GRB 020914

r Williams     Sat Sep 14 12:29   31/1443  File_s102256_12.70_predse                                                         U 56 Ne
 U 56 Neil Gehrels       Sat Sep 14 13:57   67/2560  Re: Thursday lunch
 U 57 HETE Operator      Sat Sep 14 22:51   45/1810  Trigger Notice
 U 58 Roger Williams     Sun Sep 15 00:14   49/2223  File_hsi_20020913_225050.
 U 59 Roger Williams     Sun Sep 15 00:14 12831/346782 File_hsi_20020913_225050.
 U 60 Roger Williams     Sun Sep 15 11:27 19400/1648063 File_qp102258_2A1_04.11_0
? set askcc
? mail
To: gcn
Subject: IPN annulus for GRB020914
Cc:
K. Hurley and T. Cline, on behalf of the Ulysses, Konus, and HETE GRB teams,

E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team, report:


Ulysses and Konus-Wind observed this GRB at 78798 seconds.
We have triangulated it to an annulus with raidus 39.932 +/- 0.066 degrees
(3 sigma) centered at RA, Decl (2000)=170.909, 39.244.  More details
can be obtained for this event at a later time.

^C
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^C"/export/home/khurley/dead.letter" 11/410
Interrupt
? mail
To: gcn
Subject: IPN annulus for GRB020914
Cc:
K. Hurley and T. Cline, on behalf of the Ulysses and Konus GRB teams,and

E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team, report:


Ulysses and Konus-Wind observed this GRB at 78798 seconds.
We have triangulated it to an annulus with radius 39.932 +/- 0.066 degrees
(3 sigma) centered at RA, Decl (2000)=170.909, 39.244.  More details
can be obtained for this event at a later time.

K. Hurley, on behalf of the Ulysses GRB team,

T. Cline, on behalf of the Ulysses and Konus-Wind GRB teams, and

E. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team, report:

Despite the extraneous text in GCN 1543
Loading...
 
  (caused by the fact that it was
sent while I was on travel and working from an unfamiliar terminal,
apologies for the confusion) the numbers given for the annulus center
and radius were correct.  The message is repeated below for clarity,
with some additional information.

Ulysses and Konus-Wind observed this GRB at 78798 seconds.  As observed
by Ulysses, it had a duration ~8 seconds, a 25-100 keV fluence of
8x10^-7 erg/cm2, and a peak flux over 0.5 s of 6.7x10^-7 erg/cm2.
We have triangulated it to an annulus with radius 39.932 +/- 0.066
degrees (3 sigma) centered at RA, Decl (2000) 170.909, +39.244 degrees.
In addition, a preliminary analysis of the Konus ecliptic latitude
response indicates that this event came from above ecliptic latitude
+30 degrees.  The small circle which describes this ecliptic latitude
intersects the annulus at approximately RA, Decl (2000)=211.4, +19.4
degrees and at 115.0, +51.9 degrees.

Mars Odysssey did not detect this burst, so it will not be possible
to derive a true error box for it.  However, some improvements
in the triangulation and ecliptic latitude are possible.