K-ART (Korea Array Radio Telescope) and Monitoring of Radio Transients

Details K-ART (Korea Array Radio Telescope) and Monitoring of Radio Transients K-ART (Korea Array Radio Telescope) and Monitoring of Radio Transients

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..56k&link_type=abstract

"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November

Physics

Scientific paper

Korea Array Radio Telescope (K-ART), a proto-type radio array telescope, is designed for 300-450 MHz wavebands. The system is located in the Jeju Island of the South Korea, and is currently in its testing mode since last mid-October 2010. It is primarily designed for monitoring solar activity and radio transients. K-ART has a capacity to monitor transients for about 2 hours per day, with a spatial resolution of about 10 minutes and a timing resolution of milliseconds. The sensitivity is expected to be a few mJy or less. We propose to monitor radio transients such as X-ray binaries, cataclysmic variables and quasars, on the target-of-opportunity mode, in addition to the scheduled observation.

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