Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... ClassљIndex . ... StelIndexBuffer Class Reference abstract . Generic index buffer interface usable with all Renderer backends. ... virtualљ . ... voidљ . addIndex (const uint index) . ... virtual voidљ . ... index . ... virtual void StelIndexBuffer::addIndex_ . ... virtual void StelIndexBuffer::clear_ . ... virtual void StelIndexBuffer::lock_ . ... virtual void StelIndexBuffer::setIndex_ . ... virtual void StelIndexBuffer::unlock_ . ...

lsst.coordConv љ unknown . ... Classes . Files . ... Site . ... coordConv::Site Class Reference . ... Site (double meanLong , double meanLat , double elev ) . ... site longitude, ignoring pole wander (deg, positive eastward) More... љ . ... Definition at line 10 of file site.h . coordConv::Site::Site . ... double coordConv::Site::azCorr . ... double coordConv::Site::corrLat . ... double coordConv::Site::corrLong . ... double coordConv::Site::diurAbMag . ... double coordConv::Site::elev . ...

... Classes . ... casa::UDFMSCal . ... static UDFBase * . makeHA (const String &) . ... static UDFBase * casa::UDFMSCal::makeAZEL1 . ... static UDFBase * casa::UDFMSCal::makeAZEL2 . ... static UDFBase * casa::UDFMSCal::makeHA . ... Function to create an object. static UDFBase * casa::UDFMSCal::makeHA1 . ... static UDFBase * casa::UDFMSCal::makeHA2 . ... static UDFBase * casa::UDFMSCal::makeLAST . ... static UDFBase * casa::UDFMSCal::makeLAST1 . ... static UDFBase * casa::UDFMSCal::makeLAST2 . ...

... Classes . ... Dust :: ThinShell . ... ThinShell (double *energy, double *lum, double R , size_t n) . ThinShell (std::valarray< double > & energies , std::valarray< double > & speclum , double R ) . ... std::valarray< double > . energies . Array of energies at which the luminosity is known. std::valarray< double > . ... energy , . ... Energy array should be in units of Joules. ... References energies , and speclum . ... More precisely this is energy per unit volume per unit energy interval. ...

... GPI Data Pipeline 1.0 documentation . GPI Data Pipeline Developer?s Guide . ... Editing Documentation (Including this Website) . ... Show Source . ... The documentation source code is available as part of the pipeline source code, in the documentation subdirectory inside the pipeline root. ... Pipeline primitive documentation is taken semi-automatically from the pipeline primitive headers in IDL, including the structured header comments used to populate the pipeline?s primitives config file. ...

... The DD tag element specifies a term definition, and follows one or more DT elements. ... CLASS . ... The CLASS attribute is most commonly used to attach a different style to some element, but it is recommended that where practical class names should be picked on the basis of the element's semantics, as this will permit other uses, such as restricting search through documents by matching on element class names. ... CLEAR . ... The CLEAR attribute allows you to move down unconditionally: . ...

... Class . Use . ... Packages that use ImageStatistics . ... Returns an ImageStatistics object generated using the specified measurement options and histogram bin count. ... Returns an ImageStatistics object generated using the specified measurement options, histogram bin count and histogram range. ... Draws the histogram using the specified title and ImageStatistics. ... ParticleAnalyzer. drawParticle ( ImageProcessor drawIP, Roi roi, ImageStatistics stats, ImageProcessor mask) . ... class . ...

... 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. ...

The position of the objects on the sky were generally measured to a precision between 1 and 4 arcsec. ... For the stars, the position is always at epoch 2000, whatever J2000 or B1950 coordinates are printed. ... The celestial position is given as coordinates in 4 different systems: . ... B1950 . ... Galactic coordinates in the reference frame called "new" system, adopted by IAU in 1958. Galactic pole at B124900.0+272400, node at ra=282.25,l=33 deg (inclination 62.6 deg). ... 1 arcsec . ...

The current Java Class Library for access to FITS files was designed for the VLT Data Flow System pipeline subsystem. ... all types of headers are decoded, . ... As the code has not been optimized, data access is slow e.g. on a 160 MHz machine and no JIT, 32-bit real images are read at 50k values/sec, 16-bit integer images at 80k values/sec while table data are read at 10k values/sec. FITS keywords are decoded at a rate of 2-3k keywords/sec depending significantly on their types. ...