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http://www.stsci.edu/hst/acs/documents/handbooks/current/c03_intro_acs4.html.

1. ACS Instrument Handbook for Cycle 20
... ACS Instrument Handbook . ... Advanced Camera for Surveys Instrument Handbook for Cycle 20 > Chapter 3: Introduction to ACS > 3.3 Instrument Design . ... The nonfunctioning HRC has a 1024 x 1024 SITe CCD, with 21 x 21 µm pixels that provided ~0.028 x 0.025 arcsecond/pixel spatial resolution with critical sampling at 6300 е. This gave the HRC a nominal 29 x 26 arcsecond field of view. ... The ACS design incorporates two main optical channels: one for the WFC, and one which is shared by the HRC and...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/documents/handbooks/cycle20/c03_intro_acs4.html -- 126.1 Кб -- 05.02.2013
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2. http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/HEXTE_cal_ROTHSCHILD.pdf
HEXTE Phoswich Detector 6/19/2006 Calibration Workshop, Iceland 2006 1 HEXTE Features Aperture Modulator AGC Detector "Mu Metal" Housing 6/19/2006 Calibration Workshop, Iceland 2006 Particle Monitor 2 RXTE/HEXTE Design and Calibration · Calibration begins with instrument design. ... 6/19/2006 Calibration Workshop, Iceland 2006 7 HEXTE Calibration -- Energy Resolution All of the detectors could not be taken to the synchrotron beam for detailed calibration. ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/icwg/presentations/HEXTE_cal_ROTHSCHILD.pdf -- 497.8 Кб -- 19.06.2006
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3. The Focal Plane Instruments
Next: The Transmission Gratings Up: The Instruments Previous: The Instruments . ... A conventional cross-grid charge detector reads out the photo-induced charge cloud and the electronics determine an arrival time to 16s, and the position with a resolution of about 18 m or 0.37 arcsec. ... The Massachusetts Institute of Technology's Center for Space Research, in collaboration with Lincoln Laboratories, developed the detector system and manufactured the CCDs; Lockheed-Martin integrated the instrument. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/images/chandra/crete_astro-ph/node4.html -- 4.1 Кб -- 07.12.1999
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4. CRIRES - VLT High-Resolution IR Echelle Spectrometer
... Instrument Status . Science Verification . ... CRIRES . ... SV observer shall submit their proposals using the Science Verification proposal template Proposers are asked to provide at least a short summary of the science goal, coordinates and magnitudes of GS and science target, a finding chart , the observing wavelength ID, as specified in appendix A of the UM and DIT, NDIT settings of science detectors as computed with the exposure time calculator (see below). ... with a 0.2 arcsec slit. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~rsiebenm/crires/ -- 20.5 Кб -- 10.07.2006
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5. Calibration and Performance Control for the VLT Instrumentation
Next: The ESO VLT CCD Detectors Software . ... Up: Instrument-Specific Software . ... The framework for data calibration and analysis of the VLT instrumentation is presented, based on the concepts of a calibration plan, pipeline calibration, quality control, and archiving of calibrated data for a ground-based observatory. ... Quality Control Pipeline provides quality assessment for instrument performance data and observing conditions, and tests the results of the Reduction Pipeline. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/ballesterp.html -- 9.3 Кб -- 23.06.1998
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6. Instrument Response Correction
. Next: Using a Standard Up: Echelle Spectra Previous: Flat Field Correction . љ . Using a Standard Star . Fitting the Blaze Function . Rein Warmels . Mon Jan 22 15:08:15 MET 1996
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node166.html -- 2.6 Кб -- 23.02.1996
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7. Arcad Instruments
SHORT DESCRIPTIONS OF INSTRUMENTS . ... Particle detector RIEP-2802 was developed and built in Russia. ... The combined Soviet-French ONCH-TBF onboard instrument had in memory modes the data only from several filter-banks in the range from 10 Hz to 16 kHz (while in the real-time telemetry modes, the measurements included 5-component wave-form data in the range 10 Hz - 1.5 kHz for 3 magnetic and 2 electric field components, or a wide-band mode in the range 10 Hz - 15 kHz, and several filter banks). ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/history/arcadinstr.html -- 2.8 Кб -- 31.10.1997
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/history/arcadinstr.html -- 2.8 Кб -- 31.10.1997
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8. WISPI Optical Specifications
The basic characteristics of the instrument are set by the aperture, focal length and resolution of the image forming lens, the dispersion of the spectrometer, and the sensitivity of the detector. ... The lens is internally focused, and maintains acceptable focus (2 pixels in the detector plane) over a typical spectral coverage of one grating setting. ... along the spatial dimension of a 25mm square detector in the final spectral image plane the 400mm lens is 3.2њ. ... Diffraction grating . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/wispi/wisp_specs.html -- 4.8 Кб -- 10.05.2010
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9. Optical static Fourier spectrometer
Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/~lapchuk/my_web/Spectrometer.htm -- 10.1 Кб -- 21.02.2000
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