... Up: Fitting of Data Previous: Function Specification . ... C C.INPUT ARGUMENTS : C NIND INTEGER Number of independent variables C X ( NIND ) REAL Array of NIND elements with the C independent variable C NPAR INTEGER Number of parameters C PARAM ( NPAR ) DOUBLE PRECISION Array of NPAR elements with the C values of the parameters C C.OUTPUT ARGUMENTS : C Y DOUBLE PRECISION Value of the function C DERIV ( NPAR ) DOUBLE PRECISION Array of ... Array Arguments .. ...

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• Function Specification
• Outline of the Available Methods
• Parameter estimation

... disprm Struct Reference . ... Returned ) Pointer to the first element of an array of int* containing pointers to the first elements of the arrays of integer distortion parameters for each axis. double ** disprm::dparm . Returned ) Pointer to the first element of an array of double* containing pointers to the first elements of the arrays of floating point distortion parameters for each axis. int disprm::i_naxis . ... Returned ) The number of distortion functions. struct wcserr * disprm::err . ...

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• Pulsar Group PmWiki/Other Variables
• USER-INTERFACE general subroutines
• WCSLIB: cel.h File Reference

... synth : find optimum fit by adjusting abundances v turb , v sin i , and v rad . ... syn_... <p1> <p2> : Initialise parameter for synth . syn_vturb <vturb> [<dv>]; Initialise v turb (km/s) for a fit using synth (default 5) . ... abundance <elid> <abun> <dabu> : Initialise abundances for synth . ... General remarks on the initialisation of abundances in synth A solar abundance will be assumed for any elements not specified. ... Initialise abundances and microturbulence for synth (obsolete) . ...

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• Influence of Climate Variables on Tree-Ring Widths of Different Species
• lte-codes: sterne model atmospheres

Main Page Data Structures File List Data Fields Globals . ... Go to the source code of this file. struct . ... Data for OI_ARRAY FITS table. ... write_oi_array (fitsfile *fptr, oi_array array, int extver, int *status) . ... Data for OI_ARRAY FITS table. typedef struct _target target . ... Data for OI_TARGET FITS table. typedef struct _oi_wavelength oi_wavelength . Data for OI_WAVELENGTH FITS table. typedef struct _oi_vis_record oi_vis_record . ... fptr , . ... array data struct, see exchange.h . ...

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• OptInt PmWiki : PmWiki / Other Variables
• OptInt PmWiki : PmWiki / Debug Variables
• OptInt PmWiki : Other Variables

Following designations of elements/ parameters are used in AMPLE. ... mean anomaly . ... Node . ... Apart conventional orbital elements AMPLE gives possibility to calculate for each minor planet the following often used functions: . ... MOID . ... To calculate MOID user should order the name or the number of the major or minor planet through dialog. ... To calculate CT user should order the name or the number of the major or minor planet through dialog as it is proposed for MOID calculation. ...

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• ENGAMPLE

Viewing contents of file ;'/net/www/deutsch/idl/idllib/iuedac/iuelib/pro/baserem.pro' ; ;************************************************************************ ;+ ;*NAME: ; ; BASEREM 30 SEPTEMBER 1980 ; ;*CLASS: ; ;*CATEGORY: ; ;*PURPOSE: ; ; To fit a polynomial of order NDEG to a user-specified ; spectral region for removing a baseline from a spectral feature. CALLING SEQUENCE: ; ; BASEREM,X,Y,NDEG,XL,XR,A,YBF,CHIS ; ;*PARAMETERS: ; ; X (REQ) (I) (1) (I L F D) ; Array of independent variables. ...

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• http://www.naic.edu/~tghosh/software/pcheck.pro
• Details of Rotang
• Debugging and Tracing

... Fortran . Storage rules Dummy argument is a quantity in the specification of a procedure, function or subroutine. Actual argument is a quantity in the call of a procedure, function or subroutine. ... Becomes 101 END PROGRAM EXAMPLE SUBROUTINE SUB(X, Y, Z) IMPLICIT NONE REAL, INTENT(IN) :: X REAL, INTENT(INOUT) :: Y REAL, INTENT(OUT) :: Z Y = Y**2 Z = X + Y END SUBROUTINE SUB In Fortran there is really only one kind of argument usage, called argument association. ...

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• Tutorial on Fortran 90, Digital UNIX
• Explanation of certain terms
• Specifications

... In laboratory the design and a manufacturing techniques mirror aspherical optics are developed ("fokon", ellipsoid, aspherical mirror).Such optical elements are made of widespread aluminium alloys on the standard equipment without use diamond turning. ... Using: optical blocks of not image optical devices for transitions, collimation, focus (concentration) radiations in a wide spectral range from UV to IR. Focusing and collimation of light; . ... circle aperture/ring aperture; . ... Back Forward . ...

