新しい情報です。 可視光transientとconsistentな位置に、大変明るいX線afterglowが見つかり ました。 下記の情報が正しければ、今までで一番明るいX線afterglowだと思われます。 理研 吉田 From: Luigi Piro - BeppoSAX Mission Scientist <piro@ias.rm.cnr.it> To: BEPPOSAX GRB ALERT LIST_2:;; ;; Subject: BeppoSAX MAIL n. 99/3: GRB990123: X-ray afterglow Date: Fri, 23 Jan 1998 20:13:14 +0000 (GMT) BeppoSAX MAIL n. 99/3: GRB990123: X-ray afterglow A BeppoSAX follow-up of GRB990123 initiated around 15:40 UT, i.e. 6 hr after the burst Preliminary analysis of the first 20 minutes of the data at SOC shows a previously unknown strong source (about 10**-11 c.g.s in the 1.6-10 keV ) in the center of the WFC error circle. Preliminary coordinates are: R.A.(2000)= 231.374 DEC(2000)= +44.758 The error radius is 1.5' Considering its strenght, this X-ray source is very likely the X-ray afterglow of GB990123 We will continue to observe it to monitor its temporal evolution 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: -39-06-4993-4007 I-00133 Roma | phone BeppoSAX center: -39-06-4079-6393 Italy | fax(CNR) : -39-06-20660188 #__________________________________#___________________________________________#