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The Chandra Deep Field–South: Optical Spectroscopy. I.

  • Authors: G. P. Szokoly, J. Bergeron, G. Hasinger, I. Lehmann, L. Kewley, V. Mainieri, M. Nonino, P. Rosati, R. Giacconi, R. Gilli, R. Gilmozzi, C. Norman, M. Romaniello, E. Schreier, P. Tozzi, J. X. Wang, W. Zheng, and A. Zirm

Szokoly et al. 2004 The Astrophysical Journal Supplement Series 155 271.

  • Provider: AAS Journals

Caption: Fig. 1.

Spatial distribution of the X‐ray sources with and without spectroscopic observations. Object classes are marked as in Fig. 2. The area covered by our spectroscopic masks (solid line), the imaging survey (long‐dashed line), the K20 survey area (short‐dashed line) and an 8﹩\arcmin﹩ radius circle, centered on the nominal CDFS pointing (3h32m28﹩\fs﹩0, −27°48﹩\arcmin﹩30﹩\arcsec﹩ J2000; dotted line) is also shown.

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