CD-48 14223 , the SIMBAD biblio

CD-48 14223 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.12.03CET16:43:14


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
2021AJ....162..221S 65       D     X         2 10 ~ Critical analysis of TESS transit photometric data: improved physical properties for five exoplanets. SAHA S. and SENGUPTA S.
2021ApJ...914...56A 19       D               1 55 ~ On a possible solution to the tidal realignment problem for hot Jupiters. ANDERSON K.R., WINN J.N. and PENEV K.
2020A&A...635A..73B viz 18       D               3 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.
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.
2019AJ....158..141Z viz 17       D               2 51 ~ Two new HATNet hot Jupiters around A stars and the first glimpse at the occurrence rate of hot Jupiters from TESS. ZHOU G., HUANG C.X., BAKOS G.A., 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.
2019AJ....158..243P viz 17       D               1 160 ~ A search for multiplanet systems with TESS using a Bayesian N-body retrieval and machine learning. PEARSON K.A.
2018A&A...609A.116R viz 17       D               1 143005 9 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..165P viz 17       D               1 83 4 Empirical tidal dissipation in exoplanet hosts from tidal spin-up. PENEV K., BOUMA L.G., WINN J.N., et al.
2018ApJ...853...37S 17       D               2 153 7 Evidence of an upper bound on the masses of planets and its implications for giant planet formation. SCHLAUFMAN K.C.
2018ApJ...856..155G 102       D       C       7 149 ~ Giant planets: good neighbors for habitable worlds? GEORGAKARAKOS N., EGGL S. and DOBBS-DIXON I.
2018MNRAS.474.5158G viz 17       D               1 131 8 A library of ATMO forward model transmission spectra for hot Jupiter exoplanets. GOYAL J.M., MAYNE N., SING D.K., et al.
2017A&A...600A..69A 84         O X         2 58 7 SWEET-Cat update and FASMA. A new minimization procedure for stellar parameters using high-quality spectra. ANDREASEN D.T., SOUSA S.G., TSANTAKI M., et al.
2017A&A...602A.107B viz 17       D               2 476 14 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 17       D               2 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA 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.
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.
2014MNRAS.440.1982H viz 483     A D S   X C       11 23 31 Transiting hot Jupiters from WASP-South, Euler and TRAPPIST:
WASP-95b to WASP-101b.
HELLIER C., ANDERSON D.R., COLLIER CAMERON A., et al.
2014MNRAS.442.1844B 16       D               1 81 26 Discrepancies between isochrone fitting and gyrochronology for exoplanet host stars? BROWN D.J.A.

goto View the references in ADS


2021.12.03-16:43:14

© Université de Strasbourg/CNRS

    • Contact