KOI-3278 , the SIMBAD biblio

KOI-3278 , the SIMBAD biblio (65 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:14:04


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Title First 3 Authors
2011A&A...529A..89D viz 15       D               1 3298 98 Global stellar variability study in the field-of-view of the Kepler satellite. DEBOSSCHER J., BLOMME J., AERTS C., et al.
2013A&A...557L..10N viz 15       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2013A&A...560A...4R viz 15       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014AJ....147..119C viz 15       D               1 8013 91 Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al.
2014Sci...344..275K 12 2 51 KOI-3278: a self-lensing binary star system. KRUSE E. and AGOL E.
2014A&A...568L...9Z 1341 T   A S   X C       32 2 10 The evolution of the self-lensing binary
KOI-3278: evidence of extra energy sources during CE evolution.
ZOROTOVIC M., SCHREIBER M.R. and PARSONS S.G.
2015ApJ...801....3M viz 16       D               1 3357 109 Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. MAZEH T., PERETS H.B., McQUILLAN A., et al.
2015ApJS..217...16R viz 16       D               1 8625 149 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2015MNRAS.449.2194P 55       D     X         2 99 33 14 new eclipsing white dwarf plus main-sequence binaries from the SDSS and Catalina surveys. PARSONS S.G., AGURTO-GANGAS C., GANSICKE B.T., et al.
2015ApJ...807..135L 39           X         1 10 7 Nearby stars as gravitational wave detectors. LOPES I. and SILK J.
2015ApJ...807..170H viz 16       D               1 2117 10 Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. HOLCZER T., SHPORER A., MAZEH T., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015MNRAS.452.1754P 78           X         2 4 6 The first pre-supersoft X-ray binary. PARSONS S.G., SCHREIBER M.R., GANSICKE B.T., et al.
2016ApJ...820...53H 118           X         3 1 1 Degeneracy between lensing and occultation in the analysis of self-lensing phenomena. HAN C.
2016ApJ...822...86M viz 16       D               1 6130 337 False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al.
2016ApJS..225....9H viz 16       D               1 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2016ApJS..225...32B viz 16       D               2 1473 266 Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. BREWER J.M., FISCHER D.A., VALENTI J.A., et al.
2017AJ....153...71F viz 16       D               1 3575 164 The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. FURLAN E., CIARDI D.R., EVERETT M.E., et al.
2016MNRAS.463.2125P viz 39           X         1 438 38 The white dwarf binary pathways survey - I. A sample of FGK stars with white dwarf companions. PARSONS S.G., REBASSA-MANSERGAS A., SCHREIBER M.R., et al.
2017MNRAS.465.2634A viz 16       D               1 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2016PASP..128h2001H 39           X         1 160 254 Hot subluminous stars. HEBER U.
2017AJ....154..107P viz 16       D               1 1306 226 The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets. PETIGURA E.A., HOWARD A.W., MARCY G.W., et al.
2017AJ....154..108J viz 16       D               1 3237 137 The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al.
2018AJ....155..144K 321           X C       7 23 22 Discovery of three self-lensing binaries from Kepler. KAWAHARA H., MASUDA K., MacLEOD M., et al.
2018ApJ...855..115B viz 16       D               1 1305 5 Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. BERGER T.A., HOWARD A.W. and BOESGAARD A.M.
2018MNRAS.474.2094A viz 16       D               1 1073 143 Inferring probabilistic stellar rotation periods using Gaussian processes. ANGUS R., MORTON T., AIGRAIN S., et al.
2018ApJ...861..149F viz 16       D               1 2261 6 The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2018ApJ...869L..29L 16       D               1 13 4 Observations of spin-down in post-mass-transfer stars and the possibility for blue straggler gyrochronology. LEINER E., MATHIEU R.D., GOSNELL N.M., et al.
2019ApJ...875...29M viz 16       D               1 2918 72 A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. MARTINEZ C.F., CUNHA K., GHEZZI L., et al.
2019MNRAS.487.1040M 41           X         1 16 4 The post-common-envelope binary nucleus of the planetary nebula IC 4776: neither an anomalously long orbital period nor a Wolf-Rayet binary. MISZALSKI B., MANICK R., VAN WINCKEL H., et al.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019ApJ...880...33Y 999 T   A     X C       23 1 ~ The mass of the white dwarf companion in the self-lensing binary
KOI-3278: Einstein versus Newton.
YAHALOMI D.A., SHVARTZVALD Y., AGOL E., et al.
2019ApJ...881L...3M 84               F     1 8 28 Self-lensing discovery of a 0.2 M☉ white dwarf in an unusually wide orbit around a Sun-like star. MASUDA K., KAWAHARA H., LATHAM D.W., et al.
2019MNRAS.490.2550I 16       D               1 97 38 Speaking with one voice: simulations and observations discuss the common envelope α parameter. IACONI R. and DE MARCO O.
