Next: The Schedule File Up: THE SCHED USER MANUAL Version Previous: Satellite Tracking Contents . This chapter covers the main input files that SCHED reads. ... See the SCHED Input and Output Files section of this manual for brief descriptions of the files and pointers to the standard versions. ... Summary List of SCHED Parameters . ... List of Frequency File Parameters . Setup Files . Standard Setup Files . ... Summary List of Setup File Parameters . Details of Setup File Parameters . ...

Next: ASTROMET/EDIT Up: Available Commands Previous: Available Commands . This command computes the astrometric transformation parameters for the input data set using a least-square fitting algorithm. The input data is assumed to be two MIDAS tables with fixed columns names. ... ASTROMET/TRANSFORM only computes the transformation parameters. ... R_A Real column containing the right ascension in degrees; . ... XCEN Real column to contain the X measurement; . ...

... Several of the tasks in the spectral package share a common set of parameters. ... Each task in the spectral package has a hidden parameter which points to the pkgpars parameter file. The parameters stored here include the observed data sets and the model descriptor, and instrument-specific parameters. ... The observed counts and error data set contained in the table file ( *_obs.tab ) produced by qpspec will be the input data for subsequent spectral tasks. ...

... A couple of new tasks have also been added; including, SAACLEAN to the NICMOS package, 'tweakshifts' to the DITHER package and a Python interface to SExtractor. Updated or New Tasks: ===================== 1. NEW TASKS: - 'tweakshifts' added to the DITHER package: This prototype version of 'tweakshifts' provides an automated interface for computing residual shifts between input exposures being combined using MultiDrizzle or PyDrizzle. ... Changes to CALSTIS: - Updated to Version 2.19. ...

... ONLY include the controls you are actually using. ... only used if > -100 !Profile_xmax = 1.2 !-101 ! ... only used if > -100 Profile_other_ymax = -101 ! ... step number. negative means use default. ... negative means use same value as for window CONV_file_aspect_ratio = -1 ! negative means use same value as for window ! ... negative means use same value as for window Surf_Hist_file_aspect_ratio = -1 ! ... negative means use same value as for window Power_file_aspect_ratio = -1 ! ...

OptInt PmWiki : Pm Wiki / Include Other Pages . ... include PageName:) . ... includes a named variable from a page, Group and PageName are options . ... include FullName # fromanchor # toanchor lines = 123 self = 0 basepage = abc variable = value :) . ... You can use any page name. ... This is useful if PageName is a variable like {$Name} and you want to prevent the directive from including the current page. ... By default, Included pages or lines cannot be distinguished from other text on the page. ...

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

Stellarium 0.12.3 . ... Classes . ... Class List . Class Index . ... StelModuleMgr Class Reference . Manage a collection of StelModules including both core and plugin modules. ... void  . ... Register a new StelModule to the list The module is later referenced by its QObject name. ... unloadModule (const QString &moduleID, bool alsoDelete=true) . ... Register a new StelModule to the list The module is later referenced by its QObject name. void StelModuleMgr::setPluginLoadAtStartup . ...

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

... esorex.caller.recipe-dir=/home/quality/pipelines/vcam-1.0.7:/home/quality/pipelines/detmon . ... See extraction of config.processAB : # ====================================================================== # 2. esorex configuration file names for generic pipelines # List here the name(s) of esorex configuration file (s) of general pipeline (s) (e.g. detmon ) # RAW_TYPE: usually just one, but could be more # DET_ID: required only if you need to specify config files per detector (avoid ...

The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...

... Class . Use . ... Packages that use FileInfo . ... ij.io . ... Methods in ij that return FileInfo . ... Returns a FileInfo object containing information, including the pixel array, needed to save this image. ... Returns the FileInfo object that was used to open this image. ... Displays the dialog and returns a FileInfo object that can be used to open the image. static FileInfo . ... Returns the FileInfo object used to import the last raw image, or null if a raw image has not been imported. ...

. Intervals of available data are coded by blue color. To read availability charts user should know the descriptor ("name") of the KP subset of interest. Table annotations include also number of version for each subset. Plot resolution is exactly one pixel per hour. Data are considered as available if at least one data point is present during that hour.

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

... Average resolution at altitude H=668 km . ... Swath width at H=668 km and inclination of beginning of swath 20.48 degrees . ... Resolution at H=668 км . ... Наименование параметра . ... 1 канале . ... Полоса обзора при H=668 км . ... 1-5 спектральной зоне, не более . ... 1 спектральной зоне . 0,48-0,52 мкм . ... 0,915-0,997 мкм . ... 1-4 канал . ... 1-4 каналов . ... Спектральные характеристики каналов (по уровню 0,5): . ... For more information send a mail to: info@sputnik.infospace.ru . ...

lsst.tcc   1.2.2-3-g89ecb63 . ... Files . ... include . ... telMod.h . ... 6   #include <string> . ... 24   explicit TelMod (std::string const &filePath) { . ... 86   void loadPath (std::string const &filePath); . ... 112   std::vector<std::string> getTermNames () const ; . ... 145   std::ostream & operator<< (std::ostream &os, TelMod const &telMod); . ... double getTerm(std::string const &termName) const . ... std::vector< std::string > getTermNames() const . ... TelMod(std::string const &filePath) . ...

... Tiny Tim has been used for generating Hubble Space Telescope ( HST ) point-spread functions (PSFs) for deconvolution, algorithm testing, proposal planning, and optical studies. ... Tiny Tim is a stand-alone program for simulating HST PSFs as viewed with the on-board imaging cameras (WF/PC-1, WFPC2, FOC, COSTAR/FOC). ... The measured aberrations for FOC f/96, WF/PC-1 PC6, WFPC2, and COSTAR/FOC are used by Tiny Tim . ... Figure: FOC f/96 observed and Tiny Tim model PSFs (pre-COSTAR) at 253 nm. ...

... 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) . ...

... Next . comedi_get_cmd_generic_timed -- streaming input/output capabilities . ... int comedi_get_cmd_generic_timed (comedi_t * device, unsigned int subdevice, comedi_cmd * command, unsigned int period_ns); . The command capabilities of the subdevice indicated by the parameters device and subdevice are probed, and the results placed in the command structure pointed to by the parameter command. ... The command measures samples at a rate that corresponds to the period period_ns. ...