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| KOI-4407 , the SIMBAD biblio (42 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:26:50 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2010AstL...36..338F |
15 | D | 1 | 1150 | 6 | Proper motions and CCD photometry of stars in the region of the open cluster NGC 6866. | FROLOV V.N., ANANJEVSKAJA Y.K., GORSHANOV D.L., 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. | ||
|
2014ApJ...788L...9B |
15 | D | 1 | 293 | 26 | Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars. | BASTIEN F.A., STASSUN K.G. and PEPPER J. | ||
| 2015AJ....149...55E | 796 | D | X | 21 | 48 | 34 | High-resolution multi-band imaging for validation and characterization of small Kepler planets. | EVERETT M.E., BARCLAY T., CIARDI D.R., 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...813..130W |
16 | D | 3 | 211 | 27 | Influence of stellar multiplicity on planet formation. IV. Adaptive optics imaging of Kepler stars with multiple transiting planet candidates. | WANG J., FISCHER D.A., XIE J.-W., 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. | ||
|
2016AJ....152....8K |
16 | D | 1 | 389 | 203 | The impact of stellar multiplicity on planetary systems. I. The ruinous influence of close binary companions. | KRAUS A.L., IRELAND M.J., HUBER D., et al. | ||
|
2016AJ....152...18B |
16 | D | 5 | 1167 | 34 | Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars. | BARANEC C., ZIEGLER C., LAW N.M., et al. | ||
|
2016A&A...594A..39F |
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2016AJ....152..187M |
16 | D | 1 | 471 | 74 | A super-solar metallicity for stars with hot rocky exoplanets. | MULDERS G.D., PASCUCCI I., APAI D., et al. | ||
|
2017AJ....153...25A |
179 | 7 | Probability of the physical association of 104 blended companions to Kepler Objects of Interest using visible and near-infrared adaptive optics photometry. | ATKINSON D., BARANEC C., ZIEGLER C., 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. | ||
|
2017AJ....154..107P |
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 |
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. | ||
|
2018ApJ...855..115B |
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 |
16 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
|
2018ApJ...861..149F |
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. | ||
|
2018AJ....156...83Z |
16 | D | 1 | 337 | 14 | Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. | ZIEGLER C., LAW N.M., BARANEC C., et al. | ||
|
2018A&A...615A..49C |
16 | D | 1 | 224763 | 54 | Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. | CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al. | ||
|
2018ApJS..237...38B |
16 | D | 1 | 1111 | 42 | Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. | BREWER J.M. and FISCHER D.A. | ||
|
2018ApJ...866...99B |
16 | D | 1 | 7129 | 233 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
|
2018AJ....156..292T |
16 | D | 1 | 647 | 8 | The effects of stellar companions on the observed transiting exoplanet radius distribution. | TESKE J.K., CIARDI D.R., HOWELL S.B., et al. | ||
|
2019ApJ...875...29M |
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. | ||
|
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. | ||
|
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..108B |
16 | D | 1 | 6855 | 109 | The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. | BERGER T.A., HUBER D., GAIDOS E., 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. | ||
|
2021ApJ...909..115C |
17 | D | 1 | 2176 | 13 | Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. | CHEN D.-C., XIE J.-W., ZHOU J.-L., 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 |
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..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. | ||
|
2022AJ....163..179P |
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. | ||
|
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. | ||
|
2022A&A...663A...4S |
17 | D | 1 | 14206 | 7 | Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. | SOUBIRAN C., BROUILLET N. and CASAMIQUELA L. | ||
|
2023NatAs...7..900C |
17 | D | 1 | 1054 | ~ | On the behaviour of spin-orbit connection of exoplanets. | CANTO MARTINS B.L., MESSIAS Y.S., ARRUDA GONCALVES M.I., 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. | ||
|
2024AJ....168..129S |
18 | D | 1 | 350 | ~ | Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. | SULLIVAN K., KRAUS A.L., BERGER T.A., et al. | ||
| 2024MNRAS.534..575E | 45 | X | 1 | 51 | ~ | Orbital architectures of planet-hosting binaries - III. Testing mutual inclinations of stellar and planetary orbits in triple-star systems. | EVANS E.L., DUPUY T.J., SULLIVAN K., et al. | ||
|
2024A&A...689A.250C |
18 | D | 1 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. |