Next: Spectral Analysis Up: Commands Grouped by Previous: Transformations on Pixel . ... INTEGRATE/APERTURE Integrate flux inside aperture . INTEGRATE/LINE Integrate pixel-values over area in image . ... MODIFY/CURSOR Change pixel values in image by cursor . MODIFY/GCURSOR Change pixel values in image by graphic cursor . MODIFY/PIXEL Change pixel values in image . ... READ/IMAGE List pixel values into image . ... WRITE/IMAGE Change pixel values in image (world coordinates) . ...

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... User Guide ] Task: imstat Purpose: calculate and plot map statistics Categories: map analysis IMSTAT calculates statistics for images. ... Statistics can be found for profiles or planes, specified using the axes keyword. The data can be converted to Kelvin, by using 'options=tb' and the beam keyword. ... The options keyword gives control over the plot. ... An alternative title can be put on the plot by options=title. ... Key: in Standard keyword in. ... Key: region Standard keyword region. ...

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• PPTA Wiki | Projects / RedGW
• Image Statistics and Histograms
• Function Summary

... Let us assume to begin with that there is no source at a given location, only background. Let us calculate the probability that the observed counts at that location are due solely to background. ... The routines described in the present section are designed to take as arguments the probability cutoff (actually a cutoff in likelihood is used) and the background, or expectation value for the counts, and use them to calculate the minimum value of source counts which is detectable at those levels. ...

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• The contour method of calculating source region shape

Next: Power Law fit to Up: Spectral Analysis Previous: Error Determination . With PROS2.3 all fitting is performed using Poisson statistics , rather than Gaussian, so that results will be correct even for small counts ( ) in some channels. Power Law fit to a Point Source . Raymond Model . Two-Temperature Raymond Model . Limiting Energy Channels Input to the Fit . Multiple Data Sets . ... Fit a source with a small number of net counts . Inspection of results . ...

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• Regions and Source Parameters
• The AstroStat Slog Blog Archive Parametric Bootstrap vs. Nonparametric...
• *xflux, hxflux* - Calculation of X-ray Flux

In April 2003, a new capability was introduced in synphot for use with the Advanced Camera for Surveys (ACS) imaging modes. ... Users are now able to specify a circular aperture (radius in arcsec) to calculate the source counts within this aperture. ... These values are derived for a 0.2 arcsec radius aperture for the ETC and synphot calculations. ... ETC . synphot . ... The " aper " keyword allows the user to select an aperture (radius in arcsec) and indicate this value by typing " aper#value ". ...

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• WFPC-2 ETC Help
• density.pro (JWST Pipeline routines in IDL)
• Introduction to HST Data Handbook v8.0

Pulkovo NEO Page . ... EPOS Software Package . ... EPOS ( E phemeris P rogram for O bjects of the S olar system) is the Windows PC application for study and ephemeris support of observations of the Solar system objects. ... It controls the part of common data and transfers the control to one of the programs that solve the restricted set of tasks. ... So with the EPOS software package one can calculate the accurate ephemerides for many objects and get the quick illustration of their motion as well. ...

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... Statistic files are managed using file generation sets and scripts in the ./scripts directory of this distribution. ... Each valid update appends a line of the following form to the current element of a file generation set named peerstats : . ... This keyword allows the (otherwise constant) filegen filename prefix to be modified for file generation sets, which is useful for handling statistics logs. filegen name [ file filename ] [ type typename ] [ flag flagval ] [ link | ...

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• Configuration Options

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• New Elements of Sherpa, CIAO's Modeling and Fitting Tool
• Accessing the Digitized Sky Survey

. This diagram shows a small table with three transparent cells and illustrates how their final background is determined. The table consists of two rows. Four (labeled) cells lie in the first row, but the second cell spans the first and second row. The first, third, and fourth cells of the second row are "empty". Each non-empty cell has a red background and a double black border. Each empty cell has the table's background color (specified as #ff0) as its own. Return to image.

