Spectral variability of radio sources at low frequencies

Spectral variability of radio sources encodes information about the conditions of intervening media, source structure, and emission processes. With new low-frequency radio interferometers observing over wide fractional bandwidths, studies of spectral variability for a large population of extragalact...

Full description

Bibliographic Details
Main Authors: Ross, Kat, Callingham, J.R., Hurley-Walker, Natasha, Seymour, Nick, Hancock, Paul, Franzen, Thomas, Morgan, John, White, S.V., Bell, M.E., Patil, P.
Format: Journal Article
Language:English
Published: OXFORD UNIV PRESS 2021
Subjects:
Online Access:http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91779
_version_ 1848765590007709696
author Ross, Kat
Callingham, J.R.
Hurley-Walker, Natasha
Seymour, Nick
Hancock, Paul
Franzen, Thomas
Morgan, John
White, S.V.
Bell, M.E.
Patil, P.
author_facet Ross, Kat
Callingham, J.R.
Hurley-Walker, Natasha
Seymour, Nick
Hancock, Paul
Franzen, Thomas
Morgan, John
White, S.V.
Bell, M.E.
Patil, P.
author_sort Ross, Kat
building Curtin Institutional Repository
collection Online Access
description Spectral variability of radio sources encodes information about the conditions of intervening media, source structure, and emission processes. With new low-frequency radio interferometers observing over wide fractional bandwidths, studies of spectral variability for a large population of extragalactic radio sources are now possible. Using two epochs of observations from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey that were taken one year apart, we search for spectral variability across 100-230 MHz for 21 558 sources. We present methodologies for detecting variability in the spectrum between epochs and for classifying the type of variability: either as a change in spectral shape or as a uniform change in flux density across the bandwidth. We identify 323 sources with significant spectral variability over a year-long time-scale. Of the 323 variable sources, we classify 51 of these as showing a significant change in spectral shape. Variability is more prevalent in peaked-spectrum sources, analogous to gigahertz-peaked spectrum and compact steep-spectrum sources, compared to typical radio galaxies. We discuss the viability of several potential explanations of the observed spectral variability, such as interstellar scintillation and jet evolution. Our results suggest that the radio sky in the megahertz regime is more dynamic than previously suggested.
first_indexed 2025-11-14T11:37:40Z
format Journal Article
id curtin-20.500.11937-91779
institution Curtin University Malaysia
institution_category Local University
language English
last_indexed 2025-11-14T11:37:40Z
publishDate 2021
publisher OXFORD UNIV PRESS
recordtype eprints
repository_type Digital Repository
spelling curtin-20.500.11937-917792023-05-16T02:44:01Z Spectral variability of radio sources at low frequencies Ross, Kat Callingham, J.R. Hurley-Walker, Natasha Seymour, Nick Hancock, Paul Franzen, Thomas Morgan, John White, S.V. Bell, M.E. Patil, P. Science & Technology Physical Sciences Astronomy & Astrophysics galaxies: active radio continuum: galaxies radio continuum: general ACTIVE GALACTIC NUCLEI MOLONGLO REFERENCE CATALOG COMPACT SYMMETRIC OBJECT FREE-FREE ABSORPTION STEEP-SPECTRUM DATA RELEASE ARRAY SCINTILLATION SELECTION JETS astro-ph.GA astro-ph.GA Spectral variability of radio sources encodes information about the conditions of intervening media, source structure, and emission processes. With new low-frequency radio interferometers observing over wide fractional bandwidths, studies of spectral variability for a large population of extragalactic radio sources are now possible. Using two epochs of observations from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey that were taken one year apart, we search for spectral variability across 100-230 MHz for 21 558 sources. We present methodologies for detecting variability in the spectrum between epochs and for classifying the type of variability: either as a change in spectral shape or as a uniform change in flux density across the bandwidth. We identify 323 sources with significant spectral variability over a year-long time-scale. Of the 323 variable sources, we classify 51 of these as showing a significant change in spectral shape. Variability is more prevalent in peaked-spectrum sources, analogous to gigahertz-peaked spectrum and compact steep-spectrum sources, compared to typical radio galaxies. We discuss the viability of several potential explanations of the observed spectral variability, such as interstellar scintillation and jet evolution. Our results suggest that the radio sky in the megahertz regime is more dynamic than previously suggested. 2021 Journal Article http://hdl.handle.net/20.500.11937/91779 10.1093/mnras/staa3795 English http://purl.org/au-research/grants/arc/FT190100231 OXFORD UNIV PRESS fulltext
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
galaxies: active
radio continuum: galaxies
radio continuum: general
ACTIVE GALACTIC NUCLEI
MOLONGLO REFERENCE CATALOG
COMPACT SYMMETRIC OBJECT
FREE-FREE ABSORPTION
STEEP-SPECTRUM
DATA RELEASE
ARRAY
SCINTILLATION
SELECTION
JETS
astro-ph.GA
astro-ph.GA
Ross, Kat
Callingham, J.R.
Hurley-Walker, Natasha
Seymour, Nick
Hancock, Paul
Franzen, Thomas
Morgan, John
White, S.V.
Bell, M.E.
Patil, P.
Spectral variability of radio sources at low frequencies
title Spectral variability of radio sources at low frequencies
title_full Spectral variability of radio sources at low frequencies
title_fullStr Spectral variability of radio sources at low frequencies
title_full_unstemmed Spectral variability of radio sources at low frequencies
title_short Spectral variability of radio sources at low frequencies
title_sort spectral variability of radio sources at low frequencies
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
galaxies: active
radio continuum: galaxies
radio continuum: general
ACTIVE GALACTIC NUCLEI
MOLONGLO REFERENCE CATALOG
COMPACT SYMMETRIC OBJECT
FREE-FREE ABSORPTION
STEEP-SPECTRUM
DATA RELEASE
ARRAY
SCINTILLATION
SELECTION
JETS
astro-ph.GA
astro-ph.GA
url http://purl.org/au-research/grants/arc/FT190100231
http://hdl.handle.net/20.500.11937/91779