LP 756-24 , the SIMBAD biblio

LP 756-24 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:09:52


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Title First 3 Authors
1979ApJ...227..232B 47 50 Subdwarfs. II. The missing halo-population K subdwarfs. BESSELL M.S. and WICKRAMASINGHE D.T.
1979LHS...C......0L viz 14       D               4464 ~ A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). LUYTEN W.J.
1980ApJS...43..457E 169 64 Catalogs of proper motion stars. II. Stars brighter than visual magnitude 15 and south of declination +30 with annual proper motion between 0"7 and 1"0. EGGEN O.J.
1983ApJS...51..183E 248 34 Luminosity and motion of large proper motion stars. II. Stars with annual proper motion larger than 0.7 arc seconds. EGGEN O.J.
1985AJ.....90..123H 111 32 U.S. Naval Observatory parallaxes of faint stars. List VII. HARRINGTON R.S., DAHN C.C., KALLARAKAL V.V., et al.
1995GCTP..C......0V viz 14       D               1 7047 ~ The General Catalogue of Trigonometric Stellar Parallaxes, Fourth Edition. VAN ALTENA W.F., LEE J.T. and HOFFLEIT E.D.
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.
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.
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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