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| HATS-9 , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST16:33:15 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2015AJ....150...33B |
1694 | K | D | X C | 43 | 11 | 32 | HATS9-b and HATS10-b: two compact hot jupiters in field 7 of the K2 mission. | BRAHM R., JORDAN A., HARTMAN J.D., et al. |
|
2016ApJS..224....2H |
16 | D | 1 | 31769 | 226 | The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. | HUBER D., BRYSON S.T., HAAS M.R., et al. | ||
|
2016AJ....152...88R |
39 | X | 1 | 13 | 15 | HATS-11b AND HATS-12b: two transiting hot Jupiters orbiting subsolar metallicity stars selected for the K2 campaign 7. | RABUS M., JORDAN A., HARTMAN J.D., et al. | ||
|
2017A&A...602A.107B |
16 | D | 2 | 476 | 185 | The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets. | BONOMO A.S., DESIDERA S., BENATTI S., et al. | ||
|
2017A&A...603A..30S |
16 | D | 2 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
|
2018AJ....155...21P |
16 | D | 2 | 354 | 28 | Planet candidates from K2 campaigns 5-8 and follow-up optical spectroscopy. | PETIGURA E.A., CROSSFIELD I.J.M., ISAACSON H., et al. | ||
|
2018AJ....155..119B |
417 | D | S X | 10 | 35 | 6 | HATS-36b and 24 other transiting/eclipsing systems from the HATSouth-K2 Campaign 7 program. | BAYLISS D., HARTMAN J.D., ZHOU G., et al. | |
|
2018A&A...610A..20E |
40 | X | 1 | 115 | 9 | High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016. | EVANS D.F., SOUTHWORTH J., SMALLEY B., et al. | ||
|
2018AJ....155..165P |
16 | D | 1 | 83 | 54 | Empirical tidal dissipation in exoplanet hosts from tidal spin-up. | PENEV K., BOUMA L.G., WINN J.N., et al. | ||
|
2018AJ....155..177D |
40 | X | 1 | 124 | 2 | Stellar obliquity and magnetic activity of planet-hosting stars and eclipsing binaries based on transit chord correlation. | DAI F., WINN J.N., BERTA-THOMPSON Z., et al. | ||
|
2018ApJS..239...14J |
16 | D | 1 | 1561 | 6 | Revised exoplanet radii and habitability using Gaia data release 2. | JOHNS D., MARTI C., HUFF M., et al. | ||
|
2018AJ....156..277L |
16 | D | 1 | 306 | 50 | Sixty validated planets from K2 campaigns 5-8. | LIVINGSTON J.H., CROSSFIELD I.J.M., PETIGURA E.A., et al. | ||
|
2019AJ....157..124K |
16 | D | 1 | 603 | 7 | Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. | KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al. | ||
|
2019AJ....158...59S |
16 | D | 1 | 109 | ~ | Autoregressive planet search: feasibility study for irregular time series. | STUHR A.M., FEIGELSON E.D., CACERES G.A., et al. | ||
|
2019ApJS..244...11K |
16 | D | 1 | 2119 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
| 2019MNRAS.489.3149S | 16 | D | 1 | 66 | ~ | Estimation of singly transiting K2 planet periods with Gaia parallaxes. | SANDFORD E., ESPINOZA N., BRAHM R., et al. | ||
|
2020ApJ...890...23L |
16 | D | 1 | 4936 | 35 | Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. | LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al. | ||
| 2020A&A...641A..38G | 16 | D | 4 | 44 | ~ | TATOO: Tidal-chronology standalone tool to estimate the age of massive close-in planetary systems. | GALLET F. | ||
|
2021A&A...645A...7K |
17 | D | 1 | 1569 | 17 | Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. | KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al. | ||
|
2021ApJ...909..115C |
17 | D | 1 | 2176 | 13 | Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. | CHEN D.-C., XIE J.-W., ZHOU J.-L., et al. | ||
|
2021AJ....162..259Z |
17 | D | 1 | 1094 | 12 | Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. | ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al. | ||
|
2022MNRAS.509.1447M |
85 | F | 1 | 48 | 5 | The ultra-hot-Jupiter KELT-16 b: dynamical evolution and atmospheric properties. | MANCINI L., SOUTHWORTH J., NAPONIELLO L., et al. | ||
|
2022ApJS..259...62I |
17 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. | ||
|
2022A&A...663A.161M |
17 | D | 1 | 213 | 8 | Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. | MAGRINI L., DANIELSKI C., BOSSINI D., et al. | ||
|
2023AJ....165..262Z |
17 | D | 1 | 314 | ~ | Scaling K2. VI. Reduced Small-planet Occurrence in High-galactic-amplitude Stars. | ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al. | ||
| 2024ApJ...970...53L | 18 | D | 4 | 242 | ~ | Stellar Characterization and a Chromospheric Activity Analysis of a K2 Sample of Planet-hosting Stars. | LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al. | ||
|
2024A&A...688A.193D |
18 | D | 1 | 182 | ~ | Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars. | DA SILVA R., DANIELSKI C., DELGADO MENA E., et al. | ||
|
2024A&A...691A..53S |
18 | D | 1 | 4078 | ~ | SWEET-Cat: A view on the planetary mass-radius relation. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
| 2025ApJS..281...61L | 19 | D | 4 | 643 | ~ | Stellar Characterization, Magnesium Abundances, and Chromospheric Activity Analysis of Stars with Confirmed Exoplanets from the K2 Mission. | LOAIZA-TACURI V., SOUTO D., QUISPE-HUAYNASI F., et al. | ||
| 2026AJ....171..157S | 20 | D | 2 | 480 | ~ | Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr. | SCHMIDT S.P. and SCHLAUFMAN K.C. |