... ekstest (ekstest-2.2.5) [xmmsas_20080701_1801-8.0.0] . ... To run the task ekstest using the input FITS file 'lightcurve.ds' and its associated GTI file 'gti.ds', with the single distribution Kolmogorov-Smirnov test and and the flare test where the flare must be at least 3 above the mean and at least 5 bins wide and then write the results both into a new FITS file called 'test.fit' and also write the results to the screen, a command such as, . ...

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• Description

... In our numerical experiments we have mainly considered two test objects provided by R. Hanisch and characterized by different types of brightness distribution; one of the objects simulates an elliptical galaxy and the other one a star cluster with size 512 512 and 256 256 pixels, respectively. ... The best performances in the restoration of the star cluster image are provided by the R-L algorithm and the LWPOS one; they give accuracies of 6%and 5%, respectively (see Table 1). ...

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• covar2ellipse.pro (JWST Pipeline routines in IDL)
• Structure of the Large Magellanic Cloud (LMC)
• Stellar Photometry

grd2cpt - Read a grdfile and make a color palette file grd2cpt grdfile [ -C cptmaster ] [ -I ] [ -L minlimit / maxlimit ] [ -S zstart / zstop / zinc ] [ -V ] [ -Z ] grd2cpt reads a grdfile and writes a color palette (cpt) file to standard output. The cpt file is based on an existing master cptfile of your choice, and the mapping from data value to colors is through the data's cumulative distribution function (CDF), so that the colors are histogram equalized. ... S Set steps in cpt file. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/grdhisteq.html
• Results of calculations
• Amplitude Distribution

... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

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• Results scientific researchs 10
• Results scientific researchs LRS
• Format of data description

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• casacore: casa::NegativeExpntl Class Reference
• casacore: casa::Normal Class Reference
• casacore: casa::Poisson Class Reference

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

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• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• ADASS 2003 Conference Proceedings

The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...

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• HYPERBOLOID Results Page
• Nonequilibrium distributions
• SKA-3 Experiment Description

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

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• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• http://selena.sai.msu.ru/Rod/Publications/ms34/MS059.pdf

... I.A.Dynnikov, Three-page approach to knot theory. ... Universal semigroup, Funktsional'nyi Analiz I Prilozhenija, 34 (2000), no.1, 29-40 (Russian); English translation in Functional Analysis and Its Appl. 34 (2000), no.1, 24-32. I.A.Dynnikov, Finitely presented groups and semigroups in knot theory. ... Math. 2000, no. ... English translation: Russian Math. ... A.Vershik, Numerical invariants of exponential groups, and a locally free approximation of braid groups (in Russian), Zapiski Nauchn. ...

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• Conference Moduli Spaces

spaceweb@oulu.fi - last update: 28 May 1995, 0800 UT . Advanced plasma theories are extremely important when one tries to explain, for example, the various waves and instabilities found in the plasma environment. ... In the kinetic theory it is necessary to know only the distribution function for the system of particles. ... The dependence of the distribution function on the independent variables r , v , and t is governed by an equation known as the Boltzmann equation . ... Hot plasma theory . ...

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• Venera 15 & 16
• MARSENS
• THE LOW ENERGY PLASMA COMPOSITION EXPERIMENT AMEI-2

.

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• Evolution of Intelligence
• Evidence for Dark Matter
• Low Surface Brightness Galaxy Gallery

... These data were originally part of a PhD-thesis at Leiden Observatory by M.H. Wieringa (1991). 1 name Name of source (char8, example : '76W0771*') 2 freq MHz Frequency of source detection in MHz (int, example : 327 or 608 ) 3 ra_1950 radians B1950 Right Ascension (in radians) ( real , example : 2.328327) 4 ra_1950_deg degrees B1950 Right Ascension (in degrees) ( real , example : 133.403290) 5 ra_err seconds Error in RA ( ... 70W : Umi, 327 MHz only, one field. ... Columns 21 Rows 5850...

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• HyperLeda: example of online pipeline processing
• mod_example - Apache HTTP Server
• A VLA Survey of the First Quadrant of the Galactic Plane at 1.5

... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...

