RX J1821.6+6827: A cool cluster at z =0 .81 from the ROSAT NEP survey
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- Type
- article
- Published
- 2004-08-02
- Cited by
- 19
- References
- 47
- Access
- Open access
- OpenAlex
- https://openalex.org/W2123536989
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:1884985
Keywords
ROSAT, Physics, Astrophysics, Redshift, Luminosity
References
- The ROSAT North Ecliptic Pole Survey X-Ray Data
- Catalog and Atlas from a Sensitive 1.5 GHz Radio Survey Around the North Ecliptic Pole
- Measuring Ωm with the ROSAT Deep Cluster Survey
- Overview of the ROSAT North Ecliptic Pole Survey
- Standard Solar Composition
- Measuring omega(0) using cluster evolution
- Mass estimates of X-ray clusters
- Cosmological Constraints from the Evolution of the Cluster Baryon Mass Function at z ~ 0.5
- The Canada-France Redshift Survey. II. Spectroscopic Program: Data for the 0000-00 and 1000+25 Fields
- The First Detailed X-Ray Observations of High-Redshift, Optically Selected Clusters: XMM-Newton Results for Cl 1324+3011 at z = 0.76 and Cl 1604+4304 at z = 0.90
- Abundances of the elements: Meteoritic and solar
- Observational Tests of the Mass-Temperature Relation for Galaxy Clusters
- A Very Hot High-Redshift Cluster of Galaxies: More Trouble for Ω0 = 1
- The WARPS survey - IV. The X-ray luminosity-temperature relation of high-redshift galaxy clusters
- Cooling flows and the X-ray luminosity–temperature relation for clusters
- The relation between velocity dispersion and temperature in clusters: Limiting the velocity bias
- Correlations of Richness and Global Properties in Galaxy Clusters
- The North Ecliptic Pole Supercluster
- EXOSAT observations of clusters of galaxies. I - The X-ray data. II - X-ray to optical correlations
- A catalog of intracluster gas temperatures
Cited by
- THE ORIGIN OF [O ii] IN POST-STARBURST AND RED-SEQUENCE GALAXIES IN HIGH-REDSHIFT CLUSTERS
- Kinematic analysis of a sample of X-ray luminous distant galaxy clusters - The LX − σv relation in the z > 0.6 universe
- The radio luminosity function of the NEP distant cluster radio galaxies
- THE OBSERVATIONS OF REDSHIFT EVOLUTION IN LARGE-SCALE ENVIRONMENTS (ORELSE) SURVEY. I. THE SURVEY DESIGN AND FIRST RESULTS ON CL 0023+0423 AT z = 0.84 AND RX J1821.6+6827 AT z = 0.82
- THE EVOLUTION AND ENVIRONMENTS OF X-RAY EMITTING ACTIVE GALACTIC NUCLEI IN HIGH-REDSHIFT LARGE-SCALE STRUCTURES
- The stellar population of the Rosat North Ecliptic Pole survey
- THE X-RAY–OPTICAL RELATIONS FOR NINE CLUSTERS AT z = 0.7–1.1 FROM THE ORELSE SURVEY
- Scaling relations of the colour-detected cluster RzCS 052 at z= 1.016 and some other high-redshift clusters
- The X-ray properties of optically selected z > 0.6 clusters in the European Southern Observatory Distant Cluster Survey
- Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ~ 1.5
- A deep survey of the AKARI north ecliptic pole field - I. WSRT 20 cm radio survey description, observations and data reduction
- The XMM Cluster Survey: evolution of the velocity dispersion–temperature relation over half a Hubble time
- X-ray-emitting active galactic nuclei from z = 0.6 to 1.3 in the intermediate- and high-density environments of the ORELSE survey
- Erratum: The properties of radio galaxies and the effect of environment in large-scale structures at z ̃ 1
- Evaluating tests of virialization and substructure using galaxy clusters in the ORELSE survey
- Possible evidence of the radio AGN quenching of neighbouring galaxies atz∼ 1
- Persistence of the colour–density relation and efficient environmental quenching to z ∼ 1.4
- Extended Radio AGN at z ∼ 1 in the ORELSE Survey: The Confining Effect of Dense Environments
- The Central Engines of Fermi Blazars
- The stellar population of the Rosat North Ecliptic Pole survey
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