... Class . ... FRAMES NO FRAMES All Classes . ... FIELD | CONSTR | METHOD . DETAIL: FIELD | ... java.lang.Object ij.plugin.Histogram . ... public class Histogram . ... This plugin implements the Analyze/Histogram command. ... Histogram () . ... This method is called when the plugin is loaded. void . ... Methods inherited from class java.lang.Object . ... This method is called when the plugin is loaded. 'arg', which may be blank, is the argument specified for this plugin in IJ_Props.txt. ...

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• Uses of Class ij.plugin.Histogram (ImageJ API)
• ImageStatistics (ImageJ API)

Next: Listing Image Values Up: Image Analysis Previous: Image Analysis . Task histo is a fairly commonly used task, giving a number of image statistics and a simple histogram. Apart from the input image (keyword in ), it can take a region of interest ( region ), a range to determine the histogram over ( range ), and the number of bins in the histogram ( nbins ). ... region . ... If you do not like histo , or you would like a PGPLOT plot of the histogram, you could use the task imhist instead. ...

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• HIPASS Bright Galaxy Catalog
• imhist
• imheq

... Meta Index / Home Page / Description / Extraction Stage (extractor) . evselect also contains the facility to produce a general FITS histogram product, which does not have the constraints imposed on it by the OGIP compliance of light curves and spectra. ... The column from which to extract the histogram is set with the parameter histogramcolumn . ... As with light curves, one can accumulate the values of a column from the input table, instead of just counts, by setting the parameter zcolumn . ...

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• Routines for constructing histograms

Next: Data reduction: moments Up: No Title Previous: Feature enhancement: local . ... When this is done for the energy map, with the energy scale distributed logarithmically, the result is shown on Fig. ... It can be shown that the mean magnitude at each duration reproduces the mean power spectrum in log-log coordinates. Therefore, this particular presentation of the probability density function shows graphically the scale-dependent scatter around the mean energy spectrum. ...

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To construct frequency distribution (histogram) of minor planets according to value of some element/ parameter/ function user should first select Elements item in menu bar and then Histogram in drop-down menu. ... User has possibility to save histogram or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print histogram select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print . ...

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... 11dec13: histograms, average bandpass of noise for different bandwidths. radar datataking with pdev . ... Mock radar sampling was tested using digital down conversion from 280 to 40 Mhz. 21jan14: 20 Mhz pncode was added to noise and then sampled at 20Mhz. bandpasses, histograms, and energy plots were made . 11dec13: noise was input at various bandwidths. histograms and average bandpasses were made . ... Mock radar sampling was tested using digital down conversion from 280 to 40 Mhz. ... Mhz . ...

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• r2956 venus
• testing radar dataking 31oct13
• routines to access rfi rms data

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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• http://xray.sai.msu.ru/~ivan/gmt/man/grdhisteq.html
• http://xray.sai.msu.ru/~ivan/gmt/man/psrose.html

histogram -based routines * * when dayLen = 1 day and hx1 = nameBorder+1, hx2 = width-1 * then the width of a bin is 85 seconds. */ static final int histBgColor = #99cc99; static final int histFgColor = #999966; // static final int histBgColor = #66cc66; // static final int histFgColor = #999933; static final int histHiColor = #cc3333; static final ...

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• http://hea-www.harvard.edu/RD/funtools/funtools.ds9
• *upspecrdf, downspecrdf* - Transform between RDF and pre-RDF spectral tables
• Power Law fit to a Point Source

Wang-Landau sampling method Wang­Landau method is the random walk in the energy space with a flat histogram. ... If not, accept the new state with probability g(Ek) / g(Ek+1), Otherwise keep the current state unchanged (not-accept). ... MN times, ... f = f1/2, g(E0) = 1 , reset histogram H(E)=0 The algorithm may be stopped with some small value of f.e. f close enough to unity, log f = 10-9 DoS of Ising model Exact - Beale, PRL 76 (1996) 78 DoS g(E) for Ising model 16x16. ...

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... HST is subjected to cosmic rays and protons from the Earth's radiation belts. ... Cosmic ray events usually deposit significant quantities of charge in more than one pixel. ... Figure 4.7 shows a histogram of the number of affected pixels for each cosmic ray event. ... Cosmic ray events do have a clear lower cutoff at around 500 electrons of total signal. ... The number of pixels affected by cosmic ray events in a given exposure is a slightly more sensitive function of the threshold used. ...

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• Radiation Damage and Hot Pixels
• Dark Current Measurements on a State of the Art Near-IR HgCdTe 1024x1024 Array
• Index of /ftp/science/hdf/pipeline

... Imagine that for every pixel in the color image, you take its luminance value (that's how bright it appears). ... In the end, you will have a histogram which counts how many times each luminance value appears in the image (that histogram can be used to analyze the distribution of the luminance values in the image). ... For the watermark effect, we want to use the same value that we used in the Stretch Contrast step, so that the lightest color will be in fact white (255), and nothing will get clamped...

