The central velocity dispersion represents the internal motions of the stars along a column crossing the center of a galaxy or star cluster. ... The catalogue of collected velocity dispersions may be accessed in HyperLeda. vdis is the velocity dispersion given in km/s. The velocity dispersion gives to some approximation the scale for the specific kinetic energy contained in in un-ordered motions and combined with the velocity of rotation it may give an estimate of the specific kinetic energy. ...

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• Outline of the Available Methods
• The main observational parameters
• HyperLEDA documentation: parameter: multiple

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... yes . dataset . The name of the Poissonian image which it is desired to fit background to. fitsets . ... dataset list . List of names of datasets, each of which is an image which represents one of the components of the background model to be fitted. fitstyle . ... If fitstyle =`whole', the pixels of poissonset may have any value, and a standard Poisson distribution is assumed. ...

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External influences on spin parameters for INTERBALL - AP . ... The main interest is that almost all kind of external influences to parameters of motion (eclipse, normalization, ROS) are presented in the one time interval. Three upper panels illustrate the spin velocity, the angle between kinetic moment and sun direction, and the nutation.All external events are represented on the lowest panel as blue, green and yellow columns. ...

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• AZ Key parameters, 1997
• AZ Key parameters, 1998
• AZ key parameters, 1996

... Packages that use ImageStack . ... ImagePlus. setStack ( ImageStack stack) . ... ImagePlus. setStack ( ImageStack stack, int nChannels, int nSlices, int nFrames) . ... ImagePlus. setStack (java.lang.String title, ImageStack stack) . ... ImagePlus (java.lang.String title, ImageStack stack) . ... Projector. getByteRow ( ImageStack stack, int x, int y, int z, int width1, int width2, int[] line) . ... Projector. getRGBRow ( ImageStack stack, int x, int y, int z, int width1, int width2, int[] line) . ...

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• Tools (ImageJ API)
• CurveFitter (ImageJ API)
• Uses of Class ij.plugin.frame.Editor (ImageJ API)

The current set of keyword-value pairs of a task can be monitored by typing ESC K while the name of the task is present in the User Command Area. This causes (part of) the Common Output Area to be overlaid with a display containing the current user input parameters of the task. ... If there is currently a set of parameters displayed on the screen (as the result of typing ESC K ), these parameters will be edited; otherwise the name of the task is derived from the User Command Area contents. ...

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• User Parameters - Spectral-line Imaging CentralProcessor 0.11 documentation
• Polarization/Stokes Handling (stokes and select)
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

... 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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• New Features in this Release
• Program parameters
• Kernel tunable parameters

... 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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• A Python-based IRAF Task Parameter Editor
• A Computer-Based Technique for Automatic Description and Classification of
• ETCs and Observations Simulation at the VLT

... Prev . ... comedi_from_phys -- convert physical units to sample . ... lsampl_t comedi_from_phys (double data, comedi_range * range, lsampl_t maxdata); . Converts data given in physical units (data) into sample values (lsampl_t, between 0 and maxdata). The parameter rng represents the conversion information to use, and the parameter maxdata represents the maximum possible data value for the channel that the data will be written to. Conversion is not affected by out-of-range behavior. ...

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• comedi_to_phys
• Spectral energy distribution
• harak_e

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

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• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

... SGML . The text/html content type . In this section, we begin the specification of HTML 4.0, starting with the contract between authors, documents, users, and user agents. ... These recommendations are not normative and conformance with this specification does not depend on their realization. ... An HTML document is an SGML document that meets the constraints of this specification. ... A user is a person who interacts with a user agent to view, hear, or otherwise use a rendered HTML document. ...

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• Notation
• Gaussian Chirplet
• The Frequency-Frequency (FF) Plane

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• Database of Optical Properties -- Level: subpage
• AI SPbU library of scattering codes
• Model realization and some results

Next: Discussion Up: Maximum Likelihood Estimation of Previous: Model Fitting . ... When both fits are performed on a simulated image of either kind, the value of the likelihood function is very effective in choosing the ``right'' model down to typical magnitudes of or with a single-orbit WFPC exposure, and about one magnitude fainter with the expected parameters for WFPC 2 observations (see Table 1). Six orbits are required to reach one magnitude fainter with either camera.) ...

