J/A+A/691/A242ivo://CDS.VizieR/J/A+A/691/A242doi:10.26093/cds/vizier.36910242CDSIJspeert L.W.Tkachenko A.Johnston C.Aerts C.s2025-02-18T20:02:08Z2024-11-19T12:37:20ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.freclipsing-binary-starsphotometryvisible-astronomyorbitsEclipsing binaries are crucial for understanding stellar physics, allowing detailed studies of stellar masses, radii, and orbital dynamics. Recent space missions like the Transiting Exoplanet Survey Satellite (TESS) have significantly expanded the catalogue of observed eclipsing binaries with uninterrupted time series photometry, providing an opportunity for large-scale ensemble studies. This study aims to analyse the statistical properties of circularisation in a large sample of intermediate-to-high mass eclipsing binaries observed by TESS. We explore the dependence of orbital circularisation on stellar properties and orbital parameters to improve our understanding of the physical processes affecting these systems. We further aim to assess the role of stellar pulsations in circularisation. We compiled a catalogue of O- to F-type stars to search for eclipsing binary signals in the data available from the first 4 years of the TESS mission. Using automated classification and data analysis methodologies, we arrive at a well characterised sample of 14,573 eclipsing binaries. We supplement our catalogue with Gaia effective temperatures, and investigate the statistical characteristics of the sample as a function of temperature, orbital period, and scaled orbital separation. The orbital circularisation was measured with statistical methods to obtain three distinct measurements of the critical period and separation in four temperature ranges. These measurements cover a range of orbital periods and separations where both circularised and eccentric systems exist. Pulsations were identified in the g- and p-mode regimes, and a reduced fraction of eccentric systems was found among them. Our analysis revealed the dependence of orbital circularisation on stellar temperatures, also seen in other studies, and confirmed previous findings that additional dissipation is needed as compared to the predictions of turbulent viscosity and non-resonant radiative damping. We speculate that pulsations may play a role in the circularisation of close binaries. Our study highlights the need for dissipative mechanisms that can produce a wide range of critical periods from a range of initial conditions.2024A&A...691A.242Ihttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/691/A242CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)IV/38 : TESS Input Catalog - v8.0 (TIC-8) (Stassun+, 2019)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/691/A242https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/691/A242http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/691/A242https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/691/A242https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/691/A242http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/691/A242GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/691/A242/tessobaf (TESS OBAF catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/691/A242/tessobaf?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/691/A242/tessobaf?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/691/A242/tessobaf?GETtext/xml+votable180.050000true2.0323353901565-47.78146803787850.005555555555555556Cone search capability for table J/A+A/691/A242/obaf-eb1 (TESS_OBAF_EB_catalogue (partial))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/691/A242/obaf-eb1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/691/A242/obaf-eb1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/691/A242/obaf-eb1?GETtext/xml+votable180.050000true11.9564395246578-46.32970263538880.0055555555555555560/1 3 9 11 1/2-3 8-9 11 17-21 23-24 26 29 31-33 35 40 42 2/5-7 40-42 66 88-89 100-102 112-113 123 136-138 164-166 172 174-175 3/2 6-10 14-15 17-19 172-173 175 258-259 261-263 268 270-271 360 362-365 413-414 432-433 435-437 439-440 442-444 446-447 456-457 482 485-487 489-491 556-557 669-670 692 694-695 4/0-2 4 13-15 17-20 22-23 45-49 51-52 54-55 64 66 696 698-699 1024 1026-1028 1030-1031 1041-1043 1076-1078 1444-1446 1464-1466 1468-1469 1648-1649 1651 1660-1662 1736-1737 1739 1752 1754 1764 1766-1767 1780-1781 1783 1832-1833 1835-1837 1840-1842 1844-1845 1847 1852 1854-1855 1922-1923 1927 1934 1938 1952 1954-1955 2232-2234 2236-2238 2672-2673 2675 2684-2685 2772 2774-2775 5/12-14 20 22-26 29 49-51 64-65 67 84-85 87 177-179 201-203 212 214 260 268 270-271 2788-2790 4101-4103 4116-4118 4160-4161 4163 4316-4317 4319 5789-5791 5868-5869 5871 5880-5881 5883-5886 6600-6601 6603 6652-6653 6655 6952-6953 6955 7012 7014-7015 7020 7022-7023 7060-7061 7063 7128-7130 7336-7337 7339 7352-7353 7355-7357 7359 7372-7374 7384-7386 7392 7394-7397 7399-7400 7402-7403 7413-7415 7680 7682 7684 7686 7697 7700-7702 7704-7706 7728-7730 7732 7734-7735 7741-7743 7745-7747 7749 7757-7758 7812-7813 7815 8941-8943 8957-8959 10697-10699 10746-10747 10751 11092 11094-11095 6/60 62-63 84-86 109-111 113 121 123 125-127 192-194 