Interplanetary scintillation studies with the Murchison Widefield Array III: comparison of source counts and densities for radio sources and their sub-arcsecond components at 162 MHz-Reference-Cited by-同舟云学术

Interplanetary scintillation studies with the Murchison Widefield Array III: comparison of source counts and densities for radio sources and their sub-arcsecond components at 162 MHz

Published:2018-06-23 Issue:2 Volume:479 Page:2318-2327
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Chhetri R¹²,Ekers R D¹³,Morgan J¹²,Macquart J-P¹²^ORCID,Franzen T M O⁴⁵

Affiliation:

1. International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, WA 6845, Australia

2. ARC Centre of Excellence for All-Sky Astrophysics (CAASTRO), Australia

3. CSIRO Astronomy and Space Science (CASS), Marsfield, NSW 2122, Australia

4. CSIRO Astronomy and Space Science, PO Box 1130, Bentley, WA 6102, Australia

5. Netherlands Institute for Radio Astronomy (ASTRON), PO Box 2, NL-7990 AA Dwingeloo, the Netherlands

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/479/2/2318/25145193/sty1665.pdf

Reference27 articles.

1. Extragalactic Peaked-spectrum Radio Sources at Low Frequencies

2. The AT20G high-angular-resolution catalogue

3. Interplanetary scintillation studies with the Murchison Widefield Array – II. Properties of sub-arcsecond compact sources at low radio frequencies

4. Cosmological evolution of radio sources

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