1.1k citations · 2.2k across the 19 of their papers we have counts for
18 papers
Confirming the Evolution of the Dust Mass Function in Galaxies over the past 5 Billion Years
R A Beeston, H L Gomez, L Dunne +3
The amount of evolution in the dust content of galaxies over the past five billion years of cosmic history is contested in the literature. Here we present a far-infrared census of…
BEDE: Bayesian Estimates of Dust Evolution For Nearby Galaxies
P. De Vis, S. J. Maddox, H. L. Gomez +2
We build a rigorous statistical framework to provide constraints on the chemical and dust evolution parameters for nearby late-type galaxies with a wide range of gas fractions ($3\…
A Galactic Dust Devil: far-infrared observations of the Tornado Supernova Remnant candidate
Hannah Chawner, Alex D. P. Howard, Haley L. Gomez +10
We present complicated dust structures within multiple regions of the candidate supernova remnant (SNR) the `Tornado' (G357.7-0.1) using observations with Spitzer and Herschel. We…
MADX -- A simple technique for source detection and measurement using multi-band imaging from the Herschel-ATLAS survey
S. J. Maddox, L. Dunne
We describe the method used to detect sources for the Herschel-ATLAS survey. The method is to filter the individual bands using a matched filter, based on the point-spread function…
ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies
A. E. Sansom, D. H. W. Glass, G. J. Bendo +9
Unresolved gas and dust observations show a surprising diversity in the amount of interstellar matter in early-type galaxies. Using ALMA observations we resolve the ISM in z0…
GAMA/H-ATLAS: The Local Dust Mass Function and Cosmic Density as a Function of Galaxy Type - A Benchmark for Models of Galaxy Evolution
R. A. Beeston, A. H. Wright, S. Maddox +22
We present the dust mass function (DMF) of 15,750 galaxies with redshift , drawn from the overlapping area of the GAMA and {\it H-}ATLAS surveys. The DMF is derived using t…
The faint end of the 250 micron luminosity function at z < 0.5
L. Wang, P. Norberg, M. Bethermin +12
Aims. We aim to study the 250 micron luminosity function (LF) down to much fainter luminosities than achieved by previous efforts. Methods. We developed a modified stacking method…
H-ATLAS: The Far-Infrared properties of galaxies in and around the Coma Cluster
C. Fuller, J. I. Davies, M. W. L. Smith +12
We describe a far infrared survey of the Coma cluster and the galaxy filament it resides within. Our survey covers an area of 150 deg observed by H-ATLAS in fi…
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
J. Liske, I. K. Baldry, S. P. Driver +67
The Galaxy And Mass Assembly (GAMA) survey is one of the largest contemporary spectroscopic surveys of low-redshift galaxies. Covering an area of ~286 deg^2 (split among five surve…
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…
Mining the Herschel-ATLAS: submillimeter-selected blazars in equatorial fields
M. López-Caniego, J. González-Nuevo, M. Massardi +29
The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) provides an unprecedented opportunity to search for blazars at sub-mm wavelengths. We cross-matched the FIRST radio…
Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
S. P. Driver, D. T. Hill, L. S. Kelvin +52
The Galaxy And Mass Assembly (GAMA) survey has been operating since February 2008 on the 3.9-m Anglo-Australian Telescope using the AAOmega fibre-fed spectrograph facility to acqui…
Galaxy And Mass Assembly (GAMA)
Simon P. Driver, the GAMA team
The GAMA survey aims to deliver 250,000 optical spectra (3--7Ang resolution) over 250 sq. degrees to spectroscopic limits of r_{AB} <19.8 and K_{AB}<17.0 mag. Complementary imaging…
Revised masses of dust and gas of SLUGS FIR bright galaxies based on a recent CO survey
E. R. Seaquist, Lihong Yao, L. Dunne +1
Recent CO measurements of an essentially complete sub-sample of galaxies from the SCUBA Local Universe Survey (SLUGS) are used to examine their implications for dust and gas masses…
A census of metals at high and low redshifts and the connection between submillimetre sources and spheroid formation
L. Dunne, S. A. Eales, M. G. Edmunds
Deep surveys in many wavebands have shown that the rate at which stars were forming was at least a factor of 10 higher at z > 1 than today. Heavy elements (metals) are produced by…
The Canada-UK Deep Submillimeter Survey V: The Submillimeter Properties of Lyman-Break Galaxies
T. M. A. Webb, S. Eales, S. Foucaud +9
We have used 850m maps obtained as part of the Canada-UK Deep Submillimeter Survey (CUDSS) to investigate the sub-mm properties of Lyman-break galaxies (LBGs). We used three sam…
High spatial resolution observations of CUDSS14A: a SCUBA-selected Ultraluminous galaxy at high redshift
W. K. Gear, S. J. Lilly, J. A. Stevens +4
We present a high-resolution millimetre interferometric image of the brightest SCUBA-selected galaxy from the Canada-UK deep SCUBA survey (CUDSS). We make a very clear detection at…
Constraining the Radio-Submm Redshift Indicator using data from the SCUBA Local Universe Galaxy Survey
L. Dunne, D. L. Clements, S. A. Eales
Many of the faint submm sources uncovered by deep SCUBA surveys still remain unidentified at most, if not all other wavelengths. The most successful method so far of obtaining accu…