KOI-3278 , the SIMBAD biblio

KOI-3278 , the SIMBAD biblio (47 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST10:18:45


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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 16       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 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014AJ....147..119C viz 16       D               1 8010 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 1363 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 56       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 40           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 79           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 121           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 40           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 41           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 329           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 17       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 42           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 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019ApJ...880...33Y 1028 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 87               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 17       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 17       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 17       D               1 365761 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 90           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 46           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.
2022AJ....163..128W viz 18       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.
2022MNRAS.512.1843H 63       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 179           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.
2022MNRAS.513.3090S 45           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 90           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.
2022ApJ...936...33Z 90               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 90           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 269           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.
2023MNRAS.518.4579P 93           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.

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