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http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-02.pdf.
http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-02.pdf.
21. http://www.eso.org/projects/dfs/team/QA-code-review-form.doc
... Readability |Check number: 1 | Description: Header existence for each |Evaluation (always/often/sometimes/| |source file and for each method, class, |never) : | ... Description: Naming conventions existence |Evaluation (always/often/sometimes/| |(variables start with lowercase, then |never) : | ... limited and commented |(always/often/sometimes/ | ... Description: Error message are formated : when an|Evaluation | error or an exception is raised, report the |(always/often/sometimes/ | ...
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Ссылки http://www.eso.org/projects/dfs/team/QA-code-review-form.doc -- 128.5 Кб -- 29.09.2003
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22. Maximum limits
... The planning and reduction programs are distributed with array sizes set large enough to let most observers work without difficulty. However, you might need to reduce a very large data set, or to deal with a very large number of passbands (9 is the nominal limit). ... The main problem is holding the matrix of normal equations during the iterations; on the other hand, star catalogs can be made quite large without paying much of a price in terms of performance. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node304.html -- 6.8 Кб -- 23.02.1996
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23. Armagh Observatory
... August was noteworthy by having the least number of hours of bright sunshine for at least 128 years, that is, since sunshine records began at the Observatory in 1880. ... The month was also exceptionally wet, with rainfall totaling 151.4mm (5.96 inches), nearly twice the average figure (around 81 mm) for August and the seventh wettest August at Armagh since rainfall records began at the Observatory in 1838. In order to find a wetter August we have to go back 52 years, to August 1956. ...
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Ссылки http://star.arm.ac.uk/press/2008/Weather_Aug08.html -- 4.5 Кб -- 02.09.2008
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24. http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20130506.en.txt
THE RELATIVE MONTHLY MEAN SUNSPOT NUMBER ON APRIL 2013 HAS MADE W apr.= ... THE INTERNATIONAL DAILY VALUE OF RELATIVE SUNSPOT NUMBER FOR 2013, APRIL ACCORDING DATA OF 70 SOLAR OBSERVATORIES HAS MADE 1.. 53 m 6.. ... Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 29.04 - 05.05.2013 , Forecast on 06.04 - 13.05.2013, Carrington Rotations 2136 (17,78.04.2013) SUNSPOT-FORMING ACTIVITY OF THE SUN CHANGED FROM THE AVERAGE TO THE HIGH LEVELS. ... Class E(1-8A) AR RII/IV CME X / opt. ...
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Ссылки http://www.izmiran.rssi.ru/services/saf/archive/en/2013/obzor20130506.en.txt -- 7.8 Кб -- 06.05.2013
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25. http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS10.html
ARCSAT ID NUMBER: AS10 DESCRIPTIVE TITLE: A New Filter to Study Stellar Populations. ... BRIEF SCIENCE JUSTIFICATION: We propose to use a newly designed filter (named W: 845-880-nm) to measure the [ЮБ/Fe] ratio in red giants and trace the chemical evolution of stars in the Milky Wayт??s globular clusters, halo and Local Group galaxies. ... We will use the newly-acquired 2т??x2т?? filter from Manastash Ridge Observatory to start observing globular clusters. ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2014/AS10.html -- 3.5 Кб -- 08.10.2014
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26. http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HOsborn.pdf
Detecting Long Period Planets with WASP 1 University of Warwick, Gibbet Hill Road, Coventry, CV4 7AL To estimate the number of transiting planets in this period range, planetary occurrence rates from Kepler (Fressin et al, 2013) for varying spectral type & planet type were used. ... Two `stare' fields are currently available from 2011 (330,000 stars) producing a detection rate of 3.0±2.4 planets (Fig 4). ... Since 2011, WASP-N cameras have observed in `Stare' mode, with cadence of ~1-2min. ...
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Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/HOsborn.pdf -- 292.9 Кб -- 16.04.2014
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27. Three Is A Magic Number
... Three is a magic number. ... You get three as a magic number. ... Give you three. That's a magic number. It takes three legs to make a tri-pod or to make a table stand. ... When it's three you can see it's a magic number. ... Multiply backwards from three times ten.> Three time ten is.. ... Three times nine is.. ... Three times six is 18, three times five is 15 . Three times four is twelve . And three times three is nine and three times two is six. ... Yeah> That's a magic number. ...
