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Published June 2021 | Published + Accepted Version
Journal Article Open

MERGHERS pilot: MeerKAT discovery of diffuse emission in nine massive Sunyaev–Zel'dovich-selected galaxy clusters from ACT

Abstract

The MeerKAT Exploration of Relics, Giant Halos, and Extragalactic Radio Sources (MERGHERS) survey is a planned project to study a large statistical sample of galaxy clusters with the MeerKAT observatory. Here we present the results of a 16-h pilot project, observed in response to the 2019 MeerKAT Shared Risk proposal call, to test the feasibility of using MeerKAT for a large cluster study using short (0.2–2.1 h) integration times. The pilot focuses on 1.28-GHz observations of 13 massive, low-to-intermediate redshift (0.22 < z < 0.65) clusters from the Sunyaev–Zel'dovich-selected Atacama Cosmology Telescope (ACT) DR5 catalogue that show multiwavelength indications of dynamical disturbance. With a 70 per cent detection rate (9/13 clusters), this pilot study validates our proposed MERGHERS observing strategy and provides twelve detections of diffuse emission, eleven of them new, indicating the strength of MeerKAT for such types of studies. The detections (signal-to-noise ratio ≳ 6) are summarized as follows: two systems host both relic(s) and a giant radio halo, five systems host radio haloes, and two have candidate radio haloes. Power values, k-corrected to 1.4 GHz, assuming a fiducial spectral index of α = −1.3 ± 0.4, are consistent with known radio halo and relic scaling relations.

Additional Information

© 2021 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2021 March 27. Received 2021 March 23; in original form 2020 December 30. Published: 05 April 2021. The MeerKAT telescope is operated by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation, an agency of the Department of Science and Innovation. KK, DP, and SS acknowledge funding support from SARAO. JPH acknowledges support from National Science Foundation Astronomy and Astrophysics Research Program award number 1615657. MH and KM acknowledge support from the National Research Foundation of South Africa. CP acknowledges support by the European Research Council under ERC-CoG grant CRAGSMAN-646955. CS acknowledges support from the Agencia Nacional de Investigación y Desarrollo (ANID) through FONDECYT Iniciación grant no. 11191125. The research of OS is supported by the South African Research Chairs Initiative of the Department of Science and Technology and National Research Foundation. ZX is supported by the Gordon and Betty Moore Foundation. This research made use of the ASTROPY,13 (Astropy Collaboration et al. 2013, 2018), NUMPY (Harris et al. 2020), and SCIPY (Virtanen et al. 2020) PYTHON packages. ASTROPY is a community-developed core PYTHON package for astronomy. The Common Astronomy Software Applications (CASA) package is developed by an international consortium of scientists based at the National Radio Astronomical Observatory (NRAO), the European Southern Observatory (ESO), the National Astronomical Observatory of Japan (NAOJ), the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), the CSIRO division for Astronomy and Space Science (CASS), and the Netherlands Institute for Radio Astronomy (ASTRON) under the guidance of NRAO. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Data Availability: The data underlying this paper will be shared on reasonable request to the corresponding author.

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Additional details

Created:
August 20, 2023
Modified:
October 23, 2023