|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| HATS-69b , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:09:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2019AJ....157...55H |
487 | T A | D | X C | 11 | 22 | 11 |
HATS-60b- HATS-69b: 10 transiting planets from HATSouth. |
HARTMAN J.D., BAKOS G.A., BAYLISS D., et al. |
|
2019A&A...630A.135U |
16 | D | 1 | 501 | 16 | Beyond the exoplanet mass-radius relation. | ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al. | ||
|
2020AJ....160..214S |
16 | D | 1 | 129 | ~ | (nature) versus nurture: a Bayesian framework for assessing apparent correlations between planetary orbital properties and stellar ages. | SAFSTEN E.D., DAWSON R.I. and WOLFGANG A. | ||
|
2021AJ....162..263H |
17 | D | 1 | 346 | 17 | A uniform search for nearby planetary companions to hot Jupiters in TESS data reveals hot Jupiters are still lonely. | HORD B.J., COLON K.D., KOSTOV V., et al. | ||
|
2022AJ....163..228P |
17 | D | 1 | 354 | 20 | Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS. | PATEL J.A. and ESPINOZA N. | ||
| 2023A&A...672A..78M | 87 | X | 2 | 15 | ~ | Pathways of survival for exomoons and inner exoplanets. | MAKAROV V.V. and EFROIMSKY M. | ||
|
2024AJ....167....1W |
18 | D | 1 | 336 | ~ | A Blind Search for Transit Depth Variability with TESS. | WANG G. and ESPINOZA N. | ||
|
2024ApJS..270...14W |
18 | D | 1 | 333 | ~ | Long-term Variations in the Orbital Period of Hot Jupiters from Transit-timing Analysis Using TESS Survey Data. | WANG W., ZHANG Z., CHEN Z., et al. | ||
|
2024ApJS..275...32Z |
18 | D | 1 | 264 | ~ | Constraining the Presence of Companion Planets in Hot Jupiter Planetary Systems Using Transit-timing Variation Observations from TESS. | ZHANG Z., WANG W., MA X., et al. |