CD-37 1123 , the SIMBAD biblio

CD-37 1123 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST12:37:36


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Title First 3 Authors
2006A&A...460..695T viz 15       D               1891 534 Search for associations containing young stars (SACY). I. Sample and searching method. TORRES C.A.O., QUAST G.R., DA SILVA L., et al.
2009ApJS..184..138H viz 15       D               2 20623 68 XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. HAAKONSEN C.B. and RUTLEDGE R.E.
2010A&A...517A..88W 38         O X         1 253 31 Rotational velocities of nearby young stars. WEISE P., LAUNHARDT R., SETIAWAN J., et al.
2014MNRAS.442..220F viz 15       D               1 1088 3 The FEROS-Lick/SDSS observational data base of spectral indices of FGK stars for stellar population studies. FRANCHINI M., MOROSSI C., MARCANTONIO P.D., et al.
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., et al.
2018A&A...609A.116R viz 16       D               1 143018 65 Empirical photometric calibration of the Gaia red clump: Colours, effective temperature, and absolute magnitude. RUIZ-DERN L., BABUSIAUX C., ARENOU F., et al.
2018A&A...615A..49C viz 16       D               1 224763 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.
2019A&A...622L..13M viz 16       D               1 264 78 Extended stellar systems in the solar neighborhood. II. Discovery of a nearby 120° stellar stream in Gaia DR2. MEINGAST S., ALVES J. and FURNKRANZ V.
2019AJ....158...77C viz 16       D               2 156 65 TESS reveals that the nearby Pisces-Eridanus stellar stream is only 120 Myr old. CURTIS J.L., AGUEROS M.A., MAMAJEK E.E., et al.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2019A&A...632A..37B viz 162         O X C       3 30 ~ Radial-velocity jitter of stars as a function of observational timescale and stellar age. BREMS S.S., KURSTER M., TRIFONOV T., et al.
2020ApJ...890...46T viz 16       D               1 403 45 Superflares on solar-type stars from the first year observation of TESS. TU Z.-L., YANG M., ZHANG Z.J., et al.
2020A&A...635L..13A 16       D               1 43 ~ Lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1). ARANCIBIA-SILVA J., BOUVIER J., BAYO A., et al.
2020ApJ...893...67M viz 16       D               1 533 31 A relationship between stellar age and spot coverage. MORRIS B.M.
2020MNRAS.494.2429B viz 58       D     X         2 240 ~ A kinematically hot population of young stars in the solar neighbourhood. BINKS A.S., JEFFRIES R.D. and WRIGHT N.J.
2020MNRAS.494.3596D viz 16       D               1 211 32 Superflares and variability in solar-type stars with TESS in the Southern hemisphere. DOYLE L., RAMSAY G. and DOYLE J.G.
2020A&A...639A..64R viz 16       D               1 4276 26 Extended stellar systems in the solar neighborhood. IV. Meingast 1: the most massive stellar stream in the solar neighborhood. RATZENBOCK S., MEINGAST S., ALVES J., et al.
2021A&A...647A.162P viz 17       D               1 1853 ~ The AMBRE Project: Origin and evolution of sulfur in the Milky Way. PERDIGON J., DE LAVERNY P., RECIO-BLANCO A., et al.
2022ApJ...928...70C viz 17       D               1 5007 6 Pearls on a String: Numerous Stellar Clusters Strung Along the Same Orbit. CORONADO J., FURNKRANZ V. and RIX H.-W.
2024A&A...683A.125P viz 18       D               1 3561 ~ Analysis of the public HARPS/ESO spectroscopic archive Ca II H&K time series for the HARPS radial velocity database. PERDELWITZ V., TRIFONOV T., TEKLU J.T., et al.
2024AJ....167..210V viz 18       D               1 7289 ~ The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. VACH S., ZHOU G., HUANG C.X., et al.

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