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Updated: Jun 16, 2026

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Fabrication of a Low-Cost, Fiber-Coupled, and Air-Spaced Fabry-Pérot Etalon
Published on: February 3, 2023
Pressure-Scanned Echelle Grating plus Fabry-Perot Stellar Spectrophotometer
Applied Optics
|February 2, 2010
Summary
A new photoelectric stellar spectrophotometer offers 0.3-A resolution near H-alpha. This instrument utilizes a pressure-scanned Fabry-Perot etalon and echelle grating for convenient radial velocity measurements.
Area of Science:
- Astrophysics
- Stellar Spectroscopy
- Instrumentation
Background:
- Accurate stellar spectrophotometry is crucial for understanding stellar properties.
- High-resolution measurements near the H-alpha emission line provide key diagnostic information.
- Existing instruments may have limitations in resolution or ease of use for radial velocity studies.
Purpose of the Study:
- To describe a novel photoelectric stellar spectrophotometer.
- To detail its capabilities for high-resolution spectral analysis near H-alpha.
- To highlight its utility for convenient radial velocity measurements.
Main Methods:
- Development of a photoelectric stellar spectrophotometer with 0.3-Angstrom resolution.
- Integration of a Fabry-Perot etalon and an echelle grating.
- Simultaneous pressure-scanning of both optical components for spectral analysis.
Main Results:
- The instrument achieves high spectral resolution (0.3 A) near the H-alpha line (6563 A).
- A dual-component system (Fabry-Perot etalon and echelle grating) is employed.
- The system allows for convenient radial velocity corrections via pressure scanning.
Conclusions:
- The described spectrophotometer is a capable tool for high-resolution stellar spectroscopy.
- Its design facilitates efficient radial velocity determination.
- The instrument enhances observational capabilities for studies focusing on the H-alpha region.
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