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BD-09 6003b , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.05.29CEST08:28:41 |
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 |
---|---|---|---|---|---|---|---|---|---|
2016ApJS..226....7C ![]() |
16 | D | 1 | 400 | 70 | 197 candidates and 104 validated planets in K2's first five fields. | CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al. | ||
2016AJ....152..143V | 756 | A | X C | 18 | 20 | 21 | The K2-ESPRINT project V: a short-period giant planet orbiting a subgiant star. | VAN EYLEN V., ALBRECHT S., GANDOLFI D., et al. | |
2016AJ....152..182H ![]() |
41 | X | 1 | 205 | 18 | HAT-P-65b and HAT-P-66b: two transiting inflated hot Jupiters and observational evidence for the reinflation of close-in giant planets. | HARTMAN J.D., BAKOS G.A., BHATTI W., et al. | ||
2016AJ....152..185G | 44 | X | 1 | 7 | 27 | K2-97b: a (re-?)inflated planet orbiting a red giant star. | GRUNBLATT S.K., HUBER D., GAIDOS E.J., et al. | ||
2017AJ....153..142P ![]() |
510 | D | X C | 12 | 30 | 17 | Four sub-Saturns with dissimilar densities: windows into planetary cores and envelopes. | PETIGURA E.A., SINUKOFF E., LOPEZ E.D., et al. | |
2017MNRAS.464.2708S | 43 | X | 1 | 6 | 13 | K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion. | SMITH A.M.S., GANDOLFI D., BARRAGAN O., et al. | ||
2017AJ....153..211Z ![]() |
82 | X | 2 | 24 | 11 | HAT-P-67b: an extremely low density Saturn transiting an F-subgiant confirmed via Doppler tomography. | ZHOU G., BAKOS G.A., HARTMAN J.D., et al. | ||
2017AJ....153..215P ![]() |
42 | X | 1 | 13 | 19 | KELT-11b: A highly inflated sub-Saturn exoplanet transiting the V = 8 subgiant HD 93396. | PEPPER J., RODRIGUEZ J.E., COLLINS K.A., et al. | ||
2018ApJ...861L...5G | 17 | D | 1 | 9 | 1 | Do close-in giant planets orbiting evolved stars prefer eccentric orbits? | GRUNBLATT S.K., HUBER D., GAIDOS E., et al. | ||
2018AJ....156...70D | 42 | X | 1 | 15 | 1 | Characterizing K2 candidate planetary systems orbiting low-mass stars. III. A high mass and low envelope fraction for the warm Neptune K2-55b. | DRESSING C.D., SINUKOFF E., FULTON B.J., et al. | ||
2018AJ....156..182L | 84 | C | 1 | 12 | 1 | K2 targets observed with SPHERE/VLT: an M4-7 dwarf companion resolved around EPIC 206011496. | LIGI R., DEMANGEON O., BARROS S., et al. | ||
2019MNRAS.484.3233B | 43 | X | 1 | 35 | ~ | HARPS-N radial velocities confirm the low densities of the Kepler-9 planets. | BORSATO L., MALAVOLTA L., PIOTTO G., et al. | ||
2019AJ....158...45B ![]() |
43 | X | 1 | 11 | ~ | HD 1397b: a transiting warm giant planet orbiting a V = 7.8 mag subgiant star discovered by TESS. | BRAHM R., ESPINOZA N., JORDAN A., et al. | ||
2019MNRAS.488.3067H | 85 | C | 2 | 21 | ~ | WASP-166b: a bloated super-Neptune transiting a V = 9 star. | HELLIER C., ANDERSON D.R., TRIAUD A.H.M.J., et al. | ||
2019A&A...630A.135U ![]() |
17 | D | 1 | 501 | ~ | Beyond the exoplanet mass-radius relation. | ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al. | ||
2020AJ....159...41T ![]() |
17 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
2021ApJ...921...24S | 18 | D | 1 | 328 | ~ | The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. | SCHLAUFMAN K.C. and HALPERN N.D. | ||
2021AJ....162..273S | 45 | X | 1 | 6 | ~ | Lithium enrichment signatures of planetary engulfment events in evolved stars. | SOARES-FURTADO M., CANTIELLO M., MacLEOD M., et al. | ||
2023AJ....165...44G | 20 | D | 1 | 27 | ~ | TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period-Eccentricity Relation for Giant Planets Transiting Evolved Stars. | GRUNBLATT S.K., SAUNDERS N., CHONTOS A., et al. | ||
2023A&A...670A..26T | 50 | X | 1 | 16 | ~ | Occurrence rate of hot Jupiters orbiting red giant stars. | TEMMINK M. and SNELLEN I.A.G. |
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