1.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of Cape TownZA56 papers
- University of the Western CapeZA44 papers
- Istituto di Radioastronomia di BolognaIT31 papers
- University of OxfordGB22 papers
- South African Radio Astronomy ObservatoryZA17 papers
- International Centre for Radio Astronomy ResearchAU16 papers
- National Radio Astronomy ObservatoryUS16 papers
- Rhodes UniversityZA16 papers
- Commonwealth Scientific and Industrial Research OrganisationAU14 papers
- Netherlands Institute for Radio AstronomyNL14 papers
- Western Sydney UniversityAU13 papers
- Royal ObservatoryGB11 papers
12 papers · 1 filter
The Evolution of the Low-Frequency Radio AGN Population to in the ELAIS N1 Field
E. F. Ocran, A. R. Taylor, M. Vaccari +4
We study the cosmic evolution of radio sources out to using a GMRT 610 MHz survey covering 1.86 deg of the ELAIS N1 field with a minimum/median rms noise 7…
The redshift evolution of the baryonic Tully-Fisher relation in Simba
M. Glowacki, E. Elson, R. Davé
The baryonic Tully-Fisher relation (BTFR) is an important tool for constraining galaxy evolution models. As 21-cm HI emission studies have been largely restricted to low redshifts,…
New constraints on the 1.4 GHz source number counts and luminosity functions in the Lockman Hole field
Matteo Bonato, Isabella Prandoni, Gianfranco De Zotti +3
We present a study of the 1173 sources brighter than Jy detected over an area of in the Lockman Hole field. Exploiting the mu…
A Wide-area GMRT 610~MHz survey of ELAIS N1 field
C. H. Ishwara-Chandra, A. R. Taylor, D. A. Green +3
In this paper we present a wide-area 610 MHz survey of the ELAIS\,N1 field with the GMRT, covering an area of 12.8 deg at a resolution of 6 arcsec and with an rms noise of $\si…
Blind HI and OH absorption line search: first results with MALS and uGMRT processed using ARTIP
N. Gupta, P. Jagannathan, R. Srianand +32
We present details of the Automated Radio Telescope Imaging Pipeline (ARTIP) and results of a sensitive blind search for HI and OH absorbers at and , respectively. A…
J1615+5452: a remnant radio galaxy in the ELAIS-N1 field
Z. Randriamanakoto, C. H. Ishwara-Chandra, A. R. Taylor
We report the discovery of a remnant radio AGN J1615+5452 in the field of ELAIS-N1. GMRT continuum observations at 150, 325 and 610 MHz combined with archival data from the 1.4 GHz…
Unexpected Circular Radio Objects at High Galactic Latitude
Ray P. Norris, Huib T. Intema, Anna D. Kapinska +26
We have found a class of circular radio objects in the Evolutionary Map of the Universe Pilot Survey, using the Australian Square Kilometre Array Pathfinder telescope. The objects…
An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2 COSMOS field
J. M. Simpson, Ian Smail, U. Dudzeviciute +19
We present an ALMA study of the ~180 brightest sources in the SCUBA-2 map of the COSMOS field from the S2COSMOS survey, as a pilot study for AS2COSMOS - a full survey of the ~1,000…
The baryonic Tully-Fisher relation in the Simba simulation
M. Glowacki, E. Elson, R. Davé
We investigate the Baryonic Tully-Fisher Relation (BTFR) in the Simba hydrodynamical galaxy formation simulation together with a higher-resolution $(25\,…
IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane
M. Monguió, R. Greimel, J. E. Drew +47
The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys, IPHAS and UVEX, based on data from the Isaac Newton Telescope (INT) obtained between 2003 an…
Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger S190814bv
K. Ackley, L. Amati, C. Barbieri +151
On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely…
PKS 2250351: A Giant Radio Galaxy in Abell 3936
N. Seymour, M. Huynh, S. S. Shabala +27
We present a detailed analysis of the radio galaxy PKS 2250-351, a giant of 1.2 Mpc projected size, its host galaxy, and its environment. We use radio data from the Murchison Widef…