Fig. 22 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. 22.

X‐ray luminosity in the 2–10 keV band vs. the absolute K magnitude. Symbols are as in Fig. 2. We also convert the relation found between bulge luminosity and black hole mass (Marconi & Hunt 2003), by assuming that around 40% of the K‐band emission is coming from the bulge and an X‐ray luminosity of 0.1% of the Eddington limit (solid line).

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