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http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/Sinusoid1DParam_8h_source.html.

1. casacore: casa::Sinusoid1DParam< T > Class Template Reference
... Classes . ... Class List . ... casa . casa::Sinusoid1DParam< T > . ... Parameter handling for one dimensional Sinusoid class. ... AMPLITUDE , . PERIOD , . ... Sinusoid1DParam (const T &amplitude) . Sinusoid1DParam (const T &amplitude, const T &period) . Sinusoid1DParam (const T &amplitude, const T &period, const T &x0) . ... Copy constructor (deep copy). template<class W > . ... T casa::Sinusoid1DParam < T >::amplitude . ... virtual const String & casa::Sinusoid1DParam < T >::name . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/classcasa_1_1Sinusoid1DParam.html -- 33.2 Кб -- 14.02.2011
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2. Stellarium: StelScriptMgr Class Reference
... StelScriptMgr Class Reference . ... const QStringљ . ... Stops any running script. ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getDescription . ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getLicense . ... Get the rate at which the script is running as a multiple of the normal execution rate. void StelScriptMgr::pauseScript . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelScriptMgr.html -- 32.4 Кб -- 28.02.2014
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3. Uses of Class ij.macro.Program (ImageJ API)
... Class . Use . ... Packages that use Program . ij.macro . ... Uses of Program in ij.macro . Methods in ij.macro that return Program . ... Tokenizer. tokenize (java.lang.String program) . Uses a StreamTokenizer to convert an ImageJ macro file into a token stream. ... Interpreter. run ( Program pgm) . ... Interpreter. runMacro ( Program pgm, int macroLoc, java.lang.String macroName) . ... MacroRunner ( Program pgm, int address, java.lang.String name, java.lang.String argument) . ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/macro/class-use/Program.html -- 13.5 Кб -- 02.12.2010
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4. HyperLEDA documentation: parameter: lc
The luminosity class introduced by Van den Bergh (1960) has been numerically coded between 1 and 9 with the extension introduced by H.G. Corwin (SGC, 1985) between 9 and 11. The luminosity class is coded on a continuous scale which is related to the original classification as: . The original nomenclature was chosen to match the Yerkes system of stellar luminosities. HyperLeda . Questions: prugniel@obs.univ-lyon1.fr
[ Сохраненная копия ]  Ссылки http://www.sao.ru/fetch/HL/leda/param/lc.html -- 2.7 Кб -- 23.12.2013
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5. lsst.coordConv: coordConv::OtherCoordSys Class Reference
lsst.coordConv љ unknown . ... Classes . ... coordConv::OtherCoordSys Class Reference . ... OtherCoordSys (std::string const &name, double date=0, DateTypeEnum dateType= DateType_None , bool isMean =false) . ... virtual Coord љ . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom ( CoordSys const &fromCoordSys, Coord const &fromCoord, Site const &site, double tai=0) const . ... virtual Coord coordConv::OtherCoordSys::removePM . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/coordConv/html/classcoord_conv_1_1_other_coord_sys.html -- 47.5 Кб -- 07.05.2015
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6. Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/kearnsk.html -- 12.3 Кб -- 03.11.2000
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7. A More Complete Picture of the Blazar Class
. Next: FSRQs Up: THE DEEP X-RAY RADIO Previous: Redshift Distribution . DXRBS' unique combination of a dual X-ray/radio survey method and high sensitivity has opened up important, large new regions of parameter space for both blazar sub-classes, within which a large fraction of our sample (nearly 50%) lie. This section is devoted to discussing these discoveries and their impact upon our understanding of the blazar class. љ . FSRQs . BL Lacs . Paolo Padovani . 1/5/1998
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ppadovan/survey/dxrbs_paper/node13.html -- 3.5 Кб -- 03.12.2003
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8. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/javobj.htm
... The type of a wrapped Java object accessed from within JavaScript code. ... Instantiating a Java object in JavaScript. The following code creates the JavaObject theString , which is an instance of the class java.lang.String : var theString = new Packages.java.lang.String("Hello, world") Because the String class is in the java package, you can also use the java synonym and omit the Packages keyword when you instantiate the class: var theString = new java.lang.String("Hello, world") Example 2. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/javobj.htm -- 6.5 Кб -- 07.10.1999
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9. DUST: rastsizedist.hxx File Reference
. Main Page . Related Pages . Classes . Files . #include <valarray> . #include <interpolate_forwd.hxx> . Include dependency graph for rastsizedist.hxx: . This graph shows which files directly or indirectly include this file: . Go to the source code of this file. namespace . Dust . class . Dust::RastSDS . Bojan Nikolic < bojan@bnikolic.co.uk >, < b.nikolic@mrao.cam.ac.uk > . Collect all size -distribution parameters in one place . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/devman/dust/rastsizedist_8hxx.html -- 3.6 Кб -- 11.07.2008
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10. covar2ellipse.pro (JWST Pipeline routines in IDL)
... use frames summary class fields routine details file attributes . ... AUTHOR: Craig B. Markwardt, NASA/GSFC Code 662, Greenbelt, MD 20770 craigm@lheamail.gsfc.nasa.gov UPDATED VERSIONs can be found on my WEB PAGE: http://cow.physics.wisc.edu/~craigm/idl/idl.html . PURPOSE: Compute confidence limits for chi-square statistic . ... CALLING SEQUENCE: DELCHI = MPCHILIM(PROB, DOF, [/SIGMA, /CLEVEL, /SLEVEL ]) . ... result = mpchilim( p , dof , sigma= sigma , clevel= clevel , slevel= slevel ) . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~robberto/Main/Software/IDL4pipeline/covar2ellipse.html -- 25.9 Кб -- 27.02.2014
