... The ratio of output-to-input pixel dimensions are specified by the parameters binxsize and binysize ; in addition, the starting row or column can be defined using parameters offsetx and offsety . ... In this case, as one might expect, the output image contains the same number of columns as the input. ... In this case the output image is 26 pixels wide. The first column of the output image contains columns 1 and 2 of the input image, the second contains 3 and 4, and so forth. ...

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• Parameters

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 . ...

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• casacore: casa::ObjectPool< T, Key > Class Template Reference
• casacore: casa::FunctionOrder< T > Class Template Reference
• Graphical User Interface Example (3)

... 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. ...

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• Table Filtering
• Spatial Region Boundaries
• SAO RSDC Home Page - RRA - PSPC

... 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 ; } ...

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• Zen: Gendict
• Further Information and Bibliography

... way these widgets work for the user. #include gtk/gtk.h GtkWidget *hscale, *vscale; void cb_pos_menu_select( GtkWidget * item , GtkPositionType pos ) { /* Set the value position on both scale widgets */ gtk_ scale _set_ value _pos (GTK_ SCALE (hscale), pos); gtk_ scale _set_ value _pos (GTK_ SCALE (vscale), pos); } void cb_update_menu_select( GtkWidget * item , GtkUpdateType policy ) { /* Set the update policy for both ...

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• Item Factory Example
• Estimated parameters
• Echelle Spectra

... The analysis of NICMOS polarization images is aimed at determining the Stokes' Parameters, and from those the polarization angle and degree for each pixel. NICMOS Camera 1 and Camera 2 each contain three polarizers, whose principal axes of transmission are separated by 120 degrees. ... The images in the three filters need to be compared, in order to produce the Stokes' parameters. ... The Stokes parameters can then be combined to yield the polarized intensity, I p: . ...

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• http://www.stsci.edu/institute/software_hardware/stsdas/relnotes/stsdas_v34_summary.txt
• http://www.stsci.edu/documents/dhb/web/c01_intro.fm4.html
• Appendix: Recipe File XML Format GPI Data Pipeline 1.0 documentation

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/number.htm
• Program parameters
• Netscape Cookies

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• The SuperCOSMOS Sky Surveys
• TwoFitlines: An Spectrum and Line Analysis Tool
• Interactive Fitting of EUVE Emission Line Spectra

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. ...

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• OptInt PmWiki : Include Other Pages
• Computing dispersive atmospheric delay with AATM
• John Young's Home Page

... 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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• Spectrum
• Simon's Software - howto 1-3
• Sterne

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 . ...

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• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA
• CIMA Configuration Files
• Your NED Search Results

Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties . ... If necessary, data have been determined for the different crystallographic axes. ... In the following we give some examples of the data and their possible applications. Table: Summary of data measured in the Jena laboratory, which are currently available from the JPDOC. compound . ... amorph. ... Next: Silicate minerals Up: A Database of Optical Previous: Database of Optical Properties root 2003-03-06 ...

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• Linear polarization: wavelength dependence
• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage

NAME ABbuilder - DFO data organization tool SYNOPSIS ABbuilder <options> where <options> are: --raw-dir directory containing raw data --cal-dir directory containing calib data --cal-ldir directory containing symbolic links to calib files --cal-list mcalib list --vcal-dir directory containing virtual products --pro-dir where pipeline products are created --ab-dir where association blocks are created --oca-rul file containing OCA rules --instrume instrument --date YYYY-MM-DD --mode { CALIB | ...

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• Include detmon as a generic pipeline
• pyQC: overview
• Parameters

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

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• Getting Started in Actor Prolog. Hello World.
• Getting Started in Actor Prolog. Underdetermined Sets.
• Getting Started in Actor Prolog. Oil Production.

... 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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• Guide to Russia || Top Attractions

Comedi Documentation . ... Right to the source: #include <stdio.h> /* for printf() */ #include <comedilib.h> int subdev = 0; /* change this to your input subdevice */ int chan = 0; /* change this to your channel */ int range = 0; /* more on this later */ int aref = AREF_GROUND; /* more on this later */ int main(int argc,char *argv[]) { comedi_t *it; lsampl_t data; it=comedi_open("/dev/comedi0"); comedi_data_read(it,subdev,chan,range,aref,&data); printf("%d\n",data); return 0; } . ...

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• Time Functions
• The C Preprocessor
• comedi_get_version_code

... 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 ! ...

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• http://crydee.sai.msu.ru/ftproot/pub/MESA-models/M7_Z002/inlist_project
• http://crydee.sai.msu.ru/ftproot/pub/MESA-models/M8_Z002/inlist_project
• http://crydee.sai.msu.ru/ftproot/pub/MESA-models/M6_Z002/inlist_project

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. ...

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• "Stargazers" in the Classroom--additions
• WAVE EXPERIMENTS ON TAIL PROBE
• V.G. Petukhov (Khrunichev State Research and Production Space Center).

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 . ...

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• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...

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• Stellarium: StelModuleMgr Class Reference
• Stellarium: core/StelSphereGeometry.hpp File Reference
• StelTexture::StelTextureParams Struct Reference