A Catalog of 203 Galaxy Clusters Serendipitously Detected in the ROSAT PSPC Pointed Observations
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A. Hornstrup | W. Forman | H. Quintana | C. Jones | B. McNamara | A. Vikhlinin | C. Jones
[1] M. Malkan,et al. The WARPS Survey. II. The log N-log S Relation and the X-Ray Evolution of Low-Luminosity Clusters of Galaxies , 1997, astro-ph/9709189.
[2] G. Efstathiou,et al. The origin of the cosmic soft X-ray background: optical identification of an extremely deep ROSAT survey , 1997, astro-ph/9703163.
[3] W. F ORMAN,et al. Evolution of Cluster X-ray Luminosities and Radii: Results from the 160 Square Degree Rosat Survey , 1998 .
[4] R. Della Ceca,et al. The ROSAT Deep Cluster Survey: The X-Ray Luminosity Function out to z = 0.8 , 1997, astro-ph/9710308.
[5] J. Henry. A Measurement of the Density Parameter Derived from the Evolution of Cluster X-Ray Temperatures , 1997 .
[6] S. Schindler,et al. A dark cluster of galaxies at redshift z = 1 , 1997, Nature.
[7] Antonio Maggio,et al. A Method Based on Wavelet Transforms for Source Detection in Photon-counting Detector Images. I. Theory and General Properties , 1997 .
[8] R. Petre,et al. A Possible Site of Cosmic Ray Acceleration in the Supernova Remnant IC 443 , 1997, astro-ph/9702056.
[9] A. Edge,et al. The ROSAT Brightest Cluster Sample (BCS): The Cluster X-Ray Luminosity Function within z = 0.3 , 1997, astro-ph/9701179.
[10] R. Nichol,et al. On the Evolution of X-Ray Clusters at High Redshift , 1997, astro-ph/9701143.
[11] C. Frenk,et al. Projection effects in cluster catalogues , 1997, astro-ph/9701103.
[12] H. Ebeling,et al. The Environmental Dependence of Brightest Cluster Galaxies: Implications for Large-Scale Flows , 1996, astro-ph/9611083.
[13] R. Nichol,et al. Evolution in the X-Ray Cluster Luminosity Function Revisited , 1996, astro-ph/9611182.
[14] M. Malkan,et al. The Wide-Angle ROSAT Pointed X-Ray Survey of Galaxies, Groups, and Clusters. I. Method and First Results , 1996, astro-ph/9608200.
[15] A. Liddle,et al. The cluster abundance in flat and open cosmologies , 1995, astro-ph/9511007.
[16] Truong Q. Nguyen,et al. Wavelets and filter banks , 1996 .
[17] J. B. Oke,et al. The Palomar Distant Clusters Survey. I. The Cluster Catalog , 1995, astro-ph/9511011.
[18] W. Forman,et al. Detection of the Angular Correlation of Faint X-Ray Sources , 1995, astro-ph/9510040.
[19] C. Jones,et al. Matched Filter Source Detection Applied to the ROSAT PSPC and the Determination of the Number-Flux Relation , 1995 .
[20] W. Forman,et al. ROSAT Extended Medium-Deep Sensitivity Survey: Source Counts for 130 Fields , 1995 .
[21] F. Castander,et al. Deficit of distant X-ray-emitting galaxy clusters and implications for cluster evolution , 1995, Nature.
[22] C. Jones,et al. Wavelet transform analysis of the small-scale X-ray structure of the cluster Abell 1367 , 1995 .
[23] H. Tananbaum,et al. A serach for 'failed clusters' of galaxies , 1995 .
[24] R. Giacconi,et al. A FIRST DETERMINATION OF THE SURFACE DENSITY OF GALAXY CLUSTERS AT VERY LOW X--RAY FLUXES , 1995, astro-ph/9503064.
[25] J. Mohr,et al. Cosmological Constraints from Observed Cluster X-Ray Morphologies , 1995, astro-ph/9501011.
[26] G. Luppino,et al. A possible fossil galaxy group , 1994, Nature.
[27] W. Forman,et al. A catalog of intracluster gas temperatures , 1993 .
[28] S. White,et al. The Correlation function of clusters of galaxies and the amplitude of mass fluctuations in the Universe , 1993, astro-ph/9602052.
[29] P. Peebles. Principles of Physical Cosmology , 1993 .
[30] G. C. Stewart,et al. Properties of cooling flows in a flux-limited sample of clusters of galaxies , 1992 .
[31] S. Morris,et al. The extended medium sensitivity survey distant cluster sample - X-ray data and interpretation of the luminosity evolution , 1992 .
[32] J. Hughes,et al. A measurement of the value of the Hubble constant from the X-ray properties and the Sunyaev-Zel'dovich effect of Abell 665 , 1991 .
[33] Isabella M. Gioia,et al. The Einstein Observatory Extended Medium-Sensitivity Survey. II - The optical identifications , 1991 .
[34] Keith A. Arnaud,et al. A measurement of the mass fluctuation spectrum from the cluster X-ray temperature function , 1991 .
[35] William H. Press,et al. Numerical recipes , 1990 .
[36] R. Schild,et al. The Einstein Observatory Extended Medium-Sensitivity Survey. I - X-ray data and analysis , 1990 .
[37] Nick Kaiser,et al. Evolution and clustering of rich clusters , 1986 .
[38] A. Fabian,et al. Cooling flows in clusters of galaxies , 1984, Nature.
[39] C. Heiles,et al. Reddenings derived from H I and galaxy counts : accuracy and maps. , 1982 .
[40] W. Cash,et al. Parameter estimation in astronomy through application of the likelihood ratio. [satellite data analysis techniques , 1979 .
[41] P. J. E. Peebles,et al. A computer model universe - Simulation of the nature of the galaxy distribution in the Lick catalog , 1978 .
[42] M. Rees,et al. Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering , 1978 .
[43] A. Sandage. The Redshift-Distance Relation. I. Angular Diameter of First Ranked Cluster Galaxies as a Function of Redshift: the Aperture Correction to Magnitudes , 1972 .
[44] C. Chatfield,et al. Statistics for physicists , 1971 .
[45] A. Eddington,et al. The correction of statistics for accidental error , 1940 .