Abstract
Observations have been made of the infrared afterglow candidate
to GRB 030115 (GCN 1818) using the SCUBA bolometer array on
the James Clerk Maxwell Telescope located on Mauna Kea, Hawaii.
The observations took place on January 18.41 - 18.50 UT under
average but stable sky conditions. The source was not detected
at 850 microns, with a 3-sigma upper limit of ~6 mJy
to GRB 030115 (GCN 1818) using the SCUBA bolometer array on
the James Clerk Maxwell Telescope located on Mauna Kea, Hawaii.
The observations took place on January 18.41 - 18.50 UT under
average but stable sky conditions. The source was not detected
at 850 microns, with a 3-sigma upper limit of ~6 mJy
Original language | English |
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Pages (from-to) | 1 |
Number of pages | 1 |
Journal | GRB Coordinates Network |
Volume | 1832 |
Publication status | Published - 2003 |