Index of /ogle/ogle4/OCVS/blg/transits
(M. Mróz, 2023)
================================================================================
Candidates for Transiting Planets in OGLE-IV Galactic Bulge Fields
M. Mróz, P. Pietrukowicz, R. Poleski, A. Udalski, M.K. Szymański,
M. Gromadzki, K. Ulaczyk, S. Kozłowski, J. Skowron, D.M. Skowron,
I. Soszyński, P. Mróz, M. Ratajczak, K.A. Rybicki, P. Iwanek, M. Wrona
=bibcode????????
================================================================================
Keywords: exoplanets, transits, OGLE
Abstract:
This directory contains the OGLE-IV catalog of candidates for transiting
planets toward the Galactic bulge.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . this file
ident.dat 87 99 identification of stars
transits.dat 72 99 basic parameters of systems with transiting planetary candidates
model.dat 1410 99 EXOFASTv2 planetary transit models parameters (median values and errors)
transits_all.csv . 99 CSV file with all the parameters of systems with transiting planetary candidates
phot_ogle4/I/ . . I-band OGLE-IV photometry of individual stars (2010-2019)
phot_ogle4/V/ . . V-band OGLE-IV photometry of individual stars (2010-2019)
phot_ogle4.tar.gz . . gzipped phot_ogle4/ directory
fcharts/ . . finding charts of individual stars
model/ls . . postscript plots of folded light curve of transits with fitted EXOFASTv2 model (top panel) and residuals (bottom panel) of individual stars
model/covar . . postscript plots of covariances of EXOFASTv2 model parameters
model/median . . CSV files of individual system with median values and 68% confidence intervals of EXOFASTv2 model parameters
model/pdf . . PDF files of individual system with median values and 68% confidence intervals of EXOFASTv2 model parameters
paper.pdf . . PDF version of the paper Mróz et al. (2023),
??? describing the collection.
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Byte-by-byte Description of file: ident.dat
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Bytes Format Units Label Explanations
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1-12 A12 --- ID Identifier (1)
14-15 I2 h RAh Right ascension (hour)
17-18 I2 min RAm Right ascension (minute)
20-24 F5.2 s RAs Right ascension (seconds)
26-26 A1 --- DE- Declination (degree)
27-28 I2 deg DEd Declination (degree)
30-31 I2 arcmin DEm Declination (minute)
33-36 F4.1 arcsec DEs Declination (seconds)
38-53 A16 --- ID_OGLE_IV OGLE-IV identifier
55-69 A15 --- ID_OGLE_III OGLE-III identifier
71-85 A15 --- ID_OGLE_II OGLE-II identifier
87-87 A1 --- ID_OTHER Other identifiers
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Note (1): In the format OGLE-TR-NNNN, where NNNN is a 4-digit number.
Byte-by-byte Description of file: transits.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1-12 A12 --- ID Identifier (1)
14-19 F6.3 mag Imag [12.8/15.5] Intensity mean I-band magnitude
21-26 F6.3 mag Vmag [13.35/17.42] Intensity mean V-band magnitude
28-38 F11.8 d Period_0 [0.67/63.23] Orbital period (from the EXOFASTv2
model with minimal chi2)
40-45 F6.5 BJD_TDB-2450000 tc_0 [5261.03/5503.97] Time of inferior
conjunction (transit) (from the EXOFASTv2 model
with minimal chi2) (2)
47-52 F6.4 d t14_0 [0.07/0.74] Duration of transit from 1st contact
to 4th contact (from the EXOFASTv2 model with
minimal chi2) (2)
54-61 F8.6 --- delta_0 [0.0/0.05] Transit depth (Rp/Rstar)^2 (from the
EXOFASTv2 model with minimal chi2) (2)
63-67 F5.3 --- pr_pl [0.8/1.0] Probability(planet|signal) base on
VESPA (3)
69-72 F4.2 --- SNR [6.24/96.28] signal-to-noise ratio
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Note (1): In the format OGLE-TR-NNNN, where NNNN is a 4-digit number.
