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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. 7.

Finding charts and VLT spectra of the field sources. Images are based on our FORS R‐band imaging. The images are ﹩20^{\prime \prime }\times 20^{\prime \prime }﹩ in size. Next to the finding charts we show all spectroscopic observations available for the object. On the horizontal axis both the observed (bottom) and rest frame (top, if available) wavelength is shown in Å units. The vertical axis is the measured flux, ﹩f_{\lambda }﹩ in 10−18 ergs cm−2 s−1 Å−1 units. Important emission (above the spectra) and absorption (below the spectra) features used for identification are also marked.

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