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Implementation of a Reference Interferometer for Nanodetection
Published on: April 26, 2014
Accurate measurement of interferometer group delay using field-compensated scanning white light interferometer
1University of Florida, Department of Astronomy, 211 Bryant Space Science Center, Gainesville, Florida 32611, USA. xwan@astro.ufl.edu
Applied Optics
|October 12, 2010
Summary
A new field-compensated white light scanning Michelson interferometer calibrates group delay for precise radial velocity (RV) astronomy. This tool achieves high accuracy, enabling more sensitive exoplanet detection through improved astronomical measurements.
Area of Science:
- Optics and Photonics
- Astronomy and Astrophysics
Background:
- Accurate calibration of group delay in interferometers is crucial for high-precision radial velocity (RV) measurements in astronomy.
- Existing methods face challenges with low spatial coherence light sources and require frequent recalibration.
Purpose of the Study:
- To introduce a novel field-compensated white light scanning Michelson interferometer for accurate interferometer calibration.
- To enable precise group delay measurements essential for advanced astronomical observations.
Main Methods:
- Utilized a field-compensated Michelson interferometer with a translating compensation prism for optical path difference (OPD) scanning.
- Employed a multimode fiber-coupled LED (500-560 nm) as a low spatial coherence light source, ensuring phase coherence over large scanning ranges.
- Implemented dual-laser wavelength references and an iodine absorption spectrum for achromatic OPD scanning calibration and cross-verification.
Main Results:
- Achieved high optical efficiency for improved interferogram signal-to-noise ratio.
- Determined group delay with an accuracy of 1×10⁻⁵.
- Attained phase angle precision typically of 2.5×10⁻⁶ over a wide wavelength range.
Conclusions:
- The novel interferometer provides a robust and accurate calibration tool for RV experiments.
- The developed methods ensure reliable and precise group delay measurements, advancing astronomical observation capabilities.