Note (2): For detailed parameter definition see Eastman et al. (2019)
Note (3): For detailed parameter definition see Morton (2012)
Byte-by-byte Description of file: model.dat
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Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 12 A12 --- ID Identifier (1)
14- 19 F6.4 solMass mstar_0 [0.12/4.2] Stellar mass (2)
21- 25 F5.3 solMass E_mstar_0 [0.01/4.41] upper error : The
84th-50th percentile of parameter
distribution in mstar_0
27- 31 F5.3 solMass e_mstar_0 [0.0/1.0] lower error : The
50th-16th percentile of parameter
distribution in mstar_0
33- 37 F5.3 solRad rstar_0 [0.86/8.1] Stellar radius (2)
39- 43 F5.3 solRad E_rstar_0 [0.02/2.21] upper error : The
84th-50th percentile of parameter
distribution in rstar_0
45- 49 F5.3 solRad e_rstar_0 [0.02/1.9] lower error : The
50th-16th percentile of parameter
distribution in rstar_0
51- 55 F5.3 solRad rstarsed_0 [0.37/8.4] Stellar radius base on
SED model (2)
57- 61 F5.3 solRad E_rstarsed_0 [0.02/2.5] upper error : The
84th-50th percentile of parameter
distribution in rstarsed_0
63- 67 F5.3 solRad e_rstarsed_0 [0.01/1.9] lower error : The
50th-16th percentile of parameter
distribution in rstarsed_0
69- 75 F7.3 solLum lstar_0 [0.13/940.0] Stellar luminosity (2)
77- 84 F8.3 solLum E_lstar_0 [0.03/1900.0] upper error : The
84th-50th percentile of parameter
distribution in lstar_0
86- 92 F7.3 solLum e_lstar_0 [0.02/350.0] lower error : The
50th-16th percentile of parameter
distribution in lstar_0
94- 102 E9.4 erg/s/cm2 fbol_0 [0.0/0.01] Stellar bolometric
flux (2)
104- 110 E7.2 erg/s/cm2 E_fbol_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in fbol_0
112- 118 E7.2 erg/s/cm2 e_fbol_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in fbol_0
120- 126 F7.5 g/cm3 rhostar_0 [0.0/1.91] Stellar density (2)
128- 133 F6.4 g/cm3 E_rhostar_0 [0.0/1.11] upper error : The
84th-50th percentile of parameter
distribution in rhostar_0
135- 141 F7.5 g/cm3 e_rhostar_0 [0.0/0.82] lower error : The
50th-16th percentile of parameter
distribution in rhostar_0
143- 147 F5.3 cgs logg_0 [2.63/4.52] Stellar surface gravity
(2)
149- 153 F5.3 cgs E_logg_0 [0.01/0.5] upper error : The
84th-50th percentile of parameter
distribution in logg_0
155- 159 F5.3 cgs e_logg_0 [0.01/0.51] lower error : The
50th-16th percentile of parameter
distribution in logg_0
161- 167 F7.1 K teff_0 [3670.0/21600.0] Stellar effective
temperature (2)
169- 175 F7.1 K E_teff_0 [130.0/17000.0] upper error : The
84th-50th percentile of parameter
distribution in teff_0
177- 182 F6.1 K e_teff_0 [83.0/5100.0] lower error : The
50th-16th percentile of parameter
distribution in teff_0
184- 190 F7.1 K teffsed_0 [3635.0/21200.0] Stellar effective
temperature based on SED model (2)
192- 198 F7.1 K E_teffsed_0 [120.0/17000.0] upper error : The
84th-50th percentile of parameter
distribution in teffsed_0
200- 205 F6.1 K e_teffsed_0 [72.0/5200.0] lower error : The
50th-16th percentile of parameter
distribution in teffsed_0
207- 212 F6.3 dex feh_0 [-4.49/0.45] Current metalicity,
[Fe/H] (2)
214- 218 F5.3 dex E_feh_0 [0.08/3.5] upper error : The
84th-50th percentile of parameter
distribution in feh_0
220- 224 F5.3 dex e_feh_0 [0.05/3.6] lower error : The
50th-16th percentile of parameter
distribution in feh_0
226- 232 E7.2 Gyr age_0 [0.0/13.2] Age of star (2)
234- 240 E7.2 Gyr E_age_0 [0.0/12.0] upper error : The
84th-50th percentile of parameter
distribution in age_0
