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http://www.atnf.csiro.au/computing/software/gipsy/tsk/cormap.dc1.

1. Description
... This task takes an event list and makes an image in which the value in each pixel is proportional to the variability with respect to time of the flux of events which fall within that pixel. The task cycles through all the events in the list which fall within the spatial extent of the image; for each of these events, a value of the Kolmogorov-Smirnov statistic is calculated. ... Note the implication that pixels having zero variability are not zero-valued in the output image. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/evarimgen/node3.html -- 11.2 Кб -- 02.07.2008
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2. http://astro.uni-altai.ru/AFgalleries.html
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/AFgalleries.html -- 1.1 Кб -- 01.10.2012
[ Сохраненная копия ]  Ссылки http://astroclub.ru/ -- 1.2 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://astronomy.tomsk.ru/google.php -- 1.3 Кб -- 01.10.2012
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3. Target Category and Target Description [Description]
... HST Phase II Proposal Instructions for Cycle 20 > Chapter 3: Fixed and Generic Targets > 3.3 Target Category and Target Description [Description] . ... Each target must be assigned a single primary category from Table 3.2 , and at least one descriptive keyword , chosen from the appropriate Table 3.3 through Table 3.9 (see Table 3.2 for which table is appropriate for each category). ... Table 3.3: Descriptive Keywords for STAR and EXT-STAR . ... Table 3.6: Descriptive Keywords for CLUSTER OF GALAXIES...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelpCy20/ch03_targ_fixed04.html -- 130.5 Кб -- 31.05.2012
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4. http://www.atnf.csiro.au/computing/software/gipsy/tsk/flat.dc1
... BOX= Area which needs to be flat fielded [whole map] OUTSET= Output Set/Subset(s) ORDER= Order of polynomial to be fitted to the map [1] highest allowed order is 21 ** RANGE= Give range of levels to include in fit: [all levels] Input consists of two values. ... Examples for the use of the RANGE= keyword: RANGE=2, 5 (IF 2<value<5 THEN include in fit ELSE value==>blank) RANGE=5, 2 (IF 2<value<5 THEN value==>blank ELSE include in fit) At the RANGE= keyword, the values -INF and INF can be input also. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/gipsy/tsk/flat.dc1 -- 3.5 Кб -- 20.03.2000
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5. Topics in AstroStatistics
Modern AstroStatistics has emerged as a new field in recent times, informed by a Bayesian foundation, utilizing powerful computational tools like MCMC, and applied to diverse analysis and inference problems in Astronomy. ... The goal of our Special Session is to review current practices, highlight modern techniques, and explore how the transition into the realm of Big Data Astronomy can be facilitated. ... Big Computing in Astronomy: Perspectives and Challenges . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/AAS224/ -- 12.5 Кб -- 10.04.2016
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6. Pulkovo Observatory
. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/ -- 4.5 Кб -- 06.04.2009
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7. The High-Z SN Search Description
... I am an astronomer at the Australian National Universities' Research School of Astronomy and Astrophysics. We are located at Mount Stromlo Observatory, just outside of the Australian National Capitol, Canberra. The observatory has telescopes at two sites, one at Mount Stromlo, and the other near Coonabarabran. ... The work described here is not just my work, but the collective effort of more than 20 people from around the globe with whom I work on the High-Z SN search. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~brian/PUBLIC/introduction.html -- 3.7 Кб -- 01.10.2012
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8. University of Oregon Center for High Energy Physics - ATLAS
... This precise description is called the standard model of electroweak physics. ... What brings about this important difference in the mass of these "field" particles? ... The Oregon group participates in the ATLAS experiment to investigate this question. ... Since Oregon joined ATLAS early in 2006, the group has devoted its effort to the process of selection of interesting events generated by the collisions of high energy particles within the ATLAS detector. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/~uochep/atlas.html -- 3.5 Кб -- 20.12.2007
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9. Description of the RadioAstron project, english version
Orbit . ... The orbit of the RadioAstron provides four types of study: . rough images of radio sources with ultra-high angular resolution, using all baselines up to the radius of the apogee, that is much larger than Earth diameter; . ... high quality imaging of radio sources, with moderate resolution, by observing either with small projected base lines Earth-spacecraft, i.e. close to the orbital plane, or near the perigee. ... high accuracy orbit determination. ... Space Radio Telescope . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/description/orbit_eng.htm -- 7.3 Кб -- 10.05.2008
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10. 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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12. Source Positions
