EPIC 210894022.01 , the SIMBAD biblio

EPIC 210894022.01 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST13:44:27

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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
2016ApJS..226....7C viz 16       D               1 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017A&A...604A..16F 488 T K       X C       10 13 21
K2-111 b - a short period super-Earth transiting a metal poor, evolved old star. 		FRIDLUND M., GAIDOS E., BARRAGAN O., et al.
2017A&A...608A..94S 53           X         1 4 51 Constraining planet structure and composition from stellar chemistry: trends in different stellar populations. SANTOS N.C., ADIBEKYAN V., DORN C., et al.
2018AJ....155..136M viz 222       D     X C       5 521 127 275 candidates and 149 validated planets orbiting bright stars in K2 campaigns 0-10. MAYO A.W., VANDERBURG A., LATHAM D.W., et al.
2019A&A...624A..71W 69 2 Comparative analysis of the influence of Sgr A* and nearby active galactic nuclei on the mass loss of known exoplanets. WISLOCKA A.M., KOVACEVIC A.B. and BALBI A.
2019AJ....157..174O viz 17       D               1 176 61 Discovery of a third transiting planet in the Kepler-47 circumbinary system. OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al.
2019ApJS..244...11K viz 17       D               1 2120 48 Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. KRUSE E., AGOL E., LUGER R., et al.
2020AJ....159...41T viz 17       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
2020MNRAS.499.5004M viz 1858     A S   X C F     41 7 20 K2-111: an old system with two planets in near-resonance. MORTIER A., ZAPATERO OSORIO M.R., MALAVOLTA L., et al.
2021A&A...652A.110L 17       D               1 82 7 Why do more massive stars host larger planets? LOZOVSKY M., HELLED R., PASCUCCI I., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2021AJ....162..259Z viz 17       D               1 1094 12 Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al.
2022MNRAS.511.2565P 18       D               1 40 7 HyDRo: atmospheric retrieval of rocky exoplanets in thermal emission. PIETTE A.A.A., MADHUSUDHAN N. and MANDELL A.M.
2022ApJS..261...26S viz 18       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.
2023MNRAS.519.6028R 19       D               1 86 7 Exoplanet atmosphere evolution: emulation with neural networks. ROGERS J.G., MUNOZ C.J., OWEN J.E., et al.
2023ApJ...944...42U 19       D               1 56 6 The Nominal Ranges of Rocky Planet Masses, Radii, Surface Gravities, and Bulk Densities. UNTERBORN C.T., DESCH S.J., HALDEMANN J., et al.
2023NatAs...7...57M 112       D       C       2 22 2 Helium-enhanced planets along the upper edge of the radius valley. MALSKY I., ROGERS L., KEMPTON E.M.-R., et al.
2023A&A...672A.180H 917     A S   X C       18 2 7 Exoplanet characterization using conditional invertible neural networks. HALDEMANN J., KSOLL V., WALTER D., et al.
2023A&A...674A.137L 47           X         1 122 ~ Quantitative correlation of refractory elemental abundances between rocky exoplanets and their host stars. LIU Z. and NI D.
2023A&A...677A..33B viz 19       D               1 120 ~ Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities No excess of cold Jupiters in small planet systems. BONOMO A.S., DUMUSQUE X., MASSA A., et al.
2024A&A...681A..96H 50           X         1 8 ~ BICEPS: An improved characterization model for low- and intermediate-mass exoplanets. HALDEMANN J., DORN C., VENTURINI J., et al.

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