242- 248 E7.2 Gyr e_age_0 [0.0/12.0] lower error : The
50th-16th percentile of parameter
distribution in age_0
250- 254 F5.1 --- eep_0 [43.0/506.0] Equivalent
evolutionary point; fitted for MIST
models only (see http://waps.cfa.harv
ard.edu/MIST/README_tables.pdf) (2)
256- 260 F5.1 --- E_eep_0 [1.9/150.0] upper error : The
84th-50th percentile of parameter
distribution in eep_0
262- 266 F5.1 --- e_eep_0 [1.7/360.0] lower error : The
50th-16th percentile of parameter
distribution in eep_0
268- 274 F7.4 --- logmstar_0 [-0.92/0.63] Log10 mstar/msun (2)
276- 280 F5.3 --- E_logmstar_0 [0.01/0.57] upper error : The
84th-50th percentile of parameter
distribution in logmstar_0
282- 287 F6.4 --- e_logmstar_0 [0.0/0.52] lower error : The
50th-16th percentile of parameter
distribution in logmstar_0
289- 293 F5.3 mag Av_0 [0.19/4.76] V-band extinction;
fitted for SED models only (2)
295- 299 F5.3 mag E_Av_0 [0.02/1.11] upper error : The
84th-50th percentile of parameter
distribution in Av_0
301- 305 F5.3 mag e_Av_0 [0.07/1.2] lower error : The
50th-16th percentile of parameter
distribution in Av_0
307- 311 F5.2 --- errscale_0 [2.6/81.0] Error scaling for the
SED model; fitted parameter if SED
fit (2)
313- 317 F5.2 --- E_errscale_0 [0.93/42.0] upper error : The
84th-50th percentile of parameter
distribution in errscale_0
319- 323 F5.2 --- e_errscale_0 [0.75/36.0] lower error : The
50th-16th percentile of parameter
distribution in errscale_0
325- 330 F6.4 mas parallax_0 [0.18/2.44] Parallax (2)
332- 337 F6.4 mas E_parallax_0 [0.0/0.59] upper error : The
84th-50th percentile of parameter
distribution in parallax_0
339- 343 F5.3 mas e_parallax_0 [0.01/0.29] lower error : The
50th-16th percentile of parameter
distribution in parallax_0
345- 350 F6.1 pc distance_0 [411.0/5500.0] Distance to the star
(2)
352- 357 F6.1 pc E_distance_0 [22.0/5900.0] upper error : The
84th-50th percentile of parameter
distribution in distance_0
359- 364 F6.1 pc e_distance_0 [15.0/2100.0] lower error : The
50th-16th percentile of parameter
distribution in distance_0
366- 376 F11.8 d Period_0 [0.67/63.23] Orbital period (2)
378- 384 E7.2 d E_Period_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in Period_0
386- 392 E7.2 d e_Period_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in Period_0
394- 398 F5.3 R_jupiter rp_0 [0.56/5.5] Planetary radius (2)
400- 404 F5.3 R_jupiter E_rp_0 [0.03/3.3] upper error : The
84th-50th percentile of parameter
distribution in rp_0
406- 410 F5.3 R_jupiter e_rp_0 [0.03/2.0] lower error : The
50th-16th percentile of parameter
distribution in rp_0
412- 419 F8.4 M_jupiter mp_0 [0.12/580.0] Planet mass,
quantity is derived from the Chen &
Kipping (2017) exoplanet mass-radius
relations (2)
421- 428 F8.4 M_jupiter E_mp_0 [0.0/410.0] upper error : The
84th-50th percentile of parameter
distribution in mp_0
430- 437 F8.4 M_jupiter e_mp_0 [0.0/230.0] lower error : The
50th-16th percentile of parameter
distribution in mp_0
439- 447 F9.7 solMass mpsun_0 [0.0/0.56] Planet mass (2)
449- 455 E7.2 solMass E_mpsun_0 [0.0/0.39] upper error : The
84th-50th percentile of parameter
distribution in mpsun_0
457- 463 E7.2 solMass e_mpsun_0 [0.0/0.22] lower error : The
50th-16th percentile of parameter
distribution in mpsun_0
465- 477 F13.5 BJD_TDB tc_0 [2455261.03/2455503.97] Time of
inferior conjunction (transit) (2)
479- 485 F7.5 BJD_TDB E_tc_0 [0.0/2.8] upper error : The
84th-50th percentile of parameter
distribution in tc_0
487- 493 F7.5 BJD_TDB e_tc_0 [0.0/1.11] lower error : The
50th-16th percentile of parameter
distribution in tc_0
495- 507 F13.5 BJD_TDB t0_0 [2455373.67/2457369.05] Optimal
conjunction Time (2)
509- 515 F7.5 BJD_TDB E_t0_0 [0.0/1.7] upper error : The
84th-50th percentile of parameter
distribution in t0_0
517- 523 F7.5 BJD_TDB e_t0_0 [0.0/2.1] lower error : The
50th-16th percentile of parameter
distribution in t0_0
525- 531 F7.5 AU a_0 [0.01/0.34] Semi-major axis (2)
533- 539 F7.5 AU E_a_0 [0.0/0.03] upper error : The
84th-50th percentile of parameter
distribution in a_0
541- 547 F7.5 AU e_a_0 [0.0/0.05] lower error : The
50th-16th percentile of parameter
distribution in a_0
549- 554 F6.3 degrees ideg_0 [56.0/89.86] Planetary inclination
(2)
556- 561 F6.3 degrees E_ideg_0 [0.06/14.0] upper error : The
84th-50th percentile of parameter
distribution in ideg_0
563- 568 F6.3 degrees e_ideg_0 [0.06/12.0] lower error : The
50th-16th percentile of parameter
distribution in ideg_0
570- 575 F6.1 K teq_0 [403.0/4600.0] Planetary
equilibrium temperature, assuming no
albedo, perfect redistribution (2)
577- 582 F6.1 K E_teq_0 [20.0/6000.0] upper error : The
84th-50th percentile of parameter
distribution in teq_0
584- 589 F6.1 K e_teq_0 [19.0/1200.0] lower error : The
50th-16th percentile of parameter
distribution in teq_0
591- 597 E7.2 Gyr tcirc_0 [0.0/2200000.0] Tidal
circularization timescale (2)
599- 605 E7.2 Gyr E_tcirc_0 [0.0/5100000.0] upper error : The
84th-50th percentile of parameter
distribution in tcirc_0
607- 613 E7.2 Gyr e_tcirc_0 [0.0/2000000.0] lower error : The
50th-16th percentile of parameter
distribution in tcirc_0
615- 622 F8.2 m/s k_0 [10.21/38000.0] RV semi-amplitude,
quantity is derived from the Chen &
Kipping (2017) exoplanet mass-radius
relations (2)
624- 631 F8.2 m/s E_k_0 [0.54/18000.0] upper error : The
84th-50th percentile of parameter
distribution in k_0
633- 640 F8.2 m/s e_k_0 [0.82/32000.0] lower error : The
50th-16th percentile of parameter
distribution in k_0
642- 647 F6.4 --- p_0 [0.03/0.21] Rp/Rstar (2)
649- 654 F6.4 --- E_p_0 [0.0/0.04] upper error : The
84th-50th percentile of parameter
distribution in p_0
656- 661 F6.4 --- e_p_0 [0.0/0.03] lower error : The
50th-16th percentile of parameter
distribution in p_0
663- 669 F7.4 rstar ar_0 [1.04/48.4] Semi-major axis (2)
671- 675 F5.3 rstar E_ar_0 [0.02/5.8] upper error : The
84th-50th percentile of parameter
distribution in ar_0
677- 682 F6.4 rstar e_ar_0 [0.0/6.5] lower error : The
50th-16th percentile of parameter
distribution in ar_0
684- 691 F8.6 --- delta_0 [0.0/0.05] (Rp/Rstar)^2 (2)
693- 699 E7.2 --- E_delta_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in delta_0
701- 707 E7.2 --- e_delta_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in delta_0
709- 715 F7.5 --- depth_I_0 [0.0/0.05] Flux decrement in
I-band at mid transit (can differ
from delta due to grazing geometries
and limb darkening) (2)
717- 723 F7.5 --- E_depth_I_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in depth_I_0
725- 731 F7.5 --- e_depth_I_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in depth_I_0
733- 739 F7.5 --- depth_V_0 [0.0/0.06] Flux decrement in
V-band at mid transit (can differ
from delta due to grazing geometries
and limb darkening) (2)
741- 747 F7.5 --- E_depth_V_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in depth_V_0
749- 755 F7.5 --- e_depth_V_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in depth_V_0
