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WASP-104 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2023.09.22CEST08:05:35 |
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 |
---|---|---|---|---|---|---|---|---|---|
2014A&A...570A..64S ![]() |
2264 | A | D | S X C | 56 | 9 | 9 |
WASP-104b and WASP-106b: two transiting hot Jupiters in 1.75-day and 9.3-day orbits. |
SMITH A.M.S., ANDERSON D.R., ARMSTRONG D.J., et al. |
2015ApJ...806...97K | 16 | D | 1 | 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 | 16 | D | 1 | 71 | 19 | A Lucky Imaging search for stellar sources near 74 transit hosts. | WOELLERT M. and BRANDNER W. | ||
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. | ||
2018A&A...610A..20E ![]() |
167 | X | 4 | 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. | ||
2018ApJ...856..155G | 100 | D | C | 7 | 149 | 5 | Giant planets: good neighbors for habitable worlds? | GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I. | |
2018AJ....155..165P ![]() |
17 | 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....156...44M | 610 | A | X C | 14 | 6 | 4 |
WASP-104b is darker than charcoal. |
MOCNIK T., HELLIER C. and SOUTHWORTH J. | |
2018MNRAS.473.1801G | 42 | X | 1 | 78 | 1 | Exoplanet phase curves at large phase angles. Diagnostics for extended hazy atmospheres. | GARCIA MUNOZ A. and CABRERA J. | ||
2018A&A...620A..58S ![]() |
17 | D | 1 | 164 | 10 | SWEET-Cat updated. New homogenous spectroscopic parameters. | SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al. | ||
2019AJ....158..190H ![]() |
17 | 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. | ||
2019MNRAS.490.5088M ![]() |
17 | D | 2 | 214 | 32 | Search for stellar companions of exoplanet host stars by exploring the second ESA-Gaia data release. | MUGRAUER M. | ||
2020ApJ...890...23L ![]() |
17 | D | 1 | 4935 | 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. | ||
2020AJ....159..137G | 18 | D | 3 | 74 | 83 | Statistical characterization of hot Jupiter atmospheres using Spitzer's secondary eclipses. | GARHART E., DEMING D., MANDELL A., et al. | ||
2021MNRAS.500.5420C ![]() |
627 | X C | 13 | 16 | 14 | An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b. | CHEN G., PALLE E., PARVIAINEN H., et al. | ||
2021A&A...645A...7K ![]() |
18 | 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 ![]() |
18 | D | 1 | 2175 | 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. | ||
2021ApJS..255...15W | 18 | D | 1 | 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. | ||
2021ApJ...923..242G | 18 | D | 2 | 56 | ~ | Why is it so hot in here? Exploring population trends in Spitzer thermal emission observations of hot Jupiters using planet-specific, self-consistent atmospheric models. | GOYAL J.M., LEWIS N.K., WAKEFORD H.R., et al. | ||
2022ApJS..259...62I ![]() |
19 | D | 1 | 395 | 24 | TESS Transit Timing of Hundreds of Hot Jupiters. | IVSHINA E.S. and WINN J.N. |
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