... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... yes . ... If `user', the task looks for the name of the mask image set in the parameter maskset . ... Where the background level of the image is visible, the default value (= black) is preferable; however, in the case that large areas of the image fall outside the mask (but see also the parameter expandtomask ), a value of 1.0 may be better, if only to save ink on printed output. expandtomask . ...

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... The Digitized Sky Survey is now available on CD-ROMs and will be on the ST ScI archive. ... ST ScI has digitized Schmidt plates of the entire Sky. ... The software then accesses the data, decompresses the scans and returns the data in a form of a photographic intensity as a function of x and y plate pixel coordinates. ... accesses the Digitized Sky Survey (DSS) CD ROMs and decompressed the data returning a photographic intensity as a function of x and y pixel coordinates. ...

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• TwoFitlines: An Spectrum and Line Analysis Tool
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared

2.1 Ramp filters (ACS, WFPC2) . ... 2.4 Encircled energy (ACS, WFC3) . ... 2.4.3 Supported ACS Aperture Sizes . ... Parameterized keywords are generally used to access throughput tables for which the throughput is a function of some other variable in addition to wavelength. The syntax for a parameterized keyword is keyword#value , where value is a numeric (integer or float) value for the keyword to take. ... If no parameterized keyword is used in the obsmode, a default value will be used. ...

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• CDBS FOS Page
• Index
• FOCSIM Parameters fill-out form

... This section will deal with obtaining photons within specified regions of an image. Available regions are: Annulus Box Circle Ellipse Field -- entire field Irregular region based on intensity of map... i.e. region defined by contour levels. ... The imcnts task in the xray-spatial package sums the source and background counts in specified regions, and subtracts one from the other properly normalized. ... imcnts* - Find counts in an extended region, after removing an embedded point source . ...

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• *imexamine* - General analysis of image containing many sources
• Model Spectra for Spectral-Fitting Program
• Editing Files and Parameters

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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The reduction of a given magnitude m to it is given by: . ... The galaxy extraction was made with a Discriminant Analysis based on seven parameters (peak intensity over area, Mean surface brightness, Peak intensity, Axis ratio, Relative surface object/matrix, Elongation of the matrix and Diffraction cross) and calibrated with a sample of 1146 DENIS objects visually classified as "galaxy", "star" or "unknown". A visual inspection of every galaxy candidate was made on the matrix of pixels. ...

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• Documentation: LEDA: parameter: v3k
• HyperLEDA documentation: parameter: Mg2
• Parameter estimation

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Parameters of binary compact star evolution
• Parameters of the starburst
• Initial binary parameters

... The e-mail interface of the CATS is designed like CGI for the call of the basic procedures: select and match from the html-forms and the program is a lexical analyser, distinguishing keywords and parameters from the electronic letter sent to the address `cats@sao.ru'. ... The output of result is forseen in the same formats as in other forms of the access to the CATS. ... out[put] < arg1 arg2... > . ... ra [ < arg1 > ] < arg2 > < arg3 > ... min max [center] . ... window < arg1 arg2 ... > . ...

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• Determination of atmospheric parameters and calculation of chemical composition
• harak_e

... Apply a time-varying phase shift to track the object. ... This overrides the normal behaviour of using the spin axis. arcane The format for the pmotion text files is the "arcane" format (see below). ... Each source is specified by three numbers: ra dec flux The RA and DEC are in normal Miriad format, and the flux is in Jy. ... The normal format consists of 3 values per line, being time ra dec with "time" (UTC), "ra" and "dec" being the position of the object at a given time. ...

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• Access to calibrator solutions CentralProcessor 0.11 documentation
• Miscellaneous Analysis Tasks
• ccontsubtract CentralProcessor 0.11 documentation

The starting page - The catalogues page - The list of the PUL2 fields - The list of the Pul-3(Pul-3SE) fields - The list of the PUL_ERS fields . please read short description of the access form controls . ... Right Ascension (ICRF/Tycho-2) J2000 at the central epoch of obs. (hours, minutes, seconds) (Obligatory parameter) . ... proper motion in RA (*cos(DE)) (ICRF/Tycho-2). (mas/yr) . ... Check the apropriate checkbox to output these data and radiobutton to select stars within interval. ...

