A new analysis pipeline cross-correlates the time-varying stochastic gravitational-wave background with gamma-ray, X-ray, optical, and radio light curves to find electromagnetic counterparts of sub-threshold mergers, with mock-data false alarm rates that drop when multiple bands are combined.
Exploring rapid transient detection with the Athena Wide Field Imager
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abstract
X-ray transients are among the most enigmatic objects in the cosmic sky. The unpredictability and underlying nature of their transient behavior has prompted much study in recent years. While significant progress has been made in this field, a more complete understanding of such events is often hampered by the delay in the rapid follow-up of any transient event. An efficient way to mitigate this constraint would be to devise a way for near real time detection of such transient phenomena. The Athena/Wide Field Imager (WFI), with its $40' \times 40'$ field of view and large effective area, will detect a large number of X-ray variable or transient objects daily. In this work, we discuss an algorithm for the rapid on-board or ground-based detection of X-ray transients with WFI. We present a feasibility test of the algorithm using simulated Athena/WFI data and show that a fairly simple algorithm can effectively detect transient and variable sources in typical Athena/WFI observations.
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A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
A new analysis pipeline cross-correlates the time-varying stochastic gravitational-wave background with gamma-ray, X-ray, optical, and radio light curves to find electromagnetic counterparts of sub-threshold mergers, with mock-data false alarm rates that drop when multiple bands are combined.