Swift has two main types of rate'' triggers: short and long. Short trigger time scales range from 4ms to 64ms, while long triggers are 64ms to ~ 16 seconds. While both short and long trigger have criteria with one background sample (traditional one-sided’’ triggers), the long triggers can also have
criteria with two background samples (``bracketed’’ triggers) which remove
trends in the background. Both long and short triggers can select energy ranges
of 15-25, 15-50, 25-100 and 50-350 KeV. There are more than 180 short
triggering criteria and approximately 500 long triggering criteria used to
detect gamma ray bursts. To fully utilize these criteria, the thresholds must
be set correctly. The optimum thresholds are determined by a tradeoff between
avoiding false triggers and capturing as many bursts as possible. We use
realistic simulated orbital variations, which are the prime cause of false
triggers.

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