CD-49 2136 , the SIMBAD biblio

CD-49 2136 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:56:49


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Title First 3 Authors
2013AJ....146..134K viz 15       D               1 419759 301 The radial velocity experiment (RAVE): fourth data release. KORDOPATIS G., GILMORE G., STEINMETZ M., et al.
2017AJ....153...75K viz 16       D               1 451448 394 The Radial Velocity Experiment (RAVE): fifth data release. KUNDER A., KORDOPATIS G., STEINMETZ M., et al.
2017AJ....153..257O viz 16       D               1 10625 142 Comoving stars in Gaia DR1: an abundance of very wide separation comoving pairs. OH S., PRICE-WHELAN A.M., HOGG D.W., 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.
2018AJ....155..149B viz 16       D               1 9764 5 Fundamental properties of co-moving stars observed by Gaia. BOCHANSKI J.J., FAHERTY J.K., GAGNE J., et al.
2020AJ....160...83S viz 16       D               1 451375 83 The sixth Data Release of the Radial Velocity Experiment (RAVE). II. Stellar atmospheric parameters, chemical abundances, and distances. STEINMETZ M., GUIGLION G., McMILLAN P.J., et al.
2021AJ....161...24G viz 17       D               1 412 63 Vetting of 384 TESS Objects of Interest with TRICERATOPS and statistical validation of 12 planet candidates. GIACALONE S., DRESSING C.D., JENSEN E.L.N., et al.
2021AJ....162...75L viz 17       D               1 517 28 Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. LESTER K.V., MATSON R.A., HOWELL S.B., et al.
2021AJ....162..192Z viz 17       D               1 713 29 SOAR TESS survey. II. The impact of stellar companions on planetary populations. ZIEGLER C., TOKOVININ A., LATIOLAIS M., et al.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.

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