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| CPD-66 1066c , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST02:24:52 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2023MNRAS.524.1113S | 1480 | A | D | S X C F | 32 | 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 
|
44 | X | 1 | 13 | ~ | A hot super-Earth planet in the WASP-84 planetary system. | MACIEJEWSKI G., GOLONKA J., LOBODA W., et al. | ||
|
2024A&A...682A.129M
|
134 | X | 3 | 21 | ~ | The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn. | MANTOVAN G., MALAVOLTA L., DESIDERA S., et al. | ||
|
2024A&A...684L..17M
|
45 | X | 1 | 25 | ~ | Orbital obliquity of the young planet TOI-5398 b and the evolutionary history of the system. | MANTOVAN G., MALAVOLTA L., LOCCI D., et al. | ||
|
2024AJ....168..115B
|
18 | D | 1 | 224 | ~ | Different Planetary Eccentricity-period (PEP) Distributions of Small and Giant Planets. | BASHI D., MAZEH T. and FAIGLER S. | ||
|
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. | ||
| 2025MNRAS.537.3175A | 19 | D | 1 | 68 | ~ | The NCORES programme: precise planetary masses, null results, and insight into the planet mass distribution near the radius gap. | ARMSTRONG D.J., OSBORN A., BURN R., 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. | ||
| 2025AJ....170..299K | 19 | D | 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. |
