<p dir="ltr">This data release is associated with the publication "The Quasar Feedback Survey: Revealing the importance of sensitive radio imaging deeper into the radio quiet regime", published in Njeri et al. (2025), MNRAS, under review.</p><p dir="ltr">This work presents 1.4GHz and 6 GHz radio imaging, obtained from the Very Large Array for the 29 quasars from the extended sample, to lower luminosities (QFeedS-2), of the Quasar Feedback Survey (first presented in Jarvis et al. 2021, MNRAS, 503, 1780 <a href="https://doi.org/10.1093/mnras/stab549" target="_blank"><u>https://doi.org/10.1093/mnras/stab549</u></a> ). These targets are z~0.1 quasar host galaxies, selected to be luminous in [O III] emission (L[O III] > 10<sup>42.1</sup><sup> </sup>erg/s). For full details of the survey description and sample selection see Njeri et al. (2025).</p><p dir="ltr">This data release contains the C-band (~6GHz) images produced from the Very Large Array (VLA), in A-array configuration, for each of the 29 sources. The raw VLA data were obtained under proposal ID 23A-214.</p><p dir="ltr">All normal metadata, associated with astronomical images (observation details, source details, process of imaging), is included with the fits files.</p><p dir="ltr">We used the VLA Calibration Pipeline 2024.1.0.8 for casa version 6.6.1 to reduce our data. Imaging was performed using the casa tclean algorithm with Briggs weighting of r=0.5 for all radio maps.</p>
Funding
Resolving How Black Holes Influence Galaxy Evolution