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http://www.stsci.edu/hst/acs/documents/handbooks/cycle19/ix.html.

1. ACS Instrument Handbook for Cycle 20
... ACS Instrument Handbook . ... SBC . WFC . ... HRC 1 , 2 . ... small filters . ... global limit table . ... Buffer . ... SBC 16 bit . ... See HRC . ... See WFC . ... parallel measurement/table . ... serial measurement/table . ... HRC/WFC . ... buffer dumps 1 , 2 . buffer size . ... See SBC . WFC. see WFC . ... Filter Wheel . ... WFC/HRC . ... SBC Summary Table . ... WFC/HRC Summary Table . ... filters see filters . ... Memory.See Buffer . ... HRC/SBC . ... buffer . ... SBC filters . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/documents/handbooks/cycle20/ix.html -- 164.5 Кб -- 05.02.2013
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2. http://observ.pereplet.ru/images/GRB081102/grb_film.html
... GCN 8471 | ... TITLE: GCN CIRCULAR NUMBER: 8516 SUBJECT: GRB 081102: MASTER refind and final results DATE: 08/11/11 15:50:10 GMT FROM: Vladimir Lipunov at Moscow State U/Krylov Obs E. Gorbovskoy, V. Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, P.Balanutsa Sternberg Astronomical Institute, Moscow State University A. Tlatov, A.Parkhomenko Kislovodsk Solar Station of the Pulkovo Observatory V.Krushinski, I.Zalognikh Ural State GCN Circ 8470, Lipunov et al., ...
[ Сохраненная копия ]  Ссылки http://observ.pereplet.ru/images/GRB081102/grb_film.html -- 8.2 Кб -- 01.10.2012
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3. GRB observations
... Observations have received at the telescope AT-64 of the Crimean Astrophysical Observatory . GRB . ... RA(2000): 11h 45m 10.54s . DEC(2000): 17o 24' 34.44" . ... Filter: none . ... Date, time (UT) . Exposure . ... 2000.07.29 18:21:52 . 30 sec . ... RA(2000): 19h 58m 19.61s . DEC(2000): 23o 32' 35.15" . ... 120 sec . ... DEC(2000): 6o 20' 47.07" . ... 240 sec . ... DEC(2000): 51o 46' 34.93" . ... DEC(2000): -13o 04' 30" . ... DEC(2000): +55o 18' 25.0" . ... 2000-11-09T16:03:19 . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/grb/CrAO/GRB/GRB.htm -- 14.2 Кб -- 21.11.2000
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/grb/CrAO/GRB/GRB.htm -- 14.2 Кб -- 21.11.2000
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4. http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/grizli_performance.pdf
GRIZLI Science Performance Goals Includes also some performance goals for telescope and software 16 October 2011 A. Instrument specs 1. Delivered image quality, in each filter, across entire FOV Goal: 0.5" FWHM, with well-behaved PSF, at high altitude (low airmass) 2. Limiting magnitude Goal: 26th mag in griz gives S/N=10 in 3 min exposure sky-limited in all filters with no moon 3. ... Fringing Goals: (for 3 min exposure) - less than 1% in i - less than 5% in z 8. ...
[ Текст ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/ARCTIC/Development/ImagerPDR/grizli_performance.pdf -- 46.1 Кб -- 05.12.2013
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5. Meade Series 4000 Broadband Nebular Filters
... Meade Series 4000 Nebular Filters incorporate the very latest in interference coatings technology. ... Technical Basis of the Meade Broadband Nebular Filter: As shown in the transmission graph below, the Meade Broadband Nebular Filter strongly rejects the light of sodium- and mercury-vapor lights as well as natural airglow and auroral emissions. ... Meade Series 4000 Narrowband Nebular Filters . ... Meade Series 4000 Oxygen-III Nebular Filters . ... Meade Series 4000 Photo-Visual Color Filters . ...