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Ссылки http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/s/schoolhouse.rock/3.html -- 3.8 Кб -- 09.04.1995
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28. (Untitled)
There are six possible ways of object description: . a) by number(s) . ... d) by list . e) by orbital elements . ... They should be introduced as year, month, day with tenth (e.g. 20021104.1). d) Computations are performed for all objects listed in the file whose path and name should be introduced into assigned data field. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ...
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Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user9hdg.htm -- 6.7 Кб -- 10.04.2016
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29. Optimization of spectroscopic observations
... Let us first find out which way -- rise in spectral resolution with some loss in the S/N ratio or increase in the S/N ratio with a fixed spectral resolution -- is better for the purpose of reduction of equivalent width determination errors. ... N -- number of counts for 1 ? ... line equivalent width, . ... Thus if the spectral resolution is managed to be increased (i.e. to decrease )without loss in the number of counts falling at 1 ?, the equivalent width measurement error is then proportional to . ...
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Ссылки http://mavr.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 02.10.2012
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 01.10.2012
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 01.10.2012
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/ssl/PFES/node2.html -- 13.9 Кб -- 01.10.2012
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30. Population Synthesis of X-ray Sources at the Galactic Center
Next: The Model Up: No Title Previous: Radiopulsars as Sources of . In this section, we study the evolution of stellar populations on a time-scale of 10 Myr for a starburst љ occurring under conditions similar to those in the Galactic Center (see Lipunov et al. (1995d)[ 126 ]). We estimate the expected number of X-ray transient љ sources (NS + MS star), super accreting BH, and BH + supergiant binaries, all as functions of time elapsed after the burst. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node72.html -- 6.7 Кб -- 01.03.1997
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31. Apache Server Virtual Host Support
When using a large number of Virtual Hosts, Apache may run out of available file descriptors (sometimes called file handles if each Virtual Host specifies different log files. ... Unix operating systems limit the number of file descriptors that may be used by a process; the limit is typically 64, and may usually be increased up to a large hard-limit. ... If you system falls into 1 or 2 (above), then increase the file descriptor limit before starting Apache, using a script like #!/bin/sh . ...
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Ссылки http://neptun.sai.msu.su/manual/vhosts/fd-limits.html -- 3.7 Кб -- 20.06.2002
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32. http://www.asc.rssi.ru/RadioAstron/ao-1/radioastron_ao1_proposal_template.pdf
RadioAstron AO-1 prop osal Submission dead line: February 8, 23:59 UT. ... Team contact name and e-mail address: Ivan Petrov (e-mail: Ivan.Peterov@gmail.com ) Total observing time request: 100 hrs Number of independent observing segments and typical range of pro jected baselines required: 20 (3-30 Earth diameters) Specific dates and time intervals requested : If your experiment requires specific dates and UT ranges, please, indicate them: February 1, 2014: 08:00-16:00 UT -- M87 imaging ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/ao-1/radioastron_ao1_proposal_template.pdf -- 36.5 Кб -- 22.01.2013
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33. Quicksand As Black Hole Model? - an Astronomy Net Blackholes Forum Message
Blackholes Forum Message . ... Quicksand As Black Hole Model? ... For the hole to be black it must have a fuzzy edge i.e. something one is sinking into (like a black hole is like quicksand that you discover by sinking partly into it?) ... A number of oranges "probes" what it is to be an orange so "black hole" = "number" you might suppose. ... The rest of their body not in the quicksand (i.e. not in the black hole) equates to the "collection of anti-matter near the blackhole"? ... www.astronomy.net . ...
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Ссылки http://www.astronomy.net/forums/blackholes/messages/6651.shtml -- 16.7 Кб -- 09.04.2016
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34. jg0007
... 1915QB4_C22v12p1___ Informations. relative to: J1-Io: 201, J2-Europe: 134, J3-Ganymede: 85 reference frame: astrometric centre of frame: topocentre epoch of equinox: date time scale: GMT (UT1=GMT+12h) reduction: no information coordinates: apparent distance, position angle diff. refraction: removed receptor: heliometer telescope: Refractor, F = 2.5 m, D = 17.8 cm observers: Gill David, Finlay W.H. data included in standard data file: no Comments. no information Format. ... Year of the observation 4....
