Concept


Progress in astronomy and astrophysics is driven by the development of technology. Paradigm shifts in how we construct our instruments almost always usher in a flood of discoveries altering our understanding of the Universe. The VLTI/GRAVITY instrument is one of the latest demonstrations of this process, providing astronomers with unprecedented high-angular resolution measurements of stars, some exoplanets, and the environment around Sagittarius A* at the galactic centre (which contributed to the recent Nobel Prize). What is perhaps less well known is that at the core of GRAVITY beats a photonic heart. The primary beam-combination and interferometry is not done using classical bulk-optics, but rather inside a specially-made integrated photonic circuit. Over the last decade, the use of photonic technologies in astronomy – from simple optical fibres to advanced integrated circuits – has grown immensely. In fact, French astronomers and instrumentation scientists played an early pioneering role in developing and deploying these technologies, paving the road for incredible discoveries. Today, groups across France are developing revolutionary new devices and instrumentation using photonic technologies for a diverse set of astronomical fields, such as spectroscopy, high-contrast imaging, interferometry, and gravitational wave science. Further, with the tremendous growth of commercial photonic foundries across the EU, and additional photonic design companies acting as middle-men between researchers and manufacturers, making novel state-of-the-art photonic devices for astronomy has never been easier (or cheaper). The aim of this workshop is to showcase to the whole astrophysical community the most recent and exciting developments in the field of astrophotonics, and how it will impact the next generation of instrumentation. Further, this workshop aims to re-solidify the interdisciplinary links between different groups working in this field as well as “photonics-adjacent” work in material science, wavefront control, and advanced detectors for astronomy.