LP 396-24 , the SIMBAD biblio

LP 396-24 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST00:49:02

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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
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.
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.
2014ApJ...784..156D viz 15       D               1 1505 60 Trigonometric parallaxes for 1507 nearby mid-to-late M dwarfs. DITTMANN J.A., IRWIN J.M., CHARBONNEAU D., et al.
2016ApJ...818..153D viz 16       D               1 1874 9 Calibration of the MEarth photometric system: optical magnitudes and photometric metallicity estimates for 1802 nearby M-dwarfs. DITTMANN J.A., IRWIN J.M., CHARBONNEAU D., et al.
2016ApJ...821...93N viz 16       D               2 1898 209 The rotation and galactic kinematics of mid M dwarfs in the solar neighborhood. NEWTON E.R., IRWIN J., CHARBONNEAU D., et al.
2017AJ....154..191J viz 56       D     X         2 116 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 52096 ~ 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 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2022ApJ...927..122H viz 17       D               1 3750 2 Chemical Properties of the Local Disk and Halo. II. Abundances of 3745 M Dwarfs and Subdwarfs from Improved Model Fitting of Low-resolution Spectra. HEJAZI N., LEPINE S. and NORDLANDER T.

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