ClG J1113-2615 , the SIMBAD biblio

ClG J1113-2615 , the SIMBAD biblio (35 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST00:16:07


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Title First 3 Authors
2002ApJS..140..265P viz 295 90 The WARPS survey. VI. Galaxy cluster and source identifications from phase I. PERLMAN E.S., HORNER D.J., JONES L.R., et al.
2003A&A...398..879E 1 18 101 Constraining the cosmological parameters with the gas mass fraction in local and z>0.7 galaxy clusters. ETTORI S., TOZZI P. and ROSATI P.
2003ApJ...587..589M 41   K                 6 72 Chandra X-ray analysis of the massive high-redshift galaxy clusters
Cl J1113.1-2615 and Cl J0152.7-1357.
MAUGHAN B.J., JONES L.R., EBELING H., et al.
2003ApJ...593..705T 1 17 100 Iron abundance in the intracluster medium at high redshift. TOZZI P., ROSATI P., ETTORI S., et al.
2004A&A...417...13E 2 27 192 Scaling laws in X-ray galaxy clusters at redshift between 0.4 and 1.3. ETTORI S., TOZZI P., BORGANI S., et al.
2004A&A...424.1097S viz 15       D               1 1674 24 Introducing BAX: A database for X-ray clusters and groups of galaxies. SADAT R., BLANCHARD A., KNEIB J.-P., et al.
2004ApJS..150...19K viz 67 104 Chandra multiwavelength project. I. First X-ray source catalog. KIM D.-W., CAMERON R.A., DRAKE J.J., et al.
2005A&A...430...39C 15 44 X-ray source overdensities in Chandra distant cluster fields: A new probe to map the cosmic tapestry? CAPPELLUTI N., CAPPI M., DADINA M., et al.
2005ApJ...624..606J 42 105 The evolution of structure in X-ray clusters of galaxies. JELTEMA T.E., CANIZARES C.R., BAUTZ M.W., et al.
2006MNRAS.365..509M 3 12 88 The evolution of the cluster X-ray scaling relations in the Wide Angle ROSAT Pointed Survey sample at 0.6 < z < 1.0. MAUGHAN B.J., JONES L.R., EBELING H., et al.
2007A&A...462..429B         O           67 128 Tracing the evolution in the iron content of the intra-cluster medium. BALESTRA I., TOZZI P., ETTORI S., et al.
2007A&A...467..485H 15       D               2 104 26 Robust quantitative measures of cluster X-ray morphology, and comparisons between cluster characteristics. HASHIMOTO Y., BOEHRINGER H., HENRY J.P., et al.
2007A&A...472..739B 38 25 High redshift X-ray galaxy clusters. II. The LX-T relationship revisited. BRANCHESI M., GIOIA I.M., FANTI C., et al.
2008ApJS..174..117M viz 15       D               127 246 Images, structural properties, and metal abundances of galaxy clusters observed with Chandra ACIS-I at 0.1<z<1.3. MAUGHAN B.J., JONES C., FORMAN W., et al.
2008A&A...483...35S 17       D               4 38 177 Searching for cool core clusters at high redshift. SANTOS J.S., ROSATI P., TOZZI P., et al.
2008ApJ...682..821C viz 15       D               1 208 43 Bandpass dependence of X-ray temperatures in galaxy clusters. CAVAGNOLO K.W., DONAHUE M., VOIT G.M., et al.
2009MNRAS.392.1509G viz 15       D               2 208 49 The distribution of active galactic nuclei in a large sample of galaxy clusters. GILMOUR R., BEST P. and ALMAINI O.
2009A&A...501...61E 16       D               1 60 165 The cluster gas mass fraction as a cosmological probe: a revised study. ETTORI S., MORANDI A., TOZZI P., et al.
2010A&A...521A..64S 15       D               1 64 68 The evolution of cool-core clusters. SANTOS J.S., TOZZI P., ROSATI P., et al.
2011A&A...529A..65Y 15       D               2 46 19 Measuring redshifts using X-ray spectroscopy of galaxy clusters: results from Chandra data and future prospects. YU H., TOZZI P., BORGANI S., et al.
2011ApJ...740...59H viz 15       D               4 143 6 The evolution of radio galaxies and X-ray point sources in Coma cluster progenitors since z ∼ 1.2. HART Q.N., STOCKE J.T., EVRARD A.E., et al.
2011A&A...534A.109P viz 15       D               1 1770 422 The MCXC: a meta-catalogue of X-ray detected clusters of galaxies. PIFFARETTI R., ARNAUD M., PRATT G.W., et al.
2011A&A...535A...4R viz 15       D               2 225 108 Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ∼ 1.5. REICHERT A., BOEHRINGER H., FASSBENDER R., et al.
2012MNRAS.421.1583M 117 149 Self-similar scaling and evolution in the galaxy cluster X-ray luminosity-temperature relation. MAUGHAN B.J., GILES P.A., RANDALL S.W., et al.
2012MNRAS.425..477N viz 15       D               1 1763 27 γ-rays from annihilating dark matter in galaxy clusters: stacking versus single source analysis. NEZRI E., WHITE R., COMBET C., et al.
2012A&A...546A...6A viz 15       D               1 131 18 The enrichment history of the intracluster medium: a Bayesian approach. ANDREON S.
2013A&A...555A..66L viz 16       D               1 123 48 A comprehensive picture of baryons in groups and clusters of galaxies. LAGANA T.F., MARTINET N., DURRET F., et al.
2014ARep...58..587B viz 16       D               1 137 42 Chandra X-ray galaxy clusters at z < 1.4: Constraints on the inner slope of the density profiles. BABYK Y.V., DEL POPOLO A. and VAVILOVA I.B.
2015MNRAS.447.3723P 16       D               1 90 8 The Chandra Deep Group Survey - cool core evolution in groups and clusters of galaxies. PASCUT A. and PONMAN T.J.
2015MNRAS.450.2261M viz 16       D               1 321 30 The galaxy cluster outskirts probed by Chandra. MORANDI A., SUN M., FORMAN W., et al.
2016MNRAS.455..892G viz 16       D               1 353 14 The galaxy cluster concentration-mass scaling relation. GROENER A.M., GOLDBERG D.M. and SERENO M.
2016A&A...590A.126A 56       D     X         2 47 13 The relation between mass and concentration in X-ray galaxy clusters at high redshift. AMODEO S., ETTORI S., CAPASSO R., et al.
2017MNRAS.468.3322S viz 16       D               1 28168 37 CoMaLit - V. Mass forecasting with proxies: method and application to weak lensing calibrated samples. SERENO M. and ETTORI S.
2017A&A...604A.100G 47 4 On the evolution of the entropy and pressure profiles in X-ray luminous galaxy clusters at z > 0.4. GHIRARDINI V., ETTORI S., AMODEO S., et al.
2021ApJ...911...82C viz 17       D               1 388 ~ Cosmological constraints from galaxy cluster sparsity, cluster gas mass fraction, and baryon acoustic oscillation data. CORASANITI P.-S., SERENO M. and ETTORI S.

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