HerMES: Far infrared properties of known AGN in the HerMES fields
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Author
Hatziminaoglou, E.
Omont, A.
Stevens, Jason
Amblard, A.
Arumugam, V.
Auld, R.
Aussel, H.
Babbedge, T.
Blain, A.
Bock, J.
Boselli, A.
Buat, V.
Burgarella, D.
Castro-Rodríguez, N.
Cava, A.
Chanial, P.
Clements, D. L.
Conley, A.
Conversi, L.
Cooray, A.
Dowell, C.D.
Dwek, E.
Dye, S.
Eales, S.
Elbaz, D.
Farrah, D.
Fox, M.
Franceschini, A.
Gear, W.
Glenn, J.
González Solares, E.A.
Griffin, M.
Halpern, M.
Ibar, E.
Isaak, K.
Ivison, R.J.
Lagache, G.
Levenson, L.
Lu, N.
Madden, S.
Maffei, B.
Mainetti, G.
Marchetti, L.
Mortier, A.M.J.
Nguyen, H.T.
O'Halloran, B.
Oliver, S. J.
Page, M.J.
Panuzzo, P.
Papageorgiou, A.
Pearson, C.P.
Pérez-Fournon, I.
Pohlen, M.
Rawlings, J.I.
Rigopoulou, D.
Rizzo, D.
Roseboom, I.G.
Rowan-Robinson, M.
Sanchez Portal, M.
Schulz, B.
Scott, D.
Seymour, N.
Shupe, D. L.
Symeonidis, M.
Trichas, M.
Tugwell, K.E.
Vaccari, M.
Valtchanov, I.
Vigroux, L.
Wang, L.
Ward, R.
Wright, G.
Xu, C.K.
Zemcov, M.
Attention
2299/7894
Abstract
Nuclear and starburst activity are known to often occur concomitantly. Herschel-SPIRE provides sampling of the far-infrared (FIR) spectral energy distributions (SEDs) of type 1 and type 2 AGN, allowing for the separation between the hot dust (torus) and cold dust (starburst) emission. We study large samples of spectroscopically confirmed type 1 and type 2 AGN lying within the Herschel Multi-tiered Extragalactic Survey (HerMES) fields observed during the science demonstration phase, aiming to understand their FIR colour distributions and constrain their starburst contributions.