. XMM-Newton Science Analysis System . tabcalc (dscalc-2.2.1) [xmmsas_20030110_1802-5.4.1] . Meta Index / Home Page tabcalc performs arbitrary calculations on table columns. tabcalc makes use of selectlib to perform arbitrary math on table columns. Any operation supported by selectlib is allowed. The name and type of the result column can be specified on the command line. If the result column exists, it will be overwritten. Subsections . Examples . XMM-Newton SOC/SSC -- 2003-01-10

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... 173Wall Peacock We catalogue the brightest extragalactic radio sources at 2.7 GHz. ... These data were originally presented in Wall and Peacock, MNRAS, 216, 173. The values in parenthesis include (units, datatype, example). 1 iauname Name of source in IAU convention (char7, example: '0320-37') . ... 3 ra_1950 rad Right ascension of source in radians (B1950) (real, example: 0.876068) . ... 9 alpha Spectral index of source between 2.7 and 5 GHz (real, example: 0.52) . ... Longair, 1975 . ...

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• WSRT deep surveys
• BOLOGNA (B3) catalog
• BOLOGNA B2-catalog

This diagram gives one visual rendering of a table that has been marked up especially for aural rendering. The table has a centered caption above it that reads "Travel Expense Report". ... In order to group information in a useful way, the table has a central column group with three columns, labeled "Meals", "Hotels", and "Transport" from left to right. The table's first column (to the left of the central column group) lists days of travel and labels these days with the city visited. ...

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• Long description of example illustrating precedence in the collapsing borders
• Long description of example of cell background calculation
• Long description for example showing how structurally overlapping cells are

... 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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... Classes . ... casa . casa::ScalarRecordColumnDesc . ... Class to define columns of scalar records in tables. ... ScalarRecordColumnDesc (const String &name) . ... ScalarRecordColumnDesc (const String &name, const String &comment) . ... ScalarRecordColumnDesc (const String &name, const String &comment, const String &dataManName, const String &dataManGroup) . ... name . ... ColumnDesc.cc registers such functions by using these constructors. virtual String casa::ScalarRecordColumnDesc::className . ...

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• casacore: casa::MSDataDescriptionEnums Class Reference

... 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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trend1d - Fit a [weighted] [robust] polynomial [or Fourier] model for y = f(x) to xy[w] data. trend1d -F < xymrw > -N [ f ] n _ model [ r ] [ xy [ w ] file ] [ -C condition _# ] [ -H [ nrec ] ] [ -I [ confidence _ level ] ] [ -V ] [ -W ] [ -: ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] trend1d reads x,y [and w] values from the first two [three] columns on standard input [or xy [ w ] file ] and fits a regression model y = f(x) + e by [weighted] least squares. ... E.g., a robust quadratic model is -N 3 r . ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/filter1d.html
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• http://xray.sai.msu.ru/~ivan/gmt/man/sample1d.html

... JavaScript 1.1 Plugin objects are predefined JavaScript objects that you access through the navigator.plugins array. A Plugin object is a plug-in installed on the client. ... For example, the following code displays the type and description properties of the first Plugin object's first MimeType object. myPlugin=navigator.plugins[0] . ... Description . ... The following code assigns shorthand variables for the predefined LiveAudio properties. var myPluginName = navigator.plugins["LiveAudio"].name . ...

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• mod_authn_dbd - Apache HTTP Server
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... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

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As described elsewhere, each file type known to SAOtng can have user-defined analysis commands associated with it. ... A help line describing the file types . ... If more than one marker analysis file is supplied to SAOtng via the -manalysis command switch (or the SAOTNG_MANAL environment variable), then the user can specify how to present marker analysis routines in the marker analysis menu using the -analformat command line option (or the SAOTNG_ANALFORMAT environment variable). ...

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... Observers may find that they wish to perform parts of the pipeline reduction again on their data using these tasks. Typical examples will be to re-perform cosmic ray rejection, altering the input parameters or using data from separate datasets, or to perform one-dimensional spectral extraction on long-slit data or to modify the input parameters (e.g., aperture extraction box, or background region) when doing one-dimensional spectral extraction for echelle data. ... Rectify spectral images. ...

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To get an overview of section 1 (one) of the manual: man 1 intro . ... This displays a one line synopsis of each command that has this keyword in its description. To search the online manual for a command with the phrase "copy files": man -k 'copy files' . ... To check what a command does: whatis more more, page (1) - browse or page through a text file . ... To display the manual page for the cp (copy files) command: man cp . ... To print the manual page for the man command: man -t man . ...

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• Getting a description of each command
• Checking the description of a command
• About commands

trackingtime- compute LST rise, transit, and set times for sources as well as time in the keyhole . trackingtime {--help --lim --sort --usecalib --usepsr --usex102 --usefluxgt1 --zamax=zamax --zamin=zamin --exclnorise} srcfile srcfile name of cima source file to process. ... exclnorise exclude sources that never rise. trackingtime is a shell script that calls idl routines to process the srcfile and output the lst rise, transit, and set times for each source in the file. ... Source Rises | ...

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• Manpage of MAP8BITTORF
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• Index of /~phil/hardware/pdev/fpga/gx/jfft/examples/pfb32

... Structure of Data . ... Catalog . ... The SAI OCL Catalog site provides several VO-enabled modes of operation: . VO-enabled catalog data analysis from a browser . ... Endpoint URL is http://ocl.sai.msu.ru/catalog/conesearch/ . ... VO-enabled catalog analysis from a browser . Presently, this recipe works with Firefox (Windows, MacOS, Linux), Internet Explorer (Windows) and Opera (Windows) browsers with Java plugin 1.6 installed. ... Main TOPCAT window with SAI OCL catalog loaded will appear. ...

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... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...

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• Description of the OOF software architecture Bojan Nikolic web pages (r. 329)

... Corrected geomagnetic coordinates | Let us consider as an example two numerical files with names tp.cng This files contain the information about INTERBALL Tail Probe and POLAR magnetic conjugations. ... The predicted magnetic conjugations correspond to the less then 5 deg geocentric angular distance between the footprints. ... dlt - the difference between two satellites corrected geomagnetic local times (on the second line), . ... GLAT (deg) - the satellite geographical latitude, . ...

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... 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 | ...

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• ALTER FULLTEXT ... OWNER
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• ALTER FULLTEXT CONFIGURATION

Name Last modified Size Description . Parent Directory - ppm/ 2009-02-10 15:26 - tif/ 2009-02-10 15:26 - . Apache/2.4.6 (Linux/SUSE) Server at www.astro.louisville.edu Port 80

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• Index of /software/astroimagej/examples

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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... The schedule assigned id (example: AS05) for your observing program. ... Use the time you started using the telescope including when you started taking calibrations. The time you opened for on sky observations can be entered later in the activity log. UTC End Time: . ... Focus Log: . ... The focus position can be obtained under the Telescope column of the System Status in ACP or from the run log. ... When all fields are filled out press this button to email the log to the ARCSAT and community. ...

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