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• HTML Design Notebook

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• Details of Rotang
• AGES Database Search
• CIMA Auto-Observing

... ClassљIndex . ... StelRendererStatistics Class Reference . Stores and provides access to statistics about a StelRenderer backend. ... getNext (const char *&name, double &value) . Get next statistic name and value. ... Access statistic with specified index to modify it. ... while (statistics.getNext(name, value)) . ... Name of the statistic will be stored here (only a pointer to it). value . ... A clean way to do this is to use an enum with name corresponding to the name of the statistic. ...

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... Restrictions ) are used. If specified form of output is EMP then astrometric equatorial coordinates are printed in the form usual for Ephemerides of Minor Planets, with formal precision of 0.01 minute of time in R.A. and 0.1 minute of arc in declination. ... It should be noted that the near-opposition ephemerides are not calculated for bodies/ points with numbers from –12 to 0 (in case they are included into task for computation of such ephemerides only their names are displayed in the results). ...

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• IAA VLBI Analysis Center
• ENGAMPLE

... java.lang.Object ij.macro.Interpreter . ... This is the recursive descent parser/interpreter for the ImageJ macro language. ... Interprets the specified string. public java.lang.String run (java.lang.String macro, java.lang.String arg) . ... Interprets the specified tokenized macro file starting at location 0. public void run (int location) . Runs an existing macro starting at the specified program counter location. public void runMacro ( Program pgm, int macroLoc, java.lang.String macroName) . ...

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• ParticleAnalyzer (ImageJ API)
• Orthogonal_Views (ImageJ API)
• Uses of Class ij.process.ImageStatistics (ImageJ API)

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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• The Stellar Population in the NICMOS Parallel Fields
• NICMOS Software at the University of Arizona
• STScI NICMOS Software

To suspend the execution of a command for a specific amount of time use the command: sleep time_in_seconds ; command . The second command will not be carried out until the amount of time specified as an argument to the sleep command has elapsed. ... You can also enclose the commands in parentheses to group them together and then run the combined command in the background, allowing you to carry on working at the shell prompt: (sleep time_in_seconds ; command ) . ...

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• Using the fc command
• Editing a previous command line
• Testing for files and variables with the test command

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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• Gravitational Waves from Coalescing Compact Binary Stars
• The Model

... Bojan Nikolic web pages (r. 329) . ... Analysis of (radio) spectra . The RNested package is a re-implementation of the main algorithms from the radiospec package into the R statistical data analysis environment. ... packages ( "RNested" , repos = c ( "http://www.mrao.cam.ac.uk/~bn204/soft/R" , "http://cran.us.r-project.org" )) . ... RNested ? Nested Sampling in R & analysis of spectra . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Abstract
• OptInt PmWiki : PmWiki / Wiki Style Examples
• PPEUC Programme - Cosmic Microwave Background Workshop

... Linear limb darkening coefficients are taken from tables published by Van Hamme (1993, AJ 106, 2096). limb_stars Compute limb darkening fit coefficients for all stars. limb_star ( spectrum _char , filter _char ) Function. Return linear limb darkening coefficient integrated over specified bandpass. Example: print, limb_star('G0I','V') . ... Return factor to multiply the uniform disk diameter with in order to get a limb darkened diameter using the specified linear limb darkening coefficient. ...

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• ESO - telbib information
• Command line procedures
• ESO - Science Announcements

Tail Probe is one of the satellites of the INTERBALL program. ... Collection of the orbital elements | ... Flight situation analysis during operations scheduling . ... Two stages of the orbital situation analysis are presented: . ... The satellites motion calculation during the flight situation analysis is based on the orbital elements, determined by the Ballistic center at KIAM RAN. The modified (by backward integration) orbital elements are usedduring the aposteriory situation analysis. ...

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• INTERBALL AURORAL PROBE SITUATION ANALYSIS
• INTERBALL MAGION 5 SITUATION ANALYSIS
• Main research and development work completed in 2012 and ready for

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Programs . ... htcacheclean is used to keep the size of mod_cache_disk 's storage within a given size limit, or limit on inodes in use. ... If one or more URLs are specified, each URL will be deleted from the cache, if present. ... Specify limit as the total disk cache size limit. ... By passing the -a or -A options to htcacheclean , the URLs within the cache will be listed as they are found, one URL per line. ...

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• Algorithm
• Comet Halley
• mod_expires - Apache HTTP Server