ACO S 400 , the SIMBAD biblio

ACO S 400 , the SIMBAD biblio (38 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST08:16:57


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Title First 3 Authors
1989ApJS...70....1A viz 5256 1561 A catalog of rich clusters of galaxies. ABELL G.O., CORWIN H.G.Jr and OLOWIN R.P.
1990ApJS...72..567G viz 872 653 The Einstein Observatory extended medium-sensitivity survey. I. X-ray data and analysis. GIOIA M., MACCACARO T., SCHILD R.E., et al.
1990Msngr..62...45G 8 1 Galaxy populations in medium distant and distant clusters. GIRAUD E.
1991ApJS...76..813S viz 14       D               1 855 870 The Einstein Observatory extended medium-sensitivity survey. II. The optical identifications. STOCKE J.T., MORRIS S.L., GIOIA I.M., et al.
1992AJ....104.1290G 437 12 Photometric properties of three X-ray selected clusters of galaxies. GARILLI B., BOTTINI D., MACCAGNI D., et al.
1992ApJ...386..408H 109 355 The extented medium sensitivity survey distant cluster sample : X-ray data and interpretation of the luminosity evolution. HENRY J.P., GIOIA I.M., MACCACARO T., et al.
1993ApJ...410..499B 9 10 Galaxy colors in distant clusters as a test for the world model. BUZZONI A., CHINCARINI G. and MOLINARI E.
1994ApJ...422L...5L 26 85 Imaging of 16 distant EMSS clusters with z > 0.2 and Lx,44 > 4: new arcs and first consequences. LE FEVRE O., HAMMER F., ANGONIN M.C., et al.
1994ApJS...94..583G 111 245 The EMSS catalog of X-ray-selected clusters of galaxies. I. An atlas of CCD images of 41 distant clusters. GIOIA I.M. and LUPPINO G.A.
1997A&A...319..764H 19 31 Measurement of mass distribution of galaxy clusters using the giant luminous arc statistics with Le Fevre et al.'s arc survey data. HATTORI M., WATANABE K. and YAMASHITA K.
1997ApJ...481..644N 32 64 Evolution in the X-ray cluster luminosity function revisited. NICHOL R.C., HOLDEN B.P., ROMER A.K., et al.
1997ApJ...482L..13M 2 39 288 The luminosity-temperature relation at z=0.4 for clusters of galaxies. MUSHOTZKY R.F. and SCHARF C.A.
1997ApJ...489L...1H 6 10 194 A measurement of the density parameter derived from the evolution of cluster X-ray temperatures. HENRY J.P.
1998A&A...329...21S 80 85 Constraining {OMEGA}0 from X-ray properties of clusters of galaxies at high redshift. SADAT R., BLANCHARD A. and OUKBIR J.
1998ApJ...493...54C 85 84 A medium survey of the hard X-ray sky with the ASCA gas imaging spectrometer: the (2-10 keV) number counts relationship. CAGNONI I., DELLA CECA R. and MACCACARO T.
1999A&A...351..413M 23 24 The giant luminous arc statistics. II. Spherical lens models based on ROSAT HRI data. MOLIKAWA K., HATTORI M., KNEIB J.-P., et al.
1999A&AS..136..117L 65 90 A search for gravitational lensing in 38 X-ray selected clusters of galaxies. LUPPINO G.A., GIOIA I.M., HAMMER F., et al.
1999ApJ...524...22W 245 174 The LX-t and LX-σ relationships for galaxy clusters revisited. WU X.-P., XUE Y.-J. and FANG L.-Z.
2000ApJ...534..565H 2 43 259 Measuring cosmological parameters from the evolution of cluster X-ray temperatures. HENRY J.P.
2000PASJ...52..153M 70 42 Gas, iron, and gravitational mass in galaxy clusters : the general lack of cluster evolution at z < 1.0. MATSUMOTO H., TSURU T., FUKAZAWA Y., et al.
2001ApJ...553..668E 19 7 417 MACS: a quest for the most massive galaxy clusters in the universe. EBELING H., EDGE A.C. and HENRY J.P.
2002A&A...389....1A 30 58 The X-ray surface brightness profiles of hot galaxy clusters up to z ∼ 0.8: Evidence for self-similarity and constraints on Ω0. ARNAUD M., AGHANIM N. and NEUMANN D.M.
2002AJ....124.2413N 84 54 The evolution of the galaxy cluster luminosity-temperature relation. NOVICKI M.C., SORNIG M. and HENRY J.P.
2002MNRAS.329...87D viz 903 64 The 2dF Galaxy Redshift Survey: a targeted study of catalogued clusters of galaxies. DE PROPRIS R., COUCH W.J., COLLESS M., et al.
2002MNRAS.330..631E 15 11 A reanalysis of the X-ray luminosities of clusters of galaxies with 0.3<z <0.6 in the EMSS sample. ELLIS S.C. and JONES L.R.
2003ApJ...599....7O 53 112 Arc statistics in triaxial dark matter halos: testing the collisionless cold dark matter paradigm. OGURI M., LEE J. and SUTO Y.
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.
2004ApJ...609..603H 53 106 X-ray temperatures for the extended medium-sensitivity survey high-redshift cluster sample: constraints on cosmology and the dark energy equation of state. HENRY J.P.
2005ApJ...627..186W 1 13 43 The environmental dependence of galaxy colors in intermediate-redshift X-ray-selected clusters. WAKE D.A., COLLINS C.A., NICHOL R.C., et al.
2007MNRAS.379..190C 15       D               1 114 151 The observed concentration-mass relation for galaxy clusters. COMERFORD J.M. and NATARAJAN P.
2007ApJS..172..561B viz 15       D               326 183 The 400 square degree ROSAT PSPC galaxy cluster survey: catalog and statistical calibration. BURENIN R.A., VIKHLININ A., HORNSTRUP A., 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.
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.
2014MNRAS.438.3049P 79               F     1 37 10 How typical is the Coma cluster ? PIMBBLET K.A., PENNY S.J. and DAVIES R.L.
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.
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.
2020ApJS..247...25B viz 17       D               1 506 110 The SPTpol Extended Cluster Survey. BLEEM L.E., BOCQUET S., STALDER B., et al.
2021ApJS..253....3H viz 17       D               1 4198 128 The Atacama Cosmology Telescope: a catalog of >4000 Sunyaev-Zel'dovich galaxy clusters. HILTON M., SIFON C., NAESS S., et al.

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