Richard A N Brooks
The north–south asymmetry of the ALFALFA H i velocity width function
Brooks, Richard A N; Oman, Kyle A; Frenk, Carlos S
Authors
Dr Kyle Oman kyle.a.oman@durham.ac.uk
Associate Professor - Royal Society Dorothy Hodgkin Fellow
Professor Carlos Frenk c.s.frenk@durham.ac.uk
Professor
Abstract
The number density of extragalactic 21-cm radio sources as a function of their spectral line widths - the HI width function (HIWF) - is a sensitive tracer of the dark matter halo mass function (HMF). The Lambda cold dark matter model predicts that the HMF should be identical everywhere provided it is sampled in sufficiently large volumes, implying that the same should be true of the HI WF. The Arecibo Legacy Fast ALFA (ALFALFA) 21-cm survey measured the HI WF in northern and southern Galactic fields and found a systematically higher number density in the north. At face value, this is in tension with theoretical predictions. We use the Sibelius-DARK N-body simulation and the semi-analytical galaxy formation model GALFORM to create a mock ALFALFA survey. We find that the offset in number density has two origins: the sensitivity of the survey is different in the two fields, which has not been correctly accounted for in previous measurements; and the 1/Veff algorithm used for completeness corrections does not fully account for biases arising from spatial clustering in the galaxy distribution. The latter is primarily driven by a foreground overdensity in the northern field within 30 Mpc, but more distant structure also plays a role. We provide updated measurements of the ALFALFA HI WF (and HI mass function) correcting for the variations in survey sensitivity. Only when systematic effects such as these are understood and corrected for can cosmological models be tested against the HI WF.
Citation
Brooks, R. A. N., Oman, K. A., & Frenk, C. S. (2023). The north–south asymmetry of the ALFALFA H i velocity width function. Monthly Notices of the Royal Astronomical Society, 522(3), 4043-4058. https://doi.org/10.1093/mnras/stad1191
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 18, 2023 |
Online Publication Date | Apr 17, 2023 |
Publication Date | May 2, 2023 |
Deposit Date | Oct 31, 2023 |
Publicly Available Date | Nov 2, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 522 |
Issue | 3 |
Pages | 4043-4058 |
DOI | https://doi.org/10.1093/mnras/stad1191 |
Public URL | https://durham-repository.worktribe.com/output/1872057 |
Files
Published Journal Article
(3.8 Mb)
PDF
Licence
http://creativecommons.org/licenses/by/4.0/
Copyright Statement
This accepted manuscript is licensed under the Creative Commons Attribution licence.
You might also like
The impact and response of mini-haloes and the interhalo medium on cosmic reionization
(2024)
Journal Article
The FLAMINGO project: revisiting the S8 tension and the role of baryonic physics
(2023)
Journal Article
Where shadows lie: reconstruction of anisotropies in the neutrino sky
(2023)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search