430 citations · 4.1k across the 60 of their papers we have counts for
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Isothermal dust models of Herschel-ATLAS galaxies
D. J. B. Smith, M. J. Hardcastle, M. J. Jarvis +18
We use galaxies from the Herschel-ATLAS survey, and a suite of ancillary simulations based on an isothermal dust model, to study our ability to determine the effective dust tempera…
Evolution of faint radio sources in the VIDEO-XMM3 field
K. McAlpine, M. J. Jarvis, D. G. Bonfield
It has been speculated that low luminosity radio-loud AGN have the potential to serve as an important source of AGN feedback, and may be responsible for suppressing star-formation…
H-ATLAS: estimating redshifts of Herschel sources from sub-mm fluxes
E. A. Pearson, S. Eales, L. Dunne +29
Upon its completion the Herschel ATLAS (H-ATLAS) will be the largest submillimetre survey to date, detecting close to half-a-million sources. It will only be possible to measure sp…
Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies
N. Bourne, L. Dunne, G. J. Bendo +21
We present an analysis of CO molecular gas tracers in a sample of 500μm-selected Herschel-ATLAS galaxies at z<0.05 (cz<14990km/s). Using 22-500μm photometry from WISE, IRAS and Her…
GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies
M. W. Grootes, R. J. Tuffs, C. C. Popescu +32
We report the discovery of a well-defined correlation between B-band face-on central optical depth due to dust, τ^f_B, and the stellar mass surface density, μ_{*}, of nearby (z < 0…
H2O emission in high-z ultra-luminous infrared galaxies
A. Omont, Chentao Yang, P. Cox +47
Using IRAM PdBI we report the detection of H2O in six new lensed ultra-luminous starburst galaxies at high redshift, discovered in the Herschel H-ATLAS survey. The sources are dete…
H-ATLAS: The cosmic abundance of dust from the far-infrared background power spectrum
Cameron Thacker, Asantha Cooray, Joseph Smidt +22
We present a measurement of the angular power spectrum of the cosmic far-infrared background (CFIRB) anisotropies in one of the extragalactic fields of the Herschel Astrophysical T…
The Herschel view of the environment of the radio galaxy 4C+41.17 at z = 3.8
D. Wylezalek, J. Vernet, C. De Breuck +16
We present Herschel observations at 70, 160, 250, 350 and 500 micron of the environment of the radio galaxy 4C+41.17 at z = 3.792. About 65% of the extracted sources are securely i…
Herschel-ATLAS/GAMA: spatial clustering of low-redshift sub-mm galaxies
E. van Kampen, D. J. B. Smith, S. Maddox +44
We have measured the clustering properties of low-redshift (z < 0.3) sub-mm galaxies detected at 250 micron in the Herschel-ATLAS Science Demonstration Phase (SDP) field. We select…
Herschel-ATLAS: the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects
J. M. Cao Orjales, J. A. Stevens, M. J. Jarvis +20
We have used data from the Herschel-ATLAS at 250, 350 and 500 μm to determine the far-infrared (FIR) properties of 50 Broad Absorption Line Quasars (BAL QSOs). Our sample contains…
Herschel-ATLAS: Multi-wavelength SEDs and physical properties of 250 micron-selected galaxies at z < 0.5
D. J. B. Smith, L. Dunne, E. da Cunha +38
We present a pan-chromatic analysis of an unprecedented sample of 1402 250 micron-selected galaxies at z < 0.5 (mean z = 0.24) from the Herschel-ATLAS survey. We complement our Her…
A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243
R. S. Bussmann, M. A. Gurwell, Hai Fu +35
We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880um and the Keck Adaptive Optics (AO) system at Ks-band of a gravitationally lensed sub-…
The sizes, masses and specific star-formation rates of massive galaxies at 1.3<z<1.5: strong evidence in favour of evolution via minor mergers
R. J. McLure, H. J. Pearce, J. S. Dunlop +12
We report the results of a comprehensive study of the relationship between galaxy size, stellar mass and specific star-formation rate (sSFR) at redshifts 1.3<z<1.5. Based on a mass…
Blind detections of CO J = 1--0 in 11 H-ATLAS galaxies at z = 2.1--3.5 with the GBT/Zpectrometer
A. I. Harris, A. J. Baker, D. T. Frayer +29
We report measurements of the carbon monoxide ground state rotational transition (12C16O J = 1--0) with the Zpectrometer ultra-wideband spectrometer on the 100-m diameter Green Ban…
Herschel-ATLAS: Planck sources in the Phase 1 fields
D. Herranz, J. González-Nuevo, D. L. Clements +33
We present the results of a cross-correlation of the Planck Early Release Compact Source Catalog (ERCSC) with the catalog of Herschel-ATLAS sources detected in the Phase 1 fields,…
Herschel-ATLAS: towards a sample of ~1000 strongly-lensed galaxies
J. González-Nuevo, A. Lapi, S. Fleuren +39
While the selection of strongly lensed galaxies with 500μm flux density S_500>100 mJy has proven to be rather straightforward (Negrello et al. 2010), for many applications it is im…
Herschel-ATLAS: VISTA VIKING near-IR counterparts in the Phase 1 GAMA 9h data
S. Fleuren, W. Sutherland, L. Dunne +38
We identify near-infrared Ks band counterparts to Herschel-ATLAS sub-mm sources, using a preliminary object catalogue from the VISTA VIKING survey. The sub-mm sources are selected…
A Comprehensive View of a Strongly Lensed Planck-Associated Submillimeter Galaxy
Hai Fu, E. Jullo, A. Cooray +48
We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS12--00 is selected from the Herschel-Astrophys…
Spitzer IRAC identification of Herschel-ATLAS SPIRE sources
Sam Kim, Julie L. Wardlow, Asantha Cooray +28
We use spitzer-IRAC data to identify near-infrared counterparts to submillimeter galaxies detected with Herschel-SPIRE at 250um in the Herschel Astrophysical Terahertz Large Area S…
Selection constraints on high redshift quasar searches in the VISTA kilo-degree infrared galaxy survey
J. R. Findlay, W. J. Sutherland, B. P. Venemans +5
The European Southern Observatory's (ESO) Visible and Infrared Survey Telescope for Astronomy (VISTA) is a 4-m class survey telescope for wide-field near-infrared imaging. VISTA is…
Herschel-ATLAS Galaxy Counts and High Redshift Luminosity Functions: The Formation of Massive Early Type Galaxies
A. Lapi, J. Gonzalez-Nuevo, L. Fan +35
Exploiting the Herschel-ATLAS Science Demonstration Phase (SDP) survey data, we have determined the luminosity functions (LFs) at rest-frame wavelengths of 100 and 250 micron and a…
Gas and dust in a submillimeter galaxy at z = 4.24 from the Herschel ATLAS
Pierre Cox, M. Krips, R. Neri +39
We report ground-based follow-up observations of the exceptional source, ID141, one the brightest sources detected so far in the H-ATLAS cosmological survey. ID141 was observed usi…
The environment and characteristics of low redshift galaxies detected by the Herschel-ATLAS
A. Dariush, L. Cortese, S. Eales +41
We investigate the ultraviolet and optical properties and environment of low redshift galaxies detected in the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) science…
EMU: Evolutionary Map of the Universe
Ray P. Norris, A. M. Hopkins, J. Afonso +54
EMU is a wide-field radio continuum survey planned for the new Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep (rms ~ 10 m…