... Welcome to the ADLab home page! Advanced Design Laboratory of the Special Astrophysical Observatory is concerned with research on low light level imaging and development of scientific digital imaging systems. About ADLab . ... Current project "A New Generation Multipurpose CCD Controller" . Project Contents . ... Publications on the Project . ... Other Web Sites of Interest . Created: 24 March 1998 . ... people have visited our web site. ... Copyright 1998 Advanced Design Laboratory. ...

Section I: Introduction to ALFA and GALFA . Section II: System Description . ... ALFA receives 7 beams, 2 polarizations per beam, each covering 1225-1525 MHz. The 14 IF signals cover nominally the 100 to 400 MHz band. ... A high-resolution, low-bandwidth spectrometer (8K channels covering a 7 MHz bandwidth) . ... Each spectrometer board handles two polarizations from one telescope beam.The baseband signals are to be digitized by four 8-bit ADCs at 100 Msamples/sec. ... Bandwidth: . ...

Semiconductor Home > Products > Mixed Signal and Analog > CCD IMAGERS Family > . TC236P, 680- X 500-PIXEL CCD IMAGE SENSOR . Device Status: Obsolete . ... The TC236P is a frame-transfer, charge-coupled device (CCD) image sensor designed for use in single-chip color NTSC TV, computer, and special-purpose applications requiring low cost and small size. ... One important feature of the TC236P very high-resolution sensor is the ablity to capture a full 340,000 pixels per field. ... TC236P . ...

... This tool is designed to create formatted and unformatted file-by-file reports from fits headers, or fits files. fitsreport reads from a configuration file all the keys to be displayed: . ... retrieve non-FITS information (file name, path name). ... The tool reads all fits files in the given path, evaluates the configuration file fitsreport_raw.cfg (to be in ${DFO_CONFIG_DIR}) and dumps the output into out. ... This is more evident in the other config file, fitsreport_raw.cfg. ...

... GSAOI Home . Instrument . ... The Gemini South Adaptive Optics Imager (GSAOI) is a near-infrared adaptive optics camera that will be used with the Multi-Conjugate Adaptive Optics (MCAO) system on the Gemini South 8-m telescope . ... Gemini's major instrumentation goal is to develop its Multi-Conjugate Adaptive Optics (MCAO) system for scientific use on Gemini South. ... Existing adaptive optics systems use a single natural guide star or artifical laser guide star to measure this image blur. ...

The optical scheme of the instrument is sketched in Figure 1 , it is designed to match the F/20 focal ratio of the TIRGO telescope. We have, following the optical path, the window of the dewar, the order sorting filter (not in figure), a field lens, in Calcium Floride, and the slit, in the focal plane of the telescope. ... The resolving power is (for first order of grating) of about 600 in the center of J band and 950 in the center of the K band, using a slit of two pixel (3.46 arcsec). ...

OptInt PmWiki . ... Design Documentation . ... Page History | ... Software Design Documentation . ... Design Documents . ... Restore . ... Trolley Software Functional Description [EBS] . Workstation Software Functional Description [JSY] . ... Trolley Software Functional Description: INT-406-VEN-0102 [EBS] . ... July 06, 2007, at 02:52 AM by EBS - Added draft trolley software functional description . ... Software Functional Description (workstation, VME, trolley, and shear camera) [EBS/JSY/RCB] . ...

... The motivation for this task is to create one high resolution response matrix for a set of observations without the need for creating individual high resolution matrices. ... This task creates a single response matrix file using information from a list of spectrum from multiple observations, and can also combine spectra and background spectra of the same instrument and spectral order to produce final files that can be used for futher, quantitative analysis in a fitting package such as Xspec. ...

Welcome to VDP home page. ... Operation and Measurements The VDP instrument was designed for determination of integral flux vector or integral energetic spectrum at the range 0.2 - 2.4 keV of ions or electrons of magnetospheric plasma. The instrument includes 6 identical Faraday caps, located by following ways: . ... In case of constant voltage, sensor supplies the total flux of ions plus flux of electrons above 2400 eV energy, or total flux of electrons plus flux of ions above 2400 eV energy. ...