LEDA 88729 , the SIMBAD biblio

LEDA 88729 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST17:35:36


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Title First 3 Authors
1990ApJS...72..715T 1051 133 The dynamics and structure of rich clusters of galaxies. I. Velocity data. TEAGUE P.F., CARTER D. and GRAY P.M.
2003A&A...412...45P viz 15       D               1 956189 750 HYPERLEDA. I. Identification and designation of galaxies. PATUREL G., PETIT C., PRUGNIEL P., 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.
2012MNRAS.423..256H viz 15       D               1 77 16 Data and two-dimensional scaling relations for galaxies in Abell 1689: a hint of size evolution at z ∼ 0.2. HOUGHTON R.C.W., DAVIES R.L., DALLA BONTA E., 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 15       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 670875 246 The redMaPPer galaxy cluster catalog from DES science verification data. RYKOFF E.S., ROZO E., HOLLOWOOD D., et al.
2017AJ....154..251J viz 16       D               1 271 15 Galaxy populations in massive z = 0.2-0.9 clusters. I. Analysis of spectroscopy. JORGENSEN I., CHIBOUCAS K., BERKSON E., et al.
2018AJ....155..188L viz 16       D               1 13497 1 An analysis framework for understanding the origin of nuclear activity in low-power radio galaxies. LIN Y.-T., HUANG H.-J. and CHEN Y.-C.
2020ApJ...902...17S viz 16       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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