Figure 4 from MERGER-DRIVEN FUELING OF ACTIVE GALACTIC NUCLEI: SIX DUAL AND OF AGNs DISCOVERED WITH CHANDRA AND HUBBLE SPACE TELESCOPE OBSERVATIONS

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MERGER-DRIVEN FUELING OF ACTIVE GALACTIC NUCLEI: SIX DUAL AND OF AGNs DISCOVERED WITH CHANDRA AND HUBBLE SPACE TELESCOPE OBSERVATIONS

Authors: Julia M. Comerford, David Pooley, R. Scott Barrows, Jenny E. Greene, Nadia L. Zakamska, Greg M. Madejski, and Michael C. Cooper

2015 The Astrophysical Journal 806 219.

Provider: AAS Journals

Caption: Figure 4.

Mid-infrared WISE color–color plot of ﹩W1-W2﹩ ([3.4]–[4.6]) against ﹩W1-W4﹩ ([3.4]–[22]) for our 12 targets. The dashed horizontal line indicates the AGN criterion of Stern et al. (2012). The four targets above the dashed line have mid-infrared fluxes dominated by AGN emission, while the eight targets below the dashed line have mid-infrared fluxes dominated by star formation.

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