... slconv (slconv-2.0) [xmmsas_20050815_1803-6.5.0] . ... Gaia region files are organised as a table of data, with additional information in the header which both specifies the source symbols and directs how their size and orientation should be calculated from the information in the table. ... To allow for greater flexibility however slconv allows the user to copy additional columns from the input FITS source list to the gaia region file. ...

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• Description

This diagram shows the six superimposed "layers" of the CSS table model. This diagram illustrates the algorithm for calculating a cell's final background. ... The diagram shows how, looking down on the six rectangles, one may compute the background color of each cell. ... A cell without a background color in the top layer is depicted as a "window" onto the lower layers, which give its final background color. ...

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• Long description of example illustrating background calculation
• Long description of example illustrating table row height calculations and
• Long description of example illustrating a table of travel expenses

... O.B Slee , Australia Telescope National Facility, CSIRO, Sydney bslee@atnf.csiro.au ----------------------------------------------------- ... ----------------------------------- 1- 8 A8 --- Name IAU name 9 A1 --- nFlag Flagged '*' or '#' 11- 12 I2 h RAh Right Ascension B1950 (hours) 14- 15 I2 min RAm Right Ascension B1950 (minutes) 17- 20 F4.1 s RAs Right Ascension B1950 (seconds) 22 A1 --- DE- Declination B1950 (sign) 23- 24 I2 deg DEd Declination ... Dulk, G.A. Slee, O.B. 1972, Aust. ...

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• All Sky Catalog at 2.7 GHz
• BOLOGNA B2-catalog
• Product Folder: TC213, 1024- X 512-PIXEL CCD IMAGE SENSOR

... The hydrogen line is the most pronounced absorption feature in spectra of B-type stars. Two effects play the dominant role in observed behavior of : the Stark broadening of the line absorption coefficient and interstellar absorption. ... Keywords: B-type stars, H I line, Stark effect, interstellar absorption . ... Thus having a good description of the Stark effect we investigated early B-type stars, where interstellar absorption may play an important role. ... 4 (IUE observations) and Fig. ...

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• About Tables
• HDF-S Flanking Fields Data Reduction / Technical Issues
• Reference File Descriptions Logs

... Classes . ... Derived MS and CalTable columns. More... class . ... Virtual column engine to return derived MS values. ... DerivedMC_module_internal_classes . Internal DerivedMC_module classes and functions. ... Class to handle derived columns in an MS or CalTable. A MeasurementSet or CalTable can be extended with virtual columns to be able to use hourangle, azimuth/elevation, parallactic angle, and UVW as if they were stored in the table using the DerivedMSCal virtual column engine. ...

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• casacore: casa::UDFMSCal Class Reference
• casacore: casa::StandardStMan Class Reference
• casacore: casa::TableParseUpdate Class Reference

Each file type known to SAOtng can have user-defined analysis commands associated with it. ... A help line describing the file types . ... For example, the default analysis file currently contains the following: # # Analysis command descriptions: # help # file templates # file types # analysis command line counts -- number of events in region (no background) *.qp *.imh QPOE IMH uiraf '${xraybin}'/x_xspatial.e imcnts source='${filename}' region=$sregion bkgd=0 table=NONE | ...

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• The Chandra Multiwavelength Project (ChaMP) - Spectra
• Table Filtering with Indexes
• The Chandra Multiwavelength Project (ChaMP)

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

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• Yu. Burman: Publications

Up: DATA ANALYSIS Previous: More Analyz Stuff . In this section we describe some useful routines for quick-look on-line analysis of your data. For a complete description of the routines, and for a description of analyzing HI spectra, look at the Spectral Line Appendices. ... cd a9999 [or whatever your project number is . ... corinfo = List the current set-up parameters. ... That is, if you want to look at the second data dump of scan number 57401, you `just' type ``corget 57401.00002". ...

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• GALFA System Description
• DATA ANALYSIS
• Project Description

... A technique allowing automatic representation by a relatively small number of independent parameters based on the principal component analysis of data sequences is presented. ... In recent years the spectrum of observed astronomical data can be characterized as greatly varied. ... In this instance, the problem of initial description and classification of newly-observed data becomes most urgent, especially if there is a lack of preliminary observational material and theoretical expectations. ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• An Infrared Camera Reduction/Analysis Package
• The SRON-HeaD Data Analysis System

... Description . Catalog . ... In the Catalog, we publish equatorial (ЮБ 2000 , ЮД 2000 ) and galactic (l,b) coordinates of cluster centers derived as the position of overdensity in 2MASS catalog (Koposov et al. ... Distances, color-excesses and ages are the mean-square values calculated using all available evaluations from different color-magnitude diagrams. ... There are individual pages for every cluster where all available plots and parameters are published. ... 2002). ...