264-265 267 344-346 705-707 800-801 803 852-854 861-863 1044-1046 1048 1050 1053 1055 1077 1079 11165-11167 16400-16402 16476 16478-16479 16648 16650-16651 17272 17274-17275 23152-23153 23155 23480 23482-23483 23529-23531 23548-23550 26408 26410-26411 26616-26617 26619 27816 27818-27819 28052 28054-28055 28085-28087 28248-28249 28251 28524 28526-28527 29352-29353 29416-29417 29419 29432-29434 29500-29502 29548-29550 29572-29574 29592-29593 29604 29606-29607 29616 29618-29621 29623-29625 29627-29630 29649-29651 30725-30727 30732-30733 30735 30740 30742-30743 30748-30749 30751 30784 30786-30787 30792-30794 30796-30797 30799 30812-30814 30829-30831 30925-30927 30932-30933 30935 30960 30962-30963 30976-30978 30992-30994 31000 31002-31005 31007 31024 31037-31039 31256 31258-31259 35760-35761 35763 35824-35826 42784-42785 42787 42977-42979 42981-42983 42994-42997 42999 43001-43003 443757.952274030004205e-20 3.916500758235022e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/691/A242?format=asciiOpticaldefaultJ/A+A/691/A242/tessobafTESS OBAF catalogueTICIdentification number in the TESS Input Catalog (TIC)meta.id;meta.mainlongRAJ2000Right ascension (J2000) (ra)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (dec)degpos.eq.dec;meta.mainindexede_plx? TIC parallax error (e_plx)masstat.error;pos.parallaxdoublenullableGLONGalactic longitude (gallong)degpos.galactic.lonGLATGalactic latitude (gallat)degpos.galactic.latdoubleB_E(BP-RP)? Gaia upper confidence level (84%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)magstat.fit.param;phys.atmol.leveldoublenullableb_Teff? Gaia lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)Kphys.temperature.effective;phys.atmol.leveldoublenullableB_Teff? Gaia upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)Kphys.temperature.effective;phys.atmol.leveldoublenullablelogg? Gaia surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log) (logg_gspphot)log(cm.s**-2)phys.gravitydoublenullableb_logg? Gaia lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log) (logg_gspphot)log(cm.s**-2)phys.gravity;stat.mindoublenullableB_logg? Gaia upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log) (logg_gspphot)log(cm.s**-2)phys.gravity;stat.maxdoublenullableDist? Gaia distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)pcpos.distancedoublenullableb_Dist? Gaia lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)pcpos.distance;stat.fit.param;phys.atmol.leveldoublenullableB_Dist? Gaia upper confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)pcpos.distance;stat.fit.param;phys.atmol.leveldoublenullableTeff-HS? Gaia effective temperature from ESP-HS (teff_esphs)Kphys.temperature.effectivedoublenullablee_Teff-HS? Gaia uncertainty at a 68% confidence level on the effective temperature from ESP-HS (teff_esphs_uncertainty)Kstat.errordoublenullableAG-HS? Gaia intersterstellar extinction in G band from ESP-HS (g ag_esphs)magphys.absorptiondoublenullablee_AG-HS? Gaia uncertainty on AG from ESP-HS (ag_esphs_uncertainty)magstat.errordoublenullableE(B-V)-HS? Gaia reddening E(GBP-GRP) from ESP-HS (ebpminrp_esphs)magphot.color.excessdoublenullablee_E(B-V)-HS? Gaia uncertainty on E(GBP-GRP) from ESP-HS (g ebpminrp_esphs_uncertainty)magstat.errordoublenullablelogg-HS? Gaia surface gravity from ESP-HS (log) (logg_esphs)log(cm.s**-2)phys.gravitydoublenullablee_logg-HS? Gaia uncertainty at a 68% confidence level on the surface gravity from ESP-HS (log) (logg_esphs_uncertainty)log(cm.s**-2)stat.errordoublenullablevsini-HS? Gaia projected rotational velocity from ESP-HS (vsini_esphs)km/sphys.veloc.rotatdoublenullablee_vsini-HS? Gaia uncertainty on the projected rotational velocity from ESP-HS (vsini_esphs_uncertainty)km/sstat.errordoublenullableTeffMSC1? Gaia effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1)Kphys.temperature.effectivedoublenullableB_TeffMSC1? Gaia upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_upper)Kphys.temperature.effective;phys.atmol.leveldoublenullableb_TeffMSC1? Gaia lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_lower)Kphys.temperature.effective;phys.atmol.leveldoublenullableTeffMSC2? Gaia effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2)Kphys.temperature.effectivedoublenullableGaiaDupTIC? Gaia entries with a duplicate TIC entry (lower G mag is removed from consideration) (gaia_dup_tic)meta.codefloatnullablet0SPOCy1? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t0SPOCy1)dtime.epochdoublenullablePerSPOCy1? Orbital period or half the orbital period (for indistinguishable primary and secondary) (PerSPOCy1)dtime.perioddoublenullablescoreSPOCy1? Score value between 0 and 1 by ECLIPSR (see documentation) (scoreSPOCy1)stat.fit.paramfloatnullablef1SPOCy1? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y1)stat.fit.paramdoublenullablef2SPOCy1? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y1)stat.fit.paramdoublenullablef3SPOCy1? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y1)stat.fit.paramdoublenullablef4SPOCy1? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y1)stat.fit.paramdoublenullablewideSPOCy1? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wideSPOCy1)meta.codefloatnullablef3SPOCy3? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y3)stat.fit.paramdoublenullablef4SPOCy3? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y3)stat.fit.paramdoublenullablef5SPOCy3? Feature 5 that goes into the ECLIPSR score value (f1SPOCy3)stat.fit.paramdoublenullablef6SPOCy3? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y3)stat.fit.paramfloatnullableslikeSPOCy3? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y3)meta.codefloatnullablewideSPOCy3? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y3)meta.codefloatnullablet0SPOCy4? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y4)dtime.epochdoublenullableslikeQLPy1? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_likeQLPy1)meta.codefloatnullablewideQLPy1? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wideQLPy1)meta.codefloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintplx? TIC parallax (plx)maspos.parallax.trigdoublenullablef5SPOCy1? Feature 5 that goes into the ECLIPSR score value (f1SPOCy1)stat.fit.paramdoublenullableTeff? Gaia effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)Kphys.temperature.effectivedoublenullablef2QLPy4? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y4)stat.fit.paramdoublenullablef3QLPy4? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y4)stat.fit.paramdoublenullablef6SPOCy1? Feature 6 that goes into the ECLIPSR score value (f6SPOCy1)stat.fit.paramfloatnullableslikeSPOCy1? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sinelikeSPOCy1)meta.codefloatnullableELONEcliptic longitude (eclong)degpos.ecliptic.lonELATEcliptic latitude (eclat)degpos.ecliptic.latdoubleJmagJ band magnitude (Jmag)magphot.mag;em.IR.Jdoublee_Jmag? J band magnitude error (e_Jmag)magstat.error;phot.magdoublenullableHmagH band magnitude (Hmag)magphot.mag;em.IR.Hdoublee_Hmag? H band magnitude error (e_Hmag)magstat.error;phot.magdoublenullableKmagK band magnitude (Kmag)magphot.mag;em.IR.Kdoublee_Kmag? K band magnitude error (e_Kmag)magstat.error;phot.magdoublenullableGmagtic? TIC Gaia (G) magnitude (GAIAmag)magphot.mag;em.optdoublenullablee_Gmagtic? TIC Gaia (G) magnitude error (e_GAIAmag)magstat.errordoublenullableTmagTESS (T) magnitude (Tmag)magphot.mag;em.optdoublee_Tmag? TESS (T) magnitude error (e_Tmag)magstat.error;phot.magdoublenullableTefftic? TIC effective temperature (Teff)Kphys.temperature.effectivedoublenullablee_Tefftic? TIC effective temperature error (e_Teff)Kstat.errordoublenullablelumclass[ADFRW] TIC luminosity class (dwarf or unknown in this case, by design) (lumclass)src.class.luminositycharDisttic? TIC distance (d)pcpos.distancedoublenullablee_Disttic? TIC distance error (e_d)pcstat.errordoublenullableE(B-V)? TIC extinction (ebv)magphot.color.excessdoublenullablee_E(B-V)? TIC extinction error (e_ebv)magstat.errordoublenullableNumCont? TIC number of Contamination Sources (numcont)meta.numberfloatnullableContRatio? TIC contamination ratio (contratio)stat.fit.omcdoublenullableBPmagtic? TIC Gaia BP (blue) magnitude (gaiabp)magphot.mag;em.opt.Bdoublenullablee_BPmagtic? TIC Gaia BP (blue) magnitude error (e_gaiabp)magstat.errordoublenullableRPmagtic? TIC Gaia RP (red) magnitude (gaiarp)magphot.mag;em.opt.Rdoublenullablee_RPmagtic? TIC Gaia RP (red) magnitude error (e_gaiarp)magstat.errordoublenullablewdflag? TIC white dwarf flag (0 or -1 (so not 1) in this case, by design) (wdflag)meta.codefloatnullableGaiaDR3? Identification number from GAIA DR3 (GAIA_DR3)meta.idnullableBP-RP? Gaia BP-RP colour (bp_rp)magphot.color;em.opt.B;em.opt.RdoublenullableCatOri? Original external catalogue source identifier from 2MASS (original_ext_source_id)meta.id;meta.datasetcharGmag? Gaia G-band mean magnitude (phot_g_mean_mag)magphot.mag;em.optdoublenullableBPmag? Gaia integrated BP mean magnitude (phot_bp_mean_mag)magphot.mag;em.opt.BdoublenullableRPmag? Gaia integrated RP mean magnitude (phot_rp_mean_mag)magphot.mag;em.opt.RdoublenullableAG? Gaia extinction in G band from GSP- Phot Aeneas best library using BP/RP spectra (ag_gspphot)magphys.absorptiondoublenullableb_AG? Gaia lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)magphys.absorption;phys.atmol.leveldoublenullableB_AG? Gaia upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)magphys.absorption;phys.atmol.leveldoublenullableE(BP-RP)? Gaia reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)magphot.color.excessdoublenullableb_E(BP-RP)? Gaia lower confidence level (16%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)magstat.fit.param;phys.atmol.leveldoublenullableB_TeffMSC2? Gaia upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_upper)Kphys.temperature.effective;phys.atmol.leveldoublenullableb_TeffMSC2? Gaia lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_lower)Kphys.temperature.effective;phys.atmol.leveldoublenullableloggMSC1? Gaia surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1)log(cm.s**-2)phys.gravitydoublenullableB_loggMSC1? Gaia upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1_upper)log(cm.s**-2)phys.gravity;stat.maxdoublenullableb_loggMSC1? Gaia lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1_lower)log(cm.s**-2)phys.gravity;stat.mindoublenullableloggMSC2? Gaia surface gravity of the secondary from MSC using BP/RP spectra and parallax (log cgs) (logg_msc2)log(cm.s**-2)phys.gravitydoublenullableB_loggMSC2? Gaia upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (log) (logg_msc2_upper)log(cm.s**-2)phys.gravity;stat.maxdoublenullableb_loggMSC2? Gaia lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (log) (logg_msc2_lower)log(cm.s**-2)phys.gravity;stat.mindoublenullablet0SPOCy2? