Spectroscopic Observations of the Bright Afterglow of GRB021004

Computer Science

Scientific paper

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Chandra Proposal Id #03508125

Scientific paper

One of the holy grails of gamma-ray burst research is to detect X-ray line signatures from an afterglow with high statistical significance. Of all possible observations, this perhaps offers the best chance of constraining the GRB mechanism and environment, and could provide the "smoking gun" signature connecting GRBs to massive stellar deaths. In order to accomplish this, we know long observations within one day of the event are necessary.

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