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[vsolj-alert 144] GB980613 follow up with NFI
- Date: Tue, 16 Jun 1998 08:52:21 +0900 (JST)
- To: vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsolj-alert 144] GB980613 follow up with NFI
- Sender: owner-vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
GB980613 follow up with NFI
6/13のガンマ線バーストですが、X線のafterglowらしきものが受かっている
ようです。位置もかなり明確になりましたので、特に Source A を中心に可能で
あれば深いCCD撮像で観測を試みていただければと思います。等級は何とも言
えませんが、先日の富山天文台の画像で19-20等が検出できましたので、数十cm
以上の口径で可能かも知れません。USNOチャートは別に作成する予定です。
From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Tue Jun 16 08:43 JST 1998
Date: Tue, 16 Jun 1998 08:43:54 +0900 (JST)
From: Taichi Kato <tkato>
Subject: [vsnet-alert 1886] BeppoSAX GRB 980613 BFI follow up
Date: Tue, 16 Jun 1998 00:12:58 +0000 (GMT)
From: Luigi Piro - BeppoSAX Mission Scientist <saxsci@ias.rm.cnr.it>
Subject: [vsnet-alert 0] BeppoSAX GRB: GB980613 NFI follow up
BeppoSAX GRB MAIL N. 98/21
^^^^^^^^^^^^^^^^^^^^^^^^^^
GB980613: follow up with NFI
Two previously unknown X-ray sources have been found in the WFC error
circle by the MECS during the follow up observation started 9 hrs after
the GRB.
Source A is at
R.A.(2000)= 10h17m53s
Dec.(2000)= +71d27'24"
Source B is at
R.A.(2000)= 10h18m04s
Dec.(2000)= +71d33'30"
The error radius is 50".
Source B does not show substantial variability.
Source A shows a rather strong decay during the observation, and is very
likely the X-ray afterglow of GB980613
Luigi Piro
BeppoSAX Mission Scientist
#----------------------------------#------------------------------------------#
Luigi Piro | E-mail:
Istituto Astrofisica Spaziale | piro@alpha1.ias.rm.cnr.it
C.N.R. | SAX program: saxsci@alpha1.ias.rm.cnr.it
Via Fosso del Cavaliere | phone: -39-6-4993-4007
I-00133 Roma | phone BeppoSAX center: -39-6-4079-6393
Italy | fax(CNR) : -39-6-20660188
#__________________________________#___________________________________________#
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