2020A&A...636A..85S viz 16       D               1 3696 ~ Derivation of parameters for 3748 FGK stars using H-band spectra from APOGEE Data Release 14. SARMENTO P., DELGADO MENA E., ROJAS-AYALA B., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021MNRAS.501..676L 87           X         2 8 27 WD 1856 b: a close giant planet around a white dwarf that could have survived a common envelope phase. LAGOS F., SCHREIBER M.R., ZOROTOVIC M., et al.
2021MNRAS.501.1677H 44           X         1 10 21 The White Dwarf Binary Pathways Survey - IV. Three close white dwarf binaries with G-type secondary stars. HERNANDEZ M.S., SCHREIBER M.R., PARSONS S.G., et al.
2021MNRAS.504.5327A 17       D               1 7000 19 Exoplanet validation with machine learning: 50 new validated Kepler planets. ARMSTRONG D.J., GAMPER J. and DAMOULAS T.
2021ApJS..255...17S viz 17       D               1 39591 57 Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. SANTOS A.R.G., BRETON S.N., MATHUR S., et al.
2022AJ....163..128W viz 17       D               1 1570 6 The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022AJ....163..179P viz 17       D               1 2962 39 The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. PETIGURA E.A., ROGERS J.G., ISAACSON H., et al.
2022MNRAS.512.1843H 60       D     X         2 15 13 The white dwarf binary pathways survey - VI. Two close post-common envelope binaries with TESS light curves. HERNANDEZ M.S., SCHREIBER M.R., PARSONS S.G., et al.
2022MNRAS.512.2625L 170           X   F     3 10 6 The white dwarf binary pathways survey - VII. Evidence for a bi-modal distribution of post-mass transfer systems? LAGOS F., SCHREIBER M.R., PARSONS S.G., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022MNRAS.513.3090S 43           X         1 64 8 Magnetic dynamos in white dwarfs - III. Explaining the occurrence of strong magnetic fields in close double white dwarfs. SCHREIBER M.R., BELLONI D., ZOROTOVIC M., et al.
2022MNRAS.513.3587Z 85           X         2 19 13 Close detached white dwarf + brown dwarf binaries: further evidence for low values of the common envelope efficiency. ZOROTOVIC M. and SCHREIBER M.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2022ApJ...936...33Z 85               F     1 12 4 A White Dwarf-Main-sequence Binary Unveiled by Time-domain Observations from LAMOST and TESS. ZHENG L.-L., GU W.-M., SUN M., et al.
2022ApJ...936...63S 85           X         2 4 1 Modeling Long-term Variability in Stellar-compact Object Binary Systems for Mass Determinations. SORABELLA N.M., BHATTACHARYA S., LAYCOCK S.G.T., et al.
2022MNRAS.517.2867H 255           X C F     4 9 5 The white dwarf binary pathways survey - VIII. A post-common envelope binary with a massive white dwarf and an active G-type secondary star. HERNANDEZ M.S., SCHREIBER M.R., PARSONS S.G., et al.
2023ApJS..265...50C viz 17       D               1 2291 ~ Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N. CANAS C.I., BENDER C.F., MAHADEVAN S., et al.
2023MNRAS.518.4579P 87           X         2 15 1 The white dwarf binary pathways survey - IX. Three long period white dwarf plus subgiant binaries. PARSONS S.G., HERNANDEZ M.S., TOLOZA O., et al.
2024MNRAS.52711719Y 358           X C F     6 11 ~ Wide post-common envelope binaries containing ultramassive white dwarfs: evidence for efficient envelope ejection in massive asymptotic giant branch stars. YAMAGUCHI N., EL-BADRY K., FULLER J., et al.
2024A&A...686A..61B 45           X         1 9 ~ Formation of long-period post-common envelope binaries I. No extra energy is needed to explain oxygen-neon white dwarfs paired with AFGK-type main-sequence stars. BELLONI D., ZOROTOVIC M., SCHREIBER M.R., et al.
2024A&A...686A.226B 90           X         2 9 ~ The formation of the magnetic symbiotic star FN Sgr. BELLONI D., MIKOLAJEWSKA J. and SCHREIBER M.R.
2024A&A...687A..12B 2016 T K A D S   X C       43 1 ~ Formation of long-period post-common-envelope binaries II. Explaining the self-lensing binary
KOI 3278.
BELLONI D., SCHREIBER M.R. and ZOROTOVIC M.
2024PASP..136g4201Y 179           X C       3 2 ~ No Longer Impossible: The Self-lensing Binary KIC 8145411 is a Triple. YAMAGUCHI N., EL-BADRY K., CIARDI D.R., et al.
2024ApJ...971...80S 197       D     X C       4 15 ~ Stellar Spin-down in Post-mass-transfer Binary Systems. SUN M., GOSSAGE S., LEINER E.M., et al.
2024MNRAS.533.1290S viz 18       D               1 7737 ~ The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. SEE V., LU Y., AMARD L., et al.
2024ApJ...972...60X 134           X         3 6 ~ Apparently Ultralong Period Radio Signals from Self-lensed Pulsar-Black Hole Binaries. XIAO X. and SHEN R.-F.
2024PASP..136h4202Y viz 45           X         1 34 ~ Wide Post-common Envelope Binaries from Gaia: Orbit Validation and Formation Models. YAMAGUCHI N., EL-BADRY K., REES N.R., et al.
2024PASP..136l4202Y 45           X         1 29 ~ A Search for Self-lensing Binaries with TESS and Constraints on their Occurrence Rate. YAMAGUCHI N., EL-BADRY K. and SORABELLA N.M.
2026ApJ...998...34B 200           X C       3 8 ~ A Correlation between the Final Separation and Mass Ratio from Common-envelope Simulations. BORGES S.V.

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