| Authors | 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. |
| Abstract | We present a catalog of optical spectroscopic identifications of sources detected by Spitzer at 3.6 or 24 μm down to ~10 and ~280 μJy, respectively, in the SWIRE/XMM-Newton/ELAIS-S1 field and classified via line width analysis and diagnostic diagrams. A total of 1376 sources down to R ~ 24.2 mag have been identified (1362 detected at 3.6 μm, 419 at 24 μm, and 405 at both) by low-resolution optical spectroscopy carried out with FORS2, VIMOS, and EFOSC2 at the Very Large Telescope and 3.6 m ESO telescope. The spectroscopic campaigns have been carried out over the central 0.6 deg2 area of ELAIS-S1 which, in particular, has also been observed by XMM-Newton and Chandra. We find the first direct optical spectroscopic evidence that the fraction of active galactic nuclei (AGNs; mostly AGN2) increases with increasing F(24 μm)/F(R) ratio, reaching values of 70(±20)% in the range 316 < F(24 μm)/F(R) < 1000. We present an Infrared Array Camera-Multiband Imaging Photometer color-color diagram able to separate AGN1 from obscured AGN2 candidates. After having corrected for the spectroscopic incompleteness of our sample, the result is that the AGN fraction at F(24 μm) ~0.8 mJy is ~22(±7)% and decreases slowly to ~19(±5)% down to F(24 μm) ~ 0.3 mJy. |
