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| * 24 Boo b , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:37:35 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2018ApJS..239...14J 
|
16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
| 2018PASJ...70...59T | 377 | D | X C | 9 | 31 | 12 | Planets around the evolved stars 24 Boötis and {gam} Libra: A 30 d-period planet and a double giant-planet system in possible 7:3 MMR. | TAKARADA T., SATO B., OMIYA M., et al. | |
|
2019PASP..131c4401D
|
16 | D | 2 | 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...876...23G
|
16 | D | 1 | 496 | 3 | Multiple Populations of extrasolar gas giants. | GODA S. and MATSUO T. | ||
|
2021A&A...645A...7K
|
17 | D | 2 | 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. | ||
| 2022PASJ...74...92T | 85 | X | 2 | 34 | 4 | Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate. | TENG H.-Y., SATO B., TAKARADA T., et al. | ||
| 2023PASJ...75.1030T | 17 | D | 1 | 99 | ~ | Revisiting planetary systems in the Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and a multiplicity-metallicity trend around evolved stars. | TENG H.-Y., SATO B., KUZUHARA M., et al. | ||
| 2025ApJS..280...76M | 112 | D | C | 3 | 410 | ~ | Exploring Warm Jupiter Migration Pathways with Eccentricities. I. Catalog of Uniform Keplerian Fits to Radial Velocities of 200 Warm Jupiters. | MORGAN M., BOWLER B.P., TRAN Q.H., et al. |
