ | $87.62^{+0.70}_{-0.60}$ | $1155^{+44}_{-40}$ | $1.084^{+0.077}_{-0.068}$
OGLE-TR-1084 | $1.231^{+0.076}_{-0.097}$ | $1.257^{+0.066}_{-0.063}$ | $4.330^{+0.041}_{-0.053}$ | $6200^{+180}_{-180}$ | $0.23^{+0.18}_{-0.17}$ | $1320^{+57}_{-52}$ | $0.2445^{+0.0049}_{-0.0066}$ | $89.10^{+0.11}_{-0.12}$ | $677^{+20}_{-19}$ | $1.526^{+0.100}_{-0.095}$
OGLE-TR-1085 | $0.924^{+0.042}_{-0.400}$ | $1.71^{+0.23}_{-0.15}$ | $3.938^{+0.079}_{-0.370}$ | $5220^{+150}_{-350}$ | $-0.19^{+0.15}_{-2.50}$ | $1610^{+130}_{-130}$ | $0.04551^{+0.00091}_{-0.00730}$ | $81.49^{+0.56}_{-3.70}$ | $1573^{+96}_{-130}$ | $0.942^{+0.076}_{-0.044}$
OGLE-TR-1086 | $1.004^{+0.120}_{-0.090}$ | $2.07^{+1.70}_{-0.47}$ | $3.81^{+0.22}_{-0.51}$ | $5010^{+210}_{-200}$ | $0.00^{+0.38}_{-0.45}$ | $1710^{+1200}_{-350}$ | $0.0720^{+0.0058}_{-0.0023}$ | $84.5^{+3.0}_{-6.8}$ | $1310^{+340}_{-140}$ | $1.42^{+1.90}_{-0.38}$
OGLE-TR-1087 | $1.21^{+0.24}_{-0.25}$ | $2.27^{+0.43}_{-0.66}$ | $3.83^{+0.26}_{-0.19}$ | $5640^{+860}_{-730}$ | $0.17^{+0.26}_{-1.00}$ | $2400^{+410}_{-430}$ | $0.0565^{+0.0033}_{-0.0041}$ | $82.6^{+4.8}_{-2.8}$ | $1660^{+190}_{-120}$ | $1.79^{+0.44}_{-0.59}$
OGLE-TR-1088 | $0.860^{+0.064}_{-0.084}$ | $0.972^{+0.030}_{-0.035}$ | $4.398^{+0.019}_{-0.022}$ | $5670^{+620}_{-230}$ | $-0.17^{+0.17}_{-1.60}$ | $954^{+33}_{-31}$ | $0.0553^{+0.0014}_{-0.0017}$ | $89.40^{+0.42}_{-0.58}$ | $1145^{+120}_{-46}$ | $1.187^{+0.040}_{-0.037}$
OGLE-TR-1089 | $1.259^{+0.089}_{-0.100}$ | $1.294^{+0.087}_{-0.086}$ | $4.317^{+0.049}_{-0.059}$ | $6050^{+240}_{-240}$ | $0.434^{+0.092}_{-0.160}$ | $1480^{+110}_{-110}$ | $0.2910^{+0.0067}_{-0.0080}$ | $89.42^{+0.21}_{-0.16}$ | $614^{+29}_{-27}$ | $1.72^{+0.13}_{-0.14}$
OGLE-TR-1090 | $1.38^{+0.16}_{-0.26}$ | $1.83^{+0.25}_{-0.11}$ | $4.044^{+0.072}_{-0.150}$ | $6490^{+340}_{-320}$ | $-0.12^{+0.16}_{-0.47}$ | $2130^{+180}_{-140}$ | $0.0771^{+0.0031}_{-0.0048}$ | $87.7^{+1.5}_{-2.0}$ | $1548^{+85}_{-66}$ | $1.283^{+0.230}_{-0.091}$
OGLE-TR-1091 | $0.146^{+0.100}_{-0.036}$ | $0.971^{+0.082}_{-0.069}$ | $3.63^{+0.22}_{-0.13}$ | $3670^{+170}_{-100}$ | $-1.40^{+0.67}_{-1.00}$ | $620^{+65}_{-53}$ | $0.164^{+0.026}_{-0.016}$ | $88.92^{+0.37}_{-0.29}$ | $431^{+34}_{-32}$ | $1.073^{+0.100}_{-0.088}$
