Open Access Repository

The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey. II. The First Four Epochs


Downloads per month over past year

Lovell, JEJ ORCID: 0000-0001-5273-9817, Rickett, BJ, Macquart, JP, Jauncey, DL, Bignall, HE, Kedziora-Chudczer, L, Ojha, R, Pursimo, T, Dutka, M, Senkbeil, CE and Shabala, SN 2008 , 'The Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey. II. The First Four Epochs' , Astrophysical Journal, vol. 689, no. 1 , pp. 108-126 , doi: 10.1086/592485.

[img] PDF
2008.18-53932.pdf | Request a copy
Full text restricted
Available under University of Tasmania Standard License.


We report on the variability of 443 flat-spectrum, compact radio sources monitored using the VLA for 3 days in four epochs at ~4 month intervals at 5 GHz as part of the Micro-Arcsecond Scintillation-Induced Variability (MASIV) survey. Over half of these sources exhibited 2%-10% rms variations on timescales over 2 days. We analyzed the variations by two independent methods and find that the rms variability amplitudes of the sources correlate with the emission measure in the ionized interstellar medium along their respective lines of sight. We thus link the variations with interstellar scintillation of components of these sources, with some (unknown) fraction of the total flux density contained within a compact region of angular diameter in the range 10-50 μas. We also find that the variations decrease for high mean flux density sources and, most importantly, for high-redshift sources. The decrease in variability is probably due either to an increase in the apparent diameter of the source or to a decrease in the flux density of the compact fraction beyond z ~ 2. Here we present a statistical analysis of these results, and a future paper will discuss the cosmological implications in detail.

Item Type: Article
Authors/Creators:Lovell, JEJ and Rickett, BJ and Macquart, JP and Jauncey, DL and Bignall, HE and Kedziora-Chudczer, L and Ojha, R and Pursimo, T and Dutka, M and Senkbeil, CE and Shabala, SN
Keywords: galaxies: active; ISM: structure; radiation mechanisms: non-thermal; radio continuum: ISM
Journal or Publication Title: Astrophysical Journal
ISSN: 0004-637X
DOI / ID Number: 10.1086/592485
Additional Information:

© 2008 The American Astronomical Society

Item Statistics: View statistics for this item

Actions (login required)

Item Control Page Item Control Page