Einstein Probe and Synergies with Fast Optical Photometry - Francesco Coti Zelati

15 May 2026, 11:50
20m
Aula Gratton (INAF Astronomical Observatory of Rome)

Aula Gratton

INAF Astronomical Observatory of Rome

Via Frascati, 33 00078 Monte Porzio Catone

Description

Einstein Probe, launched in January 2024, is opening a new window on the transient X-ray Universe
through the wide-field capabilities of its Wide-field X-ray Telescope and the rapid, sensitive
follow-up provided by the Follow-up X-ray Telescope. In this talk, I will present the main characteristics
of the mission and its role in the discovery and characterization of X-ray transients, with
a focus on accreting compact objects. I will then discuss the synergy between Einstein Probe and
fast optical photometry, highlighting simultaneous Einstein Probe and TNG/SiFAP2 observations
of the accreting millisecond pulsar SAX J1808.4-3658 during its 2025 outburst. These data include
a thermonuclear burst observed simultaneously in X-rays and optical wavelengths, as well as coordinated
observations probing the connection between X-ray and optical pulsations across different
stages of the outburst.

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