PM J08084+2417 , the SIMBAD biblio

PM J08084+2417 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST17:51:53


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Title First 3 Authors
2011AJ....142..138L viz 15       D               1 8898 232 An all-sky catalog of bright M dwarfs. LEPINE S. and GAIDOS E.
2013MNRAS.435.2161F viz 15       D               1 8411 18 A catalogue of bright (K < 9) M dwarfs. FRITH J., PINFIELD D.J., JONES H.R.A., et al.
2015ApJ...798...41A viz 16       D               1 802 19 The near-ultraviolet luminosity function of young, early M-type dwarf stars. ANSDELL M., GAIDOS E., MANN A.W., et al.
2020AJ....160..120J viz 16       D               2 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021AJ....162..102S viz 17       D               1 439 5 Large Adaptive optics Survey for Substellar Objects around young, nearby, low-mass stars with Robo-AO. SALAMA M., OU J., BARANEC C., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022A&A...661A..29M viz 17       D               1 688 11 First eROSITA study of nearby M dwarfs and the rotation-activity relation in combination with TESS. MAGAUDDA E., STELZER B., RAETZ S., et al.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al.
2024MNRAS.533..395L viz 18       D               1 1559 ~ Atmospheric parameters and chemical abundances within 100 pc: a sample of G, K, and M main-sequence stars. LOPEZ-VALDIVIA R., ADAME L., ZAGALA LAGUNAS E., et al.

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