On-sky demonstration of an ultra-fast intensity interferometry instrument utilizing hybrid single photon counting detectors

TL;DR

This paper demonstrates an ultra-fast intensity interferometry instrument using hybrid single photon detectors on a 1-meter telescope, achieving high temporal resolution and stable measurements of stellar photon coherence.

Contribution

It introduces a novel, upgradeable intensity interferometry instrument with hybrid photon detectors, enabling high-resolution astronomical observations at visible wavelengths.

Findings

Successful measurement of photon bunching in bright stars

Achieved stable coupling of star light to detectors

Matched observed coherence times with theoretical expectations

Abstract

Intensity interferometry is a reemerging astronomical technique for performing high angular resolution studies at visible wavelengths, benefiting immensely from the recent improvements in (single) photon detection instrumentation. We developed an ultra-fast, single photon counting and highly stable intensity interferometry instrument for 1 m class optical telescopes. The instrument records on sky the expected stellar photon rates and reaches the temporal coherence times as measured in the laboratory. In addition, all components, especially the photon detection hardware, of the instrument are easily upgradeable with custom hardware currently being developed. The collimated telescope output is spectrally filtered via an ultra narrow band pass of 2 nm at a central wavelength of 405 nm. We use hybrid photon detectors (HPDs) for single photon detection and a constant fraction discriminator (CFD) for signal conditioning. A time to digital converter (TDC) is used for time stamping. The combination of HPDs and CFDs is optimized for large active area and high timing resolution. We successfully measured photon bunching of three bright A-type stars - Vega, Altair and Deneb at the 1.04 m Omicron telescope of C2PU at the Calern Observatory in the south of France. In all cases the observed coherence time fits well to both the pre-calculated expectations as well as the values measured in preceding laboratory tests. We obtained the previously estimated photon count rates at the telescope and achieved highly stable coupling of the star light to the detectors. Utilizing a new class of large area single photon detectors based on multichannel plate amplification, high resolution spatial intensity interferometry experiments are within reach at 1 m diameter class telescopes within one night of observation time for bright stars.