757- 763 F7.5 days tau_0 [0.0/0.21] Duration of ingress or
egress (2)
765- 771 F7.5 days E_tau_0 [0.0/0.15] upper error : The
84th-50th percentile of parameter
distribution in tau_0
773- 779 F7.5 days e_tau_0 [0.0/0.11] lower error : The
50th-16th percentile of parameter
distribution in tau_0
781- 786 F6.4 d t14_0 [0.07/0.74] Duration of transit
from 1st contact to 4th contact (2)
788- 793 F6.4 d E_t14_0 [0.0/0.09] upper error : The
84th-50th percentile of parameter
distribution in t14_0
795- 800 F6.4 d e_t14_0 [0.0/0.1] lower error : The
50th-16th percentile of parameter
distribution in t14_0
802- 808 F7.5 d tfwhm_0 [0.03/0.71] Duration of transit
from mid ingress to mid egress (2)
810- 815 F6.4 d E_tfwhm_0 [0.0/0.1] upper error : The
84th-50th percentile of parameter
distribution in tfwhm_0
817- 823 F7.5 d e_tfwhm_0 [0.0/0.1] lower error : The
50th-16th percentile of parameter
distribution in tfwhm_0
825- 829 F5.3 --- b_0 [0.05/1.02] Primary transit impact
parameter (2)
831- 835 F5.3 --- E_b_0 [0.01/0.39] upper error : The
84th-50th percentile of parameter
distribution in b_0
837- 841 F5.3 --- e_b_0 [0.01/0.46] lower error : The
50th-16th percentile of parameter
distribution in b_0
843- 849 F7.4 --- cosi_0 [0.0/0.56]? Cosine of planet
inclination (2)
851- 857 F7.4 --- E_cosi_0 [0.0/0.2]? upper error : The
84th-50th percentile of parameter
distribution in cosi_0
859- 865 F7.4 --- e_cosi_0 [0.0/0.23]? lower error : The
50th-16th percentile of parameter
distribution in cosi_0
867- 874 F8.3 ppm eclipsedepth25_0 [0.05/3310.0] BB eclipse depth at
2.5µm (2)
876- 883 F8.3 ppm E_eclipsedepth25_0 [0.09/2000.0] upper error : The
84th-50th percentile of parameter
distribution in eclipsedepth25_0
885- 892 F8.3 ppm e_eclipsedepth25_0 [0.03/1400.0] lower error : The
50th-16th percentile of parameter
distribution in eclipsedepth25_0
894- 899 F6.1 ppm eclipsedepth50_0 [19.1/5810.0] BB eclipse depth at
5.0µm (2)
901- 906 F6.1 ppm E_eclipsedepth50_0 [12.0/2500.0] upper error : The
84th-50th percentile of parameter
distribution in eclipsedepth50_0
908- 913 F6.1 ppm e_eclipsedepth50_0 [7.6/1900.0] lower error : The
50th-16th percentile of parameter
distribution in eclipsedepth50_0
915- 920 F6.1 ppm eclipsedepth75_0 [81.0/6950.0] BB eclipse depth at
7.5µm (2)
922- 927 F6.1 ppm E_eclipsedepth75_0 [25.0/2600.0] upper error : The
84th-50th percentile of parameter
distribution in eclipsedepth75_0
929- 934 F6.1 ppm e_eclipsedepth75_0 [19.0/2100.0] lower error : The
50th-16th percentile of parameter
distribution in eclipsedepth75_0
936- 943 F8.5 g/cm^3 rhop_0 [0.01/78.0] Planetary density (2)
945- 952 F8.5 g/cm^3 E_rhop_0 [0.0/80.0] upper error : The
84th-50th percentile of parameter
distribution in rhop_0
954- 961 F8.5 g/cm^3 e_rhop_0 [0.0/48.0] lower error : The
50th-16th percentile of parameter
distribution in rhop_0
963- 973 F11.8 days logp_0 [-0.18/1.81] Log10 period (2)
975- 981 E7.2 days E_logp_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in logp_0
983- 989 E7.2 days e_logp_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in logp_0
991- 995 F5.3 cgs loggp_0 [2.03/5.17] Log10 planetary surface
gravity (2)
997-1001 F5.3 cgs E_loggp_0 [0.01/2.21] upper error : The
84th-50th percentile of parameter
distribution in loggp_0
1003-1007 F5.3 cgs e_loggp_0 [0.01/2.0] lower error : The
50th-16th percentile of parameter
distribution in loggp_0
1009-1016 F8.5 --- safronov_0 [0.01/66.0] Safronov number (2)
1018-1025 F8.5 --- E_safronov_0 [0.0/86.0] upper error : The
