activity
19982025
most citedThe Herschel ATLAS

596 citations · 2k across the 33 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2025★ 4 cited

The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation

Maarten Baes, Andrea Gebek, Sabelo Kunene +8

The Tully-Fisher relation (TFR) is one of the most important and widely used empirical correlations in extragalactic astronomy. Apart from its importance as a secondary distance in…

astro-ph.GA2024

MeerKAT Observations of Herschel Protocluster Candidates

Y. Ding, D. L. Clements, L. L. Leeuw +9

High-redshift protoclusters consisting of dusty starbursts are thought to play an important role in galaxy evolution. Their dusty nature makes them bright in the FIR/submm but diff…

astro-ph.GA2023★ 24 cited

The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps

Andrea Gebek, Maarten Baes, Benedikt Diemer +6

Cold gas in galaxies provides a crucial test to evaluate the realism of cosmological hydrodynamical simulations. To extract the atomic and molecular hydrogen properties of the simu…

astro-ph.GA2022★ 8 cited

The star-formation rates of QSOs

M. Symeonidis, N. Maddox, M. J. Jarvis +13

We examine the far-IR properties of a sample of 5391 optically selected QSOs in the 0.5<z<2.65 redshift range down to log[nuLnu,2500 (erg/s)]>44.7, using SPIRE data from Herschel-A…

astro-ph.GA2020★ 45 cited

MIGHTEE: Are giant radio galaxies more common than we thought?

J. Delhaize, I. Heywood, M. Prescott +31

We report the discovery of two new giant radio galaxies (GRGs) using the MeerKAT International GHz Tiered Extragalactic Exploration (MIGHTEE) survey. Both GRGs were found within a…

astro-ph.GA2020★ 4 cited

Cosmic evolution of molecular gas mass density from an empirical relation between and

G. Orellana-González, E. Ibar, R. Leiton +8

Historically, GHz radio emission has been used extensively to characterize the star-formation activity in galaxies. In this work, we look for empirical relations amongst the radio…

astro-ph.GA2020★ 6 cited

SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data

T. Cheng, D. L. Clements, J. Greenslade +21

We measure the 850-m source densities of 46 candidate protoclusters selected from the Planck High-z catalogue (PHz) and the Planck Catalogue of Compact Sources (PCCS) that were…

astro-ph.GA2019★ 24 cited

SCUBA-2 observations of candidate starbursting protoclusters selected by Planck and Herschel-SPIRE

T. Cheng, D. L. Clements, J. Greenslade +21

We present SCUBA-2 850-m observations of 13 candidate starbursting protoclusters selected using Planck and Herschel data. The cumulative number counts of the 850-m sources in…

astro-ph.GA2014★ 2 cited

Dust in the Radio Galaxy and Merger Remnant NGC 1316 (Fornax A)

Bernard Duah Asabere, Cathy Horellou, Hartmut Winkler +2

We present dust maps of NGC 1316 (Fornax A), a well-studied early-type galaxy located in the outskirts of the Fornax cluster. We used the Large APEX BOlometer CAmera (LABOCA), oper…

astro-ph.GA2012★ 10 cited

Magnetic Field in The Isolated Massive Dense Clump IRAS 20126+4104

Hiroko Shinnaga, Giles Novak, John E. Vaillancourt +8

We measured polarized dust emission at 350um towards the high-mass star forming massive dense clump IRAS 20126+4104 using the SHARC II Polarimeter, SHARP, at the Caltech Submillime…