Next: File Formats Required Up: OPTOPUS Commands and Previous: Optopus commands . Below follows a description of all parameters that can be set by the SET/OPTOPUS command, the commands which use these parameters and the default values. ... If an OPTOPUS command the default value is not used the command will, in addition to actual OPTOPUS operation, also overwrite the setting of this parameter and hence will change the default value. ... set the equinox . ... Table: Command parameters . ...

... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... Aperture Coordinate System . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... Position . ...

... New item added to the "rejflags" parameter. Version 1.17 - 2002-08-19 (UL) ------------ + now DEPENDs on package sas + a few transparent changes to improve C++ standard compliance Version 1.16 - 2002-05-29 ( JDR ) ------------ - requires rgslib-1.29 - added ON_NODE_INTERFACE to --rejflags parameter default - replaced NEXT_TO_CCD_BORDER with ON_WINDOW_BORDER - propagates EXPIDSTR from input to output, if present Version 1.15 - 2002-05-09 ( JDR ) ------------ - requires param-2.0 ...

... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...

Routines can now be called with keyword arguments and can use default arguments, that means that some arguments can be given with keywords instead of position and some do not have to be given at all, in which case a standard or default value is used. ... IMPLICIT NONE INTERFACE SUBROUTINE SOLVE (A, B, N) INTEGER, INTENT (IN) : : N REAL, INTENT(OUT) : : A REAL, INTENT(IN), OPTIONAL : : B END SUBROUTINE SOLVE END INTERFACE REAL X ! ... You will use keyword arguments and default arguments so that . ...

... SphereParams Struct Reference . ... SphereParams (const float radius) . ... Definition at line 50 of file StelGeometryBuilder.hpp . ... Definition at line 103 of file StelGeometryBuilder.hpp . ... Definition at line 120 of file StelGeometryBuilder.hpp . ... Definition at line 112 of file StelGeometryBuilder.hpp . ... Definition at line 118 of file StelGeometryBuilder.hpp . ... Definition at line 110 of file StelGeometryBuilder.hpp . ... Definition at line 114 of file StelGeometryBuilder.hpp . ...

... 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: ...

... Calculations of at least two runs with different values of a parameter are required in order to discover to what extent the results depend on the , if at all. ... In order to study how the final statistical distributions depend on the initial functions, the method of Green functions is used. ... Then we can restore any distribution on this parameter (with a certain accuracy) by summing the results for each interval with the appropriate weight. ...

... The initial descriptions of the FITS format provided a simplified method for describing the physical coordinate values of the image pixels, but deliberately did not specify any of the detailed conventions required to convey the complexities of actual image projections. ... They were CRPIX n for the reference pixel location on pixel axis n , CRVAL n for the coordinate value at that pixel, CDELT n for the increment at that pixel in the coordinate value, and CTYPE n for the type of coordinate. ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

function idlabel, idstr ,idx,Zbeda=Zbeda,Ibeda=Ibeda,Wbeda=Wbeda,Lbeku=Lbeku,$ wform = wform , wstyle = wstyle ,sep=sep, intex = intex , _extra=e ;+ ;function idlabel ; return a string array containg a nicely formatted set of labels, ; appropriate for each of the IDs in an ID structure. ; ;syntax ; label=idlabel( idstr ,idx,/Zbeda,/Ibeda,/Wbeda,/Lbeku,$ ; wform = wform , wstyle = wstyle ,sep=sep, intex = ...

/misc/gauss2.pro' ; ;*********************************************************************** ;+ ;*NAME: GAUSS2 ;*CLASS: ; numerical function ;*CATEGORY: ; ;*PURPOSE: TO CALCULATE A GAUSSIAN FUNCTION ; ;*CALLING SEQUENCE: ; GAUSS ,X,X0,DX, YMAX ,Y ; ;*PARAMETERS: ; X ( REQ ) (I) (0 1) (I L F D) ; required scalar or vector containing the independent variable(s) ; ; X0 ( REQ ) (I) (0) (F D) ; required scalar giving the center of the Gaussian ... If DX = 0, the delta function is returned. ...

lte-codes . Sterne . ... In 2006, Behara and Jeffery introduced a new file format for the model atmospheres produced by STERNE and used by SPECTRUM and SFIT. ... allow depth-dependent descriptions of composition, and . ... model.lambda_ref <lambda ref > . ... abundance < elem > < abund > . ... structure.abundance < elem > : ( needs N depth ) . ab elem,1 , ab elem,2 , ..., ab elem,Ndepth > . ... structure.tau_ref : ( needs N depth ) . ... structure.opac_ref : ( needs N depth ) . ...

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 . ...

... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

... 8, ``Celestial Mechanics'', 2002 Parameterization of the Solar Radiation Pressure model for GPS satellites I. S. Gayazov Institute of Applied Astronomy, St. Petersburg, Russia The treatment of solar radiation pressure (SRP) effect until now is the main problem in precise modeling of GPS satellite orbits. ... In practice, however, all seven parameters of the empirical model cannot be confidently determined from phase observations. ... Bar­Sever Y. E. A new model for GPS yaw attitude. ...

Azimuth Drive Box Replacement . ... A. Start with drive box with soft spring preload Drive #2 . ... Loosen horizontal foot . ... Loosen horizontal foot the remaining amount , push preload foot in to ring and work drive box away from disc. Once clear of disc raise hoist and remove drive box . ... Lift new box in place - do not contact drive disc with box . ... Connect tangential link and set alignment using drive box to disc clearance and foot centering as metrics . ... Repeat for each box. ...

... Thus all regions of the 0.94-2.50 micron wavelength range accessible from Mauna Kea can be recorded using five fixed angle gratings. ... Grating Angle . ... Efficiencies for the NIFS gratings are shown above. The NIFS spectrograph uses a Bouwers collimator and a refractive camera. ... With these assumptions, the NIFS system efficiency including the Gemini telescope optics but excluding the transmission of the adaptive optics system is about 0.17 e - /photon at J , and 0.22 e - /photon at H and K . ...

program test_spline implicit none ! define sizes of arrays integer, parameter :: m = 20 ! size of arrays used by NAG to store spline integer, parameter :: lck = m + 4 ! size of NAG work array integer, parameter :: lwk = 6 * m + 16 ! find the kind of a high precision variable, by finding kind(1.0d0) integer, parameter :: dp = kind(1.0d0) integer :: i, ifail ! NAG requires high precision variables real(dp) :: x(m), y(m), & lambda(lck), c(lck), work(lwk), & xv, yv ! ...

... 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 ...