The Square Kilometre Array (SKA): publications

Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths

\mnras 421 (2012) 3027-3059-3027-3059

Authors:

N Bourne, SJ Maddox, L Dunne, R Auld, M Baes, IK Baldry, DG Bonfield, A Cooray, SM Croom, A Dariush, G de Zotti, SP Driver, S Dye, S Eales, HL Gomez, J González-Nuevo, AM Hopkins, E Ibar, MJ Jarvis, A Lapi, B Madore, MJ Micha lowski, M Pohlen, CC Popescu, EE Rigby, M Seibert, DJB Smith, RJ Tuffs, PVD Werf, S Brough, S Buttiglione, A Cava, DL Clements, CJ Conselice, J Fritz, R Hopwood, RJ Ivison, DH Jones, LS Kelvin, J Liske, J Loveday, P Norberg, ASG Robotham, G Rodighiero, P Temi

Herschel-ATLAS: Planck sources in the Phase 1 fields

ArXiv e-prints (2012)

Authors:

D Herranz, J González-Nuevo, DL Clements, M Clemens, G De Zotti, M López-Caniego, A Lapi, G Rodighiero, L Danese, H Fu, A Cooray, M Baes, GJ Bendo, L Bonavera, FJ Carrera, H Dole, S Eales, RJ Ivison, M Jarvis, G Lagache, M Massardi, MJ Michalowski, M Negrello, E Rigby, D Scott, E Valiante, I Valtchanov, P Van der Werf, R Auld, S Buttiglione, A Dariush, L Dunne, R Hopwood, C Hoyos, E Ibar, S Maddox

Herschel-ATLAS: Toward a Sample of 1000 Strongly Lensed Galaxies

\apj 749 (2012) 65-65

Authors:

J González-Nuevo, A Lapi, S Fleuren, S Bressan, L Danese, G De Zotti, M Negrello, Z-Y Cai, L Fan, W Sutherland, M Baes, AJ Baker, DL Clements, A Cooray, H Dannerbauer, L Dunne, S Dye, S Eales, DT Frayer, AI Harris, R Ivison, MJ Jarvis, MJ Micha lowski, M López-Caniego, G Rodighiero, K Rowlands, S Serjeant, D Scott, P van der Werf, R Auld, S Buttiglione, A Cava, A Dariush, J Fritz, R Hopwood, E Ibar, S Maddox, E Pascale, M Pohlen, E Rigby, D Smith, P Temi

Spectroscopy of broad-line blazars from 1LAC

Astrophysical Journal 748:1 (2012)

Authors:

MS Shaw, RW Romani, G Cotter, SE Healey, PF Michelson, ACS Readhead, JL Richards, W Max-Moerbeck, OG King, WJ Potter

Abstract:

We report on optical spectroscopy of 165 flat spectrum radio quasars (FSRQs) in the Fermi 1LAC sample, which have helped allow a nearly complete study of this population. Fermi FSRQs show significant evidence for non-thermal emission even in the optical; the degree depends on the γ-ray hardness. They also have smaller virial estimates of hole mass than the optical quasar sample. This appears to be largely due to a preferred (axial) view of the γ-ray FSRQ and non-isotropic (H/R ∼ 0.4) distribution of broad-line velocities. Even after correction for this bias, the Fermi FSRQs show higher mean Eddington ratios than the optical population. A comparison of optical spectral properties with Owens Valley Radio Observatory radio flare activity shows no strong correlation. © 2012 The American Astronomical Society. All rights reserved.

Assessing luminosity correlations via cluster analysis: Evidence for dual tracks in the radio/X-ray domain of black hole X-ray binaries

(2012)

Authors:

Elena Gallo, Brendan Miller, Rob Fender

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