activity
20102017
most citedHerschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years

248 citations · 2.3k across the 32 of their papers we have counts for

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Showing astro-ph.COShow all

16 papers · 1 filter

astro-ph.CO2015★ 39 cited

Toward a tomographic analysis of the cross-correlation between Planck CMB lensing and H-ATLAS galaxies

Federico Bianchini, Andrea Lapi, Matteo Calabrese +9

We present an improved and extended analysis of the cross-correlation between the map of the Cosmic Microwave Background (CMB) lensing potential derived from the \emph{Planck} miss…

astro-ph.CO2014★ 89 cited

Cross-correlation between the CMB lensing potential measured by Planck and high-z sub-mm galaxies detected by the Herschel-ATLAS survey

F. Bianchini, P. Bielewicz, A. Lapi +15

We present the first measurement of the correlation between the map of the cosmic microwave background (CMB) lensing potential derived from the \emph{Planck} nominal mission data a…

astro-ph.CO2013★ 58 cited

Herschel-ATLAS: Modelling the first strong gravitational lenses

S. Dye, M. Negrello, R. Hopwood +14

We have determined the mass-density radial profiles of the first five strong gravitational lens systems discovered by the Herschel Astrophysical Terahertz Large Area Survey (H-ATLA…

astro-ph.CO2013★ 216 cited

Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z>1.5

R. S. Bussmann, I. Perez-Fournon, S. Amber +46

Strong gravitational lenses are now being routinely discovered in wide-field surveys at (sub)millimeter wavelengths. We present Submillimeter Array (SMA) high-spatial resolution im…

astro-ph.CO2013★ 51 cited

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…

astro-ph.CO2013★ 59 cited

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…

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.CO2013★ 30 cited

Far-infrared spectroscopy of a lensed starburst: a blind redshift from Herschel

R. D. George, R. J. Ivison, R. Hopwood +20

We report the redshift of HATLAS J132427.0+284452 (hereafter HATLAS J132427), a gravitationally lensed starburst galaxy, the first determined 'blind' by the Herschel Space Observat…

astro-ph.CO2013★ 18 cited

A Herschel-ATLAS study of dusty spheroids: probing the minor-merger process in the local Universe

S. Kaviraj, K. Rowlands, M. Alpaslan +7

We use multi-wavelength (0.12 - 500 micron) photometry from Herschel-ATLAS, WISE, UKIDSS, SDSS and GALEX, to study 23 nearby spheroidal galaxies with prominent dust lanes (DLSGs).…

astro-ph.CO2013★ 34 cited

GAMA/H-ATLAS: Linking the Properties of Sub-mm Detected and Undetected Early-Type Galaxies: I. z0.06 Sample

N. K. Agius, A. E. Sansom, C. C. Popescu +34

We present two large, nearby (0.013z0.06) samples of Early-Type Galaxies (ETGs): a visually classified sample of 220 ETGs, created using source-matched data from the Gala…

astro-ph.CO2013★ 48 cited

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…

astro-ph.CO2012★ 106 cited

Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 micron to 1mm

S. P. Driver, A. S. G. Robotham, L. Kelvin +40

We use the GAMA I dataset combined with GALEX, SDSS and UKIDSS imaging to construct the low-redshift (z<0.1) galaxy luminosity functions in FUV, NUV, ugriz, and YJHK bands from wit…

astro-ph.CO2012★ 157 cited

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…

astro-ph.CO2011★ 119 cited

H-ATLAS/GAMA: Dusty early-type galaxies and passive spirals

K. Rowlands, L. Dunne, S. Maddox +38

We present the dust properties and star-formation histories of local submillimetre-selected galaxies in Herschel-ATLAS, classified by optical morphology. The early-type galaxies (E…

astro-ph.CO2010★ 248 cited

Herschel-ATLAS: Rapid evolution of dust in galaxies in the last 5 billion years

L. Dunne, H. Gomez, E. da Cunha +38

We present the first direct and unbiased measurement of the evolution of the dust mass function of galaxies over the past 5 billion years of cosmic history using data from the Scie…

astro-ph.CO2010★ 13 cited

Which halos host Herschel-ATLAS galaxies in the local Universe?

Qi Guo, Shaun Cole, Cedric G. Lacey +40

We measure the projected cross-correlation between low redshift (z < 0.5) far-IR selected galaxies in the SDP field of the Herschel-ATLAS (H-ATLAS) survey and optically selected ga…