Megahertz peaked-spectrum sources in the Bo\"otes field I - a route towards finding high-redshift AGN?
Rocco Coppejans (1), David Cseh (1), Wendy L. Williams (2,3), Sjoert, van Velzen (4), Heino Falcke (1,3,5) ((1) Department of Astrophysics/IMAPP, Radboud University Nijmegen The Netherlands, (2) Leiden Observatory Leiden, University The Netherlands

TL;DR
This study presents a high-resolution 324.5MHz radio survey of the Boötes field, identifying megahertz peaked-spectrum sources that are promising candidates for high-redshift active galactic nuclei, demonstrating the method's effectiveness.
Contribution
The paper introduces a new high-resolution low-frequency radio survey and demonstrates that MPS sources can be used to efficiently find high-redshift AGN candidates.
Findings
Identified 33 MPS sources in the Boötes field.
Redshifts were determined for 24 sources, with an average of 1.3.
At least five sources are at z>2, indicating potential high-redshift AGN.
Abstract
We present a 324.5MHz image of the NOAO Bo\"otes field that was made using Very Large Array (VLA) P-band observations. The image has a resolution of 5.6x5.1arcsec, a radius of and a central noise of ~0.2mJy\beam. Both the resolution and noise of the image are an order of magnitude better than what was previously available at this frequency and will serve as a valuable addition to the already extensive multiwavelength data that are available for this field. The final source catalogue contains 1370 sources and has a median 325 to 1400MHz spectral index of -0.72. Using a radio colour-colour diagram of the unresolved sources in our catalogue, we identify 33 megahertz peaked-spectrum (MPS) sources. Based on the turnover frequency linear size relation for the gigahertz peaked-spectrum (GPS) and compact steep-spectrum (CSS) sources, we expect that the MPS sources that are compact…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation
