Radio activity in H1743-322

Bibcode
2009ATel.2062....1M
Miller-Jones, James C. A.; Sivakoff, Gregory R.; Migliari, Simone; Koerding, Elmar; Rupen, Michael P.; Remillard, Ronald A.; Dhawan, Vivek; Russell, David M.; Maitra, Dipankar; Fender, Rob P.; Markoff, Sera; Heinz, Sebastian; Sarazin, Craig L.; Maccarone, Tom J.
Bibliographical reference

The Astronomer's Telegram, #2062

Advertised on:
5
2009
Number of authors
14
IAC number of authors
0
Citations
9
Refereed citations
6
Description
Following the detection of renewed activity in H1743-322 with Swift/BAT (Krimm et al., ATEL #2058), we triggered radio observations of the source using the VLA. Observations were taken on 2009 May 27 (0855-0915 UT) at 8.4 GHz, with the array in its CnB configuration. The source was detected at a level of 2.24 +/- 0.05 mJy. The uncertainty on the absolute flux density scale is of order 5%. The source is consistent with being unresolved to the beamsize of 3.3 x 2.2 arcseconds, oriented 35 degrees E of N.
Type
Non-refereed
Black holes

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