[ Сохраненная копия ]  Ссылки http://www.meade.com/catalog/meade_4000/meade_series_4000_nebular_filters.htm -- 29.2 Кб -- 06.10.2007
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6. Description
... Meta Index / Home Page attfilter performs exposure-specific attitude data filtering and Good-Time-Interval (GTI) creation driven by a single boolean selection expression. The task generates a single GTI table whose rows represent time intervals during which the spacecraft attitude did not deviate from a given reference attitude by more than a specified tolerance limit. ... Compute the median spacecraft attitude within the exposure time window. ... Astronomical position angle of spacecraft . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/attfilter/node3.html -- 11.2 Кб -- 09.07.2007
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7. A New PROS Task for Calculating HRI Source Intensities or Upper Limits
... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/chenj.html -- 11.4 Кб -- 03.11.2000
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8. Светофильтры - Celestron LPR (Light Pollution Reduction), Baader UHC-S
... Обзор LPR фильтра. Впечатления от наблюдений с LPR фильтром. ... Характеристики цветных фильтров Baader-Planetarium . Мой перевод pdf- файла о фильтрах с сайта Baader-Planetarium (379 кб) . ...
[ Сохраненная копия ]  Ссылки http://www.shvedun.ru/filters.htm -- 33.2 Кб -- 09.04.2016
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9. The AstroStat Slog Upper Limits
... Posts tagged ?Upper Limits? Nov 24th, 2007| 09:26 am | ... ArXiv] 4th week, Nov. ... This week, instead of only filtering AstroStatistics related papers from arxiv, I chose additional arxiv/astro-ph papers related to CHASC folks? astrophysical projects. ... Due to the CHACS? long history (we are celebrating the 10th birthday this year) and my being a newbie to CHASC, I may not pick up all papers related to the projects of current, former, and future CHASC members and dedicated slog readers. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/upper-limits/index.html -- 21.6 Кб -- 01.03.2014
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10. The best images from RTT150
RTT150 . ... One of the image, obtained in the May, 2003, with Andor DW436 CCD. Cluster 1541+6626, filter R, exposure 15 minutes, the resolution is 1", limiting star magnitude is 23m, the field of view is 8' x 8'. At the left: image of cluster 0720+7132 (z=0.268) obtained in the beginning of November, 2002 with RTT-150 and AP-47P CCD. 25 minutes exposure in R. The resolution is 0.7" (angular size of the image element - 0.23"), limiting stellar magnitude is 23.5-24. ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/AZT22/ENG/best.htm -- 5.4 Кб -- 18.02.2004
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11. http://www.arcetri.astro.it/irlab/instr/firt/firt.html
The TIRGO NIR photometer uses a single InSb detector with cooled low-noise amplification electronics. Detector, filters, and diaphragms are cryogenically cooled to solid nitrogen temperature. ... FIRT gives the following choice of filters and diaphragms: . Results of the TIRGO calibration program: 1986-1987" L.K. Hunt, G.Calamai, and E. Oliva Arcetri Technical Report No. ... Manuale del nuovo sistema di controllo del Fotometro del TIRGO" C.Baffa Arcetri Technical Report No. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/instr/firt/firt.html -- 2.8 Кб -- 28.07.2005
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12. SAI Space Monitoring Laboratory
Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... GRB 100131A: MASTER-Amur alert observations 76 sec after Notice time.The limit of the main telescope images is aboute 15 mag (unfiltered). ... All news ...
[ Сохраненная копия ]  Ссылки http://master.sai.msu.ru/en/news/73 -- 8.0 Кб -- 09.04.2016
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13. http://www.naic.edu/~phil/obsproblems/faaharmonics.html
... These were being caused by the FAA radar at 1350 Mhz. ... The sky signal is normally mixed to 750 Mhz with a 500 Mhz bandpass filter limiting the band. ... The 4 260 Mhz signals (actually 8 if you count both polarizations) are sent to the correlator where they pass through a 50 Mhz bandpass filter centered at 260 Mhz.The data is then down converted and sampled with an 8 bit 100 Mhz A/D converter. ... 1350 Mhz . ... 1394-1350= 44Mhz . ... The birdies will alias at 50 Mhz so in band they will be at: ....
