You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• The Face on Mars
• Copyright Information
• Processing the "Face on Mars" Images

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

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. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• The Galaxy Gallery: Messier Objects
• Low Surface Brightness Galaxy Gallery
• Fabry-Perot Images of Spiral Galaxies

... The software was originally developed as a set of Fortran routines which were available both as stand-alone executables and as IRAF tasks in the Dither package. ... This set of code formed the basis for a more automated task for aligning images to produce distortion-corrected images; namely, the Python task PyDrizzle (Section 5.3) . Finally, all the steps required to identify cosmic rays using the aligned images produced by PyDrizzle were automated in the Python task MultiDrizzle (Section 5.4) . ...

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• WFC3 Data Handbook
• HDF-S Filename Legend
• Introduction

... 1 Instruments/Modes Instrument Mode EPIC MOS Imaging EPIC pn Imaging 2 Use pipeline processing yes interactive analysis no 3 Description This task takes the EPIC images in the input list of images, divides them by the images in the input list of `exposure maps', rebins the resulting images to a user-speci ed bin size and plots the corresponding intensity (count-rate) histograms (number of image bins containing a countrate within a certain interval) to a single PostScript le. ... List of input Images...

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• http://xmm.vilspa.esa.es/sas/6.5.0/doc/inthist.ps.gz
• http://xmm.vilspa.esa.es/sas/7.1.0/doc/inthist.ps.gz
• http://xmm.vilspa.esa.es/sas/6.1.0/doc/eregionanalyse.ps.gz

... The miriad Front-End . ... Miriad Datasets . ... Inside Datasets . Scratch Files . Miriad Data Disks at Epping . Visibility Data Concepts . Miriad Visibility File Format . Miriad 's Calibration Model . ... Selecting UV Data in Miriad . Spectral Window Selection . ... Image Data Concepts . Image Datasets . ... Getting Data In and Out of Miriad . ... Reading Visibility FITS Files . ... Writing Visibility FITS Files . ... Flagging, Manipulating and Examining Visibility Data . ...

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• cmodel (Model Image Generator) CentralProcessor 0.11 documentation
• makecube CentralProcessor 0.11 documentation
• ccalapply (Calibration Applicator) CentralProcessor 0.11 documentation

... The pinhole simulation program is a computationally and memory intensive task. ... A parallel version was developed instead, to enable distributed processing on a cluster of workstations. The program makes use of the Message Passing Interface (MPI) standard for parallel processing, implemented as an API (Application Programming Interface) to the Local Area Multicomputer (LAM) programming environment developed at the Ohio Supercomputer Center. ...

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• The SuperCOSMOS Sky Surveys
• Providing a Common GUI to Image Processing Tasks under PCIPS
• ESO C Library for an Image Processing Software Environment (eclipse)

... Главная страница / Кометы и астероиды / "Нас не догонишь". Комета 217P/LINEAR, M42, M43, Бегущий Человек и пролетающие спутники. ... M42 , M43 , БегущийЧеловек , 217P/LINEAR . ... Комета C/2009 R1 (McNaught) . ... Все права на размещенные в галерее фотографии принадлежат их авторам. ... Киевский клуб любителей астрономии "Астрополис" . Движок галереи: 4images 1.7 ...

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Most of these images were obtained by Mike Bessell, Michelle Buxton, Hwankyung Sung, Ralph Sutherland and Bob Watson at SSO using a 2Kx2K Site CCD behind a Nikon or Hasselblad lens or directly on the 1m telescope. A few images are from the Hubble Space Telescope. Some of the M42 images were obtained with the KPNO 1m and ESO NTT telescope. One image is a mosaic of IRAS images. ... Details of the CCD imaging program at MSSSO. ... antenna.jpg (53KB) . ... ngc6744.jpg (59KB) . ...

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• C/2006 P1 (McNaught)
• The GMRT Array Distribution
• Comet Shoemaker-Levy 9 Impact Images

Next: Structure of Tables Up: Table File System Previous: Table File System . The purpose of image processing systems is to extract information from image data. Systems which are designed to treat large numbers of images must also be able to analyse the data extracted from the images. ... The use of tables can be divided into three main categories: internal, external, and user applications. ... The three categories are discussed separately, although there is some overlap in the applications. ...

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• Image Hardcopy
• CCD Image Quality - PixelVision
• HyperLeda: example of online pipeline processing

This WWW form allows the user simplified access to images produced by the NRAO/VLA Sky Survey (NVSS). This service determines which NVSS image is desired based on a celestial position and returns either the image directly or a Web page with a link to the file. ... The NVSS Postage stamp (small FITS file) server can be used to obtain images with other geometries.) ... Web browsers use external viewers to display files like FITS images which they do not understand. ...

