Speaker
Sergey Molkov
Description
We will present an overview of observations of rapidly rotating neutron stars
by the Pavlinsky ART-XC telescope on-board SRG mission. Despite the fact that
the telescope was designed for scanning large areas of the sky, its detectors
have a good time resolution (≈ 23 microseconds), and the onboard clock is
stable enough, which makes it possible to perform timing analysis of coherent
signals up to several hundreds Hz frequency. We will present the results of
observations of both isolated pulsars and accreting millisecond pulsars.