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| BD+02 2056c , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST07:28:19 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2023MNRAS.524.1113S | 235 | D | X C F | 4 | 85 | ~ | TESS spots a mini- interior to a hot saturn in the TOI-2000 system. | SHA L., VANDERBURG A.M., HUANG C.X., et al. | |
|
2023MNRAS.525L..43M |
740 | A | D | S X C F | 15 | 13 | ~ | A hot super-Earth planet in the WASP-84 planetary system. | MACIEJEWSKI G., GOLONKA J., LOBODA W., et al. |
| 2024MNRAS.531.3698H | 206 | ~ | Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter. | HO C.S.K., ROGERS J.G., VAN EYLEN V., et al. | |||||
|
2024A&A...689A..52B |
90 | F | 1 | 21 | ~ | Characterisation of the warm-Jupiter TOI-1130 system with CHEOPS and a photo-dynamical approach. | BORSATO L., DEGEN D., LELEU A., et al. | ||
|
2025A&A...694A..15B |
93 | X | 2 | 9 | ~ | KOBE-1: The first planetary system from the KOBE survey Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf. | BALSALOBRE-RUZA O., LILLO-BOX J., SILVA A.M., et al. | ||
| 2025ApJ...987...30M | 19 | D | 1 | 23 | ~ | Three-dimensional Orbital Architectures and Detectability of Adjacent Companions to Hot Jupiters. | MacLEAN T. and BECKER J. | ||
| 2025ApJ...991..206Z | 19 | D | 1 | 31 | ~ | The Formation of Ultra-short-period Planets under the Influence of the Nearby Planetary Companions. | ZHU J., WANG S., JI J., et al. | ||
| 2025AJ....170..299K | 47 | X | 1 | 57 | ~ | Identifying Close-in Jupiters that Arrived via Disk Migration: Evidence of Primordial Alignment, Preference of Nearby Companions and Hint of Runaway Migration. | KAWAI Y., FUKUI A., WATANABE N., et al. | ||
| 2026ApJ...997..139H | 50 | X | 1 | 20 | ~ | Shedding Light on Desert Dwellers. | HALLATT T. and MILLHOLLAND S. | ||
| 2026ApJ...997..327B | 50 | X | 1 | 10 | ~ | Warm Jupiter Tidal Migration Can Spare Inner Planets; Hot Jupiter Tidal Migration May Not. | BECKER J. |