OGLE-TR-1092 | $1.16^{+0.14}_{-0.16}$ | $2.59^{+0.17}_{-0.30}$ | $3.707^{+0.086}_{-0.140}$ | $4804^{+250}_{-83}$ | $0.20^{+0.20}_{-0.26}$ | $2292^{+500}_{-15}$ | $0.0493^{+0.0024}_{-0.0028}$ | $78.8^{+2.3}_{-1.0}$ | $1690^{+78}_{-51}$ | $1.043^{+0.170}_{-0.046}$
OGLE-TR-1093 | $1.59^{+0.26}_{-0.18}$ | $3.61^{+0.32}_{-0.29}$ | $3.518^{+0.110}_{-0.079}$ | $5220^{+590}_{-290}$ | $0.17^{+0.27}_{-0.45}$ | $2710^{+480}_{-260}$ | $0.0317^{+0.0014}_{-0.0011}$ | $57.4^{+3.4}_{-3.5}$ | $2700^{+220}_{-120}$ | $3.82^{+0.92}_{-1.10}$
OGLE-TR-1094 | $1.005^{+0.042}_{-0.053}$ | $1.65^{+0.17}_{-0.22}$ | $4.005^{+0.120}_{-0.087}$ | $4990^{+170}_{-160}$ | $0.35^{+0.14}_{-0.35}$ | $1450^{+130}_{-140}$ | $0.1095^{+0.0015}_{-0.0019}$ | $89.19^{+0.58}_{-0.88}$ | $930^{+43}_{-45}$ | $1.62^{+0.16}_{-0.21}$
OGLE-TR-1095 | $1.83^{+4.40}_{-0.89}$ | $2.04^{+0.21}_{-0.18}$ | $4.11^{+0.46}_{-0.29}$ | $9500^{+17000}_{-3100}$ | $-1.8^{+1.6}_{-1.7}$ | $5500^{+5900}_{-2100}$ | $0.0205^{+0.0100}_{-0.0040}$ | $69.9^{+14.0}_{-9.9}$ | $4600^{+6000}_{-1200}$ | $1.062^{+0.110}_{-0.092}$
OGLE-TR-1096 | $0.968^{+0.060}_{-0.110}$ | $3.51^{+0.12}_{-0.15}$ | $3.328^{+0.023}_{-0.023}$ | $4560^{+220}_{-120}$ | $0.05^{+0.34}_{-0.62}$ | $2880^{+230}_{-150}$ | $0.04410^{+0.00090}_{-0.00170}$ | $88.4^{+1.1}_{-1.7}$ | $1967^{+95}_{-56}$ | $2.446^{+0.080}_{-0.089}$
OGLE-TR-1097 | $0.873^{+0.140}_{-0.089}$ | $0.874^{+0.074}_{-0.072}$ | $4.514^{+0.056}_{-0.064}$ | $6200^{+1200}_{-1400}$ | $-1.0^{+1.3}_{-2.5}$ | $1280^{+840}_{-580}$ | $0.0926^{+0.0046}_{-0.0032}$ | $88.08^{+0.22}_{-0.24}$ | $920^{+190}_{-220}$ | $1.017^{+0.096}_{-0.093}$
OGLE-TR-1098 | $1.09^{+0.15}_{-0.16}$ | $1.272^{+0.079}_{-0.082}$ | $4.262^{+0.066}_{-0.072}$ | $5960^{+470}_{-290}$ | $0.16^{+0.25}_{-0.54}$ | $2070^{+160}_{-150}$ | $0.0656^{+0.0029}_{-0.0035}$ | $86.06^{+0.46}_{-0.45}$ | $1264^{+110}_{-64}$ | $1.76^{+0.13}_{-0.14}$
OGLE-TR-1099 | $1.01^{+0.81}_{-0.40}$ | $8.1^{+2.2}_{-1.8}$ | $2.63^{+0.23}_{-0.20}$ | $4460^{+180}_{-200}$ | $-0.26^{+0.18}_{-0.47}$ | $5500^{+1700}_{-1300}$ | $0.107^{+0.017}_{-0.015}$ | $70.9^{+3.8}_{-4.1}$ | $1870^{+170}_{-150}$ | $4.2^{+2.0}_{-1.1}$

## References

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