Fig. 3 from The Chandra Deep Survey of the Hubble Deep Field–North Area. II. Results from the Caltech Faint Field Galaxy Redshift Survey Area

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The Chandra Deep Survey of the Hubble Deep Field–North Area. II. Results from the Caltech Faint Field Galaxy Redshift Survey Area

Authors: A. E. Hornschemeier, W. N. Brandt, G. P. Garmire, D. P. Schneider, A. J. Barger, P. S. Broos, L. L. Cowie, L. K. Townsley, M. W. Bautz, D. N. Burrows, G. Chartas, E. D. Feigelson, R. E. Griffiths, D. Lumb, J. A. Nousek, L. W. Ramsey, and W. L. W. Sargent

Hornschemeier et al. 2001 The Astrophysical Journal 554 742.

Provider: AAS Journals

Caption: Fig. 3.

Raw X‐ray images in the (a) 0.5–2 keV (soft) band and (b) 2–8 keV (hard) band. The area shown matches the Caltech area indicated on the exposure map in Fig. 1. The outlined region is the HDF‐N, and the crosses mark the centers of each of the Hubble Flanking Fields (see Table 2 of W96).

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