LP 587-45 , the SIMBAD biblio

LP 587-45 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:20:34

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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
2002AJ....124.1651M viz 14       D               53 42 Faint high-latitude carbon stars discovered by the Sloan Digital Sky Survey: methods and initial results. MARGON B., ANDERSON S.F., HARRIS H.C., et al.
2003ApJ...584L..95L 31 18 The discovery of two nearby carbon dwarfs. LOWRANCE P.J., KIRKPATRICK J.D., REID I.N., et al.
2004AJ....127.2838D viz 256 43 Faint high-latitude carbon stars discovered by the Sloan Digital Sky Survey: an initial catalog. DOWNES R.A., MARGON B., ANDERSON S.F., et al.
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.
2009yCat....1.2023S viz 15       D               4348 31 Catalogue of stellar spectral classifications. SKIFF B.A.
2013ApJ...765...12G viz 15       D               1 1416 43 Innocent bystanders: carbon stars from the Sloan Digital Sky Survey. GREEN P.
2018AJ....155..252H viz 16       D               4 22 5 Distances of dwarf carbon stars. HARRIS H.C., DAHN C.C., SUBASAVAGE J.P., et al.
2018MNRAS.479.3873W 16       D               1 28 7 Dwarf carbon stars are likely metal-poor binaries and unlikely hosts to carbon planets. WHITEHOUSE L.J., FARIHI J., GREEN P.J., 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.
2019MNRAS.486.2169K viz 16       D               1 25030 80 White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14. KEPLER S.O., PELISOLI I., KOESTER D., et al.
2021MNRAS.507.4646K viz 17       D               1 2395 10 White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 16. KEPLER S.O., KOESTER D., PELISOLI I., et al.

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