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1. Database of Optical Constants -- Level: welcome
The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/JPDOC/ -- 10.8 Кб -- 19.11.2010
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2. CREATE FULLTEXT CONFIGURATION
... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-createcfg.html -- 10.1 Кб -- 13.04.2008
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3. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
... A file upload element on an HTML form. ... JavaScript 1.1: added type property . ... The HTML INPUT tag, with "file" as the value of the TYPE attribute. For a given form, the JavaScript runtime engine creates appropriate FileUpload objects and puts these objects in the elements array of the corresponding Form object. ... form . ... For all FileUpload objects, the value of the type property is "file" . ... Use the value property to obtain the file name that the user typed into a FileUpload object. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm -- 19.0 Кб -- 07.10.1999
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4. casacore: casa::PoolStack< T, Key > Class Template Reference
... casa::PoolStack< T, Key > . ... PoolStack (const Key &key) . ... template<class T, class Key> . ... Referenced by casa::PoolStack< AutoDiffRep< Double >, uInt >::get() . ... Referenced by casa::PoolStack< AutoDiffRep< Double >, uInt >::key() . ... const uInt casa::PoolStack < T, Key >:: NDEF [static] . ... Referenced by casa::PoolStack< AutoDiffRep< Double >, uInt >::empty() , casa::PoolStack< AutoDiffRep< Double >, uInt >::get() , and casa::PoolStack< AutoDiffRep< Double >, uInt >::release() . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1PoolStack.html -- 31.8 Кб -- 14.02.2011
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5. CL Script for creating daily dark files
... CL Script for creating daily dark files . ... Data . ... The latter will ensure that one will also retrieve the appropriate "weekly bias" and "weekly dark" reference files. ... The parameter file should look like this: (Where basedark means the reference weekly dark ) infiles = Input dark image(s) to be combined/normalized basedark = Name of baseline superdark file (biasfile = ) Name of reference bias file to be used (outfile = day_ dark .fits ) Name of output normalized ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/design/software/analyzing/scripts/daydark -- 24.5 Кб -- 12.04.2016
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6. Data bases of Natural Satellites. Documentation. Structure
Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/DocStructe.htm -- 11.4 Кб -- 18.05.2009
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Еще в разделе: (Показать все результаты (>479) - lnfm1.sai.msu.ru/ )

7. *tprint* - Reading a Table File Created by imcnts
... Table files like the ones created in the section on imcnts can be displayed, printed and manipulated using the tasks contained in the stsdas.ttools package. ... sp> tables # Load the relevant package ta> tprint rp90_cnt prpar=yes # .tab extension assumed # the hidden parameter prpar is set to display the header # as well as the data ta> tprint rp90_cnt # Displays only the data info ta> tprint rp90_cnt prdata- prpar+ # Displays only the header info ta> tprint rp90_cnt prparam=yes | ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node99.html -- 4.6 Кб -- 01.10.2012
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8. http://www.eso.org/~qc/dfos/ABbuilder.txt
NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~qc/dfos/ABbuilder.txt -- 8.0 Кб -- 17.02.2006
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9. WAPP Signal Processing Page
The Wideband Arecibo Pulsar Processor Signal Processing Page . ... Raw Correlation . ... The WAPP uses custom digital hardware to create estimates of correlation functions from sampled data. The digital hardware used to estimate correlation function uses quantization to represent input . After creating an estimate of input correlation functions, the Wiener-Khintchine Theorem is applied to create estimates of input Power spectral density (PSD) and Stokes parameters . ... 3 Level . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~wapp/SignalProc/SPMain.htm -- 8.9 Кб -- 20.04.2000
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10. SEEING (V1.3) --- Apr00 --- SEEING (V1.3)
seeing -- Create a simulated ground-based star image based on a model of atmospheric turbulence seeing output xdim ydim gamma fwhmx fwhmy . output = "" [image] . The name for the output image to be created. xdim = 512 [integer] . The X dimension for the output image. ydim = 512 [integer] . The Y dimension dor the output image. gamma = 1.6666 [real] . ... For a discussion of the significance of this please see the discussion below and the references given. fwhmx = 5.0 [real] . ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/imres/seeing.hlp.html -- 4.0 Кб -- 06.06.2006
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11. AstroWeb -- Internet Resources for Astronomers
... R. E. Jackson . ... H.-M. Adorf . ... D. C. Wells . ... AstroWeb is a World Wide Web (WWW) interface to a collection of Internet accessible resources aimed at the astronomical community. ... The goal of AstroWeb is to be the most complete, up to date, and useful listing of Internet accessible astronomical resources available anywhere. ... Jackson, Wells, and Adorf noticed that they and others had created largely overlapping lists of Astronomical resources. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/jacksonr1.html -- 8.9 Кб -- 03.11.2000
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