Further observational evidence for a critical ionizing luminosity in active galaxies

We report the results of a survey for H I 21-cm absorption at redshifts of z ≳ 2.6 in a new sample of radio sources with the Green Bank and Giant Metrewave Radio Telescopes. From a total of 25 targets, we report zero detections in the 16 for which optical depth limits could be obtained. Based upon t...

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Main Authors: Curran, S, Hunstead, R, Johnston, H, Whiting, M, Sadler, E, Allison, J, Bignell, C
Format: Journal article
Language:English
Published: Oxford University Press 2017
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author Curran, S
Hunstead, R
Johnston, H
Whiting, M
Sadler, E
Allison, J
Bignell, C
author_facet Curran, S
Hunstead, R
Johnston, H
Whiting, M
Sadler, E
Allison, J
Bignell, C
author_sort Curran, S
collection OXFORD
description We report the results of a survey for H I 21-cm absorption at redshifts of z ≳ 2.6 in a new sample of radio sources with the Green Bank and Giant Metrewave Radio Telescopes. From a total of 25 targets, we report zero detections in the 16 for which optical depth limits could be obtained. Based upon the detection rate for z ≥ 0.1 associated absorption, we would expect approximately four detections. Of the 11 which have previously not been searched, there is sufficient source-frame optical/ultraviolet photometry to determine the ionizing photon rate for four. Adding these to the literature, the hypothesis that there is a critical rate of QHI∼1056 ionizing photons per second (a monochromatic λ = 912 Å luminosity of LUV ∼ 1023 W Hz−1) is now significant at ≈7σ. This reaffirms our assertion that searching z ≳ 3 active galaxies for which optical redshifts are available selects sources in which the ultraviolet luminosity is sufficient to ionize all of the neutral gas in the host galaxy.
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spelling oxford-uuid:c60b1edc-141f-4a4d-9f82-41681ff346692022-03-27T06:35:20ZFurther observational evidence for a critical ionizing luminosity in active galaxiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:c60b1edc-141f-4a4d-9f82-41681ff34669EnglishSymplectic Elements at OxfordOxford University Press2017Curran, SHunstead, RJohnston, HWhiting, MSadler, EAllison, JBignell, CWe report the results of a survey for H I 21-cm absorption at redshifts of z ≳ 2.6 in a new sample of radio sources with the Green Bank and Giant Metrewave Radio Telescopes. From a total of 25 targets, we report zero detections in the 16 for which optical depth limits could be obtained. Based upon the detection rate for z ≥ 0.1 associated absorption, we would expect approximately four detections. Of the 11 which have previously not been searched, there is sufficient source-frame optical/ultraviolet photometry to determine the ionizing photon rate for four. Adding these to the literature, the hypothesis that there is a critical rate of QHI∼1056 ionizing photons per second (a monochromatic λ = 912 Å luminosity of LUV ∼ 1023 W Hz−1) is now significant at ≈7σ. This reaffirms our assertion that searching z ≳ 3 active galaxies for which optical redshifts are available selects sources in which the ultraviolet luminosity is sufficient to ionize all of the neutral gas in the host galaxy.
spellingShingle Curran, S
Hunstead, R
Johnston, H
Whiting, M
Sadler, E
Allison, J
Bignell, C
Further observational evidence for a critical ionizing luminosity in active galaxies
title Further observational evidence for a critical ionizing luminosity in active galaxies
title_full Further observational evidence for a critical ionizing luminosity in active galaxies
title_fullStr Further observational evidence for a critical ionizing luminosity in active galaxies
title_full_unstemmed Further observational evidence for a critical ionizing luminosity in active galaxies
title_short Further observational evidence for a critical ionizing luminosity in active galaxies
title_sort further observational evidence for a critical ionizing luminosity in active galaxies
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