On-Sky Single-photon Time resolution of 35 ps with White Rabbit synchronization: towards the measurement of the size of a White Dwarf star
astro-ph.IM, astro-ph.SR, physics.ins-det
Submitted: 2026-06-24
Updated: 2026-09-01
License: http://creativecommons.org/licenses/by/4.0/
The gist: The IC4Stars (Intensity Correlation for Stars) project aims to measure the diameter of the white dwarf star Sirius B, using Intensity Interferometry.
Terminology
Abstract
The IC4Stars (Intensity Correlation for Stars) project aims to measure the diameter of the white dwarf star Sirius B, using Intensity Interferometry. In this work we present our latest efforts and the milestones achieved in the last year. We report laboratory characterization of the single-photon detectors, TDC and synchronization electronics. We describe an observation campaign where we demonstrated on-sky time resolution below 35 ps RMS, synchronizing two TDCs using the White Rabbit protocol and a 30 m telecom fiber. We developed the data acquisition of the raw time tags, and an algorithm to compute the second-order correlation function.
Related papers
- A signal dedispersion algorithm for imaging-based transient searches
- AVICA: A fully automated CASA pipeline for large volume VLBI data calibration
- Spectral Map Making with SPHEREx
- Long-Integration Magnetar Burst Observatory (LIMBO): Instrument Summary and Early FRB Rate Constraints
- Towards independent event horizon imaging of the supermassive black holes in M87 and the Milky Way
- A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline