From: LARRY KLAES (ljk4_at_msn.com)
Date: Mon Jan 07 2008 - 12:18:24 PST
>From: atel_at_astronomerstelegram.org
>To: ljk4_at_msn.com
>Subject: ATel 1350. ***Instant Email Notice***: Supernovae
>Date: 7 Jan 2008 11:50:56 -0800
>
>***Instant Email Notice***: Supernovae
>
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>The Astronomer's Telegram
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>ATEL #1350 ATEL #1350
>
>Title: Discovery of Radio Emission from SN 2007uy
>Author: Alicia Soderberg (Princeton University)
>Queries: alicia_at_astro.princeton.edu
>Posted: 7 Jan 2008; 19:36 UT
>Subjects: Radio, Novae, Supernovae
>
>I observed the Type Ibc SN 2007uy (IAUC 8908) with the Very Large Array
>beginning on 2008 Jan 6.18 UT. I detect a radio transient at RA=09:09:35.30
>Dec=+33:07:09.1 with an uncertainty of 0.1 arcsec in each coordinate which
>is coincident with the optical position. At 8.46 GHz, the measured flux
>density of the source is 290 +- 30 microJy. Follow-up observations with
>the Very Large Array are ongoing. I further note that a simultaneous
>Swift/XRT observation of the SN reveals a marginally detected X-ray
>source
>near the radio SN position. Follow-up observations with Swift are planned
>and will determine if the X-ray emission can be attributed to the SN.
>I thank the VLA and Swift scheduling committees for making these ToO
>observations possible.
>
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>Password Certification: Alicia M. Soderberg (ams_at_astro.caltech.edu)
>http://www.astronomerstelegram.org/?read=1350
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