TL;DR
GRIP is an open-source data reduction toolkit that enhances null self-calibration for nulling interferometry, improving sensitivity and consistency across different instruments for exoplanet and circumstellar dust observations.
Contribution
It introduces the first unified, open-source software framework for nulling data reduction with advanced statistical calibration methods.
Findings
Achieves nulling precision down to a few 10$^{-4}$
Demonstrates consistency with existing datasets from GLINT and LBTI
Provides a versatile tool for long-term data analysis
Abstract
Nulling interferometry is a powerful observing technique to study exoplanets and circumstellar dust at separations too small for direct imaging with single-dish telescopes. With recent photonics developments and the near-future ground-based instrumental projects, it bears the potential to detect young giant planets near the snow lines of their host stars. The observable quantity of a nulling interferometer is called the null depth, its precise measurement and calibration remain challenging against instrument and atmospheric noise. Null self-calibration is a method aiming to model the statistical distribution of the nulled signal. It has proven to be more sensitive and accurate than average-based data reduction methods in nulling interferometry. The variety of existing and upcoming of nullers raises the issue of consistency of the calibration process, structure of the data and the…
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