LP 550-135 , the SIMBAD biblio

LP 550-135 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:54:55


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Title First 3 Authors
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.
2010A&A...522A..65R viz 15       D               2 77 4 New high-sensitivity, milliarcsecond resolution results from routine observations of lunar occultations at the ESO VLT. RICHICHI A., FORS O., CHEN W.-P., et al.
2014AJ....147...20N viz 15       D               2 543 170 Near-infrared metallicities, radial velocities, and spectral types for 447 nearby M dwarfs. NEWTON E.R., CHARBONNEAU D., IRWIN J., et al.
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.
2015ApJ...800...85N viz 16       D               1 525 94 An empirical calibration to estimate cool dwarf fundamental parameters from H-band spectra. NEWTON E.R., CHARBONNEAU D., IRWIN J., et al.
2015ApJ...812....3W viz 16       D               1 239 135 An activity-rotation relationship and kinematic analysis of nearby mid-to-late-type M dwarfs. WEST A.A., WEISENBURGER K.L., IRWIN J., 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.
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 45304 70 The AllWISE motion survey, part 2. KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al.
2017ApJ...834...85N viz 16       D               1 2207 217 The Hα emission of nearby M dwarfs and its relation to stellar rotation. NEWTON E.R., IRWIN J., CHARBONNEAU D., 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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL 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.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022A&A...660A..38W viz 17       D               1 736 1 Ultracool dwarfs identified using spectra in LAMOST DR7. WANG Y.-F., LUO A.-L., CHEN W.-P., 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.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al.
2024AJ....167...56C viz 18       D               1 1125 ~ The POKEMON Speckle Survey of Nearby M Dwarfs. II. Observations of 1125 Targets. CLARK C.A., VAN BELLE G.T., HORCH E.P., et al.
2026ApJ...997..244X 20       D               1 82 ~ Magnetic Activity of Ultracool Dwarfs in the LAMOST DR11. XIANG Y., GU S. and CAO D.

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