(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: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- 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. -------------------------------------------------------------------------------- Byte-by-byte Description of file: ident.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- Note (1): In the format OGLE-TR-NNNN, where NNNN is a 4-digit number. Byte-by-byte Description of file: transits.dat -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- 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 -------------------------------------------------------------------------------- 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)