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y2)dtime.epochdoublenullablePerSPOCy2? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_spoc_y2)dtime.perioddoublenullablescoreSPOCy2? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y2)stat.fit.paramfloatnullablef1SPOCy2? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y2)stat.fit.paramdoublenullablef2SPOCy2? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y2)stat.fit.paramdoublenullablef3SPOCy2? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y2)stat.fit.paramdoublenullablef4SPOCy2? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y2)stat.fit.paramdoublenullablef5SPOCy2? Feature 5 that goes into the ECLIPSR score value (f1SPOCy2)stat.fit.paramdoublenullablef6SPOCy2? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y2)stat.fit.paramfloatnullableslikeSPOCy2? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y2)meta.codefloatnullablewideSPOCy2? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y2)meta.codefloatnullablet0SPOCy3? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y3)dtime.epochdoublenullablePerSPOCy3? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_spoc_y3)dtime.perioddoublenullablescoreSPOCy3? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y3)stat.fit.paramfloatnullablef1SPOCy3? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y3)stat.fit.paramdoublenullablef2SPOCy3? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y3)stat.fit.paramdoublenullablePerSPOCy4? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_spoc_y4)dtime.perioddoublenullablescoreSPOCy4? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y4)stat.fit.paramfloatnullablef1SPOCy4? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y4)stat.fit.paramdoublenullablef2SPOCy4? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y4)stat.fit.paramdoublenullablef3SPOCy4? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y4)stat.fit.paramdoublenullablef4iSPOCy4? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y4)stat.fit.paramdoublenullablef5SPOCy4? Feature 5 that goes into the ECLIPSR score value (f1SPOCy4)stat.fit.paramdoublenullablef6SPOCy4? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y4)stat.fit.paramfloatnullableslikeSPOCy4? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y4)meta.codefloatnullablewideSPOCy4? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y4)meta.codefloatnullablet0QLPy1? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zeroQLPy1)dtime.epochdoublenullablePerQLPy1? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_qlp_y1)dtime.perioddoublenullablescoreQLPy1? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y1)stat.fit.paramfloatnullablef3QLPy1? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y1)stat.fit.paramdoublenullablef4QLPy1? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y1)stat.fit.paramdoublenullablef5QLPy1? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y1)stat.fit.paramdoublenullablef6QLPy1? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y1)stat.fit.paramfloatnullablet0QLPy2? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zeroQLPy2)dtime.epochdoublenullablePerQLPy2? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_qlp_y2)dtime.perioddoublenullablescoreQLPy2? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y2)stat.fit.paramfloatnullablef1QLPy2? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y2)stat.fit.paramdoublenullablef2QLPy2? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y2)stat.fit.paramdoublenullablef3QLPy2? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y2)stat.fit.paramdoublenullablef4QLPy2? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y2)stat.fit.paramdoublenullablef5QLPy2? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y2)stat.fit.paramdoublenullablef2QLPy3? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y3)stat.fit.paramdoublenullablef6QLPy2? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y2)stat.fit.paramfloatnullableslikeQLPy2? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_likeQLPy2)meta.codefloatnullablewideQLPy2? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wideQLPy2)meta.codefloatnullablet0QLPy3? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zeroQLPy3)dtime.epochdoublenullablePerQLPy3? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_qlp_y3)dtime.perioddoublenullablescoreQLPy3? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y3)stat.fit.paramfloatnullablef1QLPy3? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y3)stat.fit.paramdoublenullablef3QLPy3? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y3)stat.fit.paramdoublenullablef4QLPy3? