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http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/_sources/BETApipelines/ScienceFieldSpectralLineImaging.txt.

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 ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/IPL/ -- 4.8 Кб -- 05.08.1997
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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
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/galaxy.html -- 4.8 Кб -- 10.03.2004
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3. User Parameters - Spectral-line Imaging CentralProcessor 0.11 documentation
... CentralProcessor 0.11 documentation . ... There are several steps involved in running the spectral-line imaging, with several optional pre-processing steps: . ... The gains solution from the continuum self-calibration can be applied to the spectral-line MS using ccalapply. The continuum can be subtracted from the spectral-line MS using ccontsubtract The continuum is represented by either the clean model from the continuum imaging, or ? ... Whether to do the spectral-line imaging . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/BETApipelines/ScienceFieldSpectralLineImaging.html -- 22.5 Кб -- 12.04.2016
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4. Results
... We have been using it to analyze PC images of known gravitational lenses and QSOs which are candidates for lensing (Falco 1993). ... Fig. 1 plots the higher contours of the PC image of 0142 in the upper left, and its power spectrum in the upper right. ... If we fit the envelope of the power spectrum with a binary model, we find that best fit gives a separation of the two components of 1.3 PC pixels or about 58 mas. ... The lower two curves are cuts through the 0142 power spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/nisensonp.dir/section3_3.html -- 7.5 Кб -- 16.04.1994
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5. Application Commands
... ASSOCIATE/RANK table col1 col2 [action] . ... BIN/TABLE table col1 col2 [bin] [min] [max] [sigma] . creates a table, bin.tbl with averages of col2 in bins of col1 . COMPARE/2SAM table col1 col2 . ... COMPUTE/FIT image[,error] [= function[(refima)]] . ... COMPUTE/FIT table y[,error] [= function[(ind)]] . ... COMPUTE/FUNCTION image = function[(refima)] . compute function values, result as image . COMPUTE/FUNCTION table y = function[(ind)] . ... define user functions for fitting . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node399.html -- 7.2 Кб -- 23.02.1996
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6. The Co-Addition Technique Applied to Images of Galaxy Cores
... Previous: Substepping and its Application to HST Imaging . ... This is a preliminary report on an application of the co-addition technique based upon the Richardson-Lucy algorithm. The combination of high signal-to-noise ground-based images obtained with the ESO NTT using SUSI with high angular resolution HST FOC f/96 images gives new insights on the properties of galaxy cores and their potential time variability. Cores of galaxies are one of the main thrusts of present extragalactic research. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/zeilingerw.html -- 10.8 Кб -- 12.06.2006
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/zeilingerw.html -- 10.9 Кб -- 15.05.1998
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7. Contrasting optical and X-ray applications
Next: CCD Scientific Performance Up: CCD Operation Previous: CCD Operation . A visible light photon releases only one electron-hole pair, and consequently many photons must be collected in each pixel for a measurable signal to be produced. ... This use as an imaging X-ray spectrometer requires that no more than one photon is incident on each pixel in any image frame, which imposes a requirement that image collection times be limited to ~seconds for typical astronomical applications. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/user/socpub/ccd_review/node3.html -- 7.1 Кб -- 30.08.1996
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8. STScI NICMOS Software
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. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node17.html -- 9.7 Кб -- 12.06.2006
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9. *fixsaoreg* -- restore SAOimage region to original image (physical) coordinates
Next: *display, xdisplay, xexamine* - Up: Image Display in Xwindows Previous: A Region mask for . In order to view a large image/qp file with the SAOimage display, it is necessary to block or section that image. The SAOimage pixel readout is not in original image/qp coordinates (physical) but in blocked and perhaps sectioned coordinates (logical). ... In the output file, your original region has been commented out and the same region in physical coordinates has been inserted. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node65.html -- 3.9 Кб -- 01.10.2012
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10. ANR OTARIE project: transport optimization and applications
... Reconstruction of peculiar velocities of galaxies from large-scale redshift catalogues provides an exemplary application of optimal transport. ... U Frisch, S. Matarrese, R. Mohayaee, A. Sobolevsky, A reconstruction of the initial conditions of the Universe by optimal mass transportation , Nature, 417 (2002) 260-262 ( arXiv:astro-ph/0109483 ) . ... R. Mohayaee, A. Sobolevskii, The Monge Amp re Kantorovich approach to reconstruction in cosmology , Physica D (2008) accepted ( arXiv:0712.2561 ) . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/~ansobol/otarie/research.html -- 5.4 Кб -- 19.02.2009
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11. Wispi Design Notes
... 400mm f/2.8 Nikor lens: images the sky on the entrance slit. ... The optical system maintains image quality along the slit length so that each row of the image is a spectrum of that spatially selected region of the sky. 180mm f/2.8 Nikor lens: collimates the light from the slit. ... The auxiliary optical platform on WISPI now accomodates a short focal lens and a guiding/imaging video system that may use sub-pixel corrections to provide feedback to the tracking drive motors. ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/moore/wispi/wisp_const.html -- 8.6 Кб -- 10.05.2010
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12. 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 ...
