Related Experiment Video
Updated: Jun 14, 2026

High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis
Published on: December 22, 2015
Intensifier silicon vidicon spectrophotometer for line profile studies in astronomy
This study details a new spectrophotometer for astronomy, achieving high spectral resolution for observing stellar line profiles. The instrument demonstrates efficient performance with a silicon vidicon detector and a 60-cm telescope.
Area of Science:
- Astronomy
- Astrophysics
- Instrumentation
Background:
- Spectrophotometry is crucial for analyzing celestial objects.
- Previous instruments had limitations in resolution and sensitivity.
Purpose of the Study:
- To design and characterize a moderate dispersion spectrophotometer for astronomical observations.
- To evaluate and optimize the performance of an intensifier silicon vidicon detector.
Main Methods:
- Developed a spectrophotometer with a dispersion of approximately 0.1 nm.
- Utilized an intensifier silicon vidicon as the detector.
- Optimized detector operating characteristics for astronomical use.
Main Results:
- Achieved a spectral resolution of 0.15 nm.
- Recorded stellar line profiles with a signal-to-noise ratio (SNR) of 50.
- Demonstrated capability for stars of magnitude 3.74 with 10-second integration using a 60-cm telescope.
Conclusions:
- The developed spectrophotometer offers efficient and high-resolution astronomical observation capabilities.
- The optimized silicon vidicon detector enhances performance for stellar spectroscopy.
- The instrument is suitable for detailed analysis of stellar spectra.
More Related Videos
10:03Proton Transfer and Protein Conformation Dynamics in Photosensitive Proteins by Time-resolved Step-scan Fourier-transform Infrared Spectroscopy
Published on: June 27, 2014
09:53Molecular Beam Mass Spectrometry With Tunable Vacuum Ultraviolet (VUV) Synchrotron Radiation
Published on: October 30, 2012
Related Concept Videos
UV–Vis Spectrometers
IR Spectrometers
Spectrophotometry: Introduction
The essential components of a spectrophotometer include a source of electromagnetic radiation, a slot for placing a material to be analyzed, and a...
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
UV–Vis Spectroscopy: Beer–Lambert Law
Raman Spectroscopy Instrumentation: Overview
The monochromatic laser source, typically using visible or near-infrared radiation, generates a highly focused beam of light. This light interacts with the molecules of the sample, scattering some of the light. Liquid and gaseous samples are usually tested in ordinary glass capillaries, while solids can be analyzed as powders packed in capillaries or as potassium...