G 275-92 , the SIMBAD biblio

G 275-92 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.02CEST15:03:16

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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
1955LFT...C......0L 13       D               1 1843 3 Luyten's Five Tenths. LUYTEN W.J.
1974PASP...86..742R 209 63 A photometric and spectroscopic survey of large proper-motion stars. RODGERS A.W. and EGGEN O.
1979ApJ...230..786E 324 28 Luminosity and motion of large proper-motion stars. I. Stars with annual proper motion larger than 1". EGGEN O.J.
1979LHS...C......0L viz 14       D               4461 ~ A catalogue of stars with proper motions exceeding 0".5 annually (2nd edition). LUYTEN W.J.
1985ApJS...59..197B viz 14       D               1 3393 78 G.P. Kuiper's spectral classifications of proper-motion stars. BIDELMAN W.P.
1991AJ....101.1882W 527 35 VRI photometry of late dwarf common proper motion pairs. WEIS E.W.
1996AJ....112.2300W 1229 58 Photometry of stars with large proper motion. WEIS E.
2002ApJS..141..187B viz 4465 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....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.
2006MNRAS.373..705R viz 447     A D     X         13 64 19 Optical spectroscopy of high proper motion stars: new M dwarfs within 10 pc and the closest pair of subdwarfs. REYLE C., SCHOLZ R.-D., SCHULTHEIS M., et al.
1983SAAOC...7..106W 114 2 A spectroscopic survey of 113 nearby red dwarf stars. WALKER A.R.
2008AJ....136..840J 354       D     X         10 156 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.
2009AJ....137.3800J 15       D               1 145 20 Cool subdwarf investigations. II. Multiplicity. JAO W.-C., MASON B.D., HARTKOPF W.I., et al.
2014A&A...564A..90R viz 22 31 High-resolution spectroscopic atlas of M subdwarfs. Effective temperature and metallicity. RAJPUROHIT A.S., REYLE C., ALLARD F., et al.
2016ApJ...817..112S viz 16       D               1 20551 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 45305 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al.
2016A&A...591A.118S viz 16       D               1 31406 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016AJ....152..153J 241           X C       5 23 1 Cool subdwarf investigations. III. Dynamical masses of low-metallicity subdwarfs. JAO W.-C., NELAN E.P., HENRY T.J., et al.
2016A&A...596A..33R 346     A     X C       8 11 13 Spectral energy distribution of M-subdwarfs: A study of their atmospheric properties. RAJPUROHIT A.S., REYLE C., ALLARD F., et al.
2017AJ....154..191J viz 219       D     X         6 116 4 The solar neighborhood. XLII. Parallax results from the CTIOPI 0.9 m program-identifying new nearby subdwarfs using tangential velocities and locations on the H-R diagram. JAO W.-C., HENRY T.J., WINTERS J.G., et al.
1995yCat.1098....0L viz 14       D               1 52092 ~ New Luyten Catalogue of stars with proper motions larger than two tenths of an arcsecond (NLTT). LUYTEN W.J.
2019AJ....158...81C viz 17       D               1 1623 3 The independent discovery of planet candidates around low-mass stars and astrophysical false positives from the first two TESS sectors. CLOUTIER R.
2021A&A...649A...6G viz 17       D               1 89188 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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