# Lunar occultations with Aqueye+ and Iqueye

**Authors:** L. Zampieri, A. Richichi, G. Naletto, C. Barbieri, A. Burtovoi, M., Fiori, A. Glindemann, G. Umbriaco, P. Ochner, V. V. Dyachenko, M. Barbieri

arXiv: 1908.03401 · 2019-10-16

## TL;DR

This paper demonstrates the use of Aqueye+ and Iqueye instruments for high-resolution lunar occultation observations, revealing stellar sizes and binary properties with unprecedented temporal precision and multi-filter capabilities.

## Contribution

First application of Aqueye+ and Iqueye for lunar occultations, showcasing their high time resolution and multi-filter measurement capabilities for stellar observations.

## Key findings

- Measured stellar diameters consistent with literature
- Detected unresolved stars at milliarcsecond level
- First measurement of chromosphere size for μ Psc

## Abstract

We report the first-time use of the Aqueye+ and Iqueye instruments to record lunar occultation events. High-time resolution recordings in different filters have been acquired for several occultations taken from January 2016 through January 2018 with Aqueye+ at the Copernicus telescope and Iqueye at the Galileo telescope in Asiago, Italy. Light curves with different time bins were calculated in post-processing and analyzed using a least-square model-dependent method. A total of nine occultation light curves were recorded, including one star for which we could measure for the first time the size of the chromosphere ($\mu$ Psc) and one binary star for which discrepant previous determinations existed in the literature (SAO 92922). A disappearance of Alf Tau shows an angular diameter in good agreement with literature values. The other stars were found to be unresolved, at the milliarcsecond level. We discuss the unique properties of Aqueye+ and Iqueye for this kind of observations, namely the simultaneous measurement in up to four different filters thanks to pupil splitting, and the unprecedented time resolution well exceeding the microsecond level. This latter makes Aqueye+ and Iqueye suitable to observe not just occultations by the Moon, but also much faster events such as e.g. occultations by artificial screens in low orbits. We provide an outlook of future possible observations in this context.

## Full text

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## Figures

12 figures with captions in the complete paper: https://tomesphere.com/paper/1908.03401/full.md

## References

40 references — full list in the complete paper: https://tomesphere.com/paper/1908.03401/full.md

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Source: https://tomesphere.com/paper/1908.03401