activity
20062026
most citedSpectroscopic Confirmation of a Massive Red-Sequence-Selected Galaxy Cluster at z = 1.34 in the SpARCS-South Cluster Survey

167 citations · 495 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

AGN Feedback: The impact of galactic-scale radio jets on the interstellar medium in starbursting obscured AGN

M. Polletta, C. J. Lonsdale, P. Pallavi +3

A highly star-forming galaxy at z ~ 2 hosting an obscured, luminous active galactic nucleus (AGN) and a relativistic radio jet sets the stage for a cosmic crime scene. The victim i…

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.GA2018★ 36 cited

Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array

Kristina Nyland, Jeremy J. Harwood, Dipanjan Mukherjee +19

Energetic feedback by Active Galactic Nuclei (AGNs) plays an important evolutionary role in the regulation of star formation (SF) on galactic scales. However, the effects of this f…

astro-ph.GA2017★ 43 cited

The population of SNe/SNRs in the starburst galaxy Arp 220. A self-consistent analysis of 20 years of VLBI monitoring

E. Varenius, J. E. Conway, F. Batejat +6

The nearby ultra-luminous infrared galaxy (ULIRG) Arp 220 is an excellent laboratory for studies of extreme astrophysical environments. For 20 years, Very Long Baseline Interferome…

astro-ph.GA2015★ 44 cited

Radio Jet Feedback and Star Formation in Heavily Obscured Quasars at Redshifts ~0.3-3, I: ALMA Observations

Carol J. Lonsdale, Mark Lacy, Amy E. Kimball +17

We present ALMA 870 micron (345 GHz) data for 49 high redshift (0.47<z<2.85), luminous (11.7 < log L(bol) (Lsun) < 14.2) radio-powerful AGN, obtained to constrain cool dust emissio…

astro-ph.CO2012★ 10 cited

Rapid variability of the compact radio sources in Arp220. Evidence for a population of microblazars?

F. Batejat, J. E. Conway, A. Rushton +3

Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previously identified as radio supernovae or supernova remnants. Aims. In order to sea…

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…

astro-ph2008★ 167 cited

Spectroscopic Confirmation of a Massive Red-Sequence-Selected Galaxy Cluster at z = 1.34 in the SpARCS-South Cluster Survey

Gillian Wilson, Adam Muzzin, H. K. C. Yee +10

The Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS) is a z'-passband imaging survey, consisting of deep (z' ~ 24 AB) observations made from both hemispheres using th…

astro-ph2006★ 156 cited

VLBI Images of 49 Radio Supernovae in Arp 220

Colin J. Lonsdale, Philip J. Diamond, Hannah Thrall +2

We have used a Very Long Baseline Interferometry (VLBI) array at 18cm wavelength to image the nucleus of the luminous IR galaxy Arp 220 at ~1 pc linear resolution, and with very hi…