SDSS-C4 1073 , the SIMBAD biblio

SDSS-C4 1073 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST19:31:23


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Title First 3 Authors
2005AJ....130..968M viz 15       D               1 796 263 The C4 clustering algorithm: clusters of galaxies in the Sloan Digital Sky Survey. MILLER C.J., NICHOL R.C., REICHART D., et al.
2007MNRAS.379..867V viz 15       D               1 1259 308 How special are brightest group and cluster galaxies? VON DER LINDEN A., BEST P.N., KAUFFMANN G., et al.
2011MNRAS.412..947B 92       D         F     7 17 28 The stellar and hot gas content of low-mass galaxy clusters. BALOGH M.L., MAZZOTTA P., BOWER R.G., et al.
2015MNRAS.448.2530Z viz 16       D               1 625 9 The link between morphology and structure of brightest cluster galaxies: automatic identification of cDs. ZHAO D., ARAGON-SALAMANCA A. and CONSELICE C.J.
2016A&A...585A.147A 16       D               2 41 9 The amazing diversity in the hot gas content of an X-ray unbiased massive galaxy clusters sample. ANDREON S., SERRA A.L., MORETTI A., et al.
2017A&A...606A..24A 41           X         1 35 2 Variegate galaxy cluster gas content: Mean fraction, scatter, selection effects, and covariance with X-ray luminosity. ANDREON S., WANG J., TRINCHIERI G., et al.
2020ApJS..246....2A viz 17       D               1 36251 ~ GalWeight application: a publicly available catalog of dynamical parameters of 1800 galaxy clusters from SDSS-DR13, (GalWCat19). ABDULLAH M.H., WILSON G., KLYPIN A., et al.
2022MNRAS.511.2968P 18       D               1 35 ~ Do gas-poor galaxy clusters have different galaxy populations? The positive covariance of hot and cold baryons. PUDDU E. and ANDREON S.
2022MNRAS.511.4991A 18       D               1 34 4 Low X-ray surface brightness clusters: implications on the scatter of the M-T and L-T relations. ANDREON S., TRINCHIERI G. and MORETTI A.

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