Full description
We present early science results from the First Large Absorption Survey in H I (FLASH), a spectroscopically blind survey for 21-cm absorption lines in cold hydrogen (H I) gas at cosmological distances using the Australian Square Kilometre Array Pathfinder (ASKAP). We have searched for H I absorption towards 1253 radio sources in the GAMA 23 field, covering redshifts between z = 0.34 and 0.79 over a sky area of approximately 50 deg2. In a purely blind search, we did not obtain any detections of 21-cm absorbers above our reliability threshold. Assuming a fiducial value for the H I spin temperature of Tspin = 100 K and source covering fraction cf = 1, the total comoving absorption path-length sensitive to all Damped Lyman α Absorbers (DLAs; NH I ≥ 2 × 1020 cm−2) is ΔX = 6.6 ± 0.3 (Δz = 3.7 ± 0.2) and super-DLAs (NH I ≥ 2 × 1021 cm−2) is ΔX = 111 ± 6 (Δz= 63 ± 3). We estimate upper limits on the H I column density frequency distribution function that are consistent with measurements from prior surveys for redshifted optical DLAs, and nearby 21-cm emission and absorption. By cross-matching our sample of radio sources with optical spectroscopic identifications of galaxies in the GAMA 23 field, we were able to detect 21-cm absorption at z = 0.3562 towards NVSS J224500−343030, with a column density of NH I = (1.2 ± 0.1) × 1020 (Tspin/100 K) cm−2. The absorber is associated with GAMA J22450.05−343031.7, a massive early-type galaxy at an impact parameter of 17 kpc with respect to the radio source and which may contain a massive (MH I ≿ 3 × 109 M☉) gas disc. Such gas-rich early types are rare, but have been detected in the nearby Universe.Notes
External OrganisationsARC Centre of Excellence for Astrophysics in Three Dimensions (ASTRO3D); University of Oxford; Commonwealth Scientific & Industrial Research Organisation; University of Sydney; CSIRO - Australia Telescope National Facility; Netherlands Foundation for Research in Astronomy; Victoria University of Wellington; Carnegie Institution of Washington; University of Colorado Boulder; CSIRO - Space and Astronomy; Western Sydney University; Monash University (Australia); University of Hull
Associated Persons
Max Pettini (Creator)James R. Allison (Creator); Elaine M. Sadler (Creator); S. L. Ellison (Creator); Elizabeth K. Mahony (Creator); Vanessa Moss (Creator); Matthew T. Whiting (Creator); S. J. Curran (Creator); Jeremy K. Darling (Creator); A.W. Hotan (Creator); Richard W. Hunstead (Creator); Bärbel Koribalski (Creator); Kevin Pimbblet (Creator); Maxim A. Voronkov (Creator)
Max Pettini (Creator)James R. Allison (Creator); Elaine M. Sadler (Creator); S. L. Ellison (Creator); Elizabeth K. Mahony (Creator); Vanessa Moss (Creator); Matthew T. Whiting (Creator); S. J. Curran (Creator); Jeremy K. Darling (Creator); A.W. Hotan (Creator); Richard W. Hunstead (Creator); Bärbel Koribalski (Creator); Kevin Pimbblet (Creator); Maxim A. Voronkov (Creator)
Issued: 2020-05
Subjects
Astrophysics - Astrophysics of Galaxies |
galaxies: ISM |
galaxies: evolution |
galaxies: high-redshift |
galaxies: structure |
radio lines: galaxies |
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Identifiers
- global : 58ab8dc3-23d7-4a5d-a2db-9a5627122f59