SIPS J1712-0323 , the SIMBAD biblio

SIPS J1712-0323 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST05:04:10


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Title First 3 Authors
2007A&A...468..163D viz 15       D   O           1 7019 33 Southern infrared proper motion survey. II. A sample of low mass stars with µ≥0.1"/yr. DEACON N.R. and HAMBLY N.C.
2015AJ....149....5W viz 16       D               1 1773 104 The solar neighborhood. XXXV. Distances to 1404 M dwarf systems within 25 pc in the southern sky. WINTERS J.G., HAMBLY N.C., JAO W.-C., et al.
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.
2018A&A...619L...8R viz 16       D               1 14916 6 New ultra-cool and brown dwarf candidates in Gaia DR2. REYLE C.
2020AJ....160..215V viz 16       D               2 605 16 The solar neighborhood. XLVI. Revealing new M dwarf binaries and their orbital architectures. VRIJMOET E.H., HENRY T.J., JAO W.-C., et al.
2021A&A...645A.100S viz 17       D               1 1696 44 SPECULOOS: Ultracool dwarf transit survey. Target list and strategy. SEBASTIAN D., GILLON M., DUCROT E., et al.
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.
2023A&A...670A..19G viz 17       D               1 5915 6 The Fifth Catalogue of Nearby Stars (CNS5). GOLOVIN A., REFFERT S., JUST A., et al.
2024ApJS..271...55K viz 18       D               1 1067 ~ The Initial Mass Function Based on the Full-sky 20 pc Census of ∼3600 Stars and Brown Dwarfs. KIRKPATRICK J.D., MAROCCO F., GELINO C.R., et al.
2025AJ....170..213D 19       D               4 59 ~ Gravity-sensitive Spectral Indices in Ultracool Dwarfs: Investigating Correlations with Metallicity and Planet Occurrence Using SpeX and Fire Observations. DAVOUDI F., RACKHAM B.V., DE WIT J., et al.

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