Séminaire de l'INPHYNI: Sarah Tolila --- Varvara Iachkula

  • Science et Société
Publié le 4 mai 2026 – Mis à jour le 4 mai 2026
Date(s)

le 5 mai 2026

Café : 15h
Séminaire: 15h15
Lieu(x)
Salle des séminaires

Improvement of signal to noise ratio, laboratory and on-sky testing of new detectors for intensity interferometry--- TBA

Seminars of the Institut de Physique de Nice (PhD series)


Improvement of signal to noise ratio, laboratory and on-sky testing of new detectors for intensity interferometry (Sarah Tolila)

Abstract:
Interferometry in astronomy enables extremely high angular resolution by combining light from multiple telescopes. While amplitude interferometry measures both phase and amplitude, it requires strict optical stability. In contrast, intensity interferometry relies on correlations of intensity fluctuations and is more robust to atmospheric and optical imperfections. Although widely used in the mid-20th century, it was abandoned due to lower sensitivity. Recent advances in photonics, detectors, and electronics have revived interest in this technique. The IC4Stars project has made significant progress, including detector characterization and on-sky experiments at Calern. Early results are promising, and a three-telescope campaign targeting Gamma Peg is planned.

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TBA (V. Iachkula)

Abstract: TBA

TBA