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What produces the far-infrared/submm emission in the most luminous QSOs?
Myrto Symeonidis
The AGN. I examine the average spectral energy distributions (SEDs) of two samples of the most powerful, unobscured QSOs at 2<z<3.5, with rest frame optical luminosities in the 46.…
X-ray selected BALQSOs
M. J. Page, F. J. Carrera, M. Ceballos +11
We study a sample of six X-ray selected broad absorption line (BAL) quasi-stellar objects (QSOs) from the XMM-Newton Wide Angle Survey. All six objects are classified as BALQSOs us…
HELP: star formation as function of galaxy environmentwith Herschel
S. Duivenvoorden, S. Oliver, V. Buat +15
The Herschel Extragalactic Legacy Project (HELP) brings together a vast range of data from many astronomical observatories. Its main focus is on the Herschel data, which maps dust…
AGN are cooler than you think: the intrinsic far-IR emission from QSOs
M. Symeonidis, B. Giblin, M. J. Page +4
We present an intrinsic AGN SED extending from the optical to the submm, derived with a sample of unobscured, optically luminous (vLv(5100)>10^43.5 erg/s) QSOs at z<0.18 from the P…
Star Formation in Luminous Quasars at 2<z<3
Kathryn Harris, Duncan Farrah, Bernhard Schulz +22
We investigate the relation between star formation rates () and AGN properties in optically selected type 1 quasars at using data from Herschel and the SDSS. W…