uGMRT detection of associated HI 21 cm absorption at $z \approx 3.5$
J.N.H.S. Aditya, Regina Jorgenson, Vishal Joshi, Veeresh Singh, Tao, An, Yogesh Chandola

TL;DR
This paper reports the first detection of associated HI 21-cm absorption at a redshift of approximately 3.5, demonstrating that neutral hydrogen can exist in the host galaxies of highly luminous AGNs, with implications for understanding galaxy evolution.
Contribution
It presents the highest-redshift detection of associated HI 21-cm absorption and analyzes the variability and ionization state of the host galaxy's neutral hydrogen.
Findings
Detected HI 21-cm absorption at z ≈ 3.53, the highest at this redshift.
Found that the host galaxy's neutral hydrogen survives despite high UV luminosity.
Observed variability in UV luminosity and ionizing photon rate over time.
Abstract
We report a uGMRT detection of HI 21-cm absorption associated with the radio source 8C 0604+728, at . The source is at the highest redshift at which associated HI 21-cm absorption has been discovered to date, surpassing earlier known absorber at . We estimate ultraviolet luminosities of and , and ionising photon rates of and , using data at different epochs; the source shows year-scale variability in both its luminosity and photon rate. The luminosity and photon rate at later epochs are and times higher than thresholds suggested in the literature above which all the neutral hydrogen in the AGN host galaxy is expected to be ionised. The detection…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
