... Columns RA_CORR and DEC_CORR are only passed to the output summary source lists, when srcmatch is used on only one source list. ... Additionally, the number of entries per row for a given column can also be retrieved from the FITS keyword TDIMi (i being the column index). srcmatch will pass on the columns RA_CORR and DEC_CORR (generated by eposcorr ) from the input X-ray source list to the summary output list, only if the number of input source lists is 1 . ...

. The input SHELTRAN source deck follows the normal FORTRAN layout rules, apart from the above-mentioned features. No indentation of structures need to be included, as the pre-processor will automatically provide indentation in the listing. The output source deck consists of the input source deck plus the necessary generated FORTRAN statements. It contains no Comment, Eject or Note lines. The output deck is not indented.

... The quickest way to learn how each observation was performed is to use the iminfo task in the STSDAS toolbox.headers package to look at the headers of the science data. ... Number of extensions . ... Given that NICMOS data files contain multiple extensions, the number of the desired extension must always be specified. ... In order to simplify access to NICMOS FITS image extensions, each extension header contains the two keywords: EXTNAME (extension name) and EXTVER (extension version number). ...

Next: *tabplot* - Displaying a Up: Radial Profiles and Projections Previous: Radial Profiles and Projections . Obtain a radial distribution of counts for the source centered at x = 503, y = 513, in the data image xdata$snr.qp . The background is taken locally from an annulus outside the source region. ... Region descriptors can also be given on the command line, but they must be enclosed by quotes. xs> imcnts xdata$snr ``a 503 513 0 50 n=5'' . ...

... Apache HTTP Server Version 2.4 . ... Filter Input (request) and Output (response) content using sed syntax . ... sed_module . ... mod_sed is an in-process content filter. ... However, unlike sed , mod_sed doesn't take data from standard input. Instead, the filter acts on the entity data sent between client and server. mod_sed can be used as an input or output filter. mod_sed is a content filter, which means that it cannot be used to modify client or server http headers. ... mod_sed . ...

specpsf -- Form a longslit spectrum for a point source from many point spread function images specpsf refima psfwavs psfims sliwid pixwid subsam cenoff psfpos outpsf . ... The name of the input 2-dimensional reference image to supply the dimensions and header information for the output longslit Point Spread Function (PSF) spectrum image. psfwavs = "" [table file name] . ... The centre of the Point Spread Function in each input image is determined by centroiding and the slit is placed over the image. ...

... psrfits2fil converts AO psrfits files from the pdev spectrometer to sigproc filterbank program. This standalone routine will probably one day be incorporated in the sigproc filterbank program. psrfits data taken with the mock pdev spectrometer is scan based. ... The routine will read all of the psrfits files from a scan and output a single sigprog.fil file. ... Output to a single file with same format as input: . ... The psrfits files for the test data are located in /share/pdata1/pdev/ . ...

Modules | Directives | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Logging of input and output bytes per request . ... Module Identifier: . logio_module . ... This module provides the logging of input and output number of bytes received/sent per request. ... This module requires mod_log_config . This module provides no directives. Custom Log Formats . ... Apache Log Files . This modules adds two new logging directives. ...

SIMPLE = T / file does conform to FITS standard BITPIX = 8 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A .. ... IMAGEW = 4256 / image width IMAGEH = 2832 / image height ANRUN = T / Solve this field! ...

... Up: Science Data Pipelines . ... We designed and developed a package which simulates extragalactic point source data within a given field of view and SIRTF band. ... The simulator is modular and extensible to enable multi-wavelength simulations, has been optimized by utilizing parallel processing capabilities, and will be used to test pipeline software. ... The extragalactic simulator is capable of generating large numbers of galaxies within a given patch of sky for SIRTF pipeline testing. ...

This module provides for the generation of Expires HTTP headers according to user-specified criteria. ... This module controls the setting of the Expires HTTP header in server responses. The expiration date can set to be relative to either the time the source file was last modified, or to the time of the client access. ... ExpiresByType . ExpiresDefault . The ExpiresDefault and ExpiresByType directives can also be defined in a more readable syntax of the form: . ... Module: mod_expires . ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... python . tcc . mir . mirrorDevice.py . ... 30 љ DefaultTimeLim = None # a poor choice, but the best we can do until commands pay attention to predicted duration . ... 54 љ @param[in] userCmd user command that tracks this command, if any . ... 129 љ @param[in] userCmd user command that tracks this command, if any . ... 131 љ @param[in] userCmd user command that tracks this command, if any . ... tcc.mir.mirrorDevice.MirrorDevice.handleReply . ...

fitshdr - FITS-file headers manipulation tool fitshdr [options] [FITSfile_name] . ... fitshdr [options] --edit FITSfile_name . ... If You want to modify headers of FITSFILE using new FITS-header lines from HEADER file (or from stdin), You have to use this option (You can skip this option, if -H or --header option is used). ... Empty header lines are not displayed (in 'dump' mode only). --line-offsets . ... In 'dump' mode: file offset will be displayed for each header line. --no-line-offsets . ...

Stellarium 0.12.3 . ... Scripting . ... 62 љ bool preprocessScript( const QString& input, QString& output, const QString& scriptDir); . 63 љ bool preprocessScript(QFile &input, QString& output, const QString& scriptDir); . ... 114 љ bool runScript ( const QString& fileName, const QString& includePath= "" ); . ... 154 љ QMap<QString, QString> mappify( const QStringList& args, bool lowerKey= false ); . ... 158 љ bool preprocessStratoScript(QFile& input, QString& output, const QString& scriptDir); . ...

Hide Zen home . ... Index . ... Do we really need them for database indexing ? ... We need simple numbering scheme, so that for any given point we could easily calculate the number of "pixel", this is what HealPix provides and lacks HTM. ... During Rtree queries the number of index blocks read is several times greater than during Q3C queries. ... But in Q3C scheme, as we showed before, the circle is segmented, so we extract from the database only a few percents more data than occur in the circle. ...

The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...

Bojan Nikolic bn204@mrao.cam.ac.uk , bojan@bnikolic.co.uk # # Initial version January 2008 # # Tools for using Obit import os import pyfits import obitsetup import uvrngtobin import Obit, UV, UVImager, Image , ImageMosaic, OSystem, History, OErr # Fitting import ImageFit , FitModel, FitRegion def ObitSys(datapath, nowarn= ...

asncombine -- Process and combine images in one or two NICMOS associations asncombine association . ... set to yes to include error planes in co-added images error. background . ... This is useful to use different background subtractions for different images. fheader . set to yes in order to multiply the background by the value of keyword "factor" in the image header. ... Set to yes to use quadrants statistics save in the image header from previous runs of asncombine. regquad1 . ...

The idea of component-oriented programming is that in the course of implementation of various software projects a programmer (or a programmers team) accumulates a library of reused software fragments that are used in different projects. ... To solve such problems there are some special syntax means in Actor Prolog that support component-oriented programming. ... A package in Actor Prolog is a set of classes linked by implication. ... Actor Prolog supports visual component-oriented programming. ...

gmtconvert - Convert between ASCII and binary 1-D tables gmtconvert [ inputfiles ] [ -H [ nrec ] ] [ -M [ flag ] ] [ -V ] [ -: ] [ -bi [ s ] n ] [ -bo [ s ] ] gmtconvert reads its standard input [or inputfiles] and writes out the information to standard output. ... Input (and hence output) may have multiple subheaders if -M is selected. datafile ( s ) ASCII (or binary, see -bi ) file(s) holding a number of data columns. ... If used, GMT default is 1 header record. M Multiple segment file(s). ...