J/MNRAS/507/104ivo://CDS.VizieR/J/MNRAS/507/104doi:10.26093/cds/vizier.75070104CDSRowan D.M.Stanek K.Z.Jayasinghe T.Kochanek C.S.Thompson T.A.,Shappee B.J.Holoien T.W.-S.Prieto J.L.2024-11-06T20:34:18Z2024-07-24T12:41:22ZCDS support team

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

cds-question@unistra.frmilky-way-galaxyblack-holesx-ray-binary-starsvariable-starsx-ray-sourcesinfrared-astronomyvisible-astronomyThe majority of non-merging stellar mass black holes are discovered by observing high energy emission from accretion processes. Here, we pursue the large, but still mostly unstudied population of non-interacting black holes and neutron stars by searching for the tidally induced ellipsoidal variability of their stellar companions. We start from a sample of about 200000 rotational variables, semiregular variables, and eclipsing binary stars from the All-Sky Automated Survey for Supernovae. We use a {Chi}^2^ ratio test followed by visual inspection to identify 369 candidates for ellipsoidal variability. We also discuss how to combine the amplitude of the variability with mass and radius estimates for observed stars to calculate a minimum companion mass, identifying the most promising candidates for high mass companions.2021MNRAS.507..104Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/507/104CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)I/349 : StarHorse, Gaia DR2 photo-astrometric distancesJ/AcA/66/405 : Galactic bulge eclipsing & ellipsoidal binariesJ/MNRAS/504/5907 : OGLE Bulge short-period sample (Gomel+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/507/104https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/507/104http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/507/104https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/507/104https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/507/104http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/507/104GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/507/104/table1 (Properties of the 369 ELL candidates)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/507/104/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/507/104/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/507/104/table1?GETtext/xml+votable180.050000true149.6952917-44.66308330.0055555555555555566/11 445 465 946 955 1010 1383 1388 1390 1425 1495 1616 1680 1747 1899 2023 2432 2446 2512 2563 2698 2727 2854 2894 2998 3083 3117 3136 3224 3310-3311 3316 3371 3450 3465 3595 3757 4264 4389 4640 4969 5011 5666 5718 6009 6194 6455 6488 6496 6627 6986 8093 8665 8845 8961 9253 9271 9556 9718 9817 10742 11530 11542 11997 12333 12387 12445 12720 12762 12823 12833 12875 12990 13059 13064 13102 13220 13272 13492 13608 13812 13938 14076 14106 14110 14128 14165 14180 14232 14272 14346 14354 14395 14423 14435 14441 14490 14504 14790 14871 14898 14907 14919 14924 14996 15049 15052 15096 15156 15272 15334 15376 15394 15425 15616 15767 15802 15945 15986 16032 16280 18221 19256 19552 19992 20170 20213 20564 20582 20598 20733 20765 20951 21323 21378 21454 21462 21793 21960 22139 22207 22239 22404 23195 23344 23452 23547 23718 23757 23792 23937 23945 23955 23999 24028 24048 24054 24105 24108 24317 24337 24356 24549 26589 26960 28254 28503 28734 28834 28917 28994 29015 29043 29088 29225 29297 29333 29461 29516 29565 29715 29798 29873 29875 29945 29996 30035 30136 30295 30306 30383 30448 30479 30488 30514 30521 30529 30822 31366 31650 31711 31763 31822 31826 31828 31850 31855 31913 31933 31947 31963 32018 32025 32088 32113 32175 32201 32213 32293 32342 32346 32402 32532 32563 32567 33107 33111 33529 33657 34075 34239 34619 35015 35846 36179 37221 37226 37298 37322 37344 37354 37361 37392 37431 37548 37597 37612 37664 37687 37893 37909 37917 37945 37957 38030 38037 38132 38150 38330 38444 38448 38474 38496 38511 38680 39004 39096 39140 39179-39180 39194 39199 39372 39384 39563 39663 39685 39741 39771 39793 39823 39877 40352 40497 40561 40766 40799 41148 41247 41311 41316 41320 41381 41510 41562-41563 41608 41619 41684 41838 41868 42039 42156 42170 42271 42294 42301 42307 42347 42427 42448 42644 42672 42700 42711 42757 42778 42875 43067 43107 43112 43216 43287 43309 43312 43322 43336 43412 43522 43525 43560 43824 44002 44051 44359 44434 44673 45053 45198 45708 45775 45778 46748 46821 47194 47266 47375 47661 47663 47801 47809 47826 47839 47848 47854 47863 47958 48008 48067 48084 48578 48774 48811 48904 49025https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/507/104?format=asciiX-rayOpticalInfrareddefaultJ/MNRAS/507/104/table1Properties of the 369 ELL candidatesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintASASSN-VASAS-SN identifier (JHHMMSS.ss+DDMMSS.s) (asassn_name) (1)meta.id;meta.maincharPeriodPeriod (period) (1)dtime.perioddoubleEphemerisEphemeris for ELL analytic model (Ephemeris) (2)JDtime.epochdoublee2? The amplitude of the cos(2{theta}) Fourier term (e_2_) (3)stat.fit.paramfloatnullableM0? The mass scale most reliably measured by the light-curve models (M_0_) (4)solMassphys.massfloatnullableR*? Radius of the luminous primary (R_*_) (5)solRadphys.size.radiusfloatnullableM*? Luminous star mass (M_L_) (5)solMassphys.massfloatnullableMcmin? The minimum companion mass (M_cmin_) (6)solMassphys.massfloatnullable_RAPosition from name (right ascension part)degpos.eq.ra;meta.main_DEPosition from name (declination part)degpos.eq.dec;meta.main