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Mid-type M dwarfs planet occurrence rates

Authors: Hardegree-Ullman, K.K.; Cushing, M.C.; Muirhead, P.S.; Christiansen, J.L.;
Abstract

VizieR online Data Catalogue associated with article published in journal Astronomical Journal (AAS) with title 'Kepler planet occurrence rates for mid-type M dwarfs as a function of spectral type.' (bibcode: 2019AJ....158...75H)

Keywords

metallicity, Astrophysics and Astronomy, Chemical abundances, Interdisciplinary Astronomy, observational astronomy, Effective temperature, stellar spectral types, M stars, effective temperature, Observational Astronomy, stellar radii, Stellar radii, Metallicity, Stellar masses, Apparent magnitude, interdisciplinary astronomy, Physics, Exoplanets, exoplanet astronomy, Stellar distance, stellar astronomy, Exoplanet Astronomy, exoplanets, Stellar Astronomy, stellar distance, Dwarf stars, apparent magnitude, m stars, Stellar spectral types, Natural Sciences, stellar masses, dwarf stars

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average