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• The Pul_ERS astrometric catalogue. Data access form
• Proper motions of 59766 stars with respect to galaxies in 149 areas of the sky

Applying Bayesian analysis to polarisation data J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR MKSP Workshop 1 / 15 Outline 1 2 3 4 Polarisation simulations @ radio wavebands Bayesian analysis Analysis of polarisation data Conclusions J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR ...

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• OptInt PmWiki : MROIDelayLineSW / Baseline Solution Software
• Astrophysics Group MADCOW
• PPEUC Programme - Cosmic Microwave Background Workshop

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

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• The NMW survey homepage

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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• East Siberian Center for the Earth's Ionosphere Research. Ionospheric parameter

... The Earth orientation parameters UT1 and polar motion (x pol ; y pol ) are relat­ ed with the values of UT0 and VOL obtained from the LLR analysis for a station with geocentric longitude and latitude (–; OE) by the following expression: 7 UT0 \Gamma UTC = UT1 \Gamma UTC + (x pol sin – + y pol cos –) tan OE 15 V OL = x pol cos – \Gamma y pol sin – At least four normal points for each station--reflector pair at one day were accepted for the diurnal UT0 estimations. ...

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• (Untitled)
• IAA GPS Analysis Center
• NAA-2

Shell scripts can act like standard UNIX commands and take arguments from the command line. Arguments are passed from the command line into a shell program using the positional parameters $1 through to $9 . Each parameter corresponds to the position of the argument on the command line. ... For example: cat printps # This script converts ASCII files to PostScript # and sends them to the PostScript printer ps1 # It uses a local utility "a2ps" a2ps $* | lpr -Pps1 printps elm.txt vi.ref msg . ...

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• Index: P
• Using the shift command

Next: Load point data Up: Access a data file Previous: Browse through an HDS Contents . Before any data, the system configuration (consisting of the general configuration and the earth and geometric parameters) and the background and scan tables must be loaded. You do not have to load all these by individually selecting each one, just use the A CCESS L OAD INTERFEROMETRY button, which will load all items listed above it. ... INTERFEROMETRY All objects in the file, get auxilliary data . ...

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• OYSTER home page
• Loading configuration and logs
• Preparation of parameter file

Chair of solid state physics . ... Laboratory practical training on the structural analysis for 3rd year students of the Solid State Physics Chair of MIPT . ... X-ray diffraction methods in materials research . Debye method: determination of lattice parameters, identification of crystal phases . ... X-ray phase analysis: computer processing of X-ray diffraction spectra, identification of crystal phases using ICDD database . ... X-ray powder diffraction: qualitative phase analysis. ...

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Links given for particles of different shapes allows one to access our graphics illustrating the dependence of various optical properties of model scatterers on their parameters. ... Q ext , Q sca , Q abs , Q bk , albedo, g, Q pr vs x for different m . F ij vs theta for different x, m . ... Q ext , Q sca , Q abs , Q bk , albedo, g, F ij vs x for different m, alpha . F ij vs theta for different x, m, alpha . ... Q ext , Q sca , Q abs , Q bk , albedo, g, Q pr vs x for different m (TE/TM modes) . ...

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• Model realization and some results
• AI SPbU library of scattering codes
• Linear polarization: wavelength dependence

... Chapter 1. ... Problems of observational radio cosmology (6) . ... Analysis of radio astronomical data (32) . ... Data analysis system (33) . ... Actuality, goals and results to depend (45) . ... Interactive processing of continuum radio spectra of radio sources (72) . ... Creation of the astrophysical catalogs data base CATS and its application for selection and analysis of radio galaxy samples (112) . ... Data and methods (176) . ... Results of analysis of known radio galaxies data (179) . ...

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• Lectures
• Radio Sources Parameters

... ALL INTERBALL participants have free access to ALL KP from all mission experiments. ... KP for years 1995-1997 (all but the last year) are open for everybody according to the Rules of the Road. KP for years 1995-1996 are also available at the ISTP CDAWeb page . To access KP for the last year other interested researches should contact the INTERBALL Scientific Committee or respective PI . How to access KP ? ...

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• INTERBALL-TAIL KP
• INTERBALL-TAIL KP changes
• AZ Key parameters, 1998