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| KOI-2272 , the SIMBAD biblio (32 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST03:12:14 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
2013ApJS..204...24B |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
16 | D | 1 | 2864 | ~ | Evidence for spots on hot stars suggests major revision of stellar physics. | BALONA L.A. | ||
|
2020A&A...633A..99C |
16 | D | 1 | 257585 | 169 | Clusters and mirages: cataloguing stellar aggregates in the Milky Way. | CANTAT-GAUDIN T. and ANDERS F. | ||
|
2020ApJ...890...23L |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
17 | D | 2 | 4599 | 5 | LAMOST meets Gaia: The Galactic open clusters. | FU X., BRAGAGLIA A., LIU C., et al. | ||
|
2023ApJS..265...50C |
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 |
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 |
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. |