PKS 0405-385 flux-density monitoring (Kedziora-Chudczer+, 2006)

Details PKS 0405-385 flux-density monitoring (Kedziora-Chudczer+, 2006) PKS 0405-385 flux-density monitoring (Kedziora-Chudczer+, 2006)

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..73690449k&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/369/449. Originally published in: 2006MNRAS.369..449K

Computer Science

Qsos, Polarization, Radio Sources

Scientific paper

The monitoring of PKS 0405-385 commenced in 1993 November, as part of the ATCA IDV Survey (Kedziora-Chudczer et al., 2001, Cat. ) with the Australia Telescope Compact Array.1 The source showed rapid variability in total flux density at 8.6, 4.8 and 2.4GHz during these observations. The time-scale of variability, defined throughout this paper as HWHP of auto-correlation function of flux density, was faster than 2h (the frequency of sampling used in the survey).
(2 data files).

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