HAT-P-54 , the SIMBAD biblio

HAT-P-54 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:45:20

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
2015AJ....149..149B viz 1053   K A D     X C       27 11 10
HAT-P-54b: a hot Jupiter transiting a 0.6 m☉ star in field 0 of the K2 mission. 		BAKOS G.A., HARTMAN J.D., BHATTI W., et al.
2015AJ....149..166H viz 55       D     X         2 64 86 HATS-6b: a warm Saturn transiting an early M dwarf star, and a set of empirical relations for characterizing K and M dwarf planet hosts. HARTMAN J.D., BAYLISS D., BRAHM R., et al.
2015ApJ...806...97K 133       D     X C       3 93 15 Polarization in exoplanetary systems caused by transits, grazing transits, and starspots. KOSTOGRYZ N.M., YAKOBCHUK T.M. and BERDYUGINA S.V.
2015A&A...579A.129W 133       D     X         4 71 19 A Lucky Imaging search for stellar sources near 74 transit hosts. WOELLERT M. and BRANDNER W.
2016ApJS..222...14V viz 55       D     X         2 209 177 Planetary candidates from the first year of the K2 mission. VANDERBURG A., LATHAM D.W., BUCHHAVE L.A., et al.
2016ApJ...827....8N 371       D     X         10 43 105 Friends of hot jupiters. IV. Stellar companions beyond 50 au might facilitate giant planet formation, but most are unlikely to cause Kozai-Lidov migration. NGO H., KNUTSON H.A., HINKLEY S., et al.
2016ApJS..226....7C viz 16       D               5 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017A&A...601A...6K 79               F     1 15 2 Polarimetry of transiting planets: Differences between plane-parallel and spherical host star atmosphere models. KOSTOGRYZ N.M., YAKOBCHUK T.M., BERDYUGINA S.V., et al.
2017A&A...602A.107B viz 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 viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJ...856..155G viz 96       D       C       9 149 5 Giant planets: good neighbors for habitable worlds? GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I.
2018ApJS..239...14J viz 16       D               1 1561 6 Revised exoplanet radii and habitability using Gaia data release 2. JOHNS D., MARTI C., HUFF M., et al.
2018A&A...620A..58S viz 16       D               1 164 10 SWEET-Cat updated. New homogenous spectroscopic parameters. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2019ApJS..244...11K viz 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.
2019ApJS..244...43Z viz 16       D               1 1328 22 Unbiased distribution of binary parameters from LAMOST and Kepler observations. ZHANG J., QIAN S.-B., WU Y., et al.
2019AJ....158..190H viz 16       D               1 343 61 Hot Jupiters are destroyed by tides while their host stars are on the main sequence. HAMER J.H. and SCHLAUFMAN K.C.
2020ApJ...890...23L viz 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.
2021A&A...645A...7K viz 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.
2021ApJS..255...15W 59       D     X         2 82 15 Transiting exoplanet monitoring project (TEMP). VI. The homogeneous refinement of system parameters for 39 transiting hot Jupiters with 127 new light curves. WANG X.-Y., WANG Y.-H., WANG S., et al.
2021RAA....21..292W viz 17       D               4 9395 19 LAMOST Time-Domain survey: first results of four K2 plates. WANG S., ZHANG H.-T., BAI Z.-R., et al.
2022ApJS..259...62I viz 17       D               1 395 24 TESS Transit Timing of Hundreds of Hot Jupiters. IVSHINA E.S. and WINN J.N.
2022ApJS..261...26S viz 17       D               1 1893 2 Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. SU T., ZHANG L.-Y., LONG L., et al.
2023ApJS..264...12H viz 17       D               2 1697 2 Stellar Chromospheric Activities Revealed from the LAMOST-K2 Time-domain Survey. HAN H., WANG S., BAI Y., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2023A&A...676A..90R viz 17       D               1 273 ~ The GAPS programme at TNG XLIV. Projected rotational velocities of 273 exoplanet-host stars observed with HARPS-N. RAINER M., DESIDERA S., BORSA F., et al.
2024AJ....168..183T 197       D       C F     5 41 ~ Gaussian Process Models Impact the Inferred Properties of Giant Planets around Active Stars. TRAN Q.H. and BOWLER B.P.
2024A&A...689A..53B viz 18       D               1 194 ~ The TROY project III. Exploring co-orbitals around low-mass stars. BALSALOBRE-RUZA O., LILLO-BOX J., BARRADO D., et al.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2025RNAAS...9..275M 19       D               1 365 ~ An In-depth Study of Brown Dwarfs with TESS. MARCADON F. and PRSA A.
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.

goto View the references in ADS