Monitoring Compact Extragalactic Radio Sources at 4.8 and 8.6 GHz Using the 32-m Radio Telescope of the Svetloe Radio Astronomy Observatory

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

2

Scientific paper

We present the results of monitoring of the integrated fluxes of variable extragalactic sources at 4.8 and 8.6 GHz at the Svetloe Radio Astronomy Observatory (Institute of Applied Astronomy, Russian Academy of Sciences) from 1999 up to the present. More than 1000 observations of 36 sources have been carried out over this monitoring interval. We describe some of the most interesting flares detected in a number of sources, including the well-known objects 0851+202, 3C 345, and BL Lac. Even observations of variability at two frequencies can be very useful for planning astrophysical and astrometric observations. We briefly discuss the possibility of enhancing the effectiveness of the monitoring by expanding the range of frequencies to 22 GHz and adding polarization observations.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Monitoring Compact Extragalactic Radio Sources at 4.8 and 8.6 GHz Using the 32-m Radio Telescope of the Svetloe Radio Astronomy Observatory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Monitoring Compact Extragalactic Radio Sources at 4.8 and 8.6 GHz Using the 32-m Radio Telescope of the Svetloe Radio Astronomy Observatory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Monitoring Compact Extragalactic Radio Sources at 4.8 and 8.6 GHz Using the 32-m Radio Telescope of the Svetloe Radio Astronomy Observatory will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-890846

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.