LP 942-92 , the SIMBAD biblio

LP 942-92 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST16:32:13


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Title First 3 Authors
1979LHS...C......0L viz 14       D               4464 ~ A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). LUYTEN W.J.
2002ApJS..141..187B viz 4468 67 Revised coordinates and proper motions of the stars in the Luyten half-second catalog. BAKOS G.A., SAHU K.C. and NEMETH P.
2003A&A...397..575P viz 6208 39 The Liverpool-Edinburgh high proper motion survey. POKORNY R.S., JONES H.R.A. and HAMBLY N.C.
2003AJ....125..332J 208 35 The solar neighborhood. VII. Discovery and characterization of nearby multiples in the CTIO parallax investigation. JAO W.-C., HENRY T.J., SUBASAVAGE J.P., et al.
2003ApJ...582.1011S viz 35377 223 Improved astrometry and photometry for the Luyten catalog. II. Faint stars and the revised catalog. SALIM S. and GOULD A.
2008AJ....136..840J 313       D     X C       8 156 33 Cool subdwarf investigations. I. New thoughts on the spectral types of K and M subdwarfs. JAO W.-C., HENRY T.J., BEAULIEU T.D., et al.
2011AJ....141..117J 15       D               3 57 38 The solar neighborhood. XXIV. Parallax results from the CTIOPI 0.9 M program: stars with µ ≥ 1".0/yr (MOTION sample) and subdwarfs. JAO W.-C., HENRY T.J., SUBASAVAGE J.P., et al.
2013MNRAS.434.1005Z 15       D               1 189 17 A spectroscopic and proper motion search of Sloan digital sky survey: red subdwarfs in binary systems. ZHANG Z.H., PINFIELD D.J., BURNINGHAM B., et al.
2016ApJ...817..112S viz 16       D               1 20555 25 A proper motion survey using the first sky pass of NEOWISE-reactivation data. SCHNEIDER A.C., GRECO J., CUSHING M.C., et al.
1995yCat.1098....0L viz 14       D               1 52096 ~ New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). LUYTEN W.J.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.

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