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y3)stat.fit.paramdoublenullablef5QLPy3? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y3)stat.fit.paramdoublenullablef6QLPy3? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y3)stat.fit.paramfloatnullableslikeQLPy3? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_likeQLPy3)meta.codefloatnullablewideQLPy3? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wideQLPy3)meta.codefloatnullablet0QLPy4? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zeroQLPy4)dtime.epochdoublenullablePerQLPy4? Orbital period or half the orbital period (for indistinguishable primary and secondary) (period_qlp_y4)dtime.perioddoublenullablescoreQLPy4? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y4)stat.fit.paramfloatnullablef1QLPy4? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y4)stat.fit.paramdoublenullablef4QLPy4? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y4)stat.fit.paramdoublenullablef5QLPy4? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y4)stat.fit.paramdoublenullablef6QLPy4? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y4)stat.fit.paramfloatnullableslikeQLPy4? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_likeQLPy4)meta.codefloatnullablewideQLPy4? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wideQLPy4)meta.codefloatnullablescore? Score value between 0 and 1 by ECLIPSR (see documentation) (score)stat.fit.paramfloatnullableslike? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like)meta.codefloatnullablewide? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide)meta.codefloatnullable2MASSIdentification number from 2MASS (TWOMASS)meta.idcharf1QLPy1? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y1)stat.fit.paramdoublenullablef2QLPy1? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y1)stat.fit.paramdoublenullableJ/A+A/691/A242/obaf-eb1TESS_OBAF_EB_catalogue (partial)TmagTESS (T) magnitude (Tmag)magphot.mag;em.optdoublee_Tmag? TESS (T) magnitude error (e_Tmag)magstat.error;phot.magdoublenullableTefftic? TIC effective temperature (Teff)Kphys.temperature.effectivedoublenullableGmagtic? TIC Gaia (G) magnitude (GAIAmag)magphot.mag;em.optdoublenullablee_Gmagtic? TIC Gaia (G) magnitude error (e_GAIAmag)magstat.errordoublenullablee_Tefftic? TIC effective temperature error (e_Teff)Kstat.errordoublenullablelumclass[ADFRW] TIC luminosity class (dwarf or unknown in this case, by design) (lumclass)src.class.luminositycharDisttic? TIC distance (d)pos.distancedoublenullablee_Disttic? TIC distance error (e_d)stat.errordoublenullableE(B-V)tic? TIC extinction (ebv)magphot.color.excessdoublenullablee_E(B-V)tic? TIC extinction error (e_ebv)magstat.errordoublenullableNumCont? TIC number of Contamination Sources (numcont)meta.numberfloatnullableContRatio? TIC contamination ratio (contratio)stat.fit.omcdoublenullableBPmagtic? TIC Gaia BP (blue) magnitude (gaiabp)magphot.mag;em.opt.Bdoublenullablee_RPmagtic? TIC Gaia RP (red) magnitude error (e_gaiarp)magstat.errordoublenullablewdflag? TIC white dwarf flag (0 or -1 (so not 1) in this case, by design) (wdflag)meta.codefloatnullableGaiaDR3? Identification number from GAIA DR3 (GAIA_DR3)meta.idnullableBP-RP? Gaia BP-RP colour (bp_rp)magphot.color;em.opt.B;em.opt.RdoublenullableGmag? Gaia G-band mean magnitude (phot_g_mean_mag)magphot.mag;em.optdoublenullableBPmag? Gaia integrated BP mean magnitude (phot_bp_mean_mag)magphot.mag;em.opt.BdoublenullableRPmag? Gaia integrated RP mean magnitude (phot_rp_mean_mag)magphot.mag;em.opt.RdoublenullableAG? Gaia extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot)magphys.absorptiondoublenullableb_AG? Gaia lower confidence level (16%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_lower)magphys.absorption;phys.atmol.leveldoublenullableB_AG? Gaia upper confidence level (84%) of extinction in G band from GSP-Phot Aeneas best library using BP/RP spectra (ag_gspphot_upper)magphys.absorption;phys.atmol.leveldoublenullableE(BP-RP)? Gaia reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot)magphot.color.excessdoublenullableb_E(BP-RP)? Gaia lower confidence level (16%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_lower)magstat.fit.param;phys.atmol.leveldoublenullableB_E(BP-RP)? Gaia upper confidence level (84%) of reddening E(GBP-GRP) from GSP-Phot Aeneas best library using BP/RP spectra (ebpminrp_gspphot_upper)magstat.fit.param;phys.atmol.leveldoublenullableTeff? Gaia effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot)Kphys.temperature.effectivedoublenullableb_Teff? Gaia lower confidence level (16%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_lower)Kphys.temperature.effective;phys.atmol.leveldoublenullableB_Teff? Gaia upper confidence level (84%) of effective temperature from GSP-Phot Aeneas best library using BP/RP spectra (teff_gspphot_upper)Kphys.temperature.effective;phys.atmol.leveldoublenullablelogg? Gaia surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log ) (logg_gspphot)log(cm.s**-2)phys.gravitydoublenullableb_logg? Gaia lower confidence level (16%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log) (logg_gspphot_lower)log(cm.s**-2)phys.gravity;stat.mindoublenullableB_logg? Gaia upper