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- W1673201210 abstract "A radio continuum survey of a complete sample of distant (z = 0.3–0.8) X-ray–selected clusters has been conducted at 20 cm with the Very Large Array (VLA). The targets for this survey are the complete sample of 19 distant clusters found in the X-ray–selected Einstein Extended Medium Sensitivity Survey (EMSS) at z ≥ 0.3 and δ ≥ -20°. This survey is complete to a limiting point-source radio power level of log P ≥ 23.5 W Hz-1 (H0 = 75 km s-1 Mpc-1 and q0 = 0.1) out to ½ Abell cluster radius from the brightest cluster galaxy close to the X-ray emission centroid. Of the total of 41 radio sources detected within ½ Abell radius, 23 are associated with galaxies in these clusters. Higher angular resolution mapping of these cluster radio galaxies provides details of their structure and morphology. A comparison of the radio power levels, radio structure, position in the cluster, and the total number of these radio galaxies finds no evidence for any significant differences compared to nearby rich cluster radio galaxies. The radio luminosity function of distant cluster radio galaxies is statistically indistinguishable from that seen nearby. Taken together with the minimal evolution seen in the number of rich clusters over the same time period, this provides substantial evidence for no evolution in the population of rich cluster radio galaxies since z ∼ ½." @default.
- W1673201210 created "2016-06-24" @default.
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- W1673201210 date "1999-05-01" @default.
- W1673201210 modified "2023-10-17" @default.
- W1673201210 title "The Evolution of Cluster Radio Galaxies from [CLC][ITAL]z[/ITAL][/CLC] = 0 to [CLC][ITAL]z[/ITAL][/CLC] = 0.8" @default.
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- W1673201210 doi "https://doi.org/10.1086/300826" @default.
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