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Multiwavelength observations of fast radio bursts
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 …
more than a decade of efforts. Though several models have been proposed to explain the …
The lowest-frequency fast radio bursts: Sardinia radio telescope detection of the periodic FRB 180916 at 328 MHz
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) …
FRB 180916. J0158+ 65, observed at 328 MHz with the Sardinia Radio Telescope (SRT) …
Stellar intensity interferometry: Prospects for sub-milliarcsecond optical imaging
Using kilometric arrays of air Cherenkov telescopes at short wavelengths, intensity
interferometry may increase the spatial resolution achieved in optical astronomy by an order …
interferometry may increase the spatial resolution achieved in optical astronomy by an order …
[HTML][HTML] Optical intensity interferometry with the Cherenkov Telescope Array
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 …
Telescope Array (CTA) holds great potential for also optical stellar astronomy, in particular …
Temporal intensity interferometry: photon bunching in three bright stars
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 …
experiments of Hanbury Brown and Twiss. The photon bunching g (2)(τ, r= 0), obtained in …
Stellar intensity interferometry of Vega in photon counting mode
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 …
order spatial correlation of the light emitted from a star. The physical information provided by …
Measuring temporal photon bunching in blackbody radiation
Light from thermal blackbody radiators such as stars exhibits photon bunching behavior at
sufficiently short timescales. However, with available detector bandwidths, this bunching …
sufficiently short timescales. However, with available detector bandwidths, this bunching …
Simultaneous and panchromatic observations of the fast radio burst FRB 20180916B
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 …
search for a multi-wavelength counterpart of those events can set a tight constraint on the …
Zwicky Transient Facility constraints on the optical emission from the nearby repeating FRB 180916. J0158+ 65
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 …
facilities. Meanwhile, wide-field instruments such as the 47 deg 2 Zwicky Transient Facility …
Precise optical timing of PSR J1023+ 0038, the first millisecond pulsar detected with Aqueye+ in Asiago
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 …
Aqueye+ in Asiago. This is an independent confirmation of the detection of millisecond …