activity
20102026
most citedHerMES: SPIRE galaxy number counts at 250, 350 and 500 microns

234 citations · 1.9k across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2026

Euclid preparation. Far-infrared predictions for Euclid galaxy catalogues: cluster, protocluster, and field

Euclid Collaboration, A. Parmar, D. L. Clements +297

The MAMBO mock galaxy catalogue, based on the Millennium Simulation with empirically assigned galaxy properties, provides predictions of FIR fluxes and physical parameters of Eucli…

astro-ph.GA2026

Calibrating Mid-Infrared Emission Features As Diagnostics of Star Formation in Infrared-Luminous Galaxies via Radiative Transfer Modeling

L. Robinson, D. Farrah, A. Efstathiou +13

Luminous infrared galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.2 micro…

astro-ph.IM2025

Probing the Transient Far-IR Sky with PRIMA

David L Clements, Michael Peel

The time variable far-IR/mm sky is largely unexplored. However, when PRIMA launches, next generation ground-based CMB experiments, including Simons Observatory and CMB-S4, will be…

astro-ph.CO2025★ 1 cited

The Herschel-SPIRE Dark Field I: The deepest Herschel image of the submillimetre Universe

Chris Pearson, Thomas W. O. Varnish, Xinni Wu +4

We present the image maps, data reduction, analysis and the first source counts from the Herschel SPIRE Dark Field. The SPIRE Dark Field is an area of sky near the North Ecliptic P…

astro-ph.CO2025★ 1 cited

The Herschel-SPIRE Dark Field -- II. A P(D) fluctuation analysis of the deepest Herschel image of the submillimetre universe

Thomas W O Varnish, Xinni Wu, Chris Pearson +2

The Herschel-SPIRE Dark Field is the deepest field produced by the SPIRE instrument pushing down below the galaxy confusion limit in each of the 250, 350, 500 m bands. Standard…

astro-ph.GA2025

The assembly of supermassive black holes at in early-type galaxies from scaling relations

Duncan Farrah, Athena Engholm, Evanthia Hatziminaoglou +14

The assembly of supermassive black hole (SMBH) mass () and stellar mass () in galaxies can be studied via the redshift evolution of the rela…

astro-ph.GA2024★ 7 cited

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 m and Data Release for the COSMOS Field

Zhen-Kai Gao, Chen-Fatt Lim, Wei-Hao Wang +19

We present confusion-limited SCUBA-2 450-m observations in the COSMOS-CANDELS region as part of the JCMT Large Program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps…

astro-ph.GA2022★ 14 cited

Multi-wavelength properties of 850-m selected sources from the North Ecliptic Pole SCUBA-2 survey

H. Shim, D. Lee, Y. Kim +25

We present the multi-wavelength counterparts of 850-m selected submillimetre sources over a 2-deg field centred on the North Ecliptic Pole. In order to overcome the large be…

astro-ph.GA2018★ 173 cited

A dust-enshrouded tidal disruption event with a resolved radio jet in a galaxy merger

S. Mattila, M. Pérez-Torres, A. Efstathiou +33

Tidal disruption events (TDEs) are transient flares produced when a star is ripped apart by the gravitational field of a supermassive black hole (SMBH). We have observed a transien…

astro-ph.GA2017★ 46 cited

HERUS: The Far-IR/Submm Spectral Energy Distributions of Local ULIRGs & Photometric Atlas

D. L. Clements, C. Pearson, D. Farrah +9

We present the Herschel-SPIRE photometric atlas for a complete flux limited sample of 43 local Ultraluminous Infrared Galaxies (ULIRGs), selected at 60m by IRAS, as part of the…

astro-ph.GA2016★ 122 cited

The space density of luminous dusty star-forming galaxies at : SCUBA-2 and LABOCA imaging of ultrared galaxies from -ATLAS

R. J. Ivison, A. J. R. Lewis, A. Weiss +28

Until recently, only a handful of dusty, star-forming galaxies (DSFGs) were known at , most of them significantly amplified by gravitational lensing. Here, we have increased t…

astro-ph.GA2016★ 15 cited

The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample

Hai Fu, J. F. Hennawi, J. X. Prochaska +14

We present the first results from an on-going survey to characterize the circumgalactic medium (CGM) of the massive high-redshift galaxies detected as submillimeter galaxies (SMGs)…

astro-ph.GA2016★ 26 cited

Planck intermediate results. XLV. Radio spectra of northern extragalactic radio sources

