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Related Concept Videos

UV–Vis Spectrometers01:14

UV–Vis Spectrometers

The absorbance of UV and visible (UV–visible) radiations is measured using a UV–visible spectrophotometer. Deuterium lamps, which emit UV radiation, and tungsten lamps, which produce radiation in the visible region, are used as light sources in UV–visible spectrophotometers. A monochromator or prism is used for diffraction grating, i.e., to split the incoming radiation into different wavelengths. A system of slits is used to focus the desired wavelength on the sample cell. Samples for...
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview01:02

Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview

Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material,  molecules absorb light depending on the energy required for electronic transitions. As a result...

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Multimodal Optical Imaging Platform for Studying Cellular Metabolism
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URSULA: a twin-beam multiband computer-controlled photometer for astronomical applications.

G A De Biase, L Paternò, M Pucillo

    Applied Optics
    |February 23, 2010
    PubMed
    Summary

    A new twin-beam multiband photoelectric photometer was developed for ground-based astronomical observations. This computer-integrated instrument enhances flexibility, efficiency, and signal-to-noise ratio (SNR) for precise photometry.

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    Area of Science:

    • Astronomy
    • Astrophysics
    • Instrumentation

    Background:

    • Ground-based astronomical observations require precise photometric measurements.
    • Atmospheric transmittance variations and signal-to-noise ratio (SNR) are key challenges in photometry.

    Purpose of the Study:

    • To describe the construction and capabilities of a novel twin-beam multiband photoelectric photometer.
    • To detail the design philosophy, structure, and potential extensions of the instrument.
    • To analyze the system's dynamic behavior and precision constraints.

    Main Methods:

    • Construction of a twin-beam multiband photoelectric photometer.
    • Integration with a computer for enhanced flexibility and efficiency.
    • Utilization of photon-counting techniques to optimize SNR.
    • Minimization of atmospheric transmittance variations through structural design.

    Main Results:

    • The developed photometer demonstrates superior flexibility, reliability, and simplicity compared to existing instruments.
    • Successful testing of the system's dynamic behavior confirmed its operational stability.
    • The instrument is optimized for high-precision astronomical photoelectric photometry.

    Conclusions:

    • The new photometer offers significant advancements for ground-based astronomical observations.
    • Four units have been successfully constructed and deployed to major Italian observatories.
    • The design facilitates efficient and reliable photometric data acquisition.