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X RAY CONSTRAINTS ON THE ACTIVE GALACTIC NUCLEI PROPERTIES IN SPITZER INFRARED SPECTROGRAPH IDENTIFIED z similar to 2 ULTRALUMINOUS INFRARED GALAXIES

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Figure 1. Rest-frame Spitzer IRS spectra (solid black curves) and ±1σ errors (gray regions) in units of 10 −15 W m −2 , adapted from Figure 3 of Sajina et al
Table 2 xFLS ULIRGs
Figure 2. Rest-frame 2–10 keV luminosity vs. 5.8 μm AGN continuum luminosity for several bright ULIRGs from published literature thought to host Compton-thick or nearly Compton-thick AGNs (left) and the Chandra-observed xFLS ULIRGs (right)
Figure 3. Rest-frame L 5.8 μm vs. redshift for a select few samples of candidate Compton-thick AGNs including: mid-IR excess objects studied here (red triangles); X-ray (open green squares) and IR-selected (green circles) objects from P06; radio-excess obj
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