84th-50th percentile of parameter
distribution in safronov_0
1027-1034 F8.5 --- e_safronov_0 [0.0/51.0] lower error : The
50th-16th percentile of parameter
distribution in safronov_0
1036-1043 F8.4 1e9erg/s/cm2 fave_0 [0.0/100.0] Average Incident
flux (2)
1045-1053 F9.4 1e9erg/s/cm2 E_fave_0 [0.0/2700.0] upper error :
The 84th-50th percentile of parameter
distribution in fave_0
1055-1061 F7.4 1e9erg/s/cm2 e_fave_0 [0.0/72.0] lower error : The
50th-16th percentile of parameter
distribution in fave_0
1063-1075 F13.5 BJD_TDB ts_0 [2455259.59/2455502.92] Time of
secondary eclipse (2)
1077-1083 F7.5 BJD_TDB E_ts_0 [0.0/1.7] upper error : The
84th-50th percentile of parameter
distribution in ts_0
1085-1091 F7.5 BJD_TDB e_ts_0 [0.0/3.8] lower error : The
50th-16th percentile of parameter
distribution in ts_0
1093-1105 F13.5 BJD_TDB (2) ta_0 [2455261.74/2455505.55] Time
of Ascending node
1107-1113 F7.5 BJD_TDB (2) E_ta_0 [0.0/1.11] upper error : The
84th-50th percentile of parameter
distribution in ta_0
1115-1121 F7.5 BJD_TDB (2) e_ta_0 [0.0/3.8] lower error : The
50th-16th percentile of parameter
distribution in ta_0
1123-1135 F13.5 BJD_TDB td_0 [2455261.27/2455504.49] Time of
Descending node (2)
1137-1143 F7.5 BJD_TDB E_td_0 [0.0/1.2] upper error : The
84th-50th percentile of parameter
distribution in td_0
1145-1151 F7.5 BJD_TDB e_td_0 [0.0/3.8] lower error : The
50th-16th percentile of parameter
distribution in td_0
1153-1156 F4.2 --- vcve_0 [1.0/1.08] V_c/V_e (2)
1158-1161 F4.2 --- E_vcve_0 upper error : The 84th-50th
percentile of parameter distribution
in vcve_0
1163-1165 F3.1 --- e_vcve_0 lower error : The 50th-16th
percentile of parameter distribution
in vcve_0
1167-1173 E7.2 --- q_0 [0.0/0.53] Mass ratio (mp/mstar)
(2)
1175-1181 E7.2 --- E_q_0 [0.0/0.34] upper error : The
84th-50th percentile of parameter
distribution in q_0
1183-1189 E7.2 --- e_q_0 [0.0/0.48] lower error : The
50th-16th percentile of parameter
distribution in q_0
1191-1197 F7.5 --- pt_0 [0.01/0.93] A priori non-grazing
transit probability (2)
1199-1205 F7.5 --- E_pt_0 [0.0/0.13] upper error : The
84th-50th percentile of parameter
distribution in pt_0
1207-1213 F7.5 --- e_pt_0 [0.0/0.13] lower error : The
50th-16th percentile of parameter
distribution in pt_0
1215-1221 F7.5 --- ptg_0 [0.02/1.0] A priori transit
probability (2)
1223-1229 F7.5 --- E_ptg_0 [0.0/0.15] upper error : The
84th-50th percentile of parameter
distribution in ptg_0
1231-1237 F7.5 --- e_ptg_0 [0.0/0.15] lower error : The
50th-16th percentile of parameter
distribution in ptg_0
1239-1243 F5.3 --- u1_0 [0.09/0.51] I-band linear limb
darkening coefficient; fitted (with
prior from Claret & Bloeman, 2011)
(2)
1245-1249 F5.3 --- E_u1_0 [0.01/0.2] upper error : The
84th-50th percentile of parameter
distribution in u1_0
1251-1255 F5.3 --- e_u1_0 [0.04/0.18] lower error : The
50th-16th percentile of parameter
distribution in u1_0
1257-1261 F5.3 --- u2_0 [0.16/0.43] I-band quadratic limb
darkening coefficient; fitted (with
prior from Claret & Bloeman, 2011
(2))
1263-1267 F5.3 --- E_u2_0 [0.03/0.13] upper error : The
84th-50th percentile of parameter
distribution in u2_0
1269-1273 F5.3 --- e_u2_0 [0.03/0.12] lower error : The
50th-16th percentile of parameter
distribution in u2_0
1275-1279 F5.3 --- u1_1 [0.11/0.86] V-band linear limb
darkening coefficient; fitted (with
prior from Claret & Bloeman, 2011)
(2)
1281-1285 F5.3 --- E_u1_1 [0.04/0.34] upper error : The
