HAT-P-44 , the SIMBAD biblio

HAT-P-44 , the SIMBAD biblio (43 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:23:15

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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
2014AJ....147..128H viz 2476   K A D S   X C       63 20 15
HAT-P-44b, HAT-P-45b, and HAT-P-46b: three transiting hot jupiters in possible multi-planet systems. 		HARTMAN J.D., BAKOS G.A., TORRES G., et al.
2015ApJ...806...97K 94       D       C       2 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.
2015ApJ...812L..35F 16       D               1 42 14 A bimodal correlation between host star chromospheric emission and the surface gravity of hot jupiters. FOSSATI L., INGRASSIA S. and LANZA A.F.
2016ApJ...821...26B 39           X         1 14 11 Dynamical constraints on the core mass of hot Jupiter HAT-P-13b. BUHLER P.B., KNUTSON H.A., BATYGIN K., et al.
2017MNRAS.466..738S 16       D               1 57 10 SALT observations of the chromospheric activity of transiting planet hosts: mass-loss and star-planet interactions. STAAB D., HASWELL C.A., SMITH G.D., et al.
2017A&A...601A.104F 40           X         1 45 13 The effect of ISM absorption on stellar activity measurements and its relevance for exoplanet studies. FOSSATI L., MARCELJA S.E., STAAB D., et al.
2017A&A...602A.107B viz 79           X         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               4 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJ...856...37B 16       D               1 170 43 Jupiter analogs orbit stars with an average metallicity close to that of the Sun. BUCHHAVE L.A., BITSCH B., JOHANSEN A., et al.
2018MNRAS.474.5158G viz 16       D               1 131 85 A library of ATMO forward model transmission spectra for hot Jupiter exoplanets. GOYAL J.M., MAYNE N., SING D.K., et al.
2018ApJS..237...38B viz 16       D               1 1111 42 Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
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.
2019A&A...622A..81M viz 122           X   F     2 39 22 Ephemeris refinement of 21 hot Jupiter exoplanets with high timing uncertainties. MALLONN M., VON ESSEN C., HERRERO E., et al.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., 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.
2019MNRAS.489.5098F 122           X         3 13 ~ Atmospheric scintillation noise in ground-based exoplanet photometry. FOHRING D., WILSON R.W., OSBORN J., et al.
2020AJ....159...44C viz 41           X         1 22 ~ XO-7 b: a transiting hot Jupiter with a massive companion on a wide orbit. CROUZET N., HEALY B.F., HEBRARD G., et al.
2020MNRAS.491.2760G 41           X         1 19 ~ Periodic transit timing variations and refined system parameters of the exoplanet XO-6b. GARAI Z., PRIBULLA T., KOMZIK R., et al.
2020ApJ...890...23L viz 16       D               2 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.
2020AJ....160..120J viz 16       D               2 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021ApJ...909..115C viz 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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022AJ....163..160B viz 17       D               2 240 9 Stellar Companions to TESS Objects of Interest: A Test of Planet-Companion Alignment. BEHMARD A., DAI F. and HOWARD A.W.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., 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.
2022MNRAS.513..102C viz 17       D               1 961 6 The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al.
2022AJ....164...60S viz 17       D               2 854 2 Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? SWASTIK C., BANYAL R.K., NARANG M., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2023MNRAS.518.2068G viz 17       D               1 179 2 Chaos in multiplanetary extrasolar systems. GAJDOS P. and VANKO M.
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.
2023A&A...676A.131H 87               F     2 48 ~ Forming rocky exoplanets around K-dwarf stars. HATALOVA P., BRASSER R., MAMONOVA E., et al.
2024A&A...682A.136C viz 242       D     X         6 144 ~ The GAPS Programme at TNG LI. Investigating the correlations between transiting system parameters and host chromospheric activity. CLAUDI R., BRUNO G., FOSSATI L., et al.
2023AcA....73...57M viz 87   K A D               3 24 ~ Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. III. A Study of Ten Systems Enhanced with New Ground-Based Photometry. MACIEJEWSKI G., FERNANDEZ M., SOTA A., et al.
2024A&A...689A..99Z 134     A D     X         4 10 ~ Von Zeipel-Lidov-Kozai secondary resonances can enhance the excitation of planetary eccentricity. ZHAO S., HUANG X. and LEI H.
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.
2025AJ....169..149H 93               F     1 222 ~ Architecture Classification for Extrasolar Planetary Systems. HOWE A.R., BECKER J.C., STARK C.C., et al.
2025A&A...697A.102T viz 19       D               1 176 ~ Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel mission candidate sample. TSANTAKI M., MAGRINI L., DANIELSKI C., 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.
2025PASP..137h4402L 47           X         1 4 ~ Development of a New Ground-based Instrumentation Technique for Low-resolution Exoplanet Transmission Spectroscopy. LIMBACH M.A., SCHMIDT L.M., OELKERS R.J., 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.

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