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http://www.sao.ru/drabek/CCDP/TAPER/HTM_resume/Brandeis/MAMOGRAF/Digmammo.htm.
http://www.sao.ru/drabek/CCDP/TAPER/HTM_resume/Brandeis/MAMOGRAF/Digmammo.htm.
1. IKI IPL home page
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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2. Astronomy Plus CCD Images of Galaxies
. Go Here for Hubble Ultra Deep Field . ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu
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Ссылки http://zebu.uoregon.edu/galaxy.html -- 4.8 Кб -- 10.03.2004
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3. Галерея киевского астроклуба ''Астрополис''
... 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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Ссылки http://www.astroclub.kiev.ua/gallery/details.php?image_id=1479 -- 18.2 Кб -- 10.04.2016
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4. C/2006 P1 (McNaught)
... All images on this page are copyright Robert H. McNaught. ... There have been so many requests for high resolution copies of these images that I ask that all enquiries for these to go directly to Science Photo Library. C/2006 P1 on Jan 18, 10:22 UT. Photo: R. H. McNaught, Siding Spring Observatory. Canon 5D, 135mm, f/2.0, 2 sec exp., ISO 1600 . ... ISO 200 . ... Canon 5D, 50mm, f/2.0, 30 sec exp., ... Canon 5D, 135mm, f/2.0, 120 sec exp., ... Canon 5D, 50mm, f/2.0, 110 sec exp., ...
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Ссылки http://www.mso.anu.edu.au/~rmn/C2006P1new.htm -- 9.6 Кб -- 11.05.2007
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5. Image and Spectrum Recovery
... Determine the net instrument response desired. ... Use a numerical algorithm, the convolution network (discussed in detail below), to search for the solution that provides the desired mapping of the observed data to the desired form. ... We first made preliminary studies investigating recovery of images that have been broadened by the HST's mirror by modeling its PSF as shown in Fig. ... Our recovery procedure was applied also to spectral data, in this case to a tunable diode laser (TDL) spectrum. ...
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Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/ching.dir/section3_2.html -- 12.8 Кб -- 18.04.1994
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6. Image sampling
Next: Noise distributions Up: Basic Concepts Previous: Basic Concepts . The acquisition of a data frame involves a spatial sampling and digitalization of the continuous image formed in the focus plane of a telescope. ... The individual pixel values are obtained by convolving the continuous image with the pixel response function . With a sampling step of and the digital frame is given by . ... A frame is oversampled when while for smaller sample rates it is undersampled. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node13.html -- 6.2 Кб -- 23.02.1996
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7. Blurry images
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Parkes radio telescope . Australia Telescope Compact Array . ... Images . ... A single-dish radio telescope is not nearly as effective at detecting the fine detail in the objects it focuses on, and the radio image of an object from a single-dish radio telescope is very blurry. ... However, radio waves have wavelengths of roughly one tenth of a metre and so even large radio telescope dishes produce blurry images. ...
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Ссылки http://www.atnf.csiro.au/projects/mnrf1996/para2.html -- 50.4 Кб -- 08.04.2016
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8. Image Extraction
... Image extraction is enabled by setting the name of the output file using the parameter imageset . The name of the columns to use for the and axes of the image are set using the parameters xcolumn and ycolumn . ... If no WCS information is available for a column, then the CTYPE keyword for this axis of the image is set to the name of the column, and the other WCS keywords are set to reflect the range and binning of this column, as is done for SPEC* keywords in spectral extraction. ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/evselect/node10.html -- 10.0 Кб -- 15.08.2005
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9. NVSS Image ftp service Documentation Help for NVSS Image ftp service
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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Ссылки http://www.mrao.cam.ac.uk/projects/surveys/nrao/NVSS/findhelp.html -- 6.6 Кб -- 11.02.1999
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10. Supernova 2009js in NGC 918
Supernova 2009js in NGC 918 . This page is devoted to information on Supernova 2009js in NGC 918 . Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. Discovered independently by Lick Observatory Supernova Search (USA) and Koichi Itagaki (Japan). ... 2009/10/11.44 . 17.2 . ... Joseph Brimacombe . ...
