activity
20102026
most citedA stubbornly large mass of cold dust in the ejecta of Supernova 1987A

194 citations · 349 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026★ 1 cited

MIGHTEE: The evolving radio luminosity functions of star-forming galaxies to and the cosmic history of star formation

Nijin J. Thykkathu, Matt J. Jarvis, Imogen H. Whittam +9

A key question in extragalactic astronomy is how the star-formation rate density (SFRD) evolves over cosmic time. A powerful way of addressing this question is using radio-continuu…

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.GA2025

How accurately can obscured galaxy luminosities be measured using spectral energy distribution fitting of near- through far-infrared observations?

Duncan Farrah, Kiana Ejercito, Andreas Efstathiou +23

Infrared-luminous galaxies are important sites of stellar and black hole mass assembly at most redshifts. Their luminosities are often estimated by fitting spectral energy distribu…

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.SR2014★ 194 cited

A stubbornly large mass of cold dust in the ejecta of Supernova 1987A

M. Matsuura, E. Dwek, M. J. Barlow +33

We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out in 2012. Our dedicated photometric measurements provide new 70 micron data and im…

astro-ph.CO2011★ 113 cited

The Herschel Multi-Tiered Extragalactic Survey: SPIRE-mm Photometric Redshifts

I. G. Roseboom, R. J. Ivison, T. R. Greve +78

We investigate the potential of submm-mm and submm-mm-radio photometric redshifts using a sample of mm-selected sources as seen at 250, 350 and 500 μm by the SPIRE instrument on He…

astro-ph.CO2010★ 39 cited

Measures of star formation rates from Infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields

V. Buat, E. Giovannoli, D. Burgarella +75

The reliability of infrared (IR) and ultraviolet (UV) emissions to measure star formation rates in galaxies is investigated for a large sample of galaxies observed with the SPIRE a…