XMM-Newton Science Analysis System . ... This task is designed to select those EPIC sources (from the unified list created by the task srcmatch ) for which spectra and time series (or other source-specific products) are to be extracted in the pipeline. Two other subsidiary functions are performed: (i) widths for the bins of the time series are calculated; (ii) a single pair of start and stop times for all time series is calculated. ... Time bin widths . ... Start and stop times . ...

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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: . ...

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... 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. ...

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• COALA - Tiago Pereira
• COALA - Wolfgang Kerzendor

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). ...

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• Lunar Orbiter 4
• Lunar Orbiter 1
• Lunar Orbiter 5

This page is a mirror of the ION SADS page available at http://sads.cnes.fr:8010 . Besides the information already available on this page, there you can browse the ION QuickLook images. ... The ION experiment flown on the Interball-Aurora mission performs simultaneous ion and electron measurements. Two mass spectrometers looking in opposing directions perpendicular to the satellite spin axis, which points toward the sun, measure ions in the mass and energy ranges 1-32 amu and ~ 0 to 14,000 eV. ...

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• Mars96

OptInt PmWiki . MROI Delay Line SW / . Preliminary Design Review . ... Page History | ... MROI Delay Line Design Contract . ... MROI DL Production SW Contract . ... Software Design Documentation . ... Return to Preliminary Design Review ( Edit ) . ... The Preliminary Design Review for the Production Software Contract will take place at 8.30am MST (3.30pm GMT) on 1 February 2010. ... The Preliminary Design Review for the Production Software Contract will take place around 1 February 2010. ...

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• OptInt PmWiki : Design Documentation | History
• OptInt PmWiki : MROIDelayLineSW / Preliminary Design Review
• OptInt PmWiki : MROIDelayLineSW / Design Documentation

PROS is a multi-mission x-ray analysis software system designed to run under the Image Reduction and Analysis Facility (IRAF). The analysis of x-ray data differs from that of other wavelengths due to the nature of x-ray data. ... Programs in PROS are called tasks. Tasks are grouped by function into packages. ... The qpspec task allows users to extract a background corrected spectrum from a QPOE file for use in PROS or for export to other analysis systems. model specification and fitting . ...

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• IRAF/PROS
• PINTofALE
• Analysis Routines in SAOtng

... Status of the ELECTRON experiment . ... The objective of the ELECTRON experiment is to perform 3-D measurements of the plasma electrons in the energy range from 10 eV to 26000 eV, with good angular resolution, sensitivity and large dynamical range. ... Figure 1 presents the ELECTRON sensor. ... Click on the picture to view large one) . ... Figure 3 shows dynamical spectra with counting rate measurements performed by ELECTRON experiment during very multiple magnetopause crossings on February, 4, 1996...

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• OMNIDIRECTIONAL PLASMA SENSOR VDP
• Lunar Orbiter 4
• Lunar Orbiter 1

Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

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• A Graphical User Interface for a Development Environment (GUIDE)
• Implementation Design of the ASC Data Model
• System Interfaces to the STIS Calibration Pipeline

... Space flight . ... The L-39 two-seat training jet plane is intended for flights in regular and complex meteorological conditions at day and night time, as well as for acrobatic flying. ... A cockpit canopy is pressure-tight with a single layer glazing, the back-folding parts can be thrown off under abnormal condition by pyrotechnical systems. ... Comparable on size and assigned tasks with the American F-16 and F/A-18 fighters, the MIG - 29 is presently in the service of 23 countries of the world. ...

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... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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Top] [Prev] [Next] [Bottom] . Pipeline Processing / 16-1 . NICMOS Calibration Software / 16-2 . Basic Data Reduction: calnica / 16-3 . ... Grism Data Reduction: Calnicc / 16-16 . ... This chapter is designed to help you understand what steps are performed on your data in the routine pipeline process and to help you decide whether you should recalibrate your data with different reference files. ... Provide flowcharts and descriptions of the NICMOS pipeline calibration steps. ...

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• Resume for Robert E. Douglas, Jr.
• Software / Hardware
• STIS Instrument Design

... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• проект SCORPIO-2
• NES NES
• Advanced Design Laboratory Home Page

The Parkes 21cm Multibeam Receiver is a new facility available on the Parkes Telescope which is operated by the Australia Telescope National Facility (ATNF), CSIRO. The facility consists of a 13-beam cooled 21cm receiver system, located at the prime focus of the 64m dish. ... Completed 21cm Multibeam Receiver being hoisted up to the Parkes focus cabin. ... It is now available, in 64 MHz mode and in pulsar mode, for normal National Facility use. ... Beam 1 . Beams 2-7 . ... Frequency Range . ...

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• Channel Selection, Averaging and Doppler Correction - UV Linetypes
• The Parkes 21cm Multibeam Project
• ASKAP News: Initial system tests performed on Mk II PAF | Australia Telescope

Next: Order Definition Up: Echelle Reduction Method Previous: Retrieving demonstration and . ... That is the mapping between the space wavelength, spectral order and the space sample x , line y in the raw image. ... Sections and describe the solution of this mapping. The second step in the reduction, described in Section , is to estimate the image background. ... In the rest of this Section the algorithms used in each step of the reduction are described. ...

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• HwB: ECP Parallel (Tech) Connector
• Product Folder(Obsolete): TC244A, 786- X 488-PIXEL CCD IMAGE SENSOR
• Product Folder: TC245, 786- X 488-PIXEL CCD IMAGE SENSOR

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

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• XV-GEOREF

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . ... The software run under Windows 95, 98 NT, including Paraxial and Seidel . ... and Energy Distribution, Optical Layout, Optimization, Tolerancing etc. ... Listed Since August 20, 2005 . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• OSLO LT V5.4 Optical Software For Layout And Optimization - an Astronomy Net

... News . ... Pre-university education . ... Samara region . SSAU History . SSAU roadmap . ... Scientists of Samara University (joined SSAU and of SSU) have designed new materials for accumulator batteries, that will allow us to refuse from the use of a relatively scarce and expensive lithium in favour of a more widespread and cheap metals. ... Calculations of properties for the future substances are made with the use of a software system ToposPro, developed by the scientists of ICTMS. ...

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• The complex 'Shtil-M' No. designed in SSAU began data transmission from the

Decomposition of Galaxy Images and Galaxy Rotation Curves Mosenkov A.V.*^, Savchenko S.S.*, Sotnikova N.Ya.* ... The DECA (DEComposition Analysis) code is designed to investigate images of galaxies in an automatic regime (using the simple 'bulge+disc' model) as well as in manual mode for more detailed images and/or for multicomponent structures. ... The GRCF package was created for performing the galaxies rotation curve decomposition using the models of the bulge, the disc, and the dark halo. ...

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. Russion version . Last updated on May, 2008 . RadioAstron Mission .

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• RadioAstron main page, english version