Fig. 4 from The Chandra Deep Field–South: Optical Spectroscopy. I.

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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. 4.

Flux‐calibrated spectra of a spectrophotometric standard star, Feige 110 (Hamuy et al. 1992, 1994; Oke 1990). The dashed line is the measured flux without removing the second‐order contamination, the solid line is the spectra after the correction. Open squares are the real flux values from literature.

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