LP 194-1 , the SIMBAD biblio

LP 194-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST17:06:42

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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
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 63380 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 16       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.
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.
2020A&A...643A.122S viz 17       D               1 3788 ~ Active deep learning method for the discovery of objects of interest in large spectroscopic surveys. SKODA P., PODSZTAVEK O. and TVRDIK P.
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.
2021PASJ...73..154K 17       D               3 42 ~ Characterization of M dwarfs using optical mid-resolution spectra for exploration of small exoplanets. KOIZUMI Y., KUZUHARA M., OMIYA M., et al.

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