L 395-109 , the SIMBAD biblio

L 395-109 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST02:03:50


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Title First 3 Authors
1955LFT...C......0L 13       D               1 1843 3 Luyten's Five Tenths. LUYTEN W.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.
2002AJ....124.1190L viz 217 96 New high proper motion stars from the Digitized Sky Survey. I. Northern stars with 0".5 yr–1<µ<2".0 yr–1 at low galactic latitudes. LEPINE S., SHARA M.M. and RICH R.M.
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.
2014ApJ...781....4L viz 16       D               1 763 78 A search for a distant companion to the Sun with the wide-field infrared survey explorer. LUHMAN K.L.
2014ApJ...787..126L viz 16       D               1 821 18 Characterization of high proper motion objects from the wide-field infrared survey explorer. LUHMAN K.L. and SHEPPARD S.S.
2015MNRAS.454.4054B viz 373       D     X         10 48 4 Spectrophotometric characterization of high proper motion sources from WISE. BEAMIN J.C., IVANOV V.D., MINNITI D., 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.
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.
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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