Tracing X‐ray and HI absorption in peaked spectrum sources-Reference-Cited by-同舟云学术

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Tracing X‐ray and HI absorption in peaked spectrum sources

Published:2021-11 Issue:9-10 Volume:342 Page:1097-1101
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron Nachr

Author:

Kerrison Emily F.¹²^ORCID,Moss Vanessa A.¹²^ORCID,Sadler Elaine M.¹²³^ORCID,Allison James R.³⁴^ORCID

Affiliation:

1. Sydney Institute for Astronomy, School of Physics A28 University of Sydney Sydney New South Wales Australia

2. CSIRO Space and Astronomy Epping New South Wales Australia

3. ARC Centre of Excellence for All‐Sky Astrophysics in 3 Dimensions (ASTRO 3D)

4. Sub‐Department of Astrophysics, Department of Physics University of Oxford Oxford UK

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210095

Reference23 articles.

1. Allison J. R. Sadler E. M. Amaral A. D.et al.2021 arXiv e‐prints arXiv:2110.00469.

2. Astropy: A community Python package for astronomy

3. The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package

4. Unification of the Radio and Optical Properties of Gigahertz Peak Spectrum and Compact Steep‐Spectrum Radio Sources

5. Extragalactic Peaked-spectrum Radio Sources at Low Frequencies

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1. H i absorption associated with Norma’s brightest cluster galaxy;Monthly Notices of the Royal Astronomical Society;2022-12-19

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