BD+14 1881 , the SIMBAD biblio

BD+14 1881 , the SIMBAD biblio (43 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST06:53:53

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
1975A&A....41..447H 49 2 Physical investigations of star chains. HAHN G. and HAUPT H.F.
2016ApJ...827L..17M 39           X         1 26 22 A planet in an 840 day orbit around a Kepler main-sequence a star found from phase modulation of its pulsations. MURPHY S.J., BEDDING T.R. and SHIBAHASHI H.
2016AJ....152..136Z viz 1771   K A D     X C       45 24 55
KELT-17b: a hot-Jupiter transiting an a-star in a misaligned orbit detected with Doppler tomography. 		ZHOU G., RODRIGUEZ J.E., COLLINS K.A., et al.
2017AJ....153...94C 95       D     X         3 33 15 Discovery of XO-6b: a hot Jupiter transiting a fast rotating F5 star on an oblique orbit. CROUZET N., McCULLOUGH P.R., LONG D., et al.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2017AJ....153..263M 40           X         1 10 10 KELT-18b: puffy planet, hot host, probably perturbed. McLEOD K.K., RODRIGUEZ J.E., OELKERS R.J., 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.
2017AJ....154..194L 200           X         5 31 64 KELT-20b: a giant planet with a period of p ∼ 3.5 days transiting the V ∼ 7.6 early A star HD 185603. LUND M.B., RODRIGUEZ J.E., ZHOU G., et al.
2017A&A...606A..73T viz 42           X         1 8 38 MASCARA-1 b. A hot Jupiter transiting a bright mV = 8.3 A-star in a misaligned orbit. TALENS G.J.J., ALBRECHT S., SPRONCK J.F.P., et al.
2018AJ....155...35S 122           X C       2 18 41 KELT-19Ab: a P ∼ 4.6-day hot Jupiter transiting a likely Am star with a distant stellar companion. SIVERD R.J., COLLINS K.A., ZHOU G., et al.
2017MNRAS.471.2743T 40           X         1 23 35 WASP-167b/KELT-13b: joint discovery of a hot Jupiter transiting a rapidly rotating F1V star. TEMPLE L.Y., HELLIER C., ALBROW M.D., et al.
2018A&A...609A.116R viz 16       D               1 143018 65 Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al.
2018AJ....155..139G 40           X         1 23 4 The dynamics of tightly-packed planetary systems in the presence of an outer planet: case studies using Kepler-11 and Kepler-90. GRANADOS CONTRERAS A.P. and BOLEY A.C.
2018A&A...610A...3J viz 40           X         1 17 1 Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996. JEONG G., LEE B.-C., HAN I., 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..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.
2019PASP..131h5001K 16       D               1 26 4 Detection limits of exoplanetary atmospheres with 2-m class telescopes. KABATH P., ZAK J., BOFFIN H.M.J., et al.
2019PASP..131h5002B 16       D               1 26 ~ An international survey of front-end receivers and observing performance of telescopes for radio astronomy. BOLLI P., ORFEI A., ZANICHELLI A., 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.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
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.
2020AJ....159..194V viz 16       D               1 288 ~ A statistical search for star-planet interaction in the ultraviolet using GALEX. VISWANATH G., NARANG M., MANOJ P., et al.
2020A&A...641A.145S 1506 T K A     X C       35 4 ~
KELT-17: a chemically peculiar Am star and a hot-Jupiter planet. 		SAFFE C., MIQUELARENA P., ALACORIA J., et al.
2020MNRAS.498.4680G viz 16       D               1 92 29 A library of self-consistent simulated exoplanet atmospheres. GOYAL J.M., MAYNE N., DRUMMOND B., 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.
2021A&A...647A..49S viz 727       D     X C       17 41 12 Chemical analysis of early-type stars with planets. SAFFE C., MIQUELARENA P., ALACORIA J., et al.
2021ApJ...916L...1A 59       D     X         2 57 40 A preponderance of perpendicular planets. ALBRECHT S.H., MARCUSSEN M.L., WINN J.N., 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..259...63S viz 17       D               1 10269 2 Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. SHANG L.-H., LUO A.-L., WANG L., et al.
2022MNRAS.513.2822G 1294       D S   X C F     28 12 3 Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era. GARAI Z., PRIBULLA T., KOVACS J., et al.
2022A&A...662A.101S 187       D     X C       4 25 12 High-resolution transmission spectroscopy study of ultra-hot Jupiters HAT-P-57b, KELT-17b, KELT-21b, KELT-7b, MASCARA-1b, and WASP-189b. STANGRET M., CASASAYAS-BARRIS N., PALLE E., et al.
2022A&A...662A.107S 128           X         3 29 6 TOI-1268b: The youngest hot Saturn-mass transiting exoplanet. SUBJAK J., ENDL M., CHATURVEDI P., et al.
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.
2022AJ....164..104R viz 17       D               1 105 10 A Tendency Toward Alignment in Single-star Warm-Jupiter Systems. RICE M., WANG S., WANG X.-Y., et al.
2022PASP..134h2001A viz 17       D               1 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2022A&A...668A.157S 681     A D     X         17 48 1 Are Am stars and hot-Jupiter planets related? SAFFE C., ALACORIA J., MIQUELARENA P., et al.
2023ApJ...950L...2S 87           X         2 26 1 Ponderings on the Possible Preponderance of Perpendicular Planets. SIEGEL J.C., WINN J.N. and ALBRECHT S.H.
2023AcA....73..159M viz 261   K A D     X         7 27 ~ Search for planets in hot Jupiter systems with multi-sector TESS photometry. IV. Null detections in 12 systems. MACIEJEWSKI G., SIERZPUTOWSKA J. and GOLONKA J.
2024A&A...686L...1M 18       D               2 48 ~ Gas, not dust: Migration of TESS/Gaia hot Jupiters possibly halted by the magnetospheres of protoplanetary disks. MENDIGUTIA I., LILLO-BOX J., VIOQUE M., 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...695A..27M viz 19       D               1 132 ~ Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation. MALDONADO J., MIROUH G.M., MENDIGUTIA I., 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