[ Сохраненная копия ]  Ссылки http://www.astroclub.kiev.ua/gallery/details.php?image_id=1479 -- 18.2 Кб -- 10.04.2016
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13. IRAF/STECF imaging linear polarimetry simulation and reduction package
... 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. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~jwalsh/softpol/ -- 8.2 Кб -- 02.02.2001
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14. Une image historique et intrigante de Pluton | Ciel et Espace
... Ciel Espace, le magazine qui vous guide toujours plus loin . ... les plus belles images de l'Univers d†йcrypt†йes pour vous . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Une image historique et intrigante de Pluton . ... Pour un guide complet de la mission New Horizons, avec le d†йroul†й pr†йcis, l'historique et les enjeux : rendez-vous dans Ciel & Espace de juillet-ao†Ёt , ...
[ Сохраненная копия ]  Ссылки http://www.cieletespace.fr/node/18525 -- 28.3 Кб -- 09.04.2016
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15. The Face on Mars
... The Raw Images . Table 1: List of Viking Orbiter Images of the "Face on Mars" . ... Processing the Face Images . ... In July, 1976, Viking Orbiter 1 was acquiring images of the Cydonia region of Mars as part of the search for potential landing sites for Viking Lander 2. ... Using the height field, it is also possible to view the "Face" from different look directions, by mapping the Viking Orbiter image directly on the the topography and then placing the "viewer" at different locations. ... Mars . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/face.htm -- 14.9 Кб -- 15.03.1998
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16. S.P. KOROLEV ROCKET & SPACE CORPORATION ENERGIA
... Corporation . OAO RSC Energia . President of the Corporation . ... Brief History of Rocket and Space Technology . ... Space Station MIR . ... Space Records . ... Image . ... Contribution of RSC Energia to the Russian Space Technology . International Space Station . Project History . ... First Crew . Required Resources . ... Images . ... Second Crew . ... First Russian Visiting Crew . ... Third Crew . ... Fourth Crew . ... Rockets . ... Official WEB-site of S.P.Korolev RSC Energia . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/english/sitemap.html -- 40.0 Кб -- 01.10.2012
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17. 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., ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~rmn/C2006P1new.htm -- 9.6 Кб -- 11.05.2007
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18. The IX Asian-Pacific Astronomy Olympiad 2013, applications
... Form of the application (Excel file, please, save the table in format not later Excel-1997-2003). Personal data list (please, save the data in text format *.txt), . colour photo , minimum 480x720 pixels (in accordance with the rules of ICAO , please, save the image in format *.jpg). and passport scan , resolution 150-300 dpi (please, save the image in format *.jpg). ... Dr. Michael G. Gavrilov, Founding Chairman and Coordinator of the Asian-Pacific Astronomy Olympiad (APAO) . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/iao/apao/2013/ap13bz_e.html -- 7.2 Кб -- 28.10.2013
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19. The Sparkle Plug-In
Previous Next Table of Contents . ... The Sparkle plug-in was originally written by John Beale as a stand alone program which would process a TGA image to add "sparkles" to the brightest (whitest) parts of an image. The effect, when properly applied to an image, is similar to lens flare. However, more interesting effects can be made than just lens flare. ... It could probably be changed to work with indexed color images, but I'm not sure if the effect would be the same. ... 3.5 Spike Length . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/gimp/mjhammel/gdp/plug-ins/sparkle.html -- 3.2 Кб -- 22.12.2007
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20. 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: . ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/nmw/ -- 10.7 Кб -- 18.02.2015
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