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The Chandra Deep Protocluster Survey: point source catalogues for a 400 ks observation of the z = 3 09 protocluster in SSA22

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Figure 1. Locations of some well-known extragalactic X-ray surveys con- con-ducted with Chandra (circles), XMM–Newton (squares) and ROSAT  (trian-gles) in the 0.5–2 keV flux limit versus solid angle  plane
Table 1. Journal of SSA22 Chandra observations.
Figure 4. (a) Total solid angle with at least the vignetting-corrected effective exposure indicated on the abscissa for each of the three standard bands
Table 2. Main Chandra catalogue.
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