... Parameters can be used as fixed or free parameters depending on the setting in MASK= To fix a parameter use 0. ... Use box -4 -10 9 5 and let all parameters be free in the fit : USER qfit USER QFIT FILENAME= data USER QFIT APPEND= USER QFIT AUTOVIEW=y USER QFIT INSET=n4736ave 1 Set n4736ave has 3 axes RA from -20 to 20 DEC from -31 to 20 LAMBDA from 0 to 1 BOX range for set n4736ave : RA from -20 to 20 DEC from -31 to 20 USER QFIT CLIPLOHI= ...

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• http://www.atnf.csiro.au/computing/software/gipsy/tsk/antpat.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/tsk/rotcur.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/tsk/rotmod.dc1

... The models provided are: . abs - absorption of x-rays by neutral gas with solar abundances. parameter 1 = . ... parameter 2 = . ... normalization - logarithmic value of the flux density at 1 keV in units of keV cm -2 s -1 keV -1 . ... normalization - logarithmic value of the normalization of the gaussian in units of keV cm -2 s -1 . ... absorption ( params )* model ( params ) . ... A single value for the normalization (i.e., fixed normalization) will force the program to use that value. ...

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• PoA Style Guide
• Table Filtering

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Program use
• Tunable Kernel Parameters?

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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• Initial parameters of compact stars
• Dependence on the Scenario Parameters and Initial Distributions
• Initial binary parameters

... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• Pulkovo NEO Page: Ephemeris Support

Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

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• Photometric Analysis
• GLSFit.pro (JWST Pipeline routines in IDL)
• covar2ellipse.pro (JWST Pipeline routines in IDL)

System parameters on Digital UNIX . ... Digital and Cray use the number of bytes as the KIND -parameter. ... LOGICAL Default byte word KIND number = 4 1 4 LOGICAL Default double quad KIND number = 4 8 16 INTEGER int15 int31 int63 KIND number = 2 4 8 digits = 15 31 63 radix = 2 2 2 range = 4 9 18 huge = 32767 2147483647 9223372036854775807 bit_size = 16 32 64 REAL single double quad KIND number = 4 8 16 digits = 24 53 113 maxexponent = 128 1024 16384 minexponent = -125 -1021 -16381 ...

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• Keyword arguments and default arguments
• NAG's Fortran 90

... 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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• TwoFitlines: An Spectrum and Line Analysis Tool
• Calculating the Position and Velocity Components of HST
• A Computer-Based Technique for Automatic Description and Classification of

... Creates a 1D image containing the continuum and possible emission lines. Induces absorption features on this image. ... The package contains: 4 commands: CREATE/PSF : creation of the instrumental response . COMPUTE/EMI : computation of the initial unabsorbed spectrum . COMPUTE/ABS : main program, computation of the theoretical . ... TUTORIAL/CLOUD : on line tutorial . 3 tables: EMI : contains the emission line parameters . ... ABSC : contains the absorption line parameters . ...

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• Running a Program within MIDAS
• Symbol Substitution in Command Procedures
• Documentation: LEDA: parameter:

... Meta Index / Home Page This section documents the parameters recognized by this task (if any). ... The name of the FITS dataset+table which contains the input source list. ... Switch which specifies whether the source list (after filtering with expression ) should be truncated at some maximum number, specified by parameter ncut . ... This parameter is read by the task if withlabels =`yes' and controls how source labels are assigned. ... This parameter is read if outfilestyle =`prefix'. outfile . ...

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... The described algorithm is suitable for measurements of complex images of stars. ... a) the zero-based number of stars in the complex (multicentric) image, . b) set of preliminary coordinates - x i , y i , for all stars, index i is number of a star, . ... i - index of a star in the complex image; . ... These parameters are calculated by a nonlinear method of a least squares.The main output parameters of this algorithm are x i , y i ; where the index i is number of a star in the multicentric image. ...

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... Scoring Necessary step towards more automated certification Idea: · define key QC1 parameters , check new values against trending for those · evaluate compliance: o if new within defined range, ok o if outside: nok · user may focus on nok ones, while ok is certified automatically in `confidence mode ' Required: · configure set of key parameters per product · configure comparison mode o fixed: ...