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[CANCELLED] Anisotropies in the GW sky at pulsar timing arrays

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If you have a question about this talk, please contact Thomas Colas .

Online speaker (Zoom)

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 key to determining its origin, and in particular to distinguish possible astrophysical from cosmological sources. In this talk, I discuss the sensitivity of current and future pulsar timing arrays to such anisotropies using the full covariance matrix of pulsar timing delays.

This talk is part of the Cosmology Lunch series.

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Faculty of Education, 184 Hills Road, Cambridge, CB2 8PQ, DMB, Room 2S10 Seminar Room, Henry Wellcome Building & on Zoom -https://zoom.us/meeting/register/tJAsduigrTwtEtMPh6m9S7OnOef5SaPcSYOn Room SG2, Alison Richard Building, 7 West Road, Cambridge, CB3 9DT

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