J/MNRAS/520/2386ivo://CDS.VizieR/J/MNRAS/520/2386doi:10.26093/cds/vizier/bg-g8-2ajCDSRowan D.M.Jayasinghe T.Stanek K.Z.Kochanek C.S.Thompson T.A.,Shappee B.J.Holoien T.W.-S.Prieto J.L.Giles W.2026-08-03T07:32:39Z2026-04-24T15:46:22ZCDS support team

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

cds-question@unistra.freclipsing-binary-starsphotometryvariable-starsvisible-astronomyextinctionstellar-distanceabsolute-magnitudeastronomical-reference-materialsastronomical-object-identificationx-ray-sourcesDetached eclipsing binaries are the primary tool used to measure precise masses and radii of stars. In our previous paper estimating the parameters of more than 30000 detached eclipsing binaries, we identified 766 eclipsing binaries with additional features in their All-Sky Automated Survey for Supernovae (ASAS-SN) and Transiting Exoplanet Survey Satellite light curves. Here, we characterize these 'extra-physics' systems, identifying eclipsing binaries with spotted stars, pulsating components, and candidate triple/quadruple systems. We use the Gaia, Asteroid Terrestrial-impact Last Alert System (ATLAS), Zwicky Transient Facility (ZTF), and ASAS-SN variable star catalogues to search for possible blends. We use MIST (MESA Isochrones and Stellar Tracks) isochrones and evolutionary tracks to identify systems with main-sequence, subgiant, and giant primaries and highlight systems in sparsely populated regions of the colour-magnitude diagram. We find that the orbital period distribution of spotted binaries is divided by evolutionary state and find 68 with X-ray detections. For the candidate triple/quadruples and pulsating systems, we calculate the extra orbital/pulsational period and identify systems with resonances. Finally, we highlight a number of exotic systems, including eclipsing cataclysmic variables, subdwarfs, and binaries with discs.2023MNRAS.520.2386Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/520/2386CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/517/2190 : Physical properties of ~30000 ASAS-SN EBs (Rowan+, 2022)J/MNRAS/507/104 : Ellipsoidal variables in ASAS-SN catalog (Rowan+, 2021)J/MNRAS/503/3975 : Var., period. and contact binaries in WISE (Petrosky+, 2021)J/MNRAS/370/2013 : Catalogue of close binaries (Soydugan+, 2006)J/ApJ/867/105 : ATLAS all-sky stellar ref. catalog, ATLAS-REFCAT2J/A+A/664/A96 : Multiply eclipsing candidates from TESS satelliteJ/A+A/640/A36 : OB stars TESS phot. & high-resolution spectroscopyJ/A+A/635/A193 : Catalogue of hot subdwarf stars DR2 (Geier, 2020)J/A+A/606/A92 : Gaia LMC eclipsing binary and multiple systemsJ/A+A/560/A4 : Rotation periods of active Kepler stars (Reinhold+, 2013)J/A+A/453/635 : Modelling the Galactic Interstellar ExtinctionJ/ApJS/259/50 : EA-type eclipsing binaries observed by TESS (Shi+, 2022)J/ApJS/259/66 : Eclipsing quadruple star candidates from TESS (Kostov+,2022)J/ApJS/258/16 : TESS Eclipsing Binary stars. I. Sectors 1-26 (Prsa+, 2022)J/ApJS/258/26 : Spectroscopic binaries from LAMOST MRS. I. (Zhang+, 2022)J/ApJS/249/18 : The ZTF catalog of periodic variable stars (Chen+, 2020)J/ApJS/237/28 : WISE catalog of periodic variable stars (Chen+, 2018)J/AJ/154/250 : Kepler EB classifications and rotation periods (Lurie+,2017)J/AcA/66/421 : Eclipsing binaries in the Magellanic System (Pawlak+, 2016)J/AcA/65/297 : OGLE4 LMC and SMC Cepheids (Soszynski+, 2015)J/AcA/63/323 : OGLE-III SMC eclipsing binary stars (Pawlak+, 2013)J/AcA/61/217 : VI light curves of SMC long-period variablesIX/61 : 4XMM-DR9s serendipitous source catalogue from stacksV/110 : Catalog of Cataclysmic Variables (Downes+ 2001)II/340 : XMM-OM Serendipitous Source Survey Catalogue (XMM-SUSS2.1)II/339 : Swift/UVOT Serendipitous Source Catalog (Yershov, 2015)I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)B/cb : Cataclysmic Binaries, LMXBs, and related objectsB/sb9 : SB9: 9th Catalogue of Spectroscopic