EPIC 211946007.01 , the SIMBAD biblio

EPIC 211946007.01 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST12:36:33


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Title First 3 Authors
2019AJ....157..124K viz 84           X         2 603 7 Discovery and Vetting of Exoplanets. I. Benchmarking K2 vetting tools. KOSTOV V.B., MULLALLY S.E., QUINTANA E.V., et al.
2019AJ....158...38C viz 142       D     X         4 45 22 New substellar discoveries from Kepler and K2: is there a brown dwarf desert? CARMICHAEL T.W., LATHAM D.W. and VANDERBURG A.M.
2020AJ....159..151S 187       D     X         5 51 32 TOI-503: the first known brown-dwarf Am-star binary from the TESS mission. SUBJAK J., SHARMA R., CARMICHAEL T.W., et al.
2020AJ....160...53C 145       D     X C       3 42 39 Two intermediate-mass transiting brown dwarfs from the TESS mission. CARMICHAEL T.W., QUINN S.N., MUSTILL A.J., et al.
2021A&A...645A..16P 87             C       1 18 15 TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis. PARVIAINEN H., PALLE E., ZAPATERO-OSORIO M.R., et al.
2021AJ....161...97C viz 192       D     X C       4 41 26 TOI-811b and TOI-852b: new transiting brown dwarfs with similar masses and very different radii and ages from the TESS mission. CARMICHAEL T.W., QUINN S.N., ZHOU G., et al.
2021A&A...652A.127G viz 17       D               1 64 16 Populating the brown dwarf and stellar boundary: Five stars with transiting companions near the hydrogen-burning mass limit. GRIEVES N., BOUCHY F., LENDL M., et al.
2022A&A...664A..94P viz 18       D               1 60 7 Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars. PSARIDI A., BOUCHY F., LENDL M., et al.
2023MNRAS.519.5177C 513     A D     X   F     11 49 3 Improved radius determinations for the transiting brown dwarf population in the era of Gaia and TESS. CARMICHAEL T.W.
2023AJ....166..225S 19       D               1 89 ~ Verification of Gaia Data Release 3 Single-lined Spectroscopic Binary Solutions With Three Transiting Low-mass Secondaries. SCHMIDT S.P., SCHLAUFMAN K.C., DING K., et al.

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