Radio Maps for 'Connecting outflows with radio emission in AGN at Cosmic Noon'
<p dir="ltr">This data release contains the new radio maps produced for the following publication:</p><p dir="ltr"><b>Title: </b>Connecting outflows with radio emission in AGN at Cosmic Noon<br><b>Author(s): </b>G. S. Ilha, C.M. Harrison, V. Mainieri, Ann Njeri, E. Bertola, M. Bischetti, C. Circosta, C. Cicone, G. Cresci, V.A. Fawcett, A. Georgakakis, D. Kakkad, I. Lamperti, A. Marconi, M. Perna, A. Puglisi, D. Rosario, G. Tozzi, C.Vignali , G. Zamorani</p><p dir="ltr"><b>Astronomy & Astrophysics, in press (2025).</b></p><p dir="ltr">This publication is part of the wider SUPER project (a SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback), initially introduced in Circosta et al. 2018, Astronomy & Astrophysics, 620, A82 (link: <a href="https://ui.adsabs.harvard.edu/abs/2018A&A...620A..82C//abstract" rel="noreferrer" target="_blank">https://ui.adsabs.harvard.edu/abs/2018A&A...620A..82C/</a>).</p><p dir="ltr">There are three galaxies studied in this work, and each was observed with the Very Large Array (VLA), in the C-band (central frequency of ~6GHz), in two configurations (A-array and B-array). Therefore, there are six maps in total (two for each galaxy). The details of these radio maps are described in the main publication.</p><p dir="ltr">This data release contains:</p><ol><li>Galaxy J1333+1649, A-array map: J1333+1649.Aarray.selfcal3amp_clean.125arcsec.Briggs.0.pbcorr.tt0.fits</li><li>Galaxy XID36, A-array map: XID36.briggs_plus1.fits</li><li>Galaxy CID346, A-array map: CID346.briggs_plus_1.fits</li><li>Galaxy J1333+1649 B-array map: J1333+1649.Barray.selfcal1_clean.260arcsec.Briggs.0.pbcorr.tt0.fits</li><li>Galaxy XID36, B-array map: XID36.briggs_0.fits</li><li>Galaxy CID346, B-array map: CID346.briggs_0.fits</li><li>A README containing more information</li></ol><p dir="ltr">The maps are released in fits format, including extensive metadata in the header, such as world coordinate system information.</p><p><br></p>
