LP 354-264 , the SIMBAD biblio

LP 354-264 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:56:03

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		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.
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.
2007ApJ...669.1235L 16       D               2 40 174 Revised metallicity classes for low-mass stars: dwarfs (dM), subdwarfs (sdM), extreme subdwarfs (esdM), and ultrasubdwarfs (usdM). LEPINE S., RICH R.M. and SHARA M.M.
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               1 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.
2019AJ....157...63K viz 16       D               3 93 11 Radii of 88 M subdwarfs and updated radius relations for low-metallicity M-dwarf stars. KESSELI A.Y., KIRKPATRICK J.D., FAJARDO-ACOSTA S.B., et al.
2020AJ....159...30H viz 16       D               2 1703 ~ Chemical properties of the local Galactic disk and halo. I. Fundamental properties of 1544 nearby, high proper-motion M dwarfs and subdwarfs. HEJAZI N., LEPINE S., HOMEIER D., et al.

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