LP 606-23 , the SIMBAD biblio

LP 606-23 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST13:24:03


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Title First 3 Authors
1989AJ.....98.1693R viz 1708 89 Subdwarf studies. I. UBVRI photometry of NLTT stars. RYAN S.G.
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.
2007AJ....134..778M viz 15       D               566 6 Mapping the local galactic halo. I. Optical photometry of cool subdwarf candidates. MARSHALL J.L.
2015ApJ...804...30Z viz 16       D               1 359 9 Multiplicity of the galactic senior citizens: a high-resolution search for cool subdwarf companions. ZIEGLER C., LAW N.M., BARANEC 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.
2018MNRAS.478.4513B viz 16       D               1 342691 271 The GALAH Survey: second data release. BUDER S., ASPLUND M., DUONG L., 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.
2021ApJ...907...10L viz 17       D               1 1549 37 Dynamically tagged groups of very metal-poor halo stars from the HK and Hamburg/ESO surveys. LIMBERG G., ROSSI S., BEERS T.C., et al.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2022ApJ...936L...3O 17       D               1 70 5 Antaeus: A Retrograde Group of Tidal Debris in the Milky Way's Disk Plane. ORIA P.-A., TENACHI W., IBATA R., et al.
2022A&A...665A..57L viz 17       D               1 6323 23 Substructure in the stellar halo near the Sun. I. Data-driven clustering in integrals-of-motion space. LOVDAL S.S., RUIZ-LARA T., KOPPELMAN H.H., et al.
2024A&A...684A..37C viz 18       D               1 192 ~ A Walk on the Retrograde Side (WRS) project I. Tidying-up the retrograde halo with high-resolution spectroscopy. CECCARELLI E., MASSARI D., MUCCIARELLI A., et al.

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