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| KOI-4823 , the SIMBAD biblio (16 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST04:10:01 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
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. | ||
|
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...18B |
16 | D | 2 | 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. | ||
|
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. | ||
|
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. | ||
|
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....159..124K |
16 | D | 1 | 131 | ~ | Searching the entirety of Kepler data. I. 17 new planet candidates including one Habitable Zone world. | KUNIMOTO M., MATTHEWS J.M. and NGO H. | ||
| 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. | ||
|
2023AJ....165..177S |
104 | D | X | 3 | 131 | ~ | Revising Properties of Planet-Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems. | SULLIVAN K., KRAUS A.L., HUBER D., et al. | |
|
2024AJ....168..129S |
18 | D | 2 | 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. | ||
|
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. | ||
| 2025AJ....169...29S | 19 | D | 2 | 39 | ~ | Quantifying the Contamination from nearby Stellar Companions in Gaia DR3 Photometry. | SULLIVAN K., KRAUS A.L., BERGER T.A., et al. |