84th-50th percentile of parameter
distribution in u1_1
1287-1291 F5.3 --- e_u1_1 [0.04/0.39] lower error : The
50th-16th percentile of parameter
distribution in u1_1
1293-1298 F6.3 --- u2_1 [-0.03/0.41] V-band quadratic limb
darkening coefficient; fitted (with
prior from Claret & Bloeman, 2011
(2))
1300-1304 F5.3 --- E_u2_1 [0.04/0.2] upper error : The
84th-50th percentile of parameter
distribution in u2_1
1306-1310 F5.3 --- e_u2_1 [0.02/0.18] lower error : The
50th-16th percentile of parameter
distribution in u2_1
1312-1320 E9.4 fraction variance_0 [0.0/0.01] I-band added variance
to the transit light curve (2)
1322-1328 E7.2 fraction E_variance_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in variance_0
1330-1336 E7.2 fraction e_variance_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in variance_0
1338-1345 F8.6 --- f0_0 [0.99/1.01] Baseline flux in I-band
(2)
1347-1353 E7.2 --- E_f0_0 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in f0_0
1355-1361 E7.2 --- e_f0_0 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in f0_0
1363-1370 E8.3 fraction variance_1 [0.0/0.01] V-band added variance
to the transit light curve (2)
1372-1378 E7.2 fraction E_variance_1 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in variance_1
1380-1386 E7.2 fraction e_variance_1 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in variance_1
1388-1394 F7.5 --- f0_1 [0.99/1.01] Baseline flux in V-band
(2)
1396-1402 F7.5 --- E_f0_1 [0.0/0.01] upper error : The
84th-50th percentile of parameter
distribution in f0_1
1404-1410 F7.5 --- e_f0_1 [0.0/0.01] lower error : The
50th-16th percentile of parameter
distribution in f0_1
--------------------------------------------------------------------------------
Note (1): In the format OGLE-TR-NNNN, where NNNN is a 4-digit number.
Note (2): For detailed parameter definition see Eastman et al. (2019)
Format of the files with photometry (OGLE-TR-NNNN.dat)
--------------------------------------------------------------------------
Bytes Format Units Description
--------------------------------------------------------------------------
1- 10 F10.5 days Heliocentric Julian Day - 2450000
12- 17 F6.3 mag Magnitude
19- 23 F5.3 mag Uncertainty of magnitude
--------------------------------------------------------------------------
See also:
https://www.astrouw.edu.pl/ogle/ : OGLE On-line Data Directory
https://github.com/jdeast/EXOFASTv2/ : EXOFASTv2 code
https://github.com/timothydmorton/VESPA : VESPA code
Finding charts are gzipped Postscript images. These are 1'x1' subframes
of the I-band reference frames centered on the star. White cross marks the
star. North is up and East to the left.
Figures related to the EXOFASTv2 models of transits are Encapsulated PostScript (.eps) images.
All CSV files are files with comma-separated values, with the header in the first line containing column names.
Any presentation of the scientific analysis or usage of the data from the
catalog of candidates for transiting planets toward the Galactic bulge should
include the appropriate reference(s) to OGLE paper(s).
Acknowledgements:
References:
================================================================================
Chen, J., & Kipping, D. 2017, ApJ, 834, 17.
Claret, A., & Bloemen, S. 2011, A&A, 529, A75.
Eastman, J., Rodriguez, J., Agol, E., et al. 2019, arXiv:1907.09480.
Morton, T. 2012, ApJ, 761, 6. parameter definition see Eastman et al. (2019)
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