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CD-23 1056b , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST12:50:19 |
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 |
---|---|---|---|---|---|---|---|---|---|
2011PASP..123..412W | 15 | D | 1 | 2897 | 398 | The Exoplanet Orbit Database. | WRIGHT J.T., KAKHOURI O., MARCY G.W., et al. | ||
2013A&A...549A.109B | 1 | 172 | 551 | The HARPS search for southern extra-solar planets. XXXI. The M-dwarf sample. | BONFILS X., DELFOSSE X., UDRY S., et al. | ||||
2013A&A...552A.119S | 16 | D | 1 | 1487 | 118 | Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. | SAUR J., GRAMBUSCH T., DULING S., et al. | ||
2018MNRAS.475.3090Y | 16 | D | 1 | 483 | ~ | Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission. | YI J.S., CHEN J. and KIPPING D. | ||
2019PASP..131c4401D | 17 | D | 1 | 688 | 5 | Predicted yield of transits of known radial velocity exoplanets from the TESS primary and extended missions. | DALBA P.A., KANE S.R., BARCLAY T., et al. | ||
2019ApJ...887..261M | 226 | D | X | 6 | 329 | 29 | Exomoons in the habitable zones of M dwarfs. | MARTINEZ-RODRIGUEZ H., CABALLERO J.A., CIFUENTES C., et al. | |
2021A&A...645A...7K | 17 | D | 1 | 1569 | 17 | Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. | KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al. | ||
2021PASP..133i4401D | 132 | X | 3 | 12 | 17 | Survival of exomoons around exoplanets. | DOBOS V., CHARNOZ S., PAL A., et al. | ||
2022A&A...667A.102L | 63 | D | X | 2 | 14 | 6 | The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets Project goals, target selection, and stellar characterization. | LILLO-BOX J., SANTOS N.C., SANTERNE A., et al. | |
2023AJ....165..261R | 93 | F | 1 | 15 | ~ | Warm Jupiters Beyond the Tidal Synchronization Limit may Exhibit a Wide Range of Secondary Eclipse Depths. | RAUSCHER E., COWAN N.B. and LUGER R. |