SINFONI spectra of heavily obscured AGNs in COSMOS: Evidence of outflows in a MIR/O target at z ~ 2.5

Aims. We present new data for four candidate obscured Compton-Thick (CT) quasars at z ~ 1–2.5 observed with the SINFONI VLT spectrograph in adaptive optics (AO) mode. These sources were selected from a 24 μm Spitzer MIPS survey of the COSMOS field, on the basis of red mid-infrared to optical and opt...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2015-11, Vol.583, p.A72
Hauptverfasser:	Perna, M., Brusa, M., Salvato, M., Cresci, G., Lanzuisi, G., Berta, S., Delvecchio, I., Fiore, F., Lutz, D., Le Floc’h, E., Mainieri, V., Riguccini, L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Adaptive optics Astrophysics Cosmos Diagnostic systems Emission Galaxy: evolution ISM: jets and outflows Outflow Physics Quasars quasars: emission lines Spectra
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