Planck Collaboration, P. A. R. Ade, N. Aghanim +202

Continuum spectra covering centimetre to submillimetre wavelengths are presented for a northern sample of 104 extragalactic radio sources, mainly active galactic nuclei, based on f…

astro-ph.GA2015★ 23 cited

HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4

M. P. Viero, L. Moncelsi, R. F. Quadri +28

We report contributions to cosmic infrared background (CIB) intensities originating from known galaxies and their faint companions at submillimeter wavelengths. Using the publicly-…

astro-ph.GA2015★ 66 cited

Star formation in z>1 3CR host galaxies as seen by Herschel

P. Podigachoski, P. D. Barthel, M. Haas +15

We present Herschel (PACS and SPIRE) far-infrared (FIR) photometry of a complete sample of z>1 3CR sources, from the Herschel GT project The Herschel Legacy of distant radio-loud A…

astro-ph.GA2014★ 81 cited

A Far-Infrared Spectroscopic Survey of Intermediate Redshift (Ultra) Luminous Infrared Galaxies

Georgios E. Magdis, D. Rigopoulou, R. Hopwood +16

We present Herschel far-IR photometry and spectroscopy as well as ground based CO observations of an intermediate redshift (0.21 < z < 0.88) sample of Herschel-selected (ultra)-lum…

astro-ph.GA2014★ 76 cited

HerMES: The Rest-Frame UV Emission and A Lensing Model for the z=6.34 Luminous Dusty Starburst Galaxy HFLS3

Asantha Cooray, Jae Calanog, Julie L. Wardlow +23

We discuss the restframe UV emission from the starbursting galaxy HFLS3 at z=6.34, discovered in Herschel/SPIRE data due to its red color in the submm wavelengths from 250-500 um.…

astro-ph.GA2014★ 42 cited

Herschel Observations of Far-Infrared Cooling Lines in intermediate Redshift (Ultra)-luminous Infrared Galaxies

D. Rigopoulou, R. Hopwood, G. E. Magdis +17

We report the first results from a spectroscopic survey of the [CII] 158um line from a sample of intermediate redshift (0.2<z<0.8) (ultra)-luminous infrared galaxies, (U)LIRGs (LIR…

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★ 12 cited

Cold dust but warm gas in the unusual elliptical galaxy NGC 4125

C. D. Wilson, A. Cridland, K. Foyle +19

Data from the Herschel Space Observatory have revealed an unusual elliptical galaxy, NGC 4125, which has strong and extended submillimeter emission from cold dust but only very str…

astro-ph.CO2013★ 159 cited

Planck 2013 results. XIX. The integrated Sachs-Wolfe effect

Planck Collaboration, P. A. R. Ade, N. Aghanim +245

Based on CMB maps from the 2013 Planck Mission data release, this paper presents the detection of the ISW effect, i.e., the correlation between the CMB and large-scale evolving gra…

astro-ph.CO2012★ 46 cited

The local luminosity function of star-forming galaxies derived from the Planck Early Release Compact Source Catalogue

Mattia Negrello, Marcel Clemens, Joaquin Gonzalez-Nuevo +18

The Planck Early Release Compact Source Catalog (ERCSC) has offered the first opportunity to accurately determine the luminosity function of dusty galaxies in the very local Univer…

astro-ph.CO2012★ 101 cited

Spatially resolved observations of warm ionized gas and feedback in local ULIRGs

Mark Westmoquette, Dave Clements, George Bendo +1

We present VLT/VIMOS-IFU emission-line spectroscopy of a volume limited sample of 18 southern ULIRGs selected with z<0.09 and dec<10. By covering a wide range of ULIRG types, this…

astro-ph.CO2012★ 127 cited

Submillimetre Photometry of 323 Nearby Galaxies from the Herschel Reference Survey

L. Ciesla, A. Boselli, M. W. L. Smith +23

The Herschel Reference Survey (HRS) is a guaranteed time Herschel key project aimed at studying the physical properties of the interstellar medium in galaxies of the nearby univers…