Now showing items 1-4 of 4

    • Evidence of a link between the evolution of clusters and their AGN fraction 

      van Breukelen, C.; Simpson, C.; Rawlings, S.; Akiyama, M.; Bonfield, D.; Clewley, L.; Jarvis, M.J.; Mauch, T.; Readhead, T.; Stobbart, A.M.; Swinbank, M.; Watson, M. (2009)
    • Galaxy clusters at 0.6-z-1.4 in the UKIDSS ultra deep survey early data release 

      van Breukelen, C.; Clewley, L.; Bonfield, D.; Rawlings, S.; Jarvis, M.J.; Barr, J.M.; Foucaud, S.; Almaini, O.; Cirasuolo, M.; Dalton, G.; Dunlop, J.S.; Edge, A.C.; Hirst, P.; McLure, R.J.; Page, M.J.; Sekiguchi, K.; Simpson, C.; Smail, I.; Watson, M. (2006)
    • Spectroscopic follow-up of a cluster candidate at z = 1.45 

      van Breukelen, C.; Cotter, G.; Rawlings, S.; Readhead, T.; Bonfield, D.; Clewley, L.; Ivison, R.J.; Jarvis, M.J.; Simpson, C.; Watson, M. (2007)
    • X-ray groups and clusters of galaxies in the Subaru–XMM Deep Field 

      Finoguenov, A.; Watson, M.; Tanaka, M.; Simpson, C.; Cirasuolo, M.; Dunlop, J.S.; Peacock, J.A.; Farrah, D.; Akiyama, M.; Ueda, Y.; Smolcic, V.; Stewart, G.; Rawlings, S.; van Breukelen, C.; Almaini, O.; Clewley, L.; Bonfield, D.; Jarvis, M.J.; Barr, J.M.; Foucaud, S.; McLure, R.J.; Sekiguchi, K.; Egami, E. (2010)
      We present the results of a search for galaxy clusters in the Subaru–XMM Deep Field (SXDF). We reach a depth for a total cluster flux in the 0.5–2 keV band of 2 × 10−15 erg cm−2 s−1 over one of the widest XMM–Newton ...