7–9 May 2025
Area Territoriale di Ricerca di Bologna
Europe/Rome timezone

Looking for a multi-wavelength counterpart for FRBs

Not scheduled
30m
Aula 216 (Area Territoriale di Ricerca di Bologna)

Aula 216

Area Territoriale di Ricerca di Bologna

Via Piero Gobetti 101 40129 Bologna

Speaker

Maura Pilia (Istituto Nazionale di Astrofisica (INAF))

Description

Emission outside the radio band is predicted for most models trying to explain the FRB phenomenon. Its nature, however, is still to be determined, with the exception of the possible example provided by the Galactic FRB20200428A, where X-ray emission was observed simultaneously with the radio emission, with an energy ratio E_X/E_radio = 10^5.
I will review the targeted attempts to search for the multi-wavelength counterpart of FRBs and I will highlight the results of four years of multi-wavelength campaigns targeting FRB20180916B in optical, X- and gamma-rays, simultaneously with high sensitivity radio observations. Through this campaign the deepest prompt upper limits were obtained in optical and X-rays in terms of E_MWL/E_radio.
I will discuss the challenges of such large scale campaigns and the physical implications of our findings.

Primary author

Maura Pilia (Istituto Nazionale di Astrofisica (INAF))

Presentation materials

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