On the Lx-L6μm ratio as a diagnostic for Compton-thick AGN

Astronomy and Astrophysics

Volumn 534, Issue , 2011, Pages

  Georgantopoulos, I ^a,b   Rovilos, E ^a   Akylas, A ^b   Comastri, A ^a   Ranalli, P ^a   Vignali, C ^a   Balestra, I ^c   Gilli, R ^a   Cappelluti, N ^a  

^a INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^b NATIONAL OBSERVATORY OF ATHENS   (Greece)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

infrared: galaxies; X rays: diffuse background; X rays: galaxies; X rays: general

Indexed keywords

CHANDRA; CHANDRA DEEP FIELD SOUTHS; HIGH REDSHIFT UNIVERSE; HIGH SIGNAL-TO-NOISE RATIO; INFRARED: GALAXIES; RED SHIFT; SPECTRAL ENERGY DISTRIBUTION; X-RAY LUMINOSITY; X-RAY SPECTRA; X-RAYS: DIFFUSE BACKGROUND; X-RAYS: GALAXIES; X-RAYS: GENERAL; XMM-NEWTON; XMM-NEWTON OBSERVATIONS;

FADING (RADIO); GALAXIES; SIGNAL TO NOISE RATIO; SPECTROSCOPY; X RAY SPECTROSCOPY;

LUMINANCE;

EID: 80053136016     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117400     Document Type: Article

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