ATCA radio observation of the region around IGR J18245-2452

L. Pavan, G. Wong, M. H. Wieringa, N. F. H. Tothill, M. D. Filipovic, E. Bozzo, C. Ferrigno, A. Papitto, P. Romano

    Research output: Contribution to journalArticle

    Abstract

    The new INTEGRAL transient source IGR J18245-2452 (ATel #4925 #4927 #4929 #4934 #4959 #4960 #4961 #4964) was observed with the radio Australia Telescope Compact Array on 2013-04-05 for a total of 6 hours. The array was in H214 configuration. The observation was performed at two different frequencies: 9 and 5.5 GHz. ATCA detected at both frequencies a single source in the vicinity of IGR J18245-2452, at R.A. 18h24m32.51s Dec. -24°52"²07.9"²"² (with a 90% confidence error of 0.5"²"²). This position is at 4.8"²"² from the best fit position of IGR J18245-2452 (Heinke et al., ATel #4927), estimated by Swift/XRT with an uncertainty of 3.5"²"² at a 90% confidence level (c.l.).
    Original languageEnglish
    Article number4981
    Number of pages1
    JournalAstronomer's Telegram
    Publication statusPublished - 2013

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