Research Papers and Chandra Data Products

1. - THE CHANDRA DEEP PROTOCLUSTER SURVEY: SOURCE CATALOGS FOR A 400 KS OBSERVATION OF THE z = 3.09 PROTOCLUSTER IN SSA22

  • Table 2 - Main Catalog: ASCII
  • Table A1 - Supplementary Catalog of Additional WAVDETECT Sources: ASCII
  • Figure 8 - K-Band Postage Stamp Images with X-ray Contours for all 297 Sources: PS
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  • SSA22 FITS Images (Figure 3a): 0.5-8 keV 0.5-2 keV 2-8 keV
  • SSA22 FITS Exposure Maps (Figure 3c): 0.5-8 keV 0.5-2 keV 2-8 keV
  • SSA22 FITS Background Maps: 0.5-8 keV 0.5-2 keV 2-8 keV
  • SSA22 FITS Sensitivity Maps (Figure 3d): 0.5-8 keV 0.5-2 keV 2-8 keV

    • B.D. Lehmer, D.M. Alexander, S.C. Chapman, Ian Smail, F.E. Bauer, W.N. Brandt, J.E. Geach, J.R. Mullaney, and A.M. Swinbank 2009, MNRAS, 400, 299.

    2. - THE CHANDRA DEEP PROTOCLUSTER SURVEY: EVIDENCE FOR AN ENHANCEMENT OF AGN ACTIVITY IN THE SSA22 PROTOCLUSTER AT z = 3.09

    B.D. Lehmer, D.M. Alexander, J.E. Geach, Ian Smail, A. Basu-Zych, F.E. Bauer, S.C. Chapman, Y. Matsuda, C. A. Scharf, M. Volonteri, and T. Yamada 2009, ApJ, 691, 687.

    3. - THE CHANDRA DEEP PROTOCLUSTER SURVEY: LYMAN ALPHA BLOBS ARE POWERED BY HEATING, NOT COOLING

    J.E. Geach, D.M. Alexander, B.D. Lehmer, Ian Smail, Y. Matsuda, S.C. Chapman, C.A. Scharf, R.J. Ivison, M. Volonteri, T. Yamada, A.W. Blain, R.G. Bower, F.E. Bauer, A. Basu-Zych 2009, ApJ, 700, 1.

    Chandra press conference on Geach et al. (2009): "Galaxies Coming of Age in Cosmic Blobs"

    Movie (artists impression) of Lyman-Alpha Blobs

    Local press release on Geach et al. (2009): "Cosmic blobs point to key stage in galaxy evolution"

    4. - SUBMILLIMETER ARRAY IDENTIFICATION OF THE MILLIMETER-SELECTED GALAXY SSA22-AZTEC1: A PROTOQUASAR IN A PROTOCLUSTER?

    Y. Tamura, D. Iono, D.J. Wilner, M. Kajisawa, D.M. Alexander, A. Chung, H. Ezawa, B. Hatsukade, T. Hayashino, Hughes, D.H., T. Ichikawa, S. Ikarahi, R. Kawabe, K. Kohno, B.D. Lehmer, Y. Matsuda, K. Nakanishi, T. Takata, Y.K. Uchimoto, G.W. Wilson, T. Yamada, M.S. Yun 2010, ApJ, 724, 1270.