J Delhaize
MIGHTEE: Are giant radio galaxies more common than we thought?
Delhaize, J; Heywood, I; Prescott, M; Jarvis, MJ; Delvecchio, I; Whittam, IH; White, SV; Hardcastle, MJ; Hale, CL; Afonso, J; Ao, Y; Brienza, M; Brüggen, M; Collier, JD; Daddi, E; Glowacki, M; Maddox, N; Morabito, LK; Prandoni, I; Randriamanakoto, Z; Sekhar, S; An, Fangxia; Adams, NJ; Blyth, S; Bowler, RAA; Leeuw, L; Marchetti, L; Randriamampandry, SM; Thorat, K; Seymour, N; Smirnov, O; Taylor, AR; Tasse, C; Vaccari, M
Authors
I Heywood
M Prescott
MJ Jarvis
I Delvecchio
IH Whittam
SV White
MJ Hardcastle
CL Hale
J Afonso
Y Ao
M Brienza
M Brüggen
JD Collier
E Daddi
M Glowacki
N Maddox
Professor Leah Morabito leah.k.morabito@durham.ac.uk
Professor
I Prandoni
Z Randriamanakoto
S Sekhar
Fangxia An
NJ Adams
S Blyth
RAA Bowler
L Leeuw
L Marchetti
SM Randriamampandry
K Thorat
N Seymour
O Smirnov
AR Taylor
C Tasse
M Vaccari
Abstract
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 ∼1 deg2 region inside the COSMOS field. They have redshifts of z = 0.1656 and z = 0.3363 and physical sizes of 2.4 Mpc and 2.0 Mpc, respectively. Only the cores of these GRGs were clearly visible in previous high resolution VLA observations, since the diffuse emission of the lobes was resolved out. However, the excellent sensitivity and uv coverage of the new MeerKAT telescope allowed this diffuse emission to be detected. The GRGs occupy an unpopulated region of radio power – size parameter space. Based on a recent estimate of the GRG number density, the probability of finding two or more GRGs with such large sizes at z < 0.4 in a ∼1 deg2 field is only 2.7 × 10−6, assuming Poisson statistics. This supports the hypothesis that the prevalence of GRGs has been significantly underestimated in the past due to limited sensitivity to low surface brightness emission. The two GRGs presented here may be the first of a new population to be revealed through surveys like MIGHTEE which provide exquisite sensitivity to diffuse, extended emission.
Citation
Delhaize, J., Heywood, I., Prescott, M., Jarvis, M., Delvecchio, I., Whittam, I., White, S., Hardcastle, M., Hale, C., Afonso, J., Ao, Y., Brienza, M., Brüggen, M., Collier, J., Daddi, E., Glowacki, M., Maddox, N., Morabito, L., Prandoni, I., Randriamanakoto, Z., …Vaccari, M. (2021). MIGHTEE: Are giant radio galaxies more common than we thought?. Monthly Notices of the Royal Astronomical Society, 501(3), 3833-3845. https://doi.org/10.1093/mnras/staa3837
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 9, 2020 |
Online Publication Date | Dec 14, 2020 |
Publication Date | 2021-03 |
Deposit Date | Jan 11, 2021 |
Publicly Available Date | Jul 15, 2021 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 501 |
Issue | 3 |
Pages | 3833-3845 |
DOI | https://doi.org/10.1093/mnras/staa3837 |
Public URL | https://durham-repository.worktribe.com/output/1253958 |
Related Public URLs | https://arxiv.org/abs/2012.05759 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2020 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved
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