confidence level (84%) of surface gravity from GSP-Phot Aeneas best library using BP/RP spectra (log) (logg_gspphot_upper)log(cm.s**-2)phys.gravity;stat.maxdoublenullableb_Dist? Gaia lower confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_lower)pcpos.distance;stat.fit.param;phys.atmol.leveldoublenullableB_Dist? Gaia upper confidence level (16%) of distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot_upper)pcpos.distance;stat.fit.param;phys.atmol.leveldoublenullableTeff-HS? Gaia effective temperature from ESP-HS (teff_esphs)Kphys.temperature.effectivedoublenullablee_Teff-HS? Gaia uncertainty at a 68% confidence level on the effective temperature from ESP-HS (teff_esphs_uncertainty)Kstat.errordoublenullableAG-HS? Gaia intersterstellar extinction in G band from ESP-HS (ag_esphs)magphys.absorptiondoublenullablee_AG-HS? Gaia uncertainty on AG from ESP-HS (ag_esphs_uncertainty)magstat.errordoublenullableE(B-V)-HS? Gaia reddening E(GBP-GRP) from ESP-HS (ebpminrp_esphs)magphot.color.excessdoublenullablee_E(B-V)-HS? Gaia uncertainty on E(GBP-GRP) from ESP-HS (ebpminrp_esphs_uncertainty)magstat.errordoublenullablelogg-HS? Gaia surface gravity from ESP-HS (log) (logg_esphs)log(cm.s**-2)phys.gravitydoublenullablee_logg-HS? Gaia uncertainty at a 68% confidence level on the surface gravity from ESP-HS (log) (logg_esphs_uncertainty)log(cm.s**-2)stat.errordoublenullablee_BPmagtic? TIC Gaia BP (blue) magnitude error (e_gaiabp)magstat.errordoublenullableRPmagtic? TIC Gaia RP (red) magnitude (gaiarp)magphot.mag;em.opt.RdoublenullableTeff2? Gaia effective temperature (ESP-HS takes precedent over GSP-Phot) (teff)Kphys.temperature.effectivedoublenullablewideQLPy4? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_qlp_y4)meta.codefloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTICIdentification number in the TESS Input Catalog (TIC)meta.id;meta.mainlong2MASSIdentification number from 2MASS (TWOMASS)meta.idcharRAJ2000Right ascension (J2000) (ra)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (dec)degpos.eq.dec;meta.mainindexedplx? TIC parallax (mas) (plx)maspos.parallax.trigdoublenullablee_plx? TIC parallax error (mas) (e_plx)masstat.error;pos.parallaxdoublenullableGLONGalactic longitude (degrees) (gallong)degpos.galactic.lonGLATGalactic latitude (degrees) (gallat)degpos.galactic.latdoubleELONEcliptic longitude (degrees) (eclong)degpos.ecliptic.lonELATEcliptic latitude (degrees) (eclat)degpos.ecliptic.latdoubleJmagJ band magnitude (Jmag)magphot.mag;em.IR.Jdoublee_Jmag? J band magnitude error (e_Jmag)magstat.error;phot.magdoublenullableHmagH band magnitude (Hmag)magphot.mag;em.IR.Hdoublee_Hmag? H band magnitude error (e_Hmag)magstat.error;phot.magdoublenullableKmagK band magnitude (Kmag)magphot.mag;em.IR.Kdoublee_Kmag? K band magnitude error (e_Kmag)magstat.error;phot.magdoublenullablevsini-HS? Gaia projected rotational velocity from ESP-HS (vsini_esphs)km/sphys.veloc.rotatdoublenullablee_vsini-HS? Gaia uncertainty on the projected rotational velocity from ESP-HS (vsini_esphs_uncertainty)km/sstat.errordoublenullableTeffMSC1? Gaia effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1)Kphys.temperature.effectivedoublenullablef5SPOCy1? Feature 5 that goes into the ECLIPSR score value (f_5_spoc_y1)stat.fit.paramdoublenullableB_loggMSC1? Gaia upper confidence level (84%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1_upper)log(cm.s**-2)phys.gravity;stat.maxdoublenullableb_loggMSC1? Gaia lower confidence level (16%) of surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1_lower)log(cm.s**-2)phys.gravity;stat.mindoublenullableloggMSC2? Gaia surface gravity of the secondary from MSC using BP/RP spectra and parallax (log cgs) (logg_msc2)log(cm.s**-2)phys.gravitydoublenullableB_loggMSC2? Gaia upper confidence level (84%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (log cgs) (logg_msc2_upper)log(cm.s**-2)phys.gravity;stat.maxdoublenullableb_loggMSC2? Gaia lower confidence level (16%) of surface gravity of the secondary from MSC using BP/RP spectra and parallax (log cgs) (logg_msc2_lower)log(cm.s**-2)phys.gravity;stat.mindoublenullableGaiaDupTIC? Gaia entries with a duplicate TIC entry (lower G mag is removed from consideration) (gaia_dup_tic)meta.codefloatnullableAG2? Gaia extinction in G band (ESP-HS takes precedent over GSP-Phot) (ag)magphys.absorptiondoublenullablebAG2? Gaia lower confidence level of extinction in G band (ESP-HS takes precedent over GSP-Phot) (ag_lower)magstat.errordoublenullableBAG2? Gaia upper confidence level of extinction in G band (ESP-HS takes precedent over GSP-Phot) (ag_upper)magstat.errordoublenullableE(B-V)2? Gaia reddening (ESP-HS takes precedent over GSP-Phot) (ebpminrp)magphot.color.excessdoublenullablebE(B-V)2? Gaia lower confidence level of reddening (ESP-HS takes precedent over GSP-Phot) (ebpminrp_lower)magstat.errordoublenullableBE(B-V)2? Gaia upper confidence level of reddening (ESP-HS takes precedent over GSP-Phot) (ebpminrp_upper)magstat.errordoublenullablebTeff2? Gaia lower confidence level of effective temperature (ESP-HS takes precedent over GSP-Phot) (teff_lower)Kphys.temperature.effectivedoublenullableBTeff2? Gaia upper confidence level of effective temperature (ESP-HS takes precedent over GSP-Phot) (teff_upper)Kphys.temperature.effectivedoublenullablelogg2? Gaia surface gravity (ESP-HS takes precedent over GSP-Phot) (logg)log(cm.s**-2)phys.gravitydoublenullableblogg2? Gaia lower confidence level of surface gravity (ESP-HS takes precedent over GSP-Phot) (logg_lower)log(cm.s**-2)stat.fit.param;phys.gravitydoublenullableBlogg2? Gaia upper confidence level of surface gravity (ESP-HS takes precedent over GSP-Phot) (logg_upper)log(cm.s**-2)stat.fit.param;phys.gravitydoublenullablet0SPOCy1? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y1)dtime.epochdoublenullablePerSPOCy1? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_spoc_y1)dtime.perioddoublenullablescoreSPOCy1? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y1)stat.fit.paramfloatnullablef1SPOCy1? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y1)stat.fit.paramdoublenullablef2SPOCy1? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y1)stat.fit.paramdoublenullablef3SPOCy1? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y1)stat.fit.paramdoublenullablef4SPOCy1? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y1)stat.fit.paramdoublenullableslikeSPOCy1? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y1)meta.codefloatnullablewideSPOCy1? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y1)meta.codefloatnullablet0SPOCy2? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y2)dtime.epochdoublenullablePerSPOCy2? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_spoc_y2)dtime.perioddoublenullablescoreSPOCy2? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y2)stat.fit.paramfloatnullablef1SPOCy2? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y2)stat.fit.paramdoublenullablef2SPOCy2? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y2)stat.fit.paramdoublenullablef3SPOCy2? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y2)stat.fit.paramdoublenullablef4SPOCy2? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y2)stat.fit.paramdoublenullablef5SPOCy2? Feature 5 that goes into the ECLIPSR score value (f_5_spoc_y2)stat.fit.paramdoublenullablef6SPOCy2? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y2)stat.fit.paramfloatnullableslikeSPOCy2? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y2)meta.codefloatnullablewideSPOCy2? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y2)meta.codefloatnullablet0SPOCy3? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y3)dtime.epochdoublenullablePerSPOCy3? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_spoc_y3)dtime.perioddoublenullablescoreSPOCy3? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y3)stat.fit.paramfloatnullablef1SPOCy3? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y3)stat.fit.paramdoublenullablef2SPOCy3? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y3)stat.fit.paramdoublenullablef3SPOCy3? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y3)stat.fit.paramdoublenullablef4SPOCy3? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y3)stat.fit.paramdoublenullablef5SPOCy3? Feature 5 that goes into the ECLIPSR score value (f_5_spoc_y3)stat.fit.paramdoublenullablef6SPOCy3? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y3)stat.fit.paramfloatnullableslikeSPOCy3? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y3)meta.codefloatnullablewideSPOCy3? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y3)meta.codefloatnullablet0SPOCy4? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_spoc_y4)dtime.epochdoublenullablePerSPOCy4? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_spoc_y4)dtime.perioddoublenullablescoreSPOCy4? Score value between 0 and 1 by ECLIPSR (see documentation) (score_spoc_y4)stat.fit.paramfloatnullablef1SPOCy4? Feature 1 that goes into the ECLIPSR score value (f_1_spoc_y4)stat.fit.paramdoublenullablef2SPOCy4? Feature 2 that goes into the ECLIPSR score value (f_2_spoc_y4)stat.fit.paramdoublenullablef3SPOCy4? Feature 3 that goes into the ECLIPSR score value (f_3_spoc_y4)stat.fit.paramdoublenullableslikeSPOCy4? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_spoc_y4)meta.codefloatnullablewideSPOCy4? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_spoc_y4)meta.codefloatnullablet0QLPy1? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_qlp_y1)dtime.epochdoublenullablePerQLPy1? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_qlp_y1)dtime.perioddoublenullablescoreQLPy1? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y1)stat.fit.paramfloatnullablef1QLPy1? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y1)stat.fit.paramdoublenullablef2QLPy1? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y1)stat.fit.paramdoublenullablef3QLPy1? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y1)stat.fit.paramdoublenullablef4QLPy1? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y1)stat.fit.paramdoublenullablef5QLPy1? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y1)stat.fit.paramdoublenullablef6QLPy1? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y1)stat.fit.paramfloatnullablef4QLPy2? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y2)stat.fit.paramdoublenullablef5QLPy2? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y2)stat.fit.paramdoublenullablef6QLPy2? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y2)stat.fit.paramfloatnullableslikeQLPy2? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_qlp_y2)meta.codefloatnullablewideQLPy2? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_qlp_y2)meta.codefloatnullablet0QLPy3? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_qlp_y3)dtime.epochdoublenullablePerQLPy3? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_qlp_y3)dtime.perioddoublenullablescoreQLPy3? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y3)stat.fit.paramfloatnullablef1QLPy3? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y3)stat.fit.paramdoublenullablef2QLPy3? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y3)stat.fit.paramdoublenullablef3QLPy3? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y3)stat.fit.paramdoublenullablef4QLPy3? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y3)stat.fit.paramdoublenullablef5QLPy3? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y3)stat.fit.paramdoublenullablef6QLPy3? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y3)stat.fit.paramfloatnullableslikeQLPy3? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_qlp_y3)meta.codefloatnullablewideQLPy3? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_qlp_y3)meta.codefloatnullablet0QLPy4? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_qlp_y4)dtime.epochdoublenullablePerQLPy4? Orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_qlp_y4)dtime.perioddoublenullablescoreQLPy4? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y4)stat.fit.paramfloatnullablef1QLPy4? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y4)stat.fit.paramdoublenullablef2QLPy4? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y4)stat.fit.paramdoublenullablef3QLPy4? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y4)stat.fit.paramdoublenullablef4QLPy4? Feature 4 that goes into the ECLIPSR score value (f_4_qlp_y4)stat.fit.paramdoublenullablef5QLPy4? Feature 5 that goes into the ECLIPSR score value (f_5_qlp_y4)stat.fit.paramdoublenullablef6QLPy4? Feature 6 that goes into the ECLIPSR score value (f_6_qlp_y4)stat.fit.paramfloatnullableslikeQLPy4? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_qlp_y4)meta.codefloatnullablescoreSum of score values across all datasets (SPOC and QLP years 1-4) (score)stat.fit.paramfloatslikeSum of sine_like values across all datasets (SPOC and QLP years 1-4) (sine_like)meta.codefloatwideSum of wide values across all datasets (SPOC and QLP years 1-4) (wide)meta.codefloatCatOri? Original external catalogue source identifier from 2MASS (original_ext_source_id)meta.id;meta.datasetcharDist? Gaia distance from GSP-Phot Aeneas best library using BP/RP spectra (distance_gspphot)pcpos.distancedoublenullableB_TeffMSC1? Gaia upper confidence level (84%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_upper)Kphys.temperature.effective;phys.atmol.leveldoublenullableb_TeffMSC1? Gaia lower confidence level (16%) of effective temperature of the primary from MSC using BP/RP spectra and parallax (teff_msc1_lower)Kphys.temperature.effective;phys.atmol.leveldoublenullableTeffMSC2? Gaia effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2)Kphys.temperature.effectivedoublenullableB_TeffMSC2? Gaia upper confidence level (84%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_upper)Kphys.temperature.effective;phys.atmol.leveldoublenullableb_TeffMSC2? Gaia lower confidence level (16%) of effective temperature of the secondary from MSC using BP/RP spectra and parallax (teff_msc2_lower)Kphys.temperature.effective;phys.atmol.leveldoublenullableloggMSC1? Gaia surface gravity of the primary from MSC using BP/RP spectra and parallax (log) (logg_msc1)log(cm.s**-2)phys.gravitydoublenullablef6SPOCy1? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y1)stat.fit.paramfloatnullablef4SPOCy4? Feature 4 that goes into the ECLIPSR score value (f_4_spoc_y4)stat.fit.paramdoublenullablef5SPOCy4? Feature 5 that goes into the ECLIPSR score value (f_5_spoc_y4)stat.fit.paramdoublenullablef6SPOCy4? Feature 6 that goes into the ECLIPSR score value (f_6_spoc_y4)stat.fit.paramfloatnullableslikeQLPy1? Boolean flag (0 or 1) indicating likely (purely) sinusoidal signal (sine_like_qlp_y1)meta.codefloatnullablewideQLPy1? Boolean flag (0 or 1) indicating likely wide eclipses (in phase space) (wide_qlp_y1)meta.codefloatnullablet0QLPy2? Time of superior conjunction (midpoint of primary eclipse) (TESS BJD = BJD-2457000) (t_zero_qlp_y2)dtime.epochdoublenullablePerQLPy2? orbital period or half the orbital period (for indistinguishable primary and secondary) (days) (period_qlp_y2)dtime.perioddoublenullablescoreQLPy2? Score value between 0 and 1 by ECLIPSR (see documentation) (score_qlp_y2)stat.fit.paramfloatnullablef1QLPy2? Feature 1 that goes into the ECLIPSR score value (f_1_qlp_y2)stat.fit.paramdoublenullablef2QLPy2? Feature 2 that goes into the ECLIPSR score value (f_2_qlp_y2)stat.fit.paramdoublenullablef3QLPy2? Feature 3 that goes into the ECLIPSR score value (f_3_qlp_y2)stat.fit.paramdoublenullable