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Ссылки http://lnfm1.sai.msu.ru/neb/nss/OBS_COLL/J/jg0007.html -- 3.3 Кб -- 22.06.2004
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35. Pulkovo Astrometrical Plate Database
Pulkovo Photographic Plate Database . To find a certain plate, type its number, choose instrument and click button FIND Instrument: Normal Astrograph 26-inch refractor Plate number: . To find plates with a certain sky area: choose instrument, type coordinates (R.A. and Dec.) of the center of this area, type radius of this area, type (optionally) names of required objects, and click button FIND . ...
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Ссылки http://www.puldb.ru/db/plates/index.php -- 6.7 Кб -- 01.10.2012
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36. JavaScript Random Number Tester
Minimum: 0; Average: 47; Maximum: 99 . Results divisible by: . 2: 52%, 3: 33%, 4: 25%, 5: 21%, 6: 18%, 7: 14%, 8: 12%, 9: 13%, . Range . Graph . Pct . Count . 10 . 6 . 25 . 20 . 11 . 43 . 30 . 11 . 42 . 40 . 12 . 46 . 50 . 9 . 35 . 60 . 12 . 47 . 70 . 11 . 42 . 80 . 8 . 31 . 90 . 8 . 32 . 100 . 11 . 42 .
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Ссылки http://www.sai.msu.su/~megera/tips/randtest.htm -- 3.4 Кб -- 20.08.1996
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37. Winer Observatory Benefactors
Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Winer Observatory gratefully acknowledges the generous support of those listed below. ... We thank our donors and hold them up as models of how corporations in America can behave responsibly in the communities in which they do business. ... Telescopes, parts, and accessories . ... 100,000 . ... Hughes Missile Systems . ... Miscellaneous electronics . ... Terra Universal, Inc. ... EFI Electronics Corp. ... 2013 Winer Observatory. ...
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Ссылки http://www.winer.org/Donors/Honor_Roll.php -- 22.4 Кб -- 09.04.2016
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38. XWare > APOD
... Leonid Meteors Streak . ... The 2004 Leonids meteor shower had its ups and downs. ... Spiral Galaxies in Collision . ... Stereo Phobos . ... Get out your red/blue glasses and float next to Phobos, grooved moon of Mars! ... Phobos: Doomed Moon of Mars . ... Mars, the red planet named for the Roman god of war, has two tiny moons, Phobos and Deimos, whose names are derived from the Greek for Fear and Panic. ... How old is this galaxy? ... The 1999 Leonids Meteor Shower came to an impressive crescendo. ...
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Ссылки http://www.astronet.ru/db/xware/apod.html?page=47&d=2006-02 -- 14.8 Кб -- 12.04.2016
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39. http://www.gao.spb.ru/english/publ-s/viii-rfs/p133.pdf
Instruments and Methods 133 Sky temperature resolution by microwave radiometry A.G. Kislyakov State University, Nizhny Novgorod, Russia Introduction The threshold sensitivity of a radiometer is determined by well known equation Karlov & Manenkov, 1966 " hE i = h hn i +1 hn i + N t G0 , 1 G0 1=2 : 1 Here we denote hE ias the minimum detectable increment of radiation spectral density E at a frequency . ... Equation 3 gives a correction to the expression for limit detector sensitivity Kislyakov, 1997. ...
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Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p133.pdf -- 132.7 Кб -- 21.05.2007
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40. SAO RAS - Telescopes - BTA - MSS
... Telescopes . ... The spectrograph is installed in the Nasmyth focus of the BTA telescope, the equivalent focal length is 186 m (F/31). ... The preslit device unit is marked by number 3. ... Fig. ... slit unit of the MSS, 4.1 ? ... The spectrograph slit unit consists of a mirror that redirects the light beam from the Z axis and from the calibration path at an angle of 65њ to the axis of the telescope focus into the slit, the order separation filter, the block of the slit and the shutter (Item 4 in...
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Ссылки http://www.sao.ru/hq/lizm/mss/en/tech.html -- 16.7 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://mavr.sao.ru/hq/lizm/mss/en/tech.html -- 16.7 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://mavr.sao.ru/hq/lizm/mss/en/tech.html -- 16.7 Кб -- 10.04.2016
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