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• SAI OCL Catalog Virtual Observatory

pshistogram - Bin data and plot histograms pshistogram file -Jx xscale [/ yscale ] -W bin _ width [ -2 ] [ -A ] [ -B tickinfo ] [ -C ] [ -E azimuth / elevation ] [ -G fill ] [ -H[ nrec ] ] [ -I[o] ] [ -K ] [ -L pen ] ... [r] ] [ -S ] [ -U[ / dx / dy / ][ label ] ] [ -V ] [ -X x - shift ] [ -Y y - shift ] [ -Z type ] [ -c copies ] [ -bi[s][ n ] ] pshistogram reads the first column from file [or standard input ] and calculates ... L Draw bar outline using the specified pen thickness. ...

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• Parameters of binary compact star evolution

... Here is an example of the output header of CATS data. ... SIMPLE=T / BITPIX=8 / character information NAXIS=0 / no image data array present EXTEND=T / may be standard extensions OBJECT= CATS SEARCH / CATS search result ORIGIN=SAO RAS DATE=01/01/1997 / date of file creation END XTENSION=TABLE / F-file table extension BITPIX=8 / 8-bits ... NAXIS1=93 / No. of characters per row NAXIS2=1000 / the number of lines (sources) TFIELDS=10 / there are 16 fields per row EXTNAME= CATS / object name: ...

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• SCORPIO-2 project: description
• Description of algorithm
• comedi_poll

... 1) Our CAS system will store the catalogues. ... Each catalogue should contain one or more tables. 2) The names of the catalogues should be unique, as well as the the names of tables of the SAME catalogue. ... 4) All the metadata about the CAS system, its tables, catalogues should reside in separate schema (currently "cas_metadata"). 1) The main system table of CAS is the table "catalog_list". ... short info (column "info") . ... 2) The second system table of CAS is the table "table_list". ...

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• ALTER FULLTEXT CONFIGURATION
• ALTER FULLTEXT MAPPING
• ALTER FULLTEXT ... OWNER

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. ...

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• Midas

... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...

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• ASCII files description
• Space physics cordinate systems
• SKA-3 Experiment Description

... Classes . ... Class List . Class Hierarchy . Class Members . Dust :: AttSlab . include < attslab.hxx > . Collaboration diagram for Dust::AttSlab: . ... AttSlab ( RadField *InputRF, BNLib::UnaryDD *AbsXSect) . RadField * . MkRF (double n) . Calculate the attenuated radiation field as a function of column density . RadField * Dust::AttSlab::MkRF . double . ... Return the radiation field at column density n into the slab . ... attslab.hxx . attslab.cxx . ...

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• The history of star formation and mass assembly in early-type galaxies Bojan
• Galaxy Evolution Bojan Nikolic web pages (r. 329)
• DUST: dustiface.h File Reference

Chair of solid state physics . ... The most important concepts of the modern crystallography, crystal symmetry and methods of crystal structure determination are considered. ... The main experimental aims of X-ray diffraction study of classic crystal structure and real structure are analyzed. ... Crystal lattice. ... The main diffraction schemes in representation of a reciprocal lattice: Laue method, powder diffraction method, oscillation method, X-ray diffraction on powder sample and single crystal. ...

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• X-Ray Structural Analysis

The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

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• moveProducts
• pyQC: script structure
• updateAB

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

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• FADPS - Flexible Astronomical Data Processing System

Stellarium 0.12.3 . ... TelescopeClient Class Reference abstract . ... getEnglishName (void) const . ... getInfoString (const StelCore *core, const InfoStringGroup &flags) const . ... getJ2000EquatorialPos (const StelCore *core) const =0 . ... getEquinoxEquatorialPos (const StelCore *core) const . ... getJ2000GalacticPos (const StelCore *core) const . ... getSideralPosGeometric (const StelCore *core) const . ... getPositionInfoString (const StelCore *core, const InfoStringGroup &flags) const . ...

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• Stellarium: StelQGL1InterleavedArrayVertexBufferBackend Class Reference
• Stellarium: StelQGL1ArrayVertexBufferBackend Class Reference
• Stellarium: StelQGL2InterleavedArrayVertexBufferBackend Class Reference