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• Long description of example illustrating the collapsing borders model
• Long description for example showing how structurally overlapping cells are
• Long description for the second Bach/XML formatting example

... OOF . ... OOF Index . Zernike Polys . ... The results presented here are based on same data and technique as presented in part 1 ; the only difference is that the Zernike Polynomials are defined on a circle of diameter 90m instead of 100m. The reason for doing this is that MUSTANG only illuminates the central 90m of the dish so there is essentially no constraint in the outer 10m. However, many Zernike polynomial pairs differ there the most and so previous results were highly correlated. ...

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• Retrieval of surface from data across the MUSTANG field
• CO in NGC 1530, aperture synthesis of a barred spiral
• How to create a new tool in CASA Bojan Nikolic web pages (r. 329)

Modules | ... Apache HTTP Server Version 2.2 . ... Some files in the modules/experimental directory under the Apache distribution directory tree are provided as an example to those that wish to write modules that use the Apache API. ... If you link it into your server, enable the "example-handler" handler for a location, and then browse to that location, you will see a display of some of the tracing the example module did as the various callbacks were made. ... Using the mod_example Module . ...

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• mod_substitute - Apache HTTP Server
• mod_dav - Apache HTTP Server
• mod_dir - Apache HTTP Server

Tables give parameters of interstellar extinction and polarization curves produced by rotating homogeneous spheroids with imperfect Davis-Greenstein (IDG) orientation. table 1 (amorphous carbon, oblate particles with a/b=2.0) . table 2 (amorphous carbon, oblate particles with a/b=4.0) . table 3 (amorphous carbon, prolate particles with a/b=2.0) . table 4 (amorphous carbon, prolate particles with a/b=4.0) For model description and some results see: . ...

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• Polarization properties (transmitted radiation)
• A Nature of Polar-Ring Candidate Galaxy ZGC 2315+03
• Database of Optical Properties -- Level: subsubpage

... GSAOI Home . ... Science . ... It is widely accepted that the evolution of the large scale structure of the Universe is driven by dark matter. Understanding this dark matter continues to be one of Astronomy's great unsolved problems. Measuring the bulk motions of galaxies allows us to map the overall mass distribution of the Universe in a way that is independent of the luminous matter in galaxies. ...

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• The High-Z SN Search Description
• Dark Matter in Spiral Galaxies
• GSAOI Disk Galaxies Science Page

... country name . ... Query " Moscow's celebrations hotel Moscow, Russia" would failed if search attributes separately, but could be succeeded if search their concatenation. ... hotel". ... Simple search for "Moscow": # select name, country, place, rank( idx, ftsquery ) as r from hotels, to_tsquery('Moscow') as ftsquery where idx @@ ftsquery order by r desc; name | ... Query "Moscow hotel" (rewritten by hand): # select name, country, place, rank( idx, ftsquery ) as r from hotels, to_tsquery('Moscow | ...

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• JavaScript Random Number Tester
• The Name of the Plug-In
• Building and Installing the Distribution

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Distribution of the speed w of ejecta (bold curve) relative to a platform moving with a horizontal speed of 1650 m/s and at an altitude h=30 km above the lunar surface. The assumed distribution of the ejection speeds at the surface is a power law with a low cutoff value of 100 m/s and an exponent of 1.2. ... The same conclusion holds for the speed distribution of particles near the surface. ...

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• Galactic distribution and absolute magnitudes
• sfit help file
• C.S. Jeffery, Research Astronomer

... support coversheet file _cs.html . ... PANL2 for nightlog information; asm (thru qcm) ; dataproducts..calib for pre-existing ANC files . ... twin ancillary fits files (LOGS and PLTS) . ... merge2Fits is a helper tool which prepares all input for creating product ancillary fits files. ... straightforward ingestion with existing tools: cdbIngest can handle any kind of product fits file . ... Ancillary fits files: content . The content of ancillary fits files is controlled by merge2Fits . ... LOGS . ...

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• checkConsist
• VLTI Calibrator Selection Help Page
• ESO - Release of Photometric Catalogue Data Resulting from the VISTA Magellanic