昨日のX線トランジェント(X線新星)ですが、2 Crab から 0.5 Crab 以下に減衰 していること、発表された位置が少し違っている(時角で約1m西にあるようで す)。なお光学対応天体はまだ検出の報告はありません。 Date: Wed, 1 Apr 1998 19:02:41 -0500 (EST) From: Jean Swank <swank@pcasun1.gsfc.nasa.gov> To: xtej0421+560 -- Carole Haswell <chaswell@star.cpes.susx.ac.uk>, dasmith@space.mit.edu, ehm@space.mit.edu, Tod Strohmayer <stroh@pcasun1.gsfc.nasa.gov>, gehrels@lheavx.gsfc.nasa.gov, giommi@napa.sdc.asi.it, HARMON@SSLMOR.msfc.nasa.gov, jeanz@purple.sron.ruu.nl, JeffMcClintock <jem@head-cfa.harvard.edu>, rhjellmi@aoc.nrao.edu, rr@space.mit.edu, xteplan <xteplan@xgo2.nascom.nasa.gov>, shrader@grossc.gsfc.nasa.gov, vsnet-alert@kusastro.kyoto-u.ac.jp, "WalterH.G.Lewin" <lewin@space.mit.edu> Message-ID: <vsolj-alert60@hoge.baba.hajime.jp> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII Precedence: list X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24] X-Sequence: vsnet-alert 0 Subject: [vsnet-alert 0] xtej0421+560 Errors-To: owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp Interim report to interested parties: I know some of you are planning observations at other wavelengths or are anxious about how the observations will be planned, what we know about the source and who will have access to the data. I should inform you of some developments. 1.) Source intensity Last night the source reached the equivalent of ~ 2 Crab in the PCA, ~ 1 Crab in HEXTE. But it has declined till it is less than 0.5 Crab recently in the ASM. 2.) We think the position needs correcting, but do not have an accurate one for you. The position given in the cirular (which has not come out) is 65.253, 56.058, with an error of ~4'. Last night we executed 4 raster scans over the source. It is clear that the dec pretty good, but the ra looks closer to 65.0 than to 65.25 degrees, so that the error is underestimated. We should be able to get a position to a couple of arc minutes from the scans. By an accident of where the satellite was and the data streams, we seem to be missing, so far, the real time per detector rates (called Standard 1 and 2). We are attempting to get these data as soon as possible. A few more concidences slowed this progress, such as fall out from a need to change passwords and tighten computer security. The disposition of the observations I will comment more on shortly. Ron has been in transit between GSFC and MIT. Jean