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• NVSS Image ftp service (5 August 1998)
• VLSS Image ftp service Documentation Help for VLSS Image ftp service
• OptInt PmWiki : Images | History

... FIELD | ... METHOD . ... java.lang.Object ij.plugin.filter.MaximumFinder . ... public class MaximumFinder . ... 32768 pixels in width or height version 01-Nov-2009 Bugfix: extra lines in segmented output eliminated; watershed is also faster now Maximum points encoded in long array for sorting instead of separete objects that need gc New output type 'List' . ... static int . ... The plugin is inferred from ImageJ by this method . ... int . ... Field Detail public static final int SINGLE_POINTS . ...

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• Alsvid - Python Programs for Processing FITS Astronomical Image Data
• Uses of Class ij.process.FloatProcessor (ImageJ API)
• Translator (ImageJ API)

Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...

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• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• POLIMODEL (V1.00) --- April99 --- POLIMODEL (V1.00)
• ST-ECF Grism Spectrum Software for NICMOS Grism Data

... Posted by hlee . ... Category: Algorithms , arXiv , Cross-Cultural , Data Processing , Imaging , Jargon | ... Category: Algorithms , arXiv , Data Processing , Fitting , Imaging , Jargon , Methods , Quotes , Stat | ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

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• Home Page for SAOimage: The Next Generation
• Image with sky grid overlaid
• *tabplot* - Plotting tables, lists or image sections

... Main page . ... Filters . ... Direct images . ... Back to SAO web page . Last update: 21 Nov 2015 . This page is designed by A.V. Moiseev . ... The SCORPIO-2 project: . ... The direct images are obrained in the 6.1х6.1 arcmin field-of-view with any available filters ...

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• LSVFO: SCORPIO filters
• SCORPIO-2 project: filters
• SCORPIO parameters

... Using the Echelle with TUI . Using the Echelle with Remark . ... Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . ... Focusing the Echelle . ... Changing the echelle guider filters . ... Configuring Remark to use the Echelle . ... Echelle User's Manual . ... The Echelle home page is http://astro.uchicago.edu/echelle . ... Echelle Description . ... Enclosure . ... schematic CAD files . schematic PDF files . ... enclosure wiring schematic . ...

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• Hardware Controllers
• Guider Image Controller Overview
• sgs summary

... The STECF IRAF layered package impol provides five tasks specifically aimed at reduction of HST imaging polarimetry data for ACS, FOC, NICMOS and WFPC2. ... Reduction of HST polarimetry data and simulation of raw polarimetry images, together with polarization vector plotting, are covered. ... hstpolsim -- Produce simulated polarization input data frames for HST instruments from images of the total signal, the linear polarization and the position angle of the polarization vectors. ...

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• ESO - Science Announcements
• Documentation
• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)

This is an interim program to convert Arecibo data into `regular' fits format files. ... Offset 5400.000000 (5399.719945) Object:U4131 Number of scans in an image:4 Number of dumps in a scan:300 Commands are (all caps required): QUIT to stop converting, DRIVE to finish entire file with same object name, UNTIL <scan> to continue for num or until reaching scan, SKIP <num> to skip to scan <num>, ASKFREQ to prompt for frequencies each time, ASKMAP to prompt for map pos. ...

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• M42 Color Images
• Press Release for the 193rd Meeting of the AAS, January, 1999
• AAS 1996 January Meeting Photo Release Images

Stellarium 0.12.3 . ... ScreenImageMgr Class Reference . ... createScreenImage (const QString &id, const QString &filename, float x, float y, float scale=1., bool visible=true, float alpha=1., float fadeDuration=1.) ... setImageAlpha (const QString &id, float alpha) . ... setImageXY (const QString &id, float x, float y, float duration=0.) ... virtual voidљ . ... the ID for the desired image. virtual void ScreenImageMgr::draw . ... the ID for the desired image. virtual void ScreenImageMgr::init . ...

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• Stellarium: ScreenImage Class Reference
• Stellarium: StelQGLTextureBackend Class Reference
• Stellarium: StelGui Class Reference

... Primary Mirror after being stripped and recoated in 3-layer protected silver (NiCr-Ag-NiCr) on 12 September 2009. image: CIMG7901.jpg . ... Primary Mirror held by (yellow) handling tool being lifted off transport container (note the tennis balls it rested on), to be put on wash cart during unpacking at VISTA on 29 March 2008. image: P1060207.jpg (taken 29/03/08) . ... VISTA Mirror Blank: Shape of 4m primary mirror blank being tested at Schott Glas in Germany. image: M1_shape_checking-300dpi.jpg . ...

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• VISTA - Images of Focal Plane
• VISTA - Images of Camera
• VISTA - images of site