Binary Orbitshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/520/2386https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/520/2386http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/520/2386https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/520/2386https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/520/2386http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/520/2386GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/520/2386/extrap (Astrometric and physical informations of our ASAS-SN extra-physics variables sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/520/2386/extrap?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/520/2386/extrap?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/520/2386/extrap?GETtext/xml+votable180.050000true113.5204311468764-17.33792490838620.0055555555555555566/12 122 164 684 725 1029 1115 1150 1222 1301 1304 1337 1347 1352 1385-1386 1405 1409 1415 1426 1488 1501 1514 1562 1589 1599 1663 1698 1738 1763 1845 1873 1940 1979 2024 2201 2371 2400 2427 2470 2500 2528 2532 2543 2787 2852 2999 3059 3063 3089 3097 3119 3138 3140 3154 3162 3176 3248 3252 3278 3307 3311 3357 3368 3436 3459 3492 3517 3594 3598 3606 3609 3615 3626 3630 3649 3706 3714 3725-3726 3735 3828 3991 4032 4039 4138-4139 4272 4281 4608 4644 4699 5627 5849 6257 6266 6442 6462 6567 6626 6775 6788 7010 7086 7118 7270 7277 7342 7578 7588 7705 7756 7869 7894 7899 7968 8001 8167 8185 8414 9261 9304 9467 9574 9775 9831 10055 10155 10191 10534 11331 11349 11367 11924 11978 12142 12795 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37691 37708 37713 37719 37729 37731 37734 37741 37751 37780 37796 37812 37869-37870 37882-37883 37892 37894-37895 37897 37901-37902 37906-37908 37912 37920 37927-37928 37934 37938 37962 37971 37991 37999 38016 38018 38020 38047 38065 38118-38119 38253 38395 38410 38440 38451 38497 38501 38531 38566 38649 38685 38709 38711 38862 39002-39003 39057 39080 39211 39221 39238 39247 39262 39270 39352 39394 39399 39510 39573-39574 39637 39652 39676 39724 39731 39746 39750 39756 39764 39802 39812 39842 39856 39874 39877 39905 39912 39924-39925 39930 39935 39943 39965 39971 40012 40071 40090 40109 40122 40126 40176 40284 40386 40455 40512 40514 40563 40604 40654 40663 40679 40808 40857 41007 41034 41132 41152 41156 41158 41174 41190 41273 41288 41299 41471 41514 41550 41584 41587 41592 41597 41621 41677-41678 41687 41737 41749 41756 41760 41765 41771 41798 41806-41807 41813 41822 41830 41858 41881 41925 41971 42043 42053 42057 42115 42143 42154 42156-42157 42161 42165 42170 42193-42194 42212 42225 42229 42240 42294 42311 42321 42351 42361 42376 42380 42442 42452 42463 42481 42503 42510 42529 42535 42561 42567 42572 42600-42601 42625 42636 42641 42654 42776 42802 42817 42831 42853-42854 42890 43012 43016 43020 43029 43038 43058 43069 43084 43091 43115 43254 43269 43347 43430 43475 43522 43546 43560-43561 43589 43605 43630 43659 44060 44080 44120 44155 44178 44550 45216 45226 45377 45576 45578 45657 45751 45805 45927 45967 46143 46543 46720 46982 47150 47181 47231 47238 47272 47295-47296 47324 47352 47578 47646 47655 47657 47692 47760 47790 47799 47814 48010 48026 48050 48068 48098 48133 48205 48240 484131.9867573869263685e-19 3.916500758235022e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/520/2386?format=asciiX-rayOpticaldefaultJ/MNRAS/520/2386/extrapAstrometric and physical informations of our ASAS-SN extra-physics variables samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDASAS-SN ID used to match with light curve (id)meta.id;meta.maincharLCASAS-SN light curvesmeta.ref.urlcharcrmIndicates data in crmatchmeta.ref.urlcharSep? Source sky separation for X-ray detection and optical ASAS-SN target positions (xray_separation)arcsecpos.angDistancedoublenullableASASSN-VASAS-SN V-band catalog designation (asassn_name)meta.id.assoccharChristy23Display the new and known ASAS-SN V