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/obsproblems/faaharmonics.html -- 5.6 Кб -- 06.06.2002
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14. Journal "Peremennye Zvezdy"
Peremennye Zvezdy", . ... Star Name: . USNO-A2.0 0900-17250765 . ... 15.85 - 18.4 (unfiltered) ; . ... During observations of a field in Aquila, we discovered a new UV-type variable star. ... For photometry of the new variable star, we applied VaST software by Sokolovsky and Lebedev (2005). ... 5 (J2000, 2MASS)), R 1 =14 m .30, R 2 =14 m .60 (USNO-B1.0). ... Coordinates of the variable star were drawn from the 2MASS catalogue (Skrutskie et al. ... Flare of USNO-A2.0 0900-17250765 . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1267921 -- 8.6 Кб -- 07.11.2012
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15. Artifacts
... Figure: A dark current CCD exposure with cosmic ray events which are removed with non--linear filters. ... Figure shows a CCD dark current exposure with cosmic ray events. ... Figure: Removal of cosmic ray events on a CCD spectral exposure with different techniques: (A) original, (B) median filter, (C) recursive filter and (D) stack comparison. ... For comparison with non--linear filter techniques, Figure D shows removal of cosmic ray events from the spectral frame discussed above. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node17.html -- 10.0 Кб -- 23.02.1996
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16. Supernova 1998an in UGC 3683
Here is an image a supernova in UGC3683. 11.4.1998. 0.08 UT, CCD ST-7, 520s. Track and Accumulate exposure (13x40s), no filter, dark and flat corrected, temp -20c, telescope used 152/2063 refractor. The image have been taken at the center of our city, Jyvaskyla. The weather was horrible (a full moon was shining and there was clouds on the sky during exposure), so I had stopped imaging in that night. ... Iґll wait for a next clear night and send a better image then. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/snimages/sn98an2.html -- 2.3 Кб -- 22.12.2007
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/SNIMAGES/sn98an2.html -- 2.3 Кб -- 10.04.2016
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17. Женские наручные fashion часы в коллекции New Line RB RoccoBarocco -
... Вид: пожарная мотопомпа ; . ... Коллекция: Осень-зима 2015/2016 . ... Пол: Женский . ... Коллекция: Весна-лето 2016 . ... title='Molokai Sunset - Quiksilver' border='0' align='left' width='120' style='margin-right: 20px;' hspace='7' vspace='5'/> Сланцы для мужчин от Quiksilver - новинка из коллекции "Весна 2015". ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku2469.html -- 21.8 Кб -- 14.02.2016
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18. http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/correlators.pdf
... An Aperture Synthesis Array Radiotelescope · A collection of simple interferometers · An array of N antennas · Processed in pairs ­ N(N-1)/2 pairs or baselines - u,v in wavelengths Complex Correlator Measures visibility or cross power ( complex ) Band limiting filter Cosine correlator 90 degree phase shift Sine correlator Base-band Correlator - with fringe rotation Common Local Oscillator Digital ... Provides an easy method of delay calibration. ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/correlators.pdf -- 124.4 Кб -- 22.05.2003
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19. Running a High-Performance Web Server for BSD
... After the edit, recompile the kernel and recompile the Apache server then reboot. ... If you're running a really busy BSD Apache server, the following are useful things to do if the system is acting sluggish: . ... Maximum # of processes . ... This machine is a server that handles lots of traffic, # so we crank that value. options NMBCLUSTERS=4096 # mbuf clusters at 4096 # # Misc. options # options CHILD_MAX=512 # maximum number of child processes options OPEN_MAX=512 # maximum fds (breaks RPC svcs)...
[ Сохраненная копия ]  Ссылки http://neptun.sai.msu.su/manual/misc/perf-bsd44.html -- 12.2 Кб -- 25.01.2002
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20. LIMIT EFFICIENCY OF CHAOTIC SIGNAL CLEANING - NDES-99
Alexander S. Dmitriev . Institute of Radioengineering and Electronics of the Russian Academy of Sciences . Mokhovaya st., 11, Moscow, 103907, Russia. ... Moscow Institute for Physics and Technology . ... The relationship between the problem of cleaning chaotic signals off noise and the information properties of the signals is shown. Some methods for chaotic signal cleaning are considered. The efficiency of these methods is evaluated by computer simulation. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/rus/InformChaosLab/papers/ndes99dkh.html -- 2.6 Кб -- 11.04.2000
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