The UKIDSS Deep eXtra-Galactic Survey

  • A. M. Swinbank
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 37)


The UKIDSS Deep eXtra-Galactic (DXS) will image an area of 35 sq.deg. at high Galactic latitudes in the J and K-band filters to a depth K = 21.0 (with 5 sq.deg. also imaged in H-band). When completed in 2012, the DXS will have used 118 nights to survey 4 of the best-studied extra-galactic fields: XMM-LSS, the Lockman Hole, SSA22 and ELAIS-N1. The principal goals of the DXS are to identify and measure the abundance of galaxy clusters at 0.8 < z < 1.5; to measure galaxy clustering in well defined samples at z > 1 (and hence measure the evolution of bias, a key test of hierarchical models); and to provide a multi-wavelength census of the luminosity density in star formation and AGN. Here, we describe some of the recent science highlights. Specifically, the discovery of a supercluster at z = 0.9 which spans >30 Mpc and has properties similar to local super-clusters (such as Hercules) and some of the first wide-field (∼3-sq.deg.) clustering measurements in EROs and DRGs.


Galaxy Cluster Cosmological Parameter Cluster Candidate High Galactic Latitude Cluster Mass Function 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


  1. Bremer, M.N., Valtchanov, I., Willis, J., Altieri, B., Andreon, S., Duc, P.A., Fang, F., Jean, C., et al.: XMM-LSS discovery of a z = 1.22 galaxy cluster. Mon. Not. R. Astron. Soc. 371, 1427 (2006)ADSCrossRefGoogle Scholar
  2. Couch, W.J., Ellis, R.S., MacLaren, I., Malin, D.F.: A uniformly selected catalogue of distant galaxy clusters. Mon. Not. R. Astron. Soc. 249, 606 (1991)ADSGoogle Scholar
  3. Eke, V.R., Cole, S., Frenk, C.S., Patrick Henry, J.: Measuring Omega_0 using cluster evolution. Mon. Not. R. Astron. Soc. 298, 1145 (1998)ADSCrossRefGoogle Scholar
  4. Evrard, A.E., MacFarland, T.J., Couchman, H.M.P., Colberg, J.M., Yoshida, N., White, S.D.M., Jenkins, A., Frenk, C.S., et al.: Galaxy clusters in hubble volume simulations: cosmological constraints from sky survey populations. Astrophys. J. 573, 7 (2002)ADSCrossRefGoogle Scholar
  5. Gladders, M.D., Yee, H.K.C.: A new method for galaxy cluster detection. I. The algorithm. Astron. J. 120, 2148 (2000)ADSCrossRefGoogle Scholar
  6. Hirst, P., Casali, M., Adamson, A., Ives, D., Kerr, T.: The UKIRT wide-field camera (WFCAM): commissioning and performance on the telescope. In: McLean, I.S., Iye, M. (eds.) Ground-based and airborne instrumentation for astronomy, Proceedings of the SPIE, vol. 6269, Orlando, FL, 25–29 May 2006Google Scholar
  7. Jenkins, A., Frenk, C.S., White, S.D.M., Colberg, J.M., Cole, S., Evrard, A.E., Couchman, H.M.P., Yoshida, N.: The mass function of dark matter haloes. Mon. Not. R. Astron. Soc. 321, 372 (2001)ADSCrossRefGoogle Scholar
  8. Kim, J.-W., Edge, A.C., Wake, D.A., Stott, J.P.: Clustering properties of high-redshift red galaxies in SA22 from the UKIDSS Deep eXtragalactic survey. Mon. Not. R. Astron. Soc. 410, 241–256 (2011). doi: 10.1111/j.1365-2966.2010.17439.x ADSCrossRefGoogle Scholar
  9. Lonsdale, C.J., Smith, H.E., Rowan-Robinson, M., Surace, J., Shupe, D., Xu, C., Oliver, S., Padgett, D., et al.: SWIRE: the SIRTF wide-area infrared extragalactic survey. Publ. Astron. Soc. Pac. 115, 897 (2003)ADSCrossRefGoogle Scholar
  10. Mullis, C.R., Rosati, P., Lamer, G., Böhringer, H., Schwope, A., Schuecker, P., Fassbender, R.: Discovery of an X-ray-luminous galaxy cluster at z=1.4. Astrophys. J. Lett. 623, L85 (2005)ADSCrossRefGoogle Scholar
  11. Reed, D.S., Bower, R., Frenk, C.S., Gao, L., Jenkins, A., Theuns, T., White, S.D.M.: The first generation of star-forming haloes. Mon. Not. R. Astron. Soc. 363, 393 (2005)ADSCrossRefGoogle Scholar
  12. Romer, A.K., Viana, P.T.P., Liddle, A.R., Mann, R.G.: A serendipitous galaxy cluster survey with XMM: expected catalog properties and scientific applications. Astrophys. J. 547, 594 (2001)ADSCrossRefGoogle Scholar
  13. Rosati, P., Borgani, S., Norman, C.: The evolution of X-ray clusters of galaxies. Annu. Rev. Astron. Astrophys. 40, 539 (2002)ADSCrossRefGoogle Scholar
  14. Stanford, S.A., Romer, A.K., Sabirli, K., Davidson, M., Hilton, M., Viana, P.T.P., Collins, C.A., Kay, S.T., et al.: The XMM cluster survey: a massive galaxy cluster at z = 1.45. Astrophys. J. Lett. 646, L13 (2006)ADSCrossRefGoogle Scholar
  15. Swinbank, A.M., Edge, A.C., Smail, I., Stott, J.P., Bremer, M., Sato, Y., van Breukelen, C., Jarvis, M., Waddington, I., Clewley, L., Bergeron, J., Cotter, G., Dye, S., Geach, J.E., Gonzalez-Solares, E., Hirst, P., Ivison, R.J., Rawlings, S., Simpson, C., Smith, G.P., Verma, A., Yamada, T.: The discovery of a massive supercluster at z = 0.9 in the UKIDSS Deep eXtragalactic survey. Mon. Not. R. Astron. Soc. 379, 1343 (2007)ADSCrossRefGoogle Scholar
  16. Tully, R.B., et al.: Alignment of clusters and galaxies on scales up to 0.1 C. Astrophys. J. 303, 25 (1986)ADSCrossRefGoogle Scholar
  17. Tully, R.B.: The galaxy luminosity function and environmental dependencies. Astron. J. 96, 73 (1988)ADSCrossRefGoogle Scholar
  18. van Breukelen, C., Clewley, L., Bonfield, D.G., Rawlings, S., Jarvis, M.J., Barr, J.M., Foucaud, S., Almaini, O., et al.: Galaxy clusters at 0.6 < z < 1.4 in the UKIDSS ultra deep survey early data release. Mon. Not. R. Astron. Soc. 373, L26 (2006)ADSCrossRefGoogle Scholar
  19. Viana, P.T.P., Liddle, A.R.: The cluster abundance in flat and open cosmologies. Mon. Not. R. Astron. Soc. 281, 323 (1996)ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 2013

Authors and Affiliations

  1. 1.Department of PhysicsDurham UniversityDurhamUK

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