GSC 06493-00315 , the SIMBAD biblio

GSC 06493-00315 , the SIMBAD biblio (8 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.07.24CEST08:14:16


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
2020AJ....160..133M 19       D               1 71 ~ TOI 694b and TIC 220568520b: two low-mass companions near the hydrogen-burning mass limit orbiting Sun-like stars. MIRELES I., SHPORER A., GRIEVES N., et al.
2020NatAs...4..650T 19       D               1 64 ~ An eclipsing substellar binary in a young triple system discovered by SPECULOOS. TRIAUD A.H.M.J., BURGASSER A.J., BURDANOV A., et al.
2019A&A...625A.150V viz 108       D       C       3 26 ~ EBLM Project. V. Physical properties of ten fully convective, very-low-mass stars. VON BOETTICHER A., TRIAUD A.H.M.J., QUELOZ D., et al.
2019ApJ...871...63M viz 18       D               2 85 ~ How to constrain your M dwarf. II. The Mass-Luminosity-Metallicity relation from 0.075 to 0.70 solar masses. MANN A.W., DUPUY T., KRAUS A.L., 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.
2015AJ....149..166H viz 16       D               1 64 40 HATS-6b: a warm Saturn transiting an early M dwarf star, and a set of empirical relations for characterizing K and M dwarf planet hosts. HARTMAN J.D., BAYLISS D., BRAHM R., et al.
2014MNRAS.437.2831Z viz 732     A D S   X C       17 23 37 The mass-radius relationship for very low mass stars: four new discoveries from the HATSouth Survey. ZHOU G., BAYLISS D., HARTMAN J.D., et al.
2014MNRAS.444.2525C 17       D               2 95 172 Improving PARSEC models for very low mass stars. CHEN Y., GIRARDI L., BRESSAN A., et al.

goto View the references in ADS


2021.07.24-08:14:16

© Université de Strasbourg/CNRS

    • Contact