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SUMMARY:Anisotropies in the GW sky at pulsar timing arrays - Valerie Domck
 e (CERN)
DTSTART:20241202T130000Z
DTEND:20241202T140000Z
UID:TALK224584@talks.cam.ac.uk
CONTACT:Thomas Colas
DESCRIPTION:Pulsar Timing Array (PTA) observations have recently gathered 
 substantial evidence for the existence of a gravitational wave background 
 in the nHz frequency band. Searching for anisotropies in this signal is ke
 y to determining its origin\, and in particular to distinguish possible as
 trophysical from cosmological sources. In this talk\, I discuss the sensit
 ivity of current and future pulsar timing arrays to such anisotropies usin
 g the full covariance matrix of pulsar timing delays.
LOCATION:CMS\, Pav. B\, CTC Common Room (B1.19) [Potter Room]
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