LP 367-113 , the SIMBAD biblio

LP 367-113 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST15:19:53

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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.
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.
2005PASP..117..676R viz 15       D               1 459 33 Probing the LHS catalog. II. Faint proper-motion stars. REID I.N. and GIZIS J.E.
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.
2014MNRAS.437.3603S viz 15       D               2 146 17 A 1500 deg2 near infrared proper motion catalogue from the UKIDSS Large Area Survey. SMITH L., LUCAS P.W., BURNINGHAM B., 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.
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.
2022ApJ...927..122H viz 17       D               1 3750 2 Chemical Properties of the Local Disk and Halo. II. Abundances of 3745 M Dwarfs and Subdwarfs from Improved Model Fitting of Low-resolution Spectra. HEJAZI N., LEPINE S. and NORDLANDER T.

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