activity
19982025
most citedThe Herschel ATLAS

596 citations · 2k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2025★ 4 cited

The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation

Maarten Baes, Andrea Gebek, Sabelo Kunene +8

The Tully-Fisher relation (TFR) is one of the most important and widely used empirical correlations in extragalactic astronomy. Apart from its importance as a secondary distance in…

astro-ph.GA2024

MeerKAT Observations of Herschel Protocluster Candidates

Y. Ding, D. L. Clements, L. L. Leeuw +9

High-redshift protoclusters consisting of dusty starbursts are thought to play an important role in galaxy evolution. Their dusty nature makes them bright in the FIR/submm but diff…

astro-ph.GA2023★ 24 cited

The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps

Andrea Gebek, Maarten Baes, Benedikt Diemer +6

Cold gas in galaxies provides a crucial test to evaluate the realism of cosmological hydrodynamical simulations. To extract the atomic and molecular hydrogen properties of the simu…

astro-ph.GA2022★ 8 cited

The star-formation rates of QSOs

M. Symeonidis, N. Maddox, M. J. Jarvis +13

We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5<z<2.65 redshift range down to log[nuLnu,2500 (erg/s)]>44.7, using SPIRE data from Herschel-A…

astro-ph.GA2020★ 45 cited

MIGHTEE: Are giant radio galaxies more common than we thought?

J. Delhaize, I. Heywood, M. Prescott +31

We report the discovery of two new giant radio galaxies (GRGs) using the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey. Both GRGs were found within a…

astro-ph.GA2020★ 4 cited

Cosmic evolution of molecular gas mass density from an empirical relation between and

G. Orellana-González, E. Ibar, R. Leiton +8

Historically, GHz radio emission has been used extensively to characterize the star-formation activity in galaxies. In this work, we look for empirical relations amongst the radio…

astro-ph.GA2020★ 6 cited

SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data

T. Cheng, D. L. Clements, J. Greenslade +21

We measure the 850-m source densities of 46 candidate protoclusters selected from the Planck High-z catalogue (PHz) and the Planck Catalogue of Compact Sources (PCCS) that were…

astro-ph.GA2019★ 24 cited

SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE

T. Cheng, D. L. Clements, J. Greenslade +21

We present SCUBA-2 850-m observations of 13 candidate starbursting protoclusters selected using Planck and Herschel data. The cumulative number counts of the 850-m sources in…

astro-ph.CO2017★ 65 cited

MeerKLASS: MeerKAT Large Area Synoptic Survey

Mario G. Santos, Michelle Cluver, Matt Hilton +35

We discuss the ground-breaking science that will be possible with a wide area survey, using the MeerKAT telescope, known as MeerKLASS (MeerKAT Large Area Synoptic Survey). The curr…

astro-ph.GA2014★ 2 cited

Dust in the Radio Galaxy and Merger Remnant NGC 1316 (Fornax A)

Bernard Duah Asabere, Cathy Horellou, Hartmut Winkler +2

We present dust maps of NGC 1316 (Fornax A), a well-studied early-type galaxy located in the outskirts of the Fornax cluster. We used the Large APEX BOlometer CAmera (LABOCA), oper…

astro-ph.CO2013★ 35 cited

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…

astro-ph.CO2012★ 58 cited

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-…

astro-ph.GA2012★ 10 cited

Magnetic Field in The Isolated Massive Dense Clump IRAS 20126+4104

Hiroko Shinnaga, Giles Novak, John E. Vaillancourt +8

We measured polarized dust emission at 350um towards the high-mass star forming massive dense clump IRAS 20126+4104 using the SHARC II Polarimeter, SHARP, at the Caltech Submillime…

astro-ph.CO2012★ 109 cited

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…

astro-ph.CO2011★ 61 cited

Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3

A. Omont, R. Neri, P. Cox +54

The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification mak…

astro-ph.CO2010★ 42 cited

Herschel-ATLAS: Statistical Properties of Galactic Cirrus in the GAMA-9 Hour Science Demonstration Phase Field

Andrea Bracco, Asantha Cooray, M. Veneziani +35

We study the Spectral Energy Distribution (SED) and the power spectrum of Galactic cirrus emission observed in the 14 deg^2 Science Demonstration Phase field of the Herschel-ATLAS…

astro-ph.CO2010★ 21 cited

Spitzer Imaging of Herschel-ATLAS Gravitationally Lensed Submillimeter Sources

R. Hopwood, J. Wardlow, A. Cooray +49

We present physical properties of two submillimeter selected gravitationally lensed sources, identified in the Herschel Astrophysical Terahertz Large Area Survey. These submillimet…

astro-ph.IM2010★ 106 cited

The first release of data from the Herschel ATLAS: the SPIRE images

E. Pascale, R. Auld, A. Dariush +25

We have reduced the data taken with the Spectral and Photometric Imaging Receiver (SPIRE) photometer on board the Herschel Space Observatory in the Science Demonstration Phase (SDP…

astro-ph.CO2010★ 99 cited

Herschel-ATLAS: The far-infrared--radio correlation at z<0.5

Matt J. Jarvis, D. J. B. Smith, D. G. Bonfield +44

We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared--radio correlation over the redshift range 0<z<0.5. Using the total far-infrared luminosity of…

astro-ph.IM2010★ 98 cited

H-ATLAS: PACS imaging for the Science Demonstration Phase

Edo Ibar, R. J. Ivison, A. Cava +26

We describe the reduction of data taken with the PACS instrument on board the Herschel Space Observatory in the Science Demonstration Phase of the Herschel-ATLAS (H-ATLAS) survey,…

astro-ph.CO2010★ 76 cited

Measurements of CO redshifts with Z-Spec for lensed submillimeter galaxies discovered in the H-ATLAS survey

R. E. Lupu, K. S. Scott, J. E. Aguirre +50

We present new observations from Z-Spec, a broadband 185-305 GHz spectrometer, of five sub-millimeter bright lensed sources selected from the Herschel Astrophysical Terahertz Large…

astro-ph.CO2010★ 69 cited

GBT Zpectrometer CO(1-0) Observations of the Strongly-Lensed Submillimeter Galaxies from the Herschel ATLAS

D. T. Frayer, A. I. Harris, A. J. Baker +45

The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) has uncovered a population of strongly-lensed submillimeter galaxies (SMGs). The Zpectrometer instrument on the Gre…

astro-ph.CO2010★ 3 cited

The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE

Asantha Cooray, Steve Eales, Scott Chapman +247

A large sub-mm survey with Herschel will enable many exciting science opportunities, especially in an era of wide-field optical and radio surveys and high resolution cosmic microwa…

astro-ph.CO2010★ 130 cited

Herschel-ATLAS: counterparts from the UV--NIR in the science demonstration phase catalogue

D. J. B. Smith, L. Dunne, S. J. Maddox +45

We present a technique to identify optical counterparts of 250 um-selected sources from the Herschel-ATLAS survey. Of the 6621 250 um > 32 mJy sources in our science demonstration…