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http://vo.astronet.ru/~karpov/pdf/2014_Karpov.pdf.

1. http://vo.astronet.ru/~karpov/pdf/2014_Sasyuk.pdf
... Skalnatґ Pleso 43, 1 ­ 2, (2014) e Mini-MegaTORTORA ­ multichannel system for wide-field optical monitoring with high temp oral resolution V. Sasyuk1 , G. Beskin2 , S. Karp ov2 , S. Bondar3 , A. Perkov3 , E. Ivanov3 , E. Katkova3 and A. Shearer4 2 Kazan Federal University, Russia Special Astrophysical Observatory of Russian Academy of Sciences, Russia 3 Insttitute for Precise Instrumentation, Russia 4 National University of Ireland, Galway, Ireland Received: November 4, 2013; Accepted: ?? ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2014_Sasyuk.pdf -- 59.3 Кб -- 06.02.2014
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2. Sensors
... European Remote Sensing Satellite (ERS-1) was launched on 17 July 1991, and the follow mission ERS-2 (with the same sensors and an Ozone monitoring instrument added) was launched on 21 April 1995. ... ERS-2 has a fixed repeat cycle of 35 days, and follows ERS-1 tracks with one day's delay. ... Swath width is 102.5 km (telemetered), spatial resolution is about 25x25 m. The Advanced SAR (ASAR) instrument is carried by ESA's ENVISAT satellite launched on 1 March 2002. ... Swath . ... Spatial Resolution...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/simp/sensors.html -- 8.2 Кб -- 25.02.2007
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3. Compressor monitor
... 06jun11: testing the compressor monitor system on the telescope. 14apr11: testing the compressor monitor system in the lab . ... Around second 400 to 500 seconds, willie iguina openned the huffman box of the compressor monitor to get access to turn off the device. ... luis added some shielding to the devices in the huffman box (.pdf) and then remeasured the rfi on 15apr11. data was only measured up to 2500 MHz on this data with the huffman box closed. 902 probe: rfi below 100 MHz way down . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/rfi/miscdevice/compressorMon/compressorMon.html -- 8.5 Кб -- 10.06.2011
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4. Optical systems and devices
To main of Laboratory . The research work and design of optical and optical-electronic devices are carries out by laboratory staff: . ... Lens: . ... In the layout 1 prism systems perform functions of dispersive element, corrector of aberrations, optical reducer. ... Spectral range 200 - 400 nm; . ... Back Forward . ... The main corrector's function are compensation of field aberrations of the main spherical mirror of a telescope (diameter of 600 mm, f'=1200 mm) and increase aperture ratio. ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/lao/optical_systems_eng.html -- 19.6 Кб -- 12.01.2010
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5. http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_10_26_93
HUBBLE SPACE TELESCOPE DAILY REPORT #1002 PERIOD COVERED: 0800 EST Daily Status Report as of 300/1200Z. 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed GHRS/2 5041 (GHRS Sensitivity Monitor - Cycle 3) The High Resolution Spectrograph was used to make 24 ultraviolet observations of standard star AGK81D266 to monitor the sensitivity of the HRS, which is expected to change slowly with time. ... Cycle 3 High) 3.7 Complete WFC 5076 (WF/PC Cycle 3 Calibration: WFC Flats Wide. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_93/hst_status_10_26_93 -- 5.3 Кб -- 27.10.1993
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6. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/pagani-cal-2012.pdf
Swift/ XRT radiation damage and results from the lab using a proton-damaged CCD Claudio Pagani (Swift/ XRT team) XMM Calibration Meeting, Leicester, 7/3/2012 XRT CCD e2v CCD -22 detector (developed for EPIC MOS camera on XMM) Operated in Photon Counting (PC) and Windowed Timing (WT) mode 4 55Fe corner sources continuously illuminate CCD corners, used to monitor CCD performance Spectral resolution at launch: FWHM = 135 eV at Mn K- (5.9 ...
[ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/pagani-cal-2012.pdf -- 1262.1 Кб -- 13.05.2014
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7. 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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