Cl* NGC 2632 JS 280 , the SIMBAD biblio

Cl* NGC 2632 JS 280 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST07:33:54


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Title First 3 Authors
1952ApJ...116..640J 171 199 Praesepe: magnitudes and colors. JOHNSON H.L.
1962ZA.....56...94E 280 1 Infrarot-Photometrie der Praesepe. EBERLEIN K.
1979AJ.....84.1586U 57 39 Photometry of Praesepe in BVRI colors. UPGREN A.R., WEIS E.W. and DELUCA E.E.
1991AJ....102.1080J 767 61 The luminosity function of Praesepe. I. A proper motion and photometric search for candidate members. JONES B.F. and STAUFFER J.R.
1991ChA&A..15..397W 258 ~ J2000.0 positions and proper motions of 257 stars in the central part of the Praesepe astrometric standard region. WANG J.-J. and JIANG P.-F.
1995A&AS..113..419W viz 933 15 High-precision study of proper motions and membership of 924 stars in the central region of Praesepe. WANG J.J., CHEN L., ZHAO J.-H., et al.
1995AJ....109.1379A viz 14       D               1 269 93 Moderate-resolution spectral standards from lambda-5600 to lambda-9000 Angstroms. ALLEN L.E. and STROM K.M.
2002AJ....124.1570A viz 5088 50 Structure of the Praesepe star cluster. ADAMS J.D., STAUFFER J.R., SKRUTSKIE M.F., et al.
2007AJ....134.2340K viz 15       D               1 1281 262 The stellar populations of Praesepe and Coma Berenices. KRAUS A.L. and HILLENBRAND L.A.
2014ApJ...784...57W viz 16       D               1 1032 18 Characterization of the Praesepe star cluster by photometry and proper motions with 2MASS, PPMXL, and Pan-STARRS. WANG P.F., CHEN W.P., LIN C.C., et al.
2014MNRAS.442.2081K viz 16       D               1 218 18 Stellar rotational periods in the planet hosting open cluster Praesepe. KOVACS G., HARTMAN J.D., BAKOS G.A., et al.
2014ApJ...795..161D viz 16       D               1 1906 99 The factory and the beehive. II. Activity and rotation in Praesepe and the Hyades. DOUGLAS S.T., AGUEROS M.A., COVEY K.R., et al.
2016ApJS..224....2H viz 16       D               1 31767 226 The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. HUBER D., BRYSON S.T., HAAS M.R., et al.
2017ApJ...839...92R viz 16       D               3 995 73 Rotation of late-type stars in Praesepe with K2. REBULL L.M., STAUFFER J.R., HILLENBRAND L.A., et al.
2017ApJ...842...83D viz 16       D               5 867 89 Poking the beehive from space: K2 rotation periods for Praesepe. DOUGLAS S.T., AGUEROS M.A., COVEY K.R., et al.
2017AJ....154..224R viz 16       D               1 3476 62 Zodiacal Exoplanets In Time (ZEIT). V. A uniform search for transiting planets in young clusters observed by K2. RIZZUTO A.C., MANN A.W., VANDERBURG A., et al.
2018AJ....155...51H viz 41           X         1 87 5 Robo-AO discovery and basic characterization of wide multiple star systems in the Pleiades, Praesepe, and NGC 2264 clusters. HILLENBRAND L.A., ZHANG C., RIDDLE R.L., et al.
2018MNRAS.476..908F viz 16       D               1 752 35 Stellar activity with LAMOST - II. Chromospheric activity in open clusters. FANG X.-S., ZHAO G., ZHAO J.-K., et al.
2019MNRAS.483.1125J viz 17       D               2 239 1 A search for radius inflation among active M-dwarfs in Praesepe. JACKSON R.J., JEFFRIES R.D., DELIYANNIS C.P., et al.
2019A&A...622A.133I viz 17       D               1 1629 47 Flares in open clusters with K2. I. M 45 (Pleiades), M 44 (Praesepe), and M 67. ILIN E., SCHMIDT S.J., DAVENPORT J.R.A., et al.
2019ApJ...879..100D viz 17       D               1 1008 100 K2 rotation periods for low-mass Hyads and a quantitative comparison of the distribution of slow rotators in the Hyades and Praesepe. DOUGLAS S.T., CURTIS J.L., AGUEROS M.A., et al.
2020ApJ...893...67M viz 17       D               1 533 31 A relationship between stellar age and spot coverage. MORRIS B.M.
2021ApJ...921..167R viz 17       D               1 1033 16 Three K2 campaigns yield rotation periods for 1013 stars in Praesepe. RAMPALLI R., AGUEROS M.A., CURTIS J.L., et al.
2022MNRAS.514.4781X viz 18       D               1 801 ~ Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey. XIANG Y., GU S. and CAO D.

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