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Saturday, August 1, 2020 | History

1 edition of User"s guide to CCD detectors at the AAT found in the catalog.

User"s guide to CCD detectors at the AAT

User"s guide to CCD detectors at the AAT

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  • 33 Currently reading

Published by Anglo-Australian Observatory in Epping, NSW .
Written in English


Edition Notes

StatementR.D. Robinson ... [et al.].
SeriesAAO UM -- 17.1
ID Numbers
Open LibraryOL16162029M

A CCD (Charge Coupled Device) is a silicon based multichannel array detector of UV, visible and near-infra light. They are used for Raman spectroscopy because they are extremely sensitive to light (and thus suitable for analysis of the inherently weak Raman signal), and allow multichannel operation (which means that the entire Raman spectrum can be detected in a single acquisition). The GCH is a Sony ICX CCD megapixel (x, μm pixels, mm x mm) running at 30 Hz. The GC is a 5 Megapixels (x, μm pixels, x mm^2) running at 15 Hz. DP Prosilica CCD User Guide: Prosilica GCH Datasheet: Prosilica GCH User Manual: Prosilica GC Datasheet: Prosilica GC User Manual.

Detector and sensor spectral response and calibration from UV, Vsible to long wave infrared (LWIR) Spectral Test Station (STS) for wavelength testing and calibration from LWIR to nanometers. It is for sensor testing, process control, calibration of flight sensors. Books & magazines. The MagPi issue 25 No-problem projects: put a new Raspberry Pi to good use with these inspiring, but do-able projects. Read it now HackSpace issue 14 wild hacks for your summer projects. Read it now Wireframe issue Keep your eyes to the skies.

In nearly all cases, the detector is called a CCD, but it really should be called a solid-state detector. Most scientific spectroscopy applications use two-dimensional full-frame CCD detectors that are photosensitive across the full active surface area. In these scientific devices, the readout registers are arranged along one edge of the detector. This manual describes the ST-7E, ST-8E, ST-9E, STE and STE CCD Camera Systems from Santa Barbara Instrument Group. For users new to the field of CCD Astronomy, Sections 2, 3 and 4 offer introductory material about CCD Cameras and their applications in Astronomy. Users who are familiar with CCD cameras may wish to skip section 2 and browse.


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User"s guide to CCD detectors at the AAT Download PDF EPUB FB2

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"A User's Guide to CCD Reductions with IRAF" (Massey ) is very thorough, but IRAF has become more difficult to install over time and is no longer supported. "A User's Guide to Stellar CCD Photometry with IRAF" (Massey and Davis ).

The Handbook of Astronomical Image Processing by Richard Berry and James Burnell. This provides a very Author: Matthew Craig. The CCD detector used has pixels which are 24 × 24 micron in size.

The plate scale of the JKT is seconds of arc / mm. Thus, each pixel subtends an angle of × seconds of arc on the sky. The manual for the instrument Users guide to CCD detectors at the AAT book telescope that you are using will usually quote a value for the plate scale.

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English. Sep kB. ERM User Manual. about CCD Cameras and their applications in Astronomy. Users who are familiar with CCD cameras may wish to skip section 2 and browse through sections 3 and 4, reading any new material.

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It is intended as a “walk-through” user guide. Commissioned in (read a brief history), the Anglo-Australian Telescope was one of the last 4-metre equatorially mounted telescopes to be constructed.

Its excellent optics, exceptional mechanical stability and precision computer control make it one of the finest telescopes in the world. Also important to the AAT's success has been its suite of state-of-the-art.

The digital camera, incorporating a charge-coupled device (CCD) detector, is by far the most common image capture mechanism employed in present-day optical microscopy. Although the charge-coupled device detector functions in an equivalent role to that of film, it has a number of superior attributes for imaging in many applications.

passing through the jaws. Light from this polished surface is reflected back to a guide camera (not supplied) via a 1¼ inch (mm) adapter ring. Alternatively, it is possible to employ a webcam, video camera of a second CCD camera for automatic guiding.

Lhires III – User Guide. A CCD chip is an array of photoelectric detectors built on a silicon base using layers of electrical components, called the architecture, printed on the surface.

This structure divides the base into a grid of separate compartments, called pixels, that hold electrical charges. A pixel is described by its size and the number of electrons it can hold. SMART CCD Detector Collect the diffraction patterns Now the sample can be mounted in a capillary Collect rotation frame(s) at appropriate swing angle of the SMART detector (like on the calibration powder) Save (and unwarp) this rotation frames Note: Of course the calibration file for a particular detector distance might also be collected after.

The Mar has a mm diameter detector head containing a 61 mm x 61 mm CCD sensor with 80 micron pixels at the phosphor and a frame rate ~ Detector Pool has three units available for loan. DP Mar User Guide: MarCCD Software Manual: Notes on Frame Shift: Mar Pump Down Procedure: EPICS areaDetector driver: Rayonix.Users who are familiar with CCD cameras may wish to skip section 2 and browse through sections 3 and 4, reading any new material.

Thoroughly experienced SBIG customers may wish to jump right to the separate Software Manual, which gives detailed and specific information about the SBIG software.CCD Camera Systems from Santa Barbara Instrument Group. This Section contains a one page Quick Start Guide followed by detailed instructions on handling, connecting and maintaining the camera.

For users new to the field of CCD Astronomy, Sections 2, 3 and 4 offer introductory material about CCD Cameras and their applications in Astronomy.