2MASS J04105425+2501266 , the SIMBAD biblio

2MASS J04105425+2501266 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:21:39


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Title First 3 Authors
2011ApJS..196....4R viz 15       D               1 1030 50 New young star candidates in the Taurus-Auriga region as selected from the Wide-field Infrared Survey Explorer. REBULL L.M., KOENIG X.P., PADGETT D.L., et al.
2014ApJ...784..126E viz 15       D               3 1466 39 A WISE survey of circumstellar disks in Taurus. ESPLIN T.L., LUHMAN K.L. and MAMAJEK E.E.
2017AJ....153...46L viz 95       D         F     4 513 65 A Survey for new members of the Taurus star-forming region with the Sloan Digital Sky Survey. LUHMAN K.L., MAMAJEK E.E., SHUKLA S.J., et al.
2017ApJ...837...95B 16       D               1 702 15 A search for L/T transition dwarfs with Pan-STARRS1 and WISE. III. Young L dwarf discoveries and proper motion catalogs in Taurus and Scorpius-Centaurus. BEST W.M.J., LIU M.C., MAGNIER E.A., et al.
2017AJ....154..134E viz 16       D               1 483 15 A survey for planetary-mass brown dwarfs in the Taurus and Perseus star-forming regions. ESPLIN T.L. and LUHMAN K.L.
2018ApJ...858...41Z viz 80             C       1 250 33 The Pan-STARRS1 proper-motion survey for young brown dwarfs in nearby star-forming regions. I. Taurus discoveries and a reddening-free classification method for ultracool dwarfs. ZHANG Z., LIU M.C., BEST W.M.J., et al.
2018AJ....156..271L viz 56       D     X         2 630 108 The stellar membership of the Taurus star-forming region. LUHMAN K.L.
2019AJ....158...54E viz 16       D               1 633 47 A survey for new members of Taurus from stellar to planetary masses. ESPLIN T.L. and LUHMAN K.L.
2019A&A...630A.137G viz 16       D               1 560 78 Structure and kinematics of the Taurus star-forming region from Gaia-DR2 and VLBI astrometry. GALLI P.A.B., LOINARD L., BOUY H., et al.
2021ApJ...920..132P viz 17       D               1 5441 33 Quantifying variability of young stellar objects in the mid-infrared over 6 years with the Near-Earth Object Wide-field Infrared Survey Explorer. PARK W., LEE J.-E., CONTRERAS PENA C., et al.

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