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Ссылки http://www.sai.msu.su/mirrors/isn/sn2009/sn2009js.html -- 8.2 Кб -- 13.02.2011
[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
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[ Сохраненная копия ] Ссылки http://www.rochesterastronomy.org/sn2009/sn2009js.html -- 8.4 Кб -- 19.04.2014
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11. http://observ.pereplet.ru/images/SN101019/sn.html
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Ссылки http://observ.pereplet.ru/images/SN101019/sn.html -- 1.2 Кб -- 01.10.2012
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12. Images
. Next: Type 12 Up: Stellar models Previous: Type 11 Contents . handles two types of images, one being the classical type FITS image or image cube, the other one being the PEARL image. The latter is a parametric image, assigning an effective temperature to each pixel. Subsections . Type 12 . Type 13 . Christian Hummel 2015-04-28
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Ссылки http://www.eso.org/~chummel/oyster/manual/node69.html -- 3.5 Кб -- 28.04.2015
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13. A collection of images
... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...
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Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/sun/T171_20001101_101547.html -- 13.0 Кб -- 28.12.2000
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14. Chandra Images for G290.1-00.8
True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Radio Images Page . ... Exposure uf . ... Exposure uf Exposure time of unfiltered event file . Exposure f Exposure time of filtered event file . ... Event 2 FITS File . ... AUX file . ... Region . ... see fit detail page for more about the fit. see chandra spectrum page for region used. Images in Several Energy Bands . ... Spectra of Several Regions . ... 1.0" . ... in central region . ... in central region, double? ...
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Ссылки http://hea-www.harvard.edu/ChandraSNR/G290.1-00.8/ -- 10.9 Кб -- 27.02.2014
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15. Digital images of magnetograms
Standard analog magnetograms (20 mm / sec) are presented in the form of digital images, . ... Observatory, . ... 1949 , 1950 , 1951 , 1952 , 1953 , 1954 . ... 1951 , 1952 , 1953 , 1954 , 1955 , 1956 , 1957 . ... 1950 , 1951 , 1952 , 1953 , 1954 , 1955 , 1956 , 1957 , . ... 1950 , 1951 , 1952 , 1953 , 1954 , 1955 , 1956 , . ... The project was conducted in 2003 by the International Council for Science ( "Rescue of Old Analogue Magnetograms by converting to digital images" , ICSU Grant–2003 Project). ...
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Ссылки http://www.wdcb.ru/stp/magnetogr_list.en.html -- 35.2 Кб -- 11.12.2014
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16. ISSA-PS, The Postage Stamp Server for IRAS Imaging Data
... The ISSA Postage Stamp Server is a Web-accessible service that delivers IRAS images to users with a minimum of effort. ... The basic idea of the ISSA Postage Stamp Server is to provide small subsets of the IRAS imaging data to users with minimal fuss and bother. ... Users retrieve the FITS images by clicking on the postage stamps, provided their Web clients are properly configured (we give instructions on how to do this). ... Users are, of course, free to do so at their end. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/vanburend2.html -- 7.6 Кб -- 03.11.2000
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17. The NMW survey homepage
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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18. Planetary Radar: Arecibo Radar Images of Asteroids
This series of delay-doppler radar images of the asteroid 4769 Castalia (also known as 1989 PB) were taken at approximately 2 minute intervals on 1989 August 22 at the Arecibo Observatory. ... These images have been stretched to look decent on a browser, rather than for accuracy. ... Thus these images have a frequency resolution of 0.24 Hz (~40 m), and a frequency sampling of 0.12 Hz, but the signal to noise ratio should be 2 times worse, as only 6 looks can be summed. ...
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Ссылки http://www.naic.edu/~nolan/radar/Castalia.html -- 4.4 Кб -- 24.02.2005
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19. Creating a watermark effect
... Imagine that for every pixel in the color image, you take its luminance value (that's how bright it appears). ... In the end, you will have a histogram which counts how many times each luminance value appears in the image (that histogram can be used to analyze the distribution of the luminance values in the image). ... For the watermark effect, we want to use the same value that we used in the Stretch Contrast step, so that the lightest color will be in fact white (255), and nothing will get clamped...
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Ссылки http://www.sai.msu.su/~megera/gimp/quintero/tutorials/watermark/watermark.html -- 6.9 Кб -- 22.12.2007
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20. Shared Skies Partnership Astronomical Image Data Archive
... Images and Data from the Shared Skies Partnership . ... Open access to selected images and data . Restricted access to user data . Restricted access for schools . Restricted access for the astronomy lab . Other Data and Image Resources . Sky View (internet virtual telescope) . SIMBAD Astronomical Database . ... International Astronomical Union Circulars (restricted access) . Sloan Digital Sky Survey Release 8 . Multimission Archive at Space Telescope . ...
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Ссылки http://www.astro.louisville.edu/shared_skies/archive/ -- 3.4 Кб -- 14.12.2014
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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