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![]() TITLE: GCN CIRCULAR NUMBER: 9396 SUBJECT: GRB 090516: Observations from Stardome Observatory DATE: 09/05/19 06:10:37 GMT FROM: Antonio Deugarte at IAA-CSIC <deugarte@iaa.es> G. W. Christie (Stardome/ New Zealand), A. de Ugarte Postigo (ESO/ Chile), and T. Natusch (Stardome/ New Zealand) on behalf of a larger collaboration report: We observed the field of GRB 090516 (Rowlinson et al. GCN 9374) with the Stardome 0.4m telescope located in Auckland
(New Zealand) starting at 09:25UT. We used a SG530 filter
that transmits wavelengths above 5300 Angstroms and a SBIG
ST-L-6303E CCD (KAF-6303E detector). A 9x300s combined
exposure with mean epoch 16.4080 May (80 minutes after the
burst) shows an object at the position of the afterglow
(Guidorzi et al. GCN 9375) measured at R = 20.8 +/- 0.2 as
compared to USNO-B1.0 stars. We note that with the GRB at
a redshift of 4.1 (de Ugarte Postigo et al. GCN 9383),
Ly-alpha falls within the R-band, so that comparison of
clear and very broad band filters such as ours with R-band
has to be handled with care.
This site was created by Robert Quimby
Database maintained by Robert Quimby, Erin McMahon, and Jeremy Murphy Information displayed on this site is compiled from GCN Circulars and other sources as indicated. |
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