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11. http://www.naic.edu/~phil/hardware/byuPhasedAr/rfischercode/userhelp.txt
... The telescope functions available in the array_pointing module are take_antenna_control() release_antenna() track ( object , duration , cross_el_offset= 0.0 , el_offset= 0.0 ) box( object , increment, box_num, duration ) box_set( object , increment, num_boxes, duration , repeat_on=True) raster( object , increment, max_x, max_y, ... The tracking duration begins after the telescope has reached the commanded position. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/hardware/byuPhasedAr/rfischercode/userhelp.txt -- 7.2 Кб -- 27.01.2010
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12. Output
. Next: Used CAL State Variables Up: Calling Parameters Previous: Input Contents . Efficiency . - An array of detection efficiency, real values between 0.0 and 1.0 for all events which should be detectable at the energy bins, spatial location and event pattern sub class required . Michael Smith 2011-09-20
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node134.html -- 3.2 Кб -- 20.09.2011
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Еще в разделе: (Показать все результаты (>13420) - xmm.vilspa.esa.es/ )

13. Astronomy Ireland's Evening Classes to begin on 8 October | International Year
... Astronomy: what is our place in the Universe? Wed 14 October . ... Donegal and Blue Stacks Festival 2009: happening right now! ... Astronomy Ireland's Evening Classes begin this Thursday, October 8, and are taking place at 10 locations nationwide. ... For more details of the classes you can see www.astronomy.ie/class . ... Thursday - October 8 - Dundalk - This lecture will take place in Dundalk to launch the October Evening Classes. ... International Year of Astronomy, Ireland National Node . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/scholars/iya/local/astronomy-classes.html -- 9.9 Кб -- 31.12.2009
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14. Ask Astro web extra: Will all white dwarfs, regardless of the class of star
... Subscriber Extras . ... Ask Astro . Web Extras . ... Behemoth black hole found in an unlikely place . ... black holes . ... Globular cluster NGC 2808, elliptical galaxy NGC 2986, and the Sextans Dwarf . ... Ask Astro web extra: Will all white dwarfs, regardless of the class of star that produced them, eventually become black dwarfs? ... Get instant access to subscriber content on Astronomy.com! ... Receive full access to our Ask Astro answers . BONUS web extras not included in the magazine . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/2010/12/ask-astro-white-dwarfs-to-black-dwarfs -- 62.7 Кб -- 10.04.2016
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15. Starspots
... Simulations were also carried out to quantify the range in parameter space which could be filled by stars varying in accordance with the spot hypothesis. ... First, an unspotted star was produced. To do this, colors of a given spectral type (taken from Bessell and Brett 1992) were converted to fluxes for a normalized distance. ... To simulate spots, between five and 40 of the grid locations were refilled with values corresponding to temperatures between 100K and 1000K cooler than the photosphere. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/period/node8.html -- 7.1 Кб -- 02.10.2012
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16. Initial Distributions of Binary Parameters
Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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17. http://www.stecf.org/conferences/adass/adassVII/reprints/christliebn.ps.gz
... Classification models A classification model (CM) consists of the following components: Class definitions are given by means of a learning sample, implicitly including the number N and names of the defined classes. ... Optimal loss factors In case of classification aim (3) a set of three optimal loss factors -- weights for di#erent kinds of misclassifications -- has to be stated (Christlieb et al. 1998). ... The classification of spectra of unknown classes can then be carried out under MIDAS. ...
[ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/christliebn.ps.gz -- 136.0 Кб -- 12.06.2006
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18. Help
... Documentation for the Python objects defined by the project is divided into separate pages for each package, module, and class. The API documentation also includes two pages containing information about the project as a whole: a trees page, and an index page. ... A description of the package. ... A summary of the classes defined by the package. ... The module contents frame contains a list of every submodule, class, type, exception, function, and variable defined by a module or package. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~mwhite/pynifs-doc/help.html -- 11.5 Кб -- 27.02.2014
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19. AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb
... Home Education Classes AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . ... Classes . AAA Fall Astronomy Class: Astronomy Basics тАУ October-November 2015 . AAA Winter Astronomy Class: Measuring Distances in Space тАУ Dec 2015 тАУ Feb 2016 . AAA Spring Astronomy Class: The Physics of Astronomy тАУ February - March 2016 . ... This MonthтАЩs Sky тАУ April 2016 . ... Dec. ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ...
[ Сохраненная копия ]  Ссылки http://www.aaa.org/education/classes/aaa-winter-astronomy-class-measuring-distances-in-space-dec-2015-feb-2016/ -- 100.6 Кб -- 10.04.2016
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20. http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf -- 2427.5 Кб -- 30.11.2014
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