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O.R. Hainaut, ESO, H. Boehnhardt, MPS, and S. Protopapa, UMd . MBOSS Home Tables Plots Credits . The absolute R magnitude M11 and colour distributions are represented as histograms and as their cummulative fraction. Grt is the spectral slope. All the plots for which at least one object is present are available in GIF and in Encapsulated PostScript. ... Note that the colours are sorted alphabetically after the M11 (absolute magnitude) and GRT (spectral slope) plots. ... GIF . EPS . ...

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... Plot histogram and time series. Flow Chart GUILD & LIGO Tools Local File (XML) Restore Events Import XML event data into an event container LDAS Meta Database Save Events Process events (Sort, Coincidence, Cluster) Create Histogram and/or Time Series Plot Histogram/ Time Series Event Containers Hierarchy "Chain" container - A set of List containers. ... Holds one event. ... Time Series - Make a Time Series (DMT TSeries container) of the event rate, values of specified column or event function. ...

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• http://zebu.uoregon.edu/~uochep/talks/talks02/G020047.pdf
• http://zebu.uoregon.edu/~uochep/docs/docs01/TALKdisturb.pdf
• http://zebu.uoregon.edu/~uochep/talks/talks02/G020254.pdf

... BIN/TABLE Create a table with averages of col2 in bins of col1 . COMPUTE/HISTOGRAM Compute histogram for a table column . COMPUTE/REGRESSION Compute column from regresion coefficients . ... COPY/TT Copy keys from table to table file . CREATE/COLUMN Create new column in a table file . CREATE/TABLE Create a table file . DELETE/COLUMN Delete column from an element in a table file . ... REGRESSION/POLYNOMIAL Compute regression between column in table file . ...

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• Operations on Tables
• Some statistical trends and distributions
• Improvement of selection criteria

. F IGURE . 1. Distributions of RR Lyrae stars in distance (a)from the Sun and (b) from the Galactic plane.The shaded part of the histogram corresponds to stars with known proper motions.The curve in the left histogram is a power-law approximation for the growth of the number of stars with distance in the intial sample for R < 1.75 kpc. is the power-law exponent. The dip in the right distribution near Z ? 250 pc is due to selection effects. discussion in the text | next figure .

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• Vertical Structure, figures
• F-stars in galactic disk, figures
• Population of Galactic globular clusters, figures

. Beresfield: histograms of hourly measured NO concentrations by month. The colors were made the same as in Figure . Note the obvious correspondence between the wind direction and the high-value tail of concentration histogram. Бересфилд: помесячная гистограмма ежечасных измерений концентрации NO. Цвета аналогичны рисунку 25. Обратите внимание на очевидное соответствие между направлением ветра и хвостом высоких значений на гистограмме концентраций.

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. Red histogram is 2dF QSO Redshift Survey . Blue histogram is Durham/AAT QSO Survey . | Front page | . | << - Number Counts | . Robert J. Smith, ">rsmith@mso.anu.edu.au Last modified: Fri Sep 24 11:39:02 EST 1999 .

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... It is notoriously difficult to identify weak cosmic ray events in long exposure observations. ... The method is to compare the probability distribution function (PDF) of cosmic ray events between an observation and a dark frame matched in exposure time. We illustrate the basic idea using dark exposures from a Tek 1024 1024 CCD with varying exposure lengths and read-out times. ... Figure: Histogram of cosmic ray events in a two hour dark frame. ... Original PostScript figure (78 kB) . ...

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• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• ADASS 2002 Conference Proceedings
• Towards Optimal Analysis of HST Crowded Stellar Fields

... Gamma-Ray Burst: A Milestone Explosion . ... Credit: R. Klebesadel, I. Strong R. Olson ( LANL ), Vela Satellite Team Explanation: Gamma-Ray Bursts (GRBs) were discovered by accident. ... Exploring the high-energy sky nearly 25 years later, the orbiting Compton Observatory's Burst and Transient Source Experiment (BATSE) , intentionally designed to detect cosmic gamma-ray bursts , was searching for clues to the GRB mystery. ... Publications with keywords: gamma-ray burst - BATSE . ...

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• XWare > APOD
• Journal "Peremennye Zvezdy"
• Астронет > Gamma-Ray Burst: A Milestone Explosion

Radio pulsars strictly periodic signals 14.03.2016 B 10 G;E 10 V / cm 12 10 2 Individual pulses and average profile of pulsar 14.03.2016 3 Average profiles of pulsars 14.03.2016 average energy distribution of pulses by phase of period. ... 14.03.2016 5 2695 Giant pulses (GPs) of pulsar Intensity, a.u. Time, ms Pulses that exceed the average profile over 30 times were called giant pulses. ... 2005) 14.03.2016 8 Individual pulses energy distribution 1937+21. ...

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