LP 467-66 , the SIMBAD biblio

LP 467-66 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST20:17:02


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Title First 3 Authors
2003AJ....126..472G viz 1090 18 Completeness of USNO-B for high proper motion stars. GOULD A.
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.
2005AJ....129.1483L viz 63382 364 A catalog of northern stars with annual proper motions larger than 0.15" (LSPM-NORTH catalog). LEPINE S. and SHARA M.M.
2010ApJS..190..100K viz 15       D               1 2858 246 Discoveries from a near-infrared proper motion survey using multi-epoch Two Micron All-Sky Survey data. KIRKPATRICK J.D., LOOPER D.L., BURGASSER A.J., et al.
2014ApJ...783..122K viz 15       D               3 200 116 The AllWISE motion survey and the quest for cold subdwarfs. KIRKPATRICK J.D., SCHNEIDER A., FAJARDO-ACOSTA S., et al.
2014ApJ...790..158A viz 15       D               1 244 10 An improved catalog of halo wide binary candidates. ALLEN C. and MONROY-RODRIGUEZ M.A.
2014ApJ...790..159M 16       D               1 48 138 The end of the MACHO era, revisited: new limits on MACHO masses from halo wide binaries. MONROY-RODRIGUEZ M.A. and ALLEN C.
2014AJ....148...60L 15       D               2 160 6 Optical BVRI photometry of common proper motion F/G/K+M wide separation binaries. LI T., MARSHALL J.L., LEPINE S., et al.
2015ApJ...804...30Z viz 359 9 Multiplicity of the galactic senior citizens: a high-resolution search for cool subdwarf companions. ZIEGLER C., LAW N.M., BARANEC C., 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.
2016ApJS..224...36K viz 16       D               2 45304 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.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.

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