2MASSI J1332244-044112 , the SIMBAD biblio

2MASSI J1332244-044112 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:21:19


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Title First 3 Authors
2003AJ....126.2421C viz 15       D               1 831 351 Meeting the cool neighbors. V. A 2MASS-Selected sample of ultracool dwarfs. CRUZ K.L., REID I.N., LIEBERT J., et al.
2007AJ....133..439C viz 15       D               307 255 Meeting the cool neighbors. IX. The luminosity function of M7-L8 ultracool dwarfs in the field. CRUZ K.L., REID I.N., KIRKPATRICK J.D., et al.
2007AJ....133.2258S viz 15       D               154 169 Activity and kinematics of ultracool dwarfs, including an amazing flare observation. SCHMIDT S.J., CRUZ K.L., BONGIORNO B.J., et al.
2007AJ....133.2825R viz 15       D               441 69 Meeting the cool neighbors. XI. Beyond the NLTT catalog. REID I.N., CRUZ K.L. and ALLEN P.R.
2007ApJ...667..520C viz 15       D               1 211 40 Southern very low mass stars and brown dwarfs in wide binary and multiple systems. CABALLERO J.A.
2009AJ....137....1F viz 15       D               1 851 248 The brown dwarf kinematics project I. Proper motions and tangential velocities for a large sample of late-type M, L, and T dwarfs. FAHERTY J.K., BURGASSER A.J., CRUZ K.L., et al.
2009ApJ...705.1416R viz 15       D               2 65 67 A volume-limited sample of 63 M7-M9.5 dwarfs. I. Space motion, kinematic age, and lithium. REINERS A. and BASRI G.
2010ApJ...710..924R 16       D               1 66 168 A volume-limited sample of 63 M7-M9.5 dwarfs. II. Activity, magnetism, and the fade of the rotation-dominated dynamo. REINERS A. and BASRI G.
2012ApJ...746...23M viz 15       D               1 242 93 The radio activity-rotation relation of ultracool dwarfs. McLEAN M., BERGER E. and REINERS A.
2013A&A...549A.131A viz 15       D               1 184 31 Volume-limited radio survey of ultracool dwarfs. ANTONOVA A., HALLINAN G., DOYLE J.G., et al.
2015ApJS..220...18B viz 16       D               1 109 32 The Brown Dwarf Kinematics Project (BDKP). IV. Radial velocities of 85 late-M and L dwarfs with MagE. BURGASSER A.J., LOGSDON S.E., GAGNE J., et al.
2016ApJS..224....2H viz 16       D               1 31769 226 The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. HUBER D., BRYSON S.T., HAAS M.R., et al.
2018ApJ...858...55P viz 299       D     X         8 19 50 K2 ultracool dwarfs survey. III. White light flares are ubiquitous in M6-l0 dwarfs. PAUDEL R.R., GIZIS J.E., MULLAN D.J., et al.
2018MNRAS.480.2153D 96       D       C       5 37 14 Investigating the rotational phase of stellar flares on M dwarfs using K2 short cadence data. DOYLE L., RAMSAY G., DOYLE J.G., et al.
2019ApJ...883..205B viz 16       D               1 500 34 The ultracool SpeXtroscopic survey. I. Volume-limited spectroscopic sample and luminosity function of M7-L5 ultracool dwarfs. BARDALEZ GAGLIUFFI D.C., BURGASSER A.J., SCHMIDT S.J., et al.
2020ApJS..247...11R viz 16       D               1 46229 22 Radial velocity photon limits for the dwarf stars of spectral classes F-M. REINERS A. and ZECHMEISTER M.
2020AJ....160...19S viz 16       D               1 825 ~ Upper limits on planet occurrence around ultracool dwarfs with K2. SAGEAR S.A., SKINNER J.N. and MUIRHEAD P.S.
2020A&A...641A.170S viz 16       D               2 796 ~ Occurrence rate of exoplanets orbiting ultracool dwarfs as probed by K2. SESTOVIC M. and DEMORY B.-O.
2021A&A...645A.100S viz 17       D               1 1696 44 SPECULOOS: Ultracool dwarf transit survey. Target list and strategy. SEBASTIAN D., GILLON M., DUCROT E., 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.527.6835K 18       D               1 181 ~ The occurrence rate of quiescent radio emission for ultracool dwarfs using a generalized semi-analytical Bayesian framework. KAO M.M. and SHKOLNIK E.L.

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