2dFGRS TGN371Z187 , the SIMBAD biblio

2dFGRS TGN371Z187 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:09:04


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Title First 3 Authors
2001MNRAS.328.1039C viz 206868 1908 The 2dF Galaxy Redshift Survey: spectra and redshifts. COLLESS M., DALTON G., MADDOX S., et al.
2011ApJ...733..105K 15       D               5 28 46 Halo gas and galaxy disk kinematics of a volume-limited sample of mg II absorption-selected galaxies at z ∼ 0.1. KACPRZAK G.G., CHURCHILL C.W., BARTON E.J., et al.
2011AJ....142..122C viz 246       D     X         7 69 4 Ca II and Na I quasar absorption-line systems in an emission-selected sample of SDSS DR7 Galaxy/Quasar projections. I. Sample selection. CHERINKA B. and SCHULTE-LADBECK R.E.
2012MNRAS.426..801B 19       D               1 22 207 Physical properties of galactic winds using background quasars. BOUCHE N., HOHENSEE W., VARGAS R., et al.
2013ApJ...776..114N viz 16       D               1 299 88 MAGIICAT I. The Mg II absorber-galaxy catalog. NIELSEN N.M., CHURCHILL C.W., KACPRZAK G.G., et al.
2013ApJ...779...87C viz 16       D               1 163 43 MAGIICAT III. Interpreting self-similarity of the circumgalactic medium with virial mass using Mg II absorption. CHURCHILL C.W., TRUJILLO-GOMEZ S., NIELSEN N.M., et al.
2014ApJ...788...45T viz 16       D               1 224162 54 Luminosity and redshift dependence of the covering factor of active galactic nuclei viewed with WISE and Sloan Digital Sky Survey. TOBA Y., OYABU S., MATSUHARA H., et al.
2015ApJ...804...83S 17       D               1 16 34 The VLT SINFONI Mg II program for line emitters (SIMPLE). II. Background quasars probing z ∼ 1 galactic winds. SCHROETTER I., BOUCHE N., PEROUX C., et al.
2017A&A...599A..71D viz 16       D               1 209270 41 Aperture-free star formation rate of SDSS star-forming galaxies. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.
2022A&A...666A.186D viz 18       D               1 194358 6 Mass-metallicity and star formation rate in galaxies: A complex relation tuned to stellar age. DUARTE PUERTAS S., VILCHEZ J.M., IGLESIAS-PARAMO J., et al.

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