BD+10 3472 , the SIMBAD biblio

BD+10 3472 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.11.28CET03:21:04


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Title First 3 Authors
2020A&A...635A..73B viz 1944       D S   X C       42 64 ~ A multiplicity study of transiting exoplanet host stars. I. High-contrast imaging with VLT/SPHERE. BOHN A.J., SOUTHWORTH J., GINSKI C., et al.
2020AJ....160..228K 18       D               1 30 ~ A search for FeH in hot-Jupiter atmospheres with high-dispersion spectroscopy. KESSELI A.Y., SNELLEN I.A.G., ALONSO-FLORIANO F.J., et al.
2020ApJ...890...23L 18       D               1 4935 ~ 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.
2019A&A...628A...9C viz 87             C       1 14 ~ Atmospheric characterization of the ultra-hot Jupiter MASCARA-2b/KELT-20b. Detection of CaII, FeII, NaI, and the Balmer series of H (Hα, Hβ, and Hγ) with high-dispersion transit spectroscopy. CASASAYAS-BARRIS N., PALLE E., YAN F., et al.
2019AJ....158..190H viz 17       D               1 343 ~ Hot Jupiters are destroyed by tides while their host stars are on the main sequence. HAMER J.H. and SCHLAUFMAN K.C.
2018A&A...610A...3J viz 43           X         1 17 ~ Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996. JEONG G., LEE B.-C., HAN I., et al.
2018AJ....155...35S 128           X C       2 18 12 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.
2018AJ....155..100J 85             C       1 23 7 KELT-21b: a hot Jupiter transiting the rapidly rotating metal-poor late-A primary of a likely hierarchical triple system. JOHNSON M.C., RODRIGUEZ J.E., ZHOU G., et al.
2017A&A...603A..30S viz 17       D               2 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2017A&A...606A..73T viz 42           X         1 8 7 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.
2017AJ....153..136S viz 17       D               1 525 31 Accurate empirical radii and masses of planets and their host stars with Gaia parallaxes. STASSUN K.G., COLLINS K.A. and GAUDI B.S.
2017AJ....153..263M 42           X         1 10 3 KELT-18b: puffy planet, hot host, probably perturbed. McLEOD K.K., RODRIGUEZ J.E., OELKERS R.J., et al.
2017AJ....154..194L 251           X C       5 31 15 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.
2017MNRAS.471.2743T 42           X         1 23 9 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.
2016AJ....152..136Z viz 41           X         1 24 23 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.
2016ApJ...827L..17M 41           X         1 26 14 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.
2016MNRAS.460.3376Z 41           X         1 20 11 Spin-orbit alignment for KELT-7b and HAT-P-56b via Doppler tomography with TRES. ZHOU G., LATHAM D.W., BIERYLA A., et al.
2015AJ....150..197H viz 3209   K A D     X C       79 24 25
HAT-P-57b: a short-period giant planet transiting a bright rapidly rotating A8V star confirmed via Doppler tomography.
HARTMAN J.D., BAKOS G.A., BUCHHAVE L.A., et al.
2007MNRAS.379..647L viz 15       D               60 13 SuperWASP-North extrasolar planet candidates: candidates from fields 17h<RA<18h. LISTER T.A., WEST R.G., WILSON D.M., et al.
2007MNRAS.380.1230C 16       D               2 73 174 Efficient identification of exoplanetary transit candidates from SuperWASP light curves. COLLIER CAMERON A., WILSON D.M., WEST R.G., et al.

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2021.11.28-03:21:04

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