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| BD+37 2118c , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:04:56 |
| 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 | 17 | D | 1 | 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. | ||
|
2024A&A...682A.129M |
1389 | A | D | X C | 31 | 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 |
134 | X | 3 | 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..116R |
45 | X | 1 | 43 | ~ | Evidence for Primordial Alignment: Insights from Stellar Obliquity Measurements for Compact Sub-Saturn Systems. | RADZOM B.T., DONG J., RICE M., 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. | ||
|
2024A&A...689A.132M |
45 | X | 1 | 25 | ~ | Revisiting the dynamical masses of the transiting planets in the young AU Mic system: Potential AU Mic b inflation at ∼20 Myr. | MALLORQUIN M., BEJAR V.J.S., LODIEU N., et al. | ||
| 2024AJ....168..271M | 45 | X | 1 | 268 | ~ | DIAmante TESS AutoRegressive Planet Search (DTARPS). III. Understanding the DTARPS-S Candidate Transiting Planet Catalogs. | MELTON E.J., FEIGELSON E.D., MONTALTO M., et al. | ||
| 2024A&A...692A..77D | 134 | K A | D | X | 4 | 7 | ~ | The GAPS programme at TNG LXIII. Photo-evaporating puzzle: Exploring the enigmatic nature of TOI-5398 b's atmospheric signal. | D'ARPA M.C., GUILLUY G., MANTOVAN G., et al. |
| 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. |