186 citations · 964 across the 18 of their papers we have counts for
18 papers
NOEMA confirmation of an optically dark ALMA-AzTEC submillimetre galaxy at . A late-stage starburst prior to quenching
Soh Ikarashi, R. J. Ivison, William I. Cowley +1
We have obtained 1 and 3 mm spectral scans of ASXDF1100.053.1 using NOEMA. ASXDF1100.053.1 is an unlensed optically dark millimetre-bright SMG with (), which…
A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
L. Wang, W. J. Pearson, W. Cowley +5
We aim to study the statistical properties of dusty star-forming galaxies, such as their number counts, luminosity functions (LF) and dust-obscured star-formation rate density (SFR…
The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
William I. Cowley, Karina I. Caputi, Smaran Deshmukh +6
In this work, we use measurements of galaxy stellar mass and two-point angular correlation functions to constrain the stellar-to-halo mass ratios (SHMRs) of passive and \np\ galaxi…
SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) II: Structural Properties and Near-Infrared Morphologies of Faint Submillimeter Galaxies
Yu-Yen Chang, Nicholas Ferraro, Wei-Hao Wang +25
We present structural parameters and morphological properties of faint 450-um selected submillimeter galaxies (SMGs) from the JCMT Large Program, STUDIES, in the COSMOS-CANDELS reg…
The vertical motion history of disk stars throughout the Galaxy
Yuan-Sen Ting, Hans-Walter Rix
It has long been known that the vertical motions of Galactic disk stars increase with stellar age, commonly interpreted as vertical heating through orbit scattering. Here we map th…
The Galaxy-Halo Connection for as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
William Cowley, Karina Caputi, Smaran Deshmukh +8
The \emph{Spitzer} Matching Survey of the UltraVISTA ultra-deep Stripes (SMUVS) provides unparalleled depth at and ~m over ~deg of the COSMOS field, all…
Spitzer Matching survey of the UltraVISTA ultra-deep Stripes (SMUVS): Full-mission IRAC Mosaics and Catalogs
M. L. N. Ashby, Karina I. Caputi, Will Cowley +9
This paper describes new deep 3.6 and 4.5 micron imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer's…
The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): the Evolution of Dusty and Non-Dusty Galaxies with Stellar Mass at z=2-6
S. Deshmukh, K. I. Caputi, M. L. N. Ashby +6
The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS) has obtained the largest ultra-deep Spitzer maps to date in a single field of the sky. We considered the sa…
SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-End Counts at 450 um
Wei-Hao Wang, Wei-Ching Lin, Chen-Fatt Lim +40
The SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES) is a three-year JCMT Large Program aiming at reaching the 450 m confusion limit in the COSMOS-CANDELS region, to study a repr…
Star formation in galaxies at z~4-5 from the SMUVS survey: a clear starburst/main-sequence bimodality for Halpha emitters on the SFR-M* plane
K. I. Caputi, S. Deshmukh, M. L. N. Ashby +7
We study a large galaxy sample from the Spitzer Matching Survey of the UltraVISTA ultra-deep Stripes (SMUVS) to search for sources with enhanced 3.6 micron fluxes indicative of str…
Predictions for deep galaxy surveys with JWST from CDM
William Cowley, Carlton Baugh, Shaun Cole +2
We present predictions for the outcome of deep galaxy surveys with the () obtained from a physical model of galaxy formation in CDM. We…
Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright sub-millimetre galaxies
William I. Cowley, Cedric G. Lacey, Carlton M. Baugh +2
Placing bright sub-millimetre galaxies (SMGs) within the broader context of galaxy formation and evolution requires accurate measurements of their clustering, which can constrain 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…
The far infra-red SEDs of main sequence and starburst galaxies
William I. Cowley, Matthieu Bethermin, Claudia del P. Lagos +3
We compare observed far infra-red/sub-millimetre (FIR/sub-mm) galaxy spectral energy distributions (SEDs) of massive galaxies ( M) derive…
The SCUBA-2 Cosmology Legacy Survey: The clustering of submillimetre galaxies in the UKIDSS UDS field
Aaron Wilkinson, Omar Almaini, Chian-Chou Chen +20
Submillimetre galaxies (SMGs) are among the most luminous dusty galaxies in the Universe, but their true nature remains unclear; are SMGs the progenitors of the massive elliptical…
The SCUBA-2 Cosmology Legacy Survey: ALMA resolves the bright-end of the sub-millimeter number counts
James Simpson, Ian Smail, Mark Swinbank +20
We present high-resolution 870-um ALMA continuum maps of 30 bright sub-millimeter sources in the UKIDSS UDS field. These sources are selected from deep, 1-square degrees 850-um map…
The Clustering Evolution of Dusty Star-Forming Galaxies
William I. Cowley, Cedric G. Lacey, Carlton M. Baugh +1
We present predictions for the clustering of galaxies selected by their emission at far infra-red (FIR) and sub-millimetre wavelengths. This includes the first predictions for the…
Simulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field variance
William I. Cowley, Cedric G. Lacey, Carlton M. Baugh +1
Recent observational evidence suggests that the coarse angular resolution ( FWHM) of single-dish telescopes at sub-mm wavelengths has biased the observed galaxy number cou…