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http://www.stsci.edu/stsci/meetings/irw/proceedings/bouyoucef.dir/section3_2.html.

1. The LWS Interactive Analysis (LIA) Package
... Up: Software Applications . Previous: Software Applications . ... 238, Astronomical Data Analysis Software and Systems X, eds. F. R. Harnden, Jr., ... Department of Physics, Queen Mary, University of London, U.K. We report on our on-going software project the LWS Interactive Analysis (LIA) , which has been developed under the IDL environment. This is a processing and analysis software package for the Long Wavelength Spectrometer (LWS) aboard the Infrared Space Observatory ( ISO). ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass00/D-03/ -- 12.4 Кб -- 04.06.2001
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2. http://www.stsci.edu/stsci/meetings/irw/proceedings/bouyoucef.ps.gz
The Restoration of HST Images and Spectra II Space Telescope Science Institute, 1994 R. J. Hanisch and R. L. White, eds. Interactive Deconvolution with Error Analysis K. Bouyoucef, D. Fraix­Burnet, and S. Roques Laboratoire d'Astrophysique, CNRS URA 285/GdR 134, Universit# e Toulouse III, 14 Avenue Edouard Belin, 31400 Toulouse, France Abstract. ... The supernova star is anisotropic in all images: the RLM and MEM solutions show several spikes which are residuals of the PSF. ...
[ Текст ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/bouyoucef.ps.gz -- 161.6 Кб -- 20.05.1994
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3. http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsenergy.ps.gz
... The input dataset is an event list created by rgsframes and is modi ed by the addition of the PI column to the PIXELS table. ... EXPOSURE Required columns: FRAME int32 frame identi er TIME real64 timestamp { PIXELS Required attributes: WINDOWX0 WINDOWY0 telemetry window: origin (node coordinates) WINDOWDX WINDOWDY telemetry window: dimensions RAWY z nominal readout row in HTR mode Required columns: FRAME int32 frame identi er RAWX RAWY y int16 coordinates ENERGY int16 uncalibrated ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/rgsenergy.ps.gz -- 44.1 Кб -- 02.07.2008
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4. http://www.iki.rssi.ru/conf/mss09/MSS-09_files/pap-eng-1.doc
Intensity of atmospheric motions in the mabl retrieved from ocean surface radar imagery M. Mityagina E-mail: mityag@iki.rssi.ru Abstract. The paper is dedicated to the theory and practice of analysis of radar images of sea surface, obtained under unstable atmospheres. In this case, the sea surface reveals wind field variations in the marine atmospheric boundary layer (MABL) caused by atmospheric convec-tive processes, accompanied by air motions with mainly vertical direction. ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/conf/mss09/MSS-09_files/pap-eng-1.doc -- 873.0 Кб -- 26.06.2009
[ Текст ]  Ссылки http://www.cosmos.ru/conf/mss09/MSS-09_files/pap-eng-1.doc -- 873.0 Кб -- 26.06.2009
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5. http://zebu.uoregon.edu/~uochep/talks/talks02/G020237.pdf
... Plot histogram and time series. Flow Chart GUILD & LIGO Tools Local File (XML) Restore Events Import XML event data into an event container LDAS Meta Database Save Events Process events (Sort, Coincidence, Cluster) Create Histogram and/or Time Series Plot Histogram/ Time Series Event Containers Hierarchy "Chain" container - A set of List containers. ... Holds one event. ... Time Series - Make a Time Series (DMT TSeries container) of the event rate, values of specified column or event function. ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks02/G020237.pdf -- 217.5 Кб -- 25.09.2002
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6. http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf
... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf -- 100.3 Кб -- 21.05.2007
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7. SAO RAS home page
... Дни открытых дверей к юбилею САО РАН (12-14 апреля 2016 г.) . Международная конференция "Dark Ages and White Nights (Spectroscopy of the CMB)" (20-24 июня 2016 г.) . ... Международная конференция MULTI-SPIN GALAXIES - 2016 (26-30 сентября 2016 г.) . Международная астрономическая конференция "Физика звезд: от коллапса до коллапса" (3-7 октября 2016 г.) Архив . ... Подробнее.. ... 10.02.16 . ... БТА в реальном времени . ... Цейсс-1000 в реальном времени . ... Последнее обновление: 22/03/2016 ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/ -- 11.4 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/ -- 11.4 Кб -- 09.04.2016
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8. Electron bombarded sensors-resolution
Electron-Bombarded, Back-Illuminated CCD Sensors . ... EBCCD PERFORMANCE: Resolution and CTF . ... Measured CTF for an SI502AB back-illuminated CCD, a GaAs SI502AB EBCCD, . ... Figure 8 depicts each sensor's measured CTF. ... The EBCCD's CTF is only slightly lower in contrast than the back-illuminated CCD's CTF and, depending upon the spatial frequency of interest, is 20% to 100% higher in contrast than the ICCD's CTF. ... Measured CTF for GaAs SI502AB EBCCD #A (1.8 keV) and SI502AB ICCD using a . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/drabek/CCDP/TUTORIAL/EBSENS/Resolut.htm -- 11.2 Кб -- 11.09.1998
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9. ChaMPlane data_archive_.html
... Fields Observed . ... Data Archive . ... Complete Optical and X-ray data for all ChaMPlane fields are available through the DS9 VO interface . ... functionality of DS9 is available to manipulate the results in addition to those provided by the "Champlane tools" You can select images, compare . ... our region of interest has been selected by drawing a red square region on the image. at bottom left the high res optical image of that selected region, and on the right is the X-ray image. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/ChaMPlane/virtual_obs.html -- 10.9 Кб -- 01.10.2012
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10. High Resolution HST Images of Pluto and Charon (ESO Press Release 09/94)
... The remote planet Pluto and its moon Charon orbit the Sun at a mean distance of almost 6,000 million kilometres, or nearly fourty times farther out than the Earth. During a recent investigation by an international group of astronomers [1], the best picture ever of Pluto and Charon [2] was secured with the European Space Agency's Faint Object Camera at the Hubble Space Telescope (HST). ... The new HST image was taken when Charon was near its maximum elongation from Pluto (0.9 arcseconds). ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ohainaut/nice/pluto.html -- 8.5 Кб -- 18.08.2004
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11. Yu. Burman: Publications
... N.A.Bobylev, Yu.M.Burman, Morse lemmas for functionals of the variational calculus, Func.Anal.Appl., ... N.A.Bobylev, Yu.M.Burman. ... N.A.Bobylev, Yu.M.Burman, A.B.Shubin, Algorithms for control with a minimal number of switchings, Automation and remote control , V.53, 5:619, 1992. ... TeX file ) . ... Quadratic Poisson brackets compatible with an algebra structure . ... Yu.M.Burman. ... Yu.M.Burman, Whitney's index formula in higher dimensions and Laplace integrals , Preprint math.DG/9801044 . ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/~burman/list_en.html -- 10.1 Кб -- 04.11.2008