LSPM J1524+2925 , the SIMBAD biblio

LSPM J1524+2925 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST09:26:10

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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
2002A&A...390L..27M 13 19 Search for nearby stars among proper motion stars selected by optical-to-infrared photometry. II. Two late M dwarfs within 10 pc. McCAUGHREAN M.J., SCHOLZ R.-D. and LODIEU N.
2002AJ....124..519R 44 131 High-resolution spectroscopy of ultracool M dwarfs. REID I.N., KIRKPATRICK J.D., LIEBERT J., et al.
2003AJ....126..921L 67 37 New high proper motion stars from the digitized sky survey. II. Northern stars with 0.5arcsec.yr–1 < µ < 2.0arcsec.yr–1 at high galactic latitudes. LEPINE S., SHARA M.M. and RICH R.M.
2003ApJ...583..451M 121 361 Rotation and activity in Mid-M to L field dwarfs. MOHANTY S. and BASRI G.
2003ApJ...598.1265S 39 32 An adaptive optics survey of M6.0-M7.5 stars: discovery of three very low mass binary systems including two probable Hyades members. SIEGLER N., CLOSE L.M., MAMAJEK E.E., et al.
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.
2005ApJ...621.1023S 74 86 Discovery of two very low mass binaries: final results of an adaptive optics survey of nearby M6.0-M7.5 stars. SIEGLER N., CLOSE L.M., CRUZ K.L., et al.
2011ApJS..197...19K viz 15       D               1 575 330 The first hundred brown dwarfs discovered by the Wide-field Infrared Survey Explorer (WISE). KIRKPATRICK J.D., CUSHING M.C., GELINO C.R., et al.
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.
2014A&A...566A.130C viz 16       D               1 336 47 Doppler imaging of exoplanets and brown dwarfs. CROSSFIELD I.J.M.
2016ApJ...817..112S viz 16       D               1 20551 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 45305 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.
2019ApJ...883..205B viz 17       D               1 500 34 The ultracool SpeXtroscopic survey. I. Volume-limited spectroscopic sample and luminosity function of M7-L5 ultracool dwarfs. BARDALEZ GAGLIUFFI D.C., BURGASSER A.J., SCHMIDT S.J., et al.
2020ApJ...891...58S viz 17       D               1 46 ~ Dim prospects for transmission spectra of ocean Earths around M stars. SUISSA G., MANDELL A.M., WOLF E.T., et al.
2020AJ....160..120J viz 17       D               2 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2021AJ....161..233K viz 17       D               1 6504 ~ Around which stars can TESS detect Earth-like planets? The Revised TESS Habitable Zone Catalog. KALTENEGGER L., PEPPER J., CHRISTODOULOU P.M., et al.
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.
2023AJ....165..149D 112       D       C       4 100 1 EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates of Planets around Late-M Dwarfs within 15 pc. DIETRICH J., APAI D., SCHLECKER M., et al.

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