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Показаны документы, содержащие фрагменты текста из документа
http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_4.html.

1. WFC3 Instrument Handbook
WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Chapter 3: Choosing the Optimum HST Instrument > 3.3 Comparison of WFC3 with Other HST Imaging Instruments . ... 3.3.2 Field of View . ... Figure 3.1 illustrates the fields of view, at the same scale, for all of the HST imaging instruments currently available on HST . Figure 3.1: Schematic diagram comparing relative sizes of the fields of view for all available HST imaging instruments. ... WFC3/IR . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/hst/wfc3/documents/handbooks/currentIHB/c03_optimum_instr4.html -- 24.0 Кб -- 12.04.2016
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2. IBIS: Technical Description
The following papers summarize the characterization and technical performance of IBIS : . ... Characterization of Fabry-Perot interferometers and multi-etalon transmission profiles. ... Righini, A., Cavallini, F., Reardon, K. P., 2010, Astronomy and Astrophysics , 515 , A85, . ... The filter wheel is located between the two interferometers. ... The interferometers can be rapidly tuned, simultaneously, so to allow sequential scanning of the spectral lines of interest (see movie in IBIS Intro ). ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/solar/IBIS/IBIS_description.html -- 33.6 Кб -- 13.12.2015
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3. Sample instrument files
. Next: A simple photometer Up: Instrument configuration and Previous: Telescope optics . љ Because the instrumental table file is rather complicated, and has a variable structure that depends on the nature of the instrument, here are some examples. A simple photometer . A modern single-channel photometer . A modern two-channel photometer . CCD photometry . Rein Warmels . Mon Jan 22 15:08:15 MET 1996
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node629.html -- 2.9 Кб -- 23.02.1996
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4. Spectral Analysis
... The x-ray spectral analysis consists of a comparison between the observed pulse height spectrum and a pulse height spectrum calculated using a given spectral model. ... To obtain the spectral parameters for an x-ray source, several steps need to be followed. For each source: . ... obtain the best fit parameters for a spectral model - repeated for each model of interest . obtain a 1-D or 2-D grid of values around the best fit values - this can be done for as many models as desired . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node135.html -- 7.8 Кб -- 01.10.2012
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Еще в разделе: (Показать все результаты (>3616) - hea-www.harvard.edu/ )

5. Meade Instruments - Telescopes, Solar Telescopes, Binoculars, Spotting Scopes
STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado€о Solar . ... Spotting Scopes . ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/ -- 73.9 Кб -- 09.04.2016
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6. East Siberian Center for the Earth's Ionosphere Research. Instruments engineer
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The instruments engineer and technical support subdivision consists of the engineer support group: 4 senior engineers, 5 engineers and 14 staff members of service personnel. Head: Zavorin A. V. The main subdivision's instrument is the Incoherent Scatter Radar . The instruments engineer and technical support subdivision's main task is technical support of Irkutsk IS radar experiments. ...
[ Сохраненная копия ]  Ссылки http://rp.iszf.irk.ru/esceir/isr/engdepen.htm -- 3.4 Кб -- 04.06.2001
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7. News Results
This source is hiding behind our Galaxy at a distance of ~18 Mpc, located at a galactic latitide of 0 degrees. ... As we look towards longer wavelengths, 60 micron, to try and penetrate the Galactic Plane, we still see confusion from galactic sources. ... If the image seems some what confusing that is because the MOST is a continuum radio telescope and when it looks in the direction of our Galaxy it detects radiation from sources within our Galaxy and from sources that may lie behind our Galaxy. ...