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dc.contributor.authorZhu, Y.
dc.contributor.authorBecker, G.D.
dc.contributor.authorBosman, S.E.I.
dc.contributor.authorKeating, L.C.
dc.contributor.authorChristenson, H.M.
dc.contributor.authorBañados, E.
dc.contributor.authorBian, F.
dc.contributor.authorDavies, F.B.
dc.contributor.authorD’Odorico, V.
dc.contributor.authorEilers, A.-C.
dc.contributor.authorFan, X.
dc.contributor.authorHaehnelt, M.G.
dc.contributor.authorKulkarni, G.
dc.contributor.authorPallottini, A.
dc.contributor.authorQin, Y.
dc.contributor.authorWang, F.
dc.contributor.authorYang, J.
dc.date.accessioned2022-03-17T01:56:36Z
dc.date.available2022-03-17T01:56:36Z
dc.date.issued2021
dc.identifier.citationZhu, Y., Becker, G. D., Bosman, S. E. I., Keating, L. C., Christenson, H. M., Bañados, E., Bian, F., Davies, F. B., D’Odorico, V., Eilers, A.-C., Fan, X., Haehnelt, M. G., Kulkarni, G., Pallottini, A., Qin, Y., Wang, F., & Yang, J. (2021). Chasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly. Astrophysical Journal.
dc.identifier.issn0004-637X
dc.identifier.doi10.3847/1538-4357/ac26c2
dc.identifier.urihttp://hdl.handle.net/10150/663540
dc.description.abstractWe present a new investigation of the intergalactic medium (IGM) near the end of reionization using “dark gaps” in the Lyα forest. Using spectra of 55 QSOs at z em > 5.5, including new data from the XQR-30 VLT Large Programme, we identify gaps in the Lyα forest where the transmission averaged over 1 comoving h −1 Mpc bins falls below 5%. Nine ultralong (L > 80 h −1 Mpc) dark gaps are identified at z < 6. In addition, we quantify the fraction of QSO spectra exhibiting gaps longer than 30 h −1 Mpc, F 30, as a function of redshift. We measure F 30 ≃ 0.9, 0.6, and 0.15 at z = 6.0, 5.8, and 5.6, respectively, with the last of these long dark gaps persisting down to z ≃5.3. Comparing our results with predictions from hydrodynamical simulations, we find that the data are consistent with models wherein reionization extends significantly below redshift six. Models wherein the IGM is essentially fully reionized that retain large-scale fluctuations in the ionizing UV background at z ≲6 are also potentially consistent with the data. Overall, our results suggest that signatures of reionization in the form of islands of neutral hydrogen and/or large-scale fluctuations in the ionizing background remain present in the IGM until at least z ≃ 5.3. © 2021. The American Astronomical Society. All rights reserved.
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.rightsCopyright © 2021. The American Astronomical Society. All rights reserved.
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleChasing the Tail of Cosmic Reionization with Dark Gap Statistics in the Ly
dc.typeArticle
dc.typetext
dc.contributor.departmentSteward Observatory, University of Arizona
dc.identifier.journalAstrophysical Journal
dc.description.noteImmediate access
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal published version
dc.source.journaltitleAstrophysical Journal
refterms.dateFOA2022-03-17T01:56:36Z


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