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  • The host galaxies of X-ray selected active galactic nuclei to z = 2.5 : structure, star formation, and their relationships from CANDELS and Herschel/PACS 

    Rosario, D.J.; McIntosh, D.H.; Van Der Wel, A.; Kartaltepe, J.; Lang, P.; Santini, P.; Wuyts, S.; Lutz, D.; Rafelski, M.; Villforth, C.; Alexander, D.M.; Bauer, F.E.; Bell, E.F.; Berta, S.; Brandt, W.N.; Conselice, C.J.; Dekel, A.; Faber, S.M.; Ferguson, H.C.; Genzel, R.; Grogin, N.A.; Kocevski, D.D.; Koekemoer, A.M.; Koo, D.C.; Lotz, J.M.; Magnelli, B.; Maiolino, R.; Mozena, M.; Mullaney, J.R.; Papovich, C.J.; Popesso, P.; Tacconi, L.J.; Trump, J.R.; Avadhuta, S.; Bassett, R.; Bell, A.; Bernyk, M.; Bournaud, F.; Cassata, P.; Cheung, E.; Croton, D.; Donley, J.; Degroot, L.; Guedes, J.; Hathi, N.; Herrington, J.; Hilton, M.; Lai, K.; Lani, C.; Martig, M.; McGrath, E.; Mutch, S.; Mortlock, A.; McPartland, C.; O'Leary, E.; Peth, M.; Pillepich, A.; Poole, G.; Snyder, D.; Straughn, A.; Telford, O.; Tonini, C.; Wandro, P. (2015-01) - Journal article
    We study the relationship between the structure and star formation rate (SFR) of X-ray selected low and moderate luminosity active galactic nuclei (AGNs) in the two Chandra Deep Fields, using Hubble Space Telescope imaging ...