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Questions and Answers
What is the purpose of assuming a source position for the GRB in the context of mapping incident photon energies?
What is the purpose of assuming a source position for the GRB in the context of mapping incident photon energies?
Why are NaI detectors used for standard analysis with observing angles less than 60 degrees?
Why are NaI detectors used for standard analysis with observing angles less than 60 degrees?
Why is the BGO detector with the smallest viewing angle to the source used in analysis?
Why is the BGO detector with the smallest viewing angle to the source used in analysis?
Why are detectors not used for analysis if portions of the spacecraft or LAT block them from viewing the source?
Why are detectors not used for analysis if portions of the spacecraft or LAT block them from viewing the source?
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How is the duration of GRBs typically defined?
How is the duration of GRBs typically defined?
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What is T90 in the context of defining GRB duration?
What is T90 in the context of defining GRB duration?
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What is the canonical observing energy range for durations defined by T90?
What is the canonical observing energy range for durations defined by T90?
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In terms of duration analysis, what aspect of GRBs is usually considered at 5% and 95% of cumulative observed fluence?
In terms of duration analysis, what aspect of GRBs is usually considered at 5% and 95% of cumulative observed fluence?
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What is the main parameter that defines the duration of a GRB?
What is the main parameter that defines the duration of a GRB?
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How does observing energy range relate to defining the duration of a GRB burst?
How does observing energy range relate to defining the duration of a GRB burst?
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