Spectroscopic identifications of Spitzer sources in the 
SWIRE/XMM-Newton/ELAIS-S1 field: a large fraction of active galactic nucleus 
with high F(24 μm)/F(R) ratio

Sacchi, N.; La Franca, F.; Feruglio, C.; Fiore, F.; Puccetti, S.; Cocchia, F.; Berta, S.; Brusa, M.; Cimatti, A.; Comastri, A.; Franceschini, A.; Gruppioni, C.; Maiolino, R.; Matute, I.; Polletta, M.; Pozzetti, L.; Pozzi, F.; Vignali, C.; Zamorani, G.; Oliver, S.; Rowan-Robinson, M.; Smith, G.; Lonsdale, C.

doi:10.1088/0004-637X/703/2/1778

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Spectroscopic identifications of Spitzer sources in the SWIRE/XMM-Newton/ELAIS-S1 field: a large fraction of active galactic nucleus with high F(24 μm)/F(R) ratio

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Berta, S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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

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Sacchi, N., La Franca, F., Feruglio, C., Fiore, F., Puccetti, S., Cocchia, F., et al. (2009). Spectroscopic identifications of Spitzer sources in the SWIRE/XMM-Newton/ELAIS-S1 field: a large fraction of active galactic nucleus with high F(24 μm)/F(R) ratio. The Astrophysical Journal, 703(2), 1778-1790. doi:10.1088/0004-637X/703/2/1778.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-BF0E-B

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