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Supplier: Excelitas Technologies Corp.
Description: : 400-1060 nm, peak @ 650 nm Dark counts specified @ less than 500 cps Digitized TTL output, 4 seperate detection channels Temperatur controlled, TE-cooled operation Light measurement up to 25 Mcps before saturation Applications Particle Sizing / Photon-Correlation-Spectroscopy
- Photosensor Type: Avalanche Photodiode
- Output Type: Photon Counting
- Cooled: Yes
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Supplier: Excelitas Technologies Corp.
Description: Applications Particle Sizing / Photon-Correlation-Spectroscopy Confocal Microscopy Adaptive optics and astronomical observations Optical range finding, LIDAR Ultra-sensitive fluorescence
- Photosensor Type: Avalanche Photodiode
- Output Type: Photon Counting
- Cooled: Yes
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Supplier: Excelitas Technologies Corp.
Description: before saturation Applications Particle Sizing / Photon-Correlation-Spectroscopy Confocal Microscopy Adaptive optics and astronomical observations Optical range finding, LIDAR Ultra-sensitive fluorescence
- Photosensor Type: Avalanche Photodiode
- Output Type: Photon Counting
- Cooled: Yes
-
Supplier: Excelitas Technologies Corp.
Description: before saturation Applications Particle Sizing / Photon-Correlation-Spectroscopy Confocal Microscopy Adaptive optics and astronomical observations Optical range finding, LIDAR Ultra-sensitive fluorescence
- Photosensor Type: Avalanche Photodiode
- Output Type: Photon Counting
- Cooled: Yes
-
Supplier: Excelitas Technologies Corp.
Description: before saturation Applications Particle Sizing / Photon-Correlation-Spectroscopy Confocal Microscopy Adaptive optics and astronomical observations Optical range finding, LIDAR Ultra-sensitive fluorescence
- Photosensor Type: Avalanche Photodiode
- Output Type: Photon Counting
- Cooled: Yes
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The PRIMA fringe sensor unit
. BibSonomy. CiteUlike. Connotea. Del.icio.us. Digg. Facebook. Mendeley. Twitter. EDPS account. Latest articles FREE. Email-alert. Free access article. Issue. A&A. Volume 507, Number 3, December I 2009. Page(s). 1739 - 1757. Section. Astronomical instrumentation. DOI
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Helping the S.A.L.T. Telescope See Further into the Cosmos
that comes from. infrared can be used to characterize the final stages of. astronomical objects. Although infrared imagers. dying massive stars as they generate powerful winds. have been in use on telescopes for quite some time,. by expelling their outer layers and finally explode as. spectrographs
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Case Study: TONiCTM incremental encoders have star potential for Astrosysteme Austria
, drives that use similar tracking capability to professional observatories. This has been made possible by employing high-resolution Renishaw encoders installed directly on the axes of the mount. Previously, even the finest astronomical mounts relying solely on mechanics couldn't solve the problems
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SmartMovesTM Spotlights: University of California Observatories (.pdf)
Astronomers -- continued. for moving an iodine cell into a beam, opening a light port,. According to a UCO data report, the beginnings of. moving a mirror into a beam and opening a mirror cover. 8- to 10-meter astronomical telescope development began at. The logic control provided by the RIO ensured
Engineering Web Search: Astronomical Spectroscopy Top
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Astronomical spectroscopy - Wikipedia, the free encyclopedia
Astronomical spectroscopy From Wikipedia, the free encyclopedia Astronomical spectroscopy is the technique of spectroscopy used in astronomy.
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Raman spectroscopy - Wikipedia, the free encyclopedia
Raman spectroscopy From Wikipedia, the free encyclopedia
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ESA Science & Technology: Astronomical Spectroscopy and...
Astronomical Spectroscopy and Virtual Observatory Workshop
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ESA Science & Technology: Workshop and spectroscopy school<br>...
this in mind we invite those in the astronomical community with an interest in high resolution X-ray spectroscopy to get together again at MSSL, in a
- GOODS: The Great Observatories Origins Deep Survey
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Home - spectroscopyNOW.com
Advances in Raman spectroscopy have led to unprecedented performance for an exhaustive list of application areas.
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Home | UW-Madison Astronomy
The Washburn Astronomical Laboratories is a new organization within the department dedicated to the development and implementation of astronomical
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Atomic Data Needs for X-ray Astronomy: Proceedings
us are those parameters needed for analysis and modeling of spectra shortward of ~ 100 Å and relevant to ionic species of astronomical interest.
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WhatIsSpectroscopy < Public < IRS
The Wikipedia's entry on astronomical spectroscopy McGraw Hill's AccessScience collection on astronomical spectroscopy
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Spectroscopy
Images Astronomical Wallpapers Discovery Spectroscopy: Unlocking the Secret in Starlight