variable stars based on g-band light curves and cross-matches of Christy et al. 2023MNRAS.519.5271C, Cat. J/MNRAS/519/5271meta.ref.urlintnullableJaya18Display the ASAS-SN catalog of variable stars of Jayasinghe 2018MNRAS.477.3145J, Cat. II/366meta.ref.urlintnullableATLASDisplay the ATLAS-REFCAT2 of Tonry et al. 2018ApJ...867..105T, Cat. J/ApJ/867/105meta.ref.urlintnullableGaiaDR3Gaia DR3 Source identifier (source)meta.id.assocprimaryTICTESS Input Catalog v8.2 identifier (TIC)meta.id.assocRAJ2000Right ascension (J2000) (RA_ICRS)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (DE_ICRS)degpos.eq.dec;meta.mainPerOrbital period (period)dtime.perioddoubleP2? The given second orbital/pulsational/rotational period (p2)dtime.perioddoublenullablef_P2Method of subtraction method used to determine period P2 in section 3.2 Extra eclipses (p2_method_i)meta.codeintGroupType of extra-physics variability (group) (1)meta.codecharf_TICTrue if TESS QLP or SPOC light curve are available at 2022 October for 734 sources (has_tess)meta.codecharSectorNumber of TESS sectors with QLP or SPOC light curves (tess_sectors)meta.numbercharGmagGaia apparent G-band magnitude (Gmag)magphot.mag;em.optdoubleGMAG? Absolute gaia G-band magnitude (absolute_g)magphot.magdoublenullableBP-RPGaia BP-RP color (bp_rp)magphot.color;em.opt.B;em.opt.RdoubleBP-RPc? Gaia BP-RP color corrected for extinction (bp_rp_corrected)magphot.color;em.opt.B;em.opt.RdoublenullableRPlx? Gaia parallax to parallax error (parallax_over_error)stat.fit.omcdoublenullablerpgeo? Bailer-Jones photogeometric distance (rpgeo)pcpos.distancedoublenullableAV? V-band extinction from mwdust (mwdust_av)magphys.absorptiondoublenullableAG? G-band extinction from mwdust (mwdust_ag)magphys.absorptiondoublenullableABP? BP-band extinction from mwdust (mwdust_abp)magphys.absorptiondoublenullableARP? RP-band extinction from mwdust (mwdust_arp)magphys.absorptiondoublenullablef_IDParallax_over_error > 10 and mwdust_av < 2 (gaia_filter)meta.codecharStateState evolutionary state based on CMD position (state) (2)meta.codecharr1ATLAS REFCAT-2 r1 statistic from Tonry et al. 2018ApJ...867..105T, Cat. J/ApJ/867/105 (r1) (3)arcsecphys.angSize;srcfloatXrayThe boolean flag for X-ray detection in 74 cases in our sample (xray_source)meta.codecharObsName of X-ray observatory (xray_observatory) (4)meta.id;instr.obstycharr_XrayLiterature reference of Heasarc X-ray source (xray_citation_key) (5)meta.ref;pos.framecharADSLink to X-ray detection paper (xray_ads_link)meta.ref.urlcharExpTime? Exposure of X-ray observation (xray_exposure)sobs.param;obsdoublenullableLX? X-ray luminosity (xray_luminosity)1e-07Wphys.luminosity;em.X-raydoublenullableJ/MNRAS/520/2386/crmatchCross-matches of extra-physics targets to Gaia, ZTF, and ATLAS with a radius of 21 arcsecrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGaiaDR3Gaia DR3 Source identifier (Source)meta.id;meta.mainGmagGaia apparent G-band magnitude (Gmag)magphot.mag;em.optdoubleNGaiaDR3? The Gaia DR3 source identifier of the nearby star (Source_x)meta.id.assocnullableNGmag? Gaia apparent G-band magnitude of the nearby star (Gmag_x)magphot.mag;em.optdoublenullableGaiaSep? Gaia angular separation (angDist_x)arcsecpos.angDistancedoublenullableZTF? ZTF identifier from Zwicky Transient Facility (ZTF)meta.id.assocchargmag? The g-band associated magnitude (ztf_gmag)magphot.mag;em.opt.BfloatnullableZTFSep? Angular separation with ZTF (ztf_separation)arcsecpos.angDistancedoublenullableATLASATLAS refcat2 designation with RAdeg and DEdeg positions (ATOID)meta.id.assoccharomag? ATLAS median o-band magnitude (ls-o-med)magphot.mag;em.optfloatnullableATLASSep? Angular separation with ATLAS (Separation)arcsecpos.angDistancedoublenullableP2? Gaia or ZTF or ATLAS period if is within 5 per cent the rotation period, spotted period, or second orbital period in the TESS light curve (p2_best_match)dtime.perioddoublenullable