2MASS J19224278-0515536 , the SIMBAD biblio

2MASS J19224278-0515536 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:01:21


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Title First 3 Authors
2006AJ....132..866R viz 15       D               1076 188 Identification of new M dwarfs in the solar neighborhood. RIAZ B., GIZIS J.E. and HARVIN J.
2009ApJS..184..138H viz 15       D               1 20623 68 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
2013ApJ...762...88M viz 15       D               1 488 304 Bayesian analysis to identify new star candidates in nearby young stellar kinematic groups. MALO L., DOYON R., LAFRENIERE D., et al.
2014ApJ...788...81M viz 15       D               2 351 123 BANYAN. III. Radial velocity, rotation, and X-ray emission of low-mass star candidates in nearby young kinematic groups. MALO L., ARTIGAU E., DOYON R., et al.
2014ApJ...792...37M 15       D               1 96 112 BANYAN. IV. Fundamental parameters of low-mass star candidates in nearby young stellar kinematic Groups–Isochronal age determination using magnetic evolutionary models. MALO L., DOYON R., FEIDEN G.A., et al.
2015MNRAS.454..593B viz 16       D               1 550 376 A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood. BELL C.P.M., MAMAJEK E.E. and NAYLOR T.
2016A&A...591A.118S viz 16       D               1 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2019MNRAS.489.2189L viz 16       D               1 616 ~ Evaluation of nearby young moving groups based on unsupervised machine learning. LEE J. and SONG I.
2021AJ....161..173T 17       D               1 43 8 The Epoch of giant planet Migration planet search program. I. Near-infrared radial velocity jitter of young Sun-like stars. TRAN Q.H., BOWLER B.P., COCHRAN W.D., et al.
2025AJ....170..103T 299       D     X C       6 122 ~ The Epoch of Giant Planet Migration Planet Search Program. III. The Occurrence Rate of Young Giant Planets inside the Water Ice Line. TRAN Q.H., BOWLER B.P., COCHRAN W.D., et al.

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