papers

Publications (16)

astro-ph.GA2014

Detailed modelling of a large sample of Herschel sources in the Lockman Hole: identification of cold dust and of lensing candidates through their anomalous SEDs

Michael Rowan-Robinson, Lingyu Wang, Julie Wardlow +12

We have studied in detail a sample of 967 SPIRE sources with 5-sigma detections at 350 and 500 micron and associations with Spitzer-SWIRE 24 micron galaxies in the HerMES-Lockman s…

astro-ph2000

The Canada-UK Deep Submillimetre Survey: The Survey of the 14-hour field

Stephen Eales, Simon Lilly, Tracy Webb +4

We have used SCUBA to survey an area of 50 square arcmin, detecting 19 sources down to a 3sigma sensitivity limit of 3.5 mJy at 850 microns. We have used Monte-Carlo simulations to…

astro-ph.GA2018

The Causes of the Red Sequence, the Blue Cloud, the Green Valley and the Green Mountain

Stephen Eales, Maarten Baes, Nathan Bourne +23

The galaxies found in optical surveys fall in two distinct regions of a diagram of optical colour versus absolute magnitude: the red sequence and the blue cloud with the green vall…

astro-ph.GA2016

The star-formation rate density from z = 0-6

Michael Rowan-Robinson, Seb Oliver, Lingyu Wang +6

We use 3035 Herschel-SPIRE 500m sources from 20.3 sq deg of sky in the HerMES Lockman, ES1 and XMM-LSS areas to estimate the star-formation rate density at z = 1-6. 500 mu sour…

astro-ph.GA2019

Spitzer catalog of Herschel-selected ultrared dusty, star-forming galaxies

Jingzhe Ma, Asantha Cooray, Hooshang Nayyeri +24

The largest Herschel extragalactic surveys, H-ATLAS and HerMES, have selected a sample of "ultrared" dusty, star-forming galaxies (DSFGs) with rising SPIRE flux densities ($S_{500}…

astro-ph.GA2017

The interstellar medium in high-redshift submillimeter galaxies as probed by infrared spectroscopy

Julie L. Wardlow, Asantha Cooray, Willow Osage +21

Submillimeter galaxies (SMGs) at are luminous in the far-infrared and have star-formation rates, SFR, of hundreds to thousands of solar masses per year. However, it is…

astro-ph.CO2012

Can dust emission be used to map the interstellar medium in high-redshift galaxies? Results from the Herschel Reference Survey

Stephen Eales, Matthew W. L. Smith, Robbie Auld +23

It has often been suggested that an alternative to the standard CO/21-cm method for estimating the mass of the interstellar medium (ISM) in a galaxy might be to estimate the mass o…

astro-ph.GA2015

H-ATLAS/GAMA: Quantifying the Morphological Evolution of the Galaxy Population Using Cosmic Calorimetry

Stephen Eales, Andrew Fullard, Matthew Allen +28

Using results from the Herschel Astrophysical Terrahertz Large-Area Survey and the Galaxy and Mass Assembly project, we show that, for galaxy masses above approximately 1.0e8 solar…

astro-ph.CO2012

The Infrared Properties of Sources Matched in the WISE all-sky and Herschel-ATLAS Surveys

Nicholas A. Bond, Dominic J. Benford, Jonathan P. Gardner +34

We describe the infrared properties of sources detected over ~36 deg^2 of sky in the GAMA 15-hr equatorial field, using data from both the Herschel Astrophysical Terahertz Large-Ar…

astro-ph.GA2025

Witnessing the violent, merger-driven formation of an extremely massive galaxy 1.7 Gyr after the Big Bang

Lura K. Pitchford, Joseph Cairns, Duncan Farrah +4

We combine near-infrared imaging in two bands from the Hubble Space Telescope (HST) with archival observations of molecular gas to study SDSS J160705.16+533558.6 (J1607), an extrem…

astro-ph2003

The Canada-UK Deep Submillimeter Survey VII: Optical and near-infrared identifications for the 14h field

Tracy Webb, Simon Lilly, David Clements +5

We present the multi-wavelength identifications for 23 sources in the Canada-UK Deep Submillimeter Survey (CUDSS) 14h field. The identifications have been selected on the basis of…

astro-ph2003

XMM-Newton Surveys of the CFRS Fields - I: The Sub-mm/X-ray relation

Timothy J. Waskett, Stephen A. Eales, Walter K. Gear +7

First results from XMM-Newton observations of the Canada France Redshift Survey (CFRS) 3hr, 10hr and 14hr fields are presented. Limited regions of two of the XMM surveys (3 and 14h…

astro-ph.GA2023

Characterisation of Herschel-selected strong lens candidates through HST and sub-mm/mm observations

Edoardo Borsato, Lucia Marchetti, Mattia Negrello +34

We have carried out HST snapshot observations at 1.1 m of 281 candidate strongly lensed galaxies identified in the wide-area extragalactic surveys conducted with the Herschel s…

astro-ph2006

Understanding Infrared Galaxy Populations: the SWIRE Legacy Survey

Michael Rowan-Robinson, Carol Lonsdale, Gene Smith +21

We discuss spectral energy distributions, photometric redshifts, redshift distributions, luminosity functions, source-counts and the far infrared to optical luminosity ratio for so…

astro-ph.CO2013

Far-infrared Fine-Structure Line Diagnostics of Ultraluminous Infrared Galaxies

Duncan Farrah, Vianney Lebouteiller, Henrik Spoon +16

We present Herschel observations of six fine-structure lines in 25 Ultraluminous Infrared Galaxies at z<0.27. The lines, [O III]52, [N III]57, [O I]63, [N II]122, [O I]145, and [C…

astro-ph2007

The Far-Infrared Surveyor (FIS) for AKARI

Mitsunobu Kawada, Hajime Baba, Peter D. Barthel +57

The Far-Infrared Surveyor (FIS) is one of two focal plane instruments on the AKARI satellite. FIS has four photometric bands at 65, 90, 140, and 160 um, and uses two kinds of array…