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• Iterative Image Restoration
• HST Image Restoration with Variable Resolution
• COS Instrument Handbook

The problem of solar wind data correlation for the observations onboard several spacecraft is very important for three points of view: . ... This problem is studied now in detail by systematic determination of ion flux and ion velocity data correlations by INTERBALL-1 (IKI group), WIND and IMP 8 (both - MIT group). ... Solar wind plasma correlation lengths from IMP 8, WIND and INTERBALL-1. ... Correlation of solar wind observations onboard several spacecraft: INTERBALL-1, IMP 8 and WIND data. ...

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• IKI SSC, INTMINS APRIL99
• Space Weather
• V.G. Petukhov (Khrunichev State Research and Production Space Center).

grdvector - Plot vector fields from grdfiles grdvector compx . ... CYLINDRICAL PROJECTIONS: -Jc lon0 / lat0 / scale (Cassini) -Jj lon0 / scale (Miller) -Jm scale ( Mercator - Greenwich and Equator as origin) -Jm lon0 / lat0 / scale ( Mercator - Give meridian and standard parallel) -Joa lon0 / lat0 / azimuth / scale (Oblique Mercator - point and azimuth) -Job lon0 / lat0 / lon1 / lat1 / scale (Oblique Mercator - two points) -Joc lon0 / ...

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• http://xray.sai.msu.ru/~polar/html/publications/citation/citation2.pdf
• Initial parameters of compact stars
• Other parameters of the evolutionary scenario

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
• http://selena.sai.msu.ru/Greg/Publications/ms38/ms090.pdf
• http://selena.sai.msu.ru/Greg/Publications/ms40/81_Ushkin_Michael.pdf

To pass several arguments from the command line to the shell: cat first_5args # This script echoes the first five arguments # supplied to the script echo The first five command line echo arguments are $1 $2 $3 $4 $5 first_5args mines a pint john o.k. The first five command line arguments are mines a pint john o.k. This passes the arguments represented by parameters $1 through $5 to the shell script. ... This processes the three files given as arguments to the command printps . ...

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• Understanding HTML and SGML
• Example of using the shift command

Hideyuki Saio Simon Jeffery are exploring models for the evolution of stars formed by the merger of two white dwarfs. The attached movie provides a simulation of the major events involved in the merger process. ... An initial binary system consists of two white dwarfs of masses M 1 and M 2 (given) with an orbital period ( P ). ... We adopt a simple expression for the white dwarf radius as a function of mass (in solar units): . ... The merged star evolution is simulated by a quadratic expansion . ...

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• Armagh Observatory
• SCL Sfit SLV Commands
• Abstract 192

... The Astronomical Society of the Pacific (ASP) presented Priscilla and Bart Bok Awards to two high School Seniors at the Intel International Science and Engineering Fair held May 10 to 15 in Reno this year. ... The Bok prize is named for Bart and Priscilla Bok. ... About 10 years ago, at the suggestion of the American Astronomical Society, the activities supported by the Bok Fund were expanded to include the joint sponsorship of an astronomy award at Intel Science and Education Fair. ...

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SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...

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• Sun orbital parameters for Computer Ephemeris for 2014 (DE200/LE200).
• MISSION WARNING
• Sun orbital parameters for Computer Ephemeris for 2015 (DE200/LE200).

... Colours of stars and galaxies hold information on intrinsic and extrinsic parameters, such as stellar temperatures and galaxy populations, selective absorption and colour changes due different dust contents and inclination angles of galaxies, as well as galaxy redshifts and evolution. ... The colour magnitude diagram of 65000 galaxies to which all above-mentioned quantities and others contribute can only be explained by comparison with simulations. ... Colours are also of technical help. ...

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• Preparation of parameter file
• List procedures
• SPECPSF (V1.00) --- May00 stecf.specres --- SPECPSF (V1.00)