Revealing a population of heavily obscured active galactic nuclei at z 0.5-1 in 
the Chandra deep field-south

Luo, B.; Brandt, W. N.; Xue, Y. Q.; Alexander, D. M.; Brusa, M.; Bauer, F. E.; Comastri, A.; Fabian, A. C.; Gilli, R.; Lehmer, B. D.; Rafferty, D. A.; Schneider, D. P.; Vignali, C.

doi:10.1088/0004-637X/740/1/37

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Revealing a population of heavily obscured active galactic nuclei at z 0.5-1 in the Chandra deep field-south

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Brusa, M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Luo, B., Brandt, W. N., Xue, Y. Q., Alexander, D. M., Brusa, M., Bauer, F. E., Comastri, A., Fabian, A. C., Gilli, R., Lehmer, B. D., Rafferty, D. A., Schneider, D. P., & Vignali, C. (2011). Revealing a population of heavily obscured active galactic nuclei at z 0.5-1 in the Chandra deep field-south. The Astrophysical Journal, 740(1):, pp. 1-15. doi:10.1088/0004-637X/740/1/37.

引用: https://hdl.handle.net/11858/00-001M-0000-0012-3326-F

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