ToO observation of a new bright transient discovered by GLAST and Swift in the Galactic plane

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Chandra Proposal Id #09400231

Scientific paper

We propose a TOO observation of a new intense transient detected by GLAST-LAT and followed by a Swift-XRT detection, at |b|<5 deg. Our goal is to determine the nature of an event similar to the intense, non-blazar, transient that EGRET saw in the Galactic plane once in its lifetime. The lack of a radio-loud source and of a known X-ray binary in the error box indicates either a new facet of Galactic compact objects or a new manifestation of a non-blazar active galaxy behind the Milky way. A significant XRT detection of a counterpart will trigger the proposed 30 ks Chandra observation to precisely locate the source in crowded Galactic regions, to constrain the X-ray decay time, and to measure the source spectrum and absorption.

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