KOI-2272 , the SIMBAD biblio

KOI-2272 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST03:12:14


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Title First 3 Authors
2013ApJS..204...24B viz 15       D               1 3274 922 Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data. BATALHA N.M., ROWE J.F., BRYSON S.T., et al.
2013ApJ...775L..11M viz 15       D               1 2010 189 Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators. McQUILLAN A., MAZEH T. and AIGRAIN S.
2014ApJS..210...19B viz 15       D               1 5860 211 Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). BURKE C.J., BRYSON S.T., MULLALLY F., et al.
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.
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.
2015ApJ...814..130M viz 16       D               1 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
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.
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.
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.
2018AJ....156..142D viz 16       D               1 1381 47 The Open Cluster Chemical Abundances and Mapping survey. II. Precision cluster abundances for APOGEE using SDSS DR14. DONOR J., FRINCHABOY P.M., CUNHA K., et al.
2018A&A...618A..93C viz 16       D               1 87620 517 A Gaia DR2 view of the open cluster population in the Milky Way. CANTAT-GAUDIN T., JORDI C., VALLENARI A., et al.
2019A&A...623A..80C viz 16       D               1 1585 60 Open clusters in APOGEE and GALAH. Combining Gaia and ground-based spectroscopic surveys. CARRERA R., BRAGAGLIA A., CANTAT-GAUDIN T., et al.
2019MNRAS.485.2380M viz 16       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., 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.
2019MNRAS.490.2112B viz 16       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2020A&A...633A..99C viz 16       D               1 257585 169 Clusters and mirages: cataloguing stellar aggregates in the Milky Way. CANTAT-GAUDIN T. and ANDERS F.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., 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.
2020A&A...640A...1C viz 16       D               1 235399 241 Painting a portrait of the Galactic disc with its stellar clusters. CANTAT-GAUDIN T., ANDERS F., CASTRO-GINARD A., et al.
2020A&A...640A.127Z viz 16       D               1 9108 33 Exploring open cluster properties with Gaia and LAMOST. ZHONG J., CHEN L., WU D., et al.
2021A&A...647A..19T viz 17       D               1 24814 55 3D kinematics and age distribution of the open cluster population. TARRICQ Y., SOUBIRAN C., CASAMIQUELA L., et al.
2021MNRAS.503.3279S viz 17       D               1 104620 56 The GALAH survey: tracing the Galactic disc with open clusters. SPINA L., TING Y.-S., DE SILVA G.M., 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..257...46G viz 17       D               1 10775 37 Stellar rotation in the Gaia era: revised open clusters' sequences. GODOY-RIVERA D., PINSONNEAULT M.H. and REBULL L.M.
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.
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.
2022ApJS..262....7H viz 17       D               1 134735 19 A Blind All-sky Search for Star Clusters in Gaia EDR3: 886 Clusters within 1.2 kpc of the Sun. HE Z., WANG K., LUO Y., et al.
2022A&A...668A...4F viz 17       D               2 4599 5 LAMOST meets Gaia: The Galactic open clusters. FU X., BRAGAGLIA A., LIU C., 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.
2023AJ....166..219D viz 17       D               1 275 ~ Understanding the Planetary Formation and Evolution in Star Clusters (UPiC). I. Evidence of Hot Giant Exoplanets Formation Timescales. DAI Y.-Z., LIU H.-G., YANG J.-Y., et al.
2024AJ....168..109S viz 18       D               2 702 ~ Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H.

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