The origin and phenomenology of the Fast Radio Burst (FRB) remains unknown despite
more than a decade of efforts. Though several models have been proposed to explain the …

We report on the lowest-frequency detection to date of three bursts from the fast radio burst
FRB 180916. J0158+ 65, observed at 328 MHz with the Sardinia Radio Telescope (SRT) …

Using kilometric arrays of air Cherenkov telescopes at short wavelengths, intensity
interferometry may increase the spatial resolution achieved in optical astronomy by an order …

With its unprecedented light-collecting area for night-sky observations, the Cherenkov
Telescope Array (CTA) holds great potential for also optical stellar astronomy, in particular …

We report the first intensity correlation measured with starlight since the historical
experiments of Hanbury Brown and Twiss. The photon bunching g (2)(τ, r= 0), obtained in …

Aims. Fast radio bursts are bright radio transients whose origins are not yet understood. The
search for a multi-wavelength counterpart of those events can set a tight constraint on the …

Stellar intensity interferometry is a technique based on the measurement of the second-
order spatial correlation of the light emitted from a star. The physical information provided by …

Light from thermal blackbody radiators such as stars exhibits photon bunching behavior at
sufficiently short timescales. However, with available detector bandwidths, this bunching …

The discovery rate of fast radio bursts (FRBs) is increasing dramatically thanks to new radio
facilities. Meanwhile, wide-field instruments such as the 47 deg 2 Zwicky Transient Facility …

We report the first detection of an optical millisecond pulsar with the fast photon counter
Aqueye+ in Asiago. This is an independent confirmation of the detection of millisecond …