2dFGRS TGN259Z043 , the SIMBAD biblio

2dFGRS TGN259Z043 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST04:06:32


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Title First 3 Authors
2002MNRAS.335...10B viz 523 57 An Hα survey of the rich cluster A 1689. BALOGH M.L., COUCH W.J., SMAIL I., et al.
2003ApJS..146..267M viz 185 22 Radio-selected galaxies in very rich clusters at z ≤ 0.25. I. Multiwavelength observations and data reduction techniques. MORRISON G.E., OWEN F.N., LEDLOW M.J., et al.
2006ApJ...644..116M 55 95 Spectroscopic confirmation of a large population of active galactic nuclei in clusters of galaxies. MARTINI P., KELSON D.D., KIM E., et al.
2011ApJ...729...22A viz 15       D               1 589 13 A multi-wavelength study of low-redshift clusters of galaxies. I. Comparison of X-ray and mid-infrared selected active galactic nuclei. ATLEE D.W., MARTINI P., ASSEF R.J., et al.
2011A&A...527A.126P viz 15       D               1 16772 65 Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey. PINEAU F.-X., MOTCH C., CARRERA F., et al.
2012ApJ...754...97H 15       D               1 85 55 LoCuSS: a dynamical analysis of X-ray active galactic nuclei in local clusters. HAINES C.P., PEREIRA M.J., SANDERSON A.J.R., et al.
2012ApJ...761..114A viz 15       D               1 499 6 A multi-wavelength study of low-redshift clusters of galaxies. II. Environmental impact on galaxy growth. ATLEE D.W. and MARTINI P.
2013ApJ...767...15R viz 16       D               1 25361 168 Measuring the ultimate halo mass of galaxy clusters: redshifts and mass profiles from the Hectospec Cluster Survey (HeCS). RINES K., GELLER M.J., DIAFERIO A., et al.
2016ApJS..224....1R viz 16       D               1 670876 246 The redMaPPer galaxy cluster catalog from DES science verification data. RYKOFF E.S., ROZO E., HOLLOWOOD D., et al.
2020ApJ...902...17S viz 17       D               1 1627 ~ The velocity dispersion function for quiescent galaxies in nine strong-lensing clusters. SOHN J., FABRICANT D.G., GELLER M.J., et al.

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