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APT5 - Galactic Gamma-Ray Sources: steady vs. transient sources

Speaker

Markwardt, Craig

Co-autors

Swift BAT Team

Talk Title

Hard X-ray Transients Observed by Swift

Abstract

The X-ray sky is highly variable, and timely follow-up observations are one key to unlocking the secrets of X-ray transients. The Swift observatory has a unique capability to perform automated follow-up observations of new and previously known X-ray transients. Sources are detected by the BAT hard X-ray instrument, and can be examined in more detail by the sensitive XRT and UVOT narrow-field instruments. This talk will summarize several of those discoveries.

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