Next: Catalog Construction Up: Observations and Analysis Previous: Source Detections . ... It was assumed that the highest signal gives the most likely position of the source. ... Comparing the summed map with the maps from the individual energy ranges, the one which produced the smallest error box was chosen to represent the source position, as long as was greater than 4, a level chosen to reflect a reasonable degree of confidence in the detection. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/EGRET2/node7.html -- 9.0 Кб -- 08.05.1998
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13. GALFA System Description
Section I: Introduction to ALFA and GALFA . Section II: System Description . ... ALFA receives 7 beams, 2 polarizations per beam, each covering 1225-1525 MHz. The 14 IF signals cover nominally the 100 to 400 MHz band. ... A high-resolution, low-bandwidth spectrometer (8K channels covering a 7 MHz bandwidth) . ... Each spectrometer board handles two polarizations from one telescope beam.The baseband signals are to be digitized by four 8-bit ADCs at 100 Msamples/sec. ... Bandwidth: . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/alfa/galfa/docs/galspect/system/galfa_desc.html -- 7.9 Кб -- 18.07.2006
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14. Long description for frame layout example
This diagram illustrates a frame-like layout with 'position: fixed'. The illustration shows a four-panel frameset. The top panel ("header") covers the entire width of the frameset and takes up 15% of the vertical space. ... To the right of the sidebar and below the header is the "main" area, whose dimensions are computed based on remaining available space. Finally, at the bottom, the "footer" area is 100px high and covers the entire width of the frameset. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/css2/images/longdesc/frame-desc.html -- 2.0 Кб -- 01.05.1998
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15. http://xray.sai.msu.ru/~ivan/gmt/man/grdvolume.html
grdvolume - Calculating volume under a surface within a contour grdvolume grdfile [ -C cval or -C low / high / delta ] [ -L base ] [ -R west / east / south / north [ r ] ] [ -S [ k ] ] [ -T ] [ -V [ l ] ] [ -Z fact [/ delta ] ] grdvolume reads a 2-D binary grd file and calculates the volume contained between the surface and the plane specified by the given contour (or zero if not given). ... Alternatively, search using all contours from low to high in steps of delta . ... Default is no scaling]. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~ivan/gmt/man/grdvolume.html -- 4.7 Кб -- 19.03.1999
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16. http://www.eso.org/projects/dfs/to-do-list/fors-to-do-close.txt
LIST OF CLOSED ACTION ITEMS * ================================= Last update: Thu Jun 28 12:29:45 MET DST 2001 ---------------------------------------------------------------------------------------------- ID Chronological number. ... Type ACTION= for a normal action item; BUG= for an item related to a bug report; CHANGE= for an item related to a change request. ... 0010 FORS sbogun/Jan 2001 CHANGE LOW ?? ... 0002 FORS sbogun/Jan 2001 CHANGE HIGH 2001-03-05 SB DONE Update FORS User Manual. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/projects/dfs/to-do-list/fors-to-do-close.txt -- 5.4 Кб -- 28.06.2001
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17. Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare
... The standard science quicklook processing produces over a dozen sky maps at each downlink, and these maps are automatically searched for potential transient point sources. ... We have found that a heuristic modification of a formula derived by Li & Ma (1983) provides reasonably accurate estimates of p -values for point source detections even for very low p -value detections. ... Case 1u. The most straightforward approach uses the signal , where . ... To get a p -value, use . ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/theilerj.html -- 14.9 Кб -- 23.06.1998
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18. SKA-3 Experiment Description
... It consists of two energy-angle analyzers EA-2 and EA-3 for low energy particles, and two identical oppositely directed time-of-flight (TOF) analyzers EM-1-1 and EM-1-2 for high energies. ... Analyzers of low energy charged particles (EA-2 and EA-3). ... The instruments allow to measure simultaneously in eight angular sectors evenly distributed in the angle 2 perpendicular to the satellite rotation axis, and sequentially in 7 energy intervals for each angular sector. ... Interval . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/ska-3dscr.htm -- 5.4 Кб -- 07.08.1997
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/ska-3dscr.htm -- 5.4 Кб -- 07.08.1997
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19. High Energy Astrophysics Today and Tomorrow
... А.М. Белобородов (Колумбийский университет, США) . ... Рабочий язык конференции - русский. ... Е.М.Чуразов, д.ф .- м.н . А.А. Вихлинин, проф. д.ф .- м.н . М.Р.Гильфанов, д.ф .- м.н . М.Н.Павлинский, д.ф .- м.н . М.Г.Ревнивцев, д.ф .- м.н . С.Ю.Сазонов. д.ф .- м.н . М.Н.Павлинский (председатель), к.ф .- м.н . А.В.Мещеряков (зам. председателя), Н.Л.Александрович, к.ф .- м.н . В.А.Арефьев, к.ф .- м.н . Р.А.Буренин, П.Болдин, Н.П.Васильева, к.ф .- м.н . А.А.Воеводкин, В.Воробьев, А.Е.Елкин, ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/conf/hea2012/ -- 19.4 Кб -- 27.02.2014
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20. Description of algorithm
... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 28.12.2007
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 11.09.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/vch/Publications/Eng/html/NN/node2.html -- 11.5 Кб -- 02.10.2012
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