K2-107 , the SIMBAD biblio

K2-107 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2023.03.26CEST10:42:34


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2017AJ....153..130E 1128       D S   X C       26 6 5 K2-60b and K2-107b. A sub-Jovian and a Jovian planet from the K2 mission. EIGMULLER P., GANDOLFI D., PERSSON C.M., et al.
2017A&A...603A..30S viz 16       D               2 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018AJ....155...21P viz 17       D               2 354 11 Planet candidates from K2 campaigns 5-8 and follow-up optical spectroscopy. PETIGURA E.A., CROSSFIELD I.J.M., ISAACSON H., et al.
2018AJ....155..136M viz 17       D               1 521 23 275 candidates and 149 validated planets orbiting bright stars in K2 campaigns 0-10. MAYO A.W., VANDERBURG A., LATHAM D.W., et al.
2018AJ....156..277L viz 17       D               1 306 ~ Sixty validated planets from K2 campaigns 5-8. LIVINGSTON J.H., CROSSFIELD I.J.M., PETIGURA E.A., et al.
2019AJ....157..124K viz 17       D               1 603 ~ Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019ApJS..244...11K viz 17       D               1 2118 ~ Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. KRUSE E., AGOL E., LUGER R., et al.
2020ApJ...890...23L viz 17       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.
2021ApJ...909..115C viz 18       D               1 2175 ~ 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.

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2023.03.26-10:42:34

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