Spectroscopic follow-up of a cluster candidate at z = 1.45
We have obtained deep optical spectroscopic data of the highest-redshift cluster candidate (z ~ 1.4, CVB13) selected by Van Breukelen et al. (2006) in a photometric optical/infrared catalogue of the Subaru XMM-Newton Deep Field. The data, which comprise 104 targeted galaxies, were taken with the DEe...
Päätekijät: | Breukelen, C, Cotter, G, Rawlings, S, Readhead, T, Bonfield, D, Clewley, L, Ivison, R, Jarvis, M, Simpson, C, Watson, M |
---|---|
Aineistotyyppi: | Journal article |
Julkaistu: |
2007
|
Samankaltaisia teoksia
-
Evidence of a link between the evolution of clusters and their AGN
fraction
Tekijä: Breukelen, C, et al.
Julkaistu: (2009) -
Galaxy clusters at 0.6 < z < 1.4 in the UKIDSS Ultra Deep Survey Early
Data Release
Tekijä: Breukelen, C, et al.
Julkaistu: (2006) -
The radio galaxy K-z relation to z ~ 4.5
Tekijä: Jarvis, M, et al.
Julkaistu: (2001) -
The radio galaxy K-z relation to z similar to 4.5
Tekijä: Jarvis, M, et al.
Julkaistu: (2001) -
The discovery of a typical radio galaxy at z = 4.88
Tekijä: Jarvis, M, et al.
Julkaistu: (2009)