BD-19 4086 , the SIMBAD biblio

BD-19 4086 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST16:37:23


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Title First 3 Authors
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..222D 1136 T K A     X C       26 13 6 Three small planets transiting the bright young field star
K2-233.
DAVID T.J., CROSSFIELD I.J.M., BENNEKE B., et al.
2018AJ....156..302D 41           X         1 117 10 Discovery of a transiting adolescent sub-Neptune exoplanet with K2. DAVID T.J., MAMAJEK E.E., VANDERBURG A., et al.
2019AJ....157...40F 42           X         1 16 7 K2-288Bb: a small temperate planet in a low-mass binary system discovered by citizen scientists. FEINSTEIN A.D., SCHLIEDER J.E., LIVINGSTON J.H., et al.
2019MNRAS.483.5534S 85             C       1 6 9 Machine-learning approaches to exoplanet transit detection and candidate validation in wide-field ground-based surveys. SCHANCHE N., CAMERON A.C., HEBRARD G., et al.
2020ApJ...890...23L viz 17       D               3 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.
2020A&A...640A..48L viz 2171 T   A D S   X C       49 27 17 Masses for the seven planets in K2-32 and
K2-233. Four diverse planets in resonant chain and the first young rocky worlds.
LILLO-BOX J., LOPEZ T.A., SANTERNE A., et al.
2020AJ....160..179M 44           X         1 44 65 TESS hunt for young and maturing exoplanets (THYME). III. A two-planet system in the 400 Myr Ursa Major group. MANN A.W., JOHNSON M.C., VANDERBURG A., et al.
2021AJ....161....2Z 45           X         1 27 38 Two young planetary systems around field stars with ages between 20 and 320 Myr from TESS. ZHOU G., QUINN S.N., IRWIN J., et al.
2021ApJ...909..115C viz 17       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.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2021Sci...374..330A 45           X         1 47 73 A compositional link between rocky exoplanets and their host stars. ADIBEKYAN V., DORN C., SOUSA S.G., et al.
2022AJ....163..289Z 90             C       1 63 7 A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235. ZHOU G., WIRTH C.P., HUANG C.X., et al.
2022A&A...663A.161M viz 18       D               1 213 8 Ariel stellar characterisation. I. Homogeneous stellar parameters of 187 FGK planet host stars: Description and validation of the method. MAGRINI L., DANIELSKI C., BOSSINI D., et al.
2023MNRAS.522.3458B 2099 T K A D S   X C F     42 12 ~ Revisiting
K2-233 spectroscopic time-series with multidimensional Gaussian processes.
BARRAGAN O., GILLEN E., AIGRAIN S., et al.
2023A&A...673A...4B 47           X         1 20 ~ The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming one. BARROS S.C.C., DEMANGEON O.D.S., ARMSTRONG D.J., et al.
2023ApJ...952...68S 47           X         1 26 ~ A Search for Stellar Siblings of the ∼200 Myr TOI-251 b Planetary System. SUN Q., WANG S.X., MANN A.W., et al.
2023A&A...676A.131H 93               F     2 48 ~ Forming rocky exoplanets around K-dwarf stars. HATALOVA P., BRASSER R., MAMONOVA E., et al.
2023A&A...675A.158D 93           X         2 27 ~ TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit. DESIDERA S., DAMASSO M., GRATTON R., et al.
2023A&A...679A..33D 47           X         1 19 ~ A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO Radial velocities lead to the detection of transits with low signal-to-noise ratio. DAMASSO M., RODRIGUES J., CASTRO-GONZALEZ A., et al.

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