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• Achievements - Page 4

... A file upload element on an HTML form. ... JavaScript 1.1: added type property . ... The HTML INPUT tag, with "file" as the value of the TYPE attribute. For a given form, the JavaScript runtime engine creates appropriate FileUpload objects and puts these objects in the elements array of the corresponding Form object. ... form . ... For all FileUpload objects, the value of the type property is "file" . ... Use the value property to obtain the file name that the user typed into a FileUpload object. ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/submit.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/reset.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/button.htm

Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) Ї Ї Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/perminov.pdf
• Pulkovo NEO Page: Ephemeris Support

The beam pattern and the polarization characteristics . of the radio telescope RATAN-600 . The Mueller matrix elements was computed via formulas [1]: . ... The BP were computed by the aperture method, proceeding from the fild distribution in the aperture of the primary mirror. The components of the main and cross-polarization components of the electric field in the vertical aperture of the primary mirror was computed in Frenel diffraction approximation. ...

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• comedi_get_cmd_src_mask
• Determination of atmospheric parameters and calculation of chemical composition
• Access via e-mail

There are some variables which are set internally by the shell and which are available to the user: Name Description . ... 0 the name of the command currently being executed. $# the number of positional arguments given to this invocation of the shell. $? the exit status of the last command executed is given as a decimal string. ... For example '1 2' 3 becomes "1 2 3" . is identical to the arguments received by the shell, the resulting list of words completely match what was given to the shell. ...

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• HTML Math
• Index: P
• The IMG (Image) Element

Underdetermined sets is a new type of data structures (terms) developed in Actor Prolog . ... The point is that an underdetermined set can include some indefinite rest (a tail) like a list in usual Prolog . At the same time, the order of elements of an underdetermined set can be arbitrary one and it does not affect results of unification of underdetermined sets. Moreover, Actor Prolog guarantees that a rest of an underdetermined set never contains elements that are explicitly given in the set. ...

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Peremennye Zvezdy", . ... Find.Chart . ... GSC 04516-02121 . ... The new variable star 2MASS J00511854+5022580 (indicated as V in the finding chart) is inside the field of view of the known variable star V364 Cas. ... The new variable star GSC 04516-02121 (indicated as V in the finding chart) is inside the field of view of the known variable star V405 Cep. ... The variable star 2MASS GSC 00770-00523 (indicated as V2 in the finding chart) is inside the field of view of the known variable star AV CMi. ...

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Stellarium 0.12.3 . ... Classes . ... Class List . ... Static Public Member Functions . CLIProcessor Class Reference . ... argsGetOption (const QStringList &argList, QString shortOpt, QString longOpt) . Check if a QStringList has a CLI-style option in it (before the first ). ... Retrieve the argument to an option from a QStringList. ... Check if a QStringList has a yes/no CLI-style option in it, and find out the argument to that parameter. ... a long-form option string, e.g. "&ndash;help" . ...

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• StelTextureMgr Class Reference
• Stellarium: StelFileMgr Class Reference

lsst.tcc   1.2.2-3-g89ecb63 . ... Namespaces . ... Files . ... All   Classes   Namespaces   Files   Functions   Variables   Typedefs   Enumerations   Enumerator   Macros   Pages . ... tcc.parse.getCoordSys Namespace Reference . ... Obtain a coordinate system from a parsed parameter. ... Make a coordinate system from its name and date. ... if the coordinate system is unrecognized . Definition at line 31 of file getCoordSys.py . ... coordinate system date, or None for default date . ...

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• lsst.tcc: tcc.msg.formatObjFields Namespace Reference
• lsst.tcc: tcc.parse.getPVTList Namespace Reference
• lsst.tcc: tcc.parse.getPVTPxPMRadVel Namespace Reference

... This page will contain a form to pass parameter values for a on-line working code producing figures illustrating the dependence of optical properties of different scatterers on their parameters. Specify the parameters and press start calculation button to produce a figure. ... Independent variable: x v a/b alpha Re(m)? another? ... Number of curves: 1 2 3 . ... Curve #1: . Particle shape: sphere spheroid another? TE/TM mode: TE TM . Other parameters: x= Re(m)= Im(m)= a/b= alpha= . ...

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• Model realization and some results
• Database of Optical Constants -- Misc: SVM code(s)
• AI SPbU library of scattering codes

... We present a pro ject of an Information system on binary stars (ISBS). ... Stars from the following catalogues will be included in the first version of ISBS: Catalog of orbital elements , masses and luminosities of close double stars ( Svechnikov Bessonova 1984); The catalogue of approximate photometric and absolute elements of eclipsing variable stars ( Svechnikov Kuznetsova 1990); The catalogue of orbital elements , masses and luminosities of detached main-sequence ...

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• ADASS 2003 Conference Proceedings
• The FITS Embedded Function Format
• Data Access Layer to Support Variable Inputs Using C

... Characteristic parameters of subsystems RR Lyrae field stars and globular clusters . ... RR Lyrae . ... 0.05 . ... lim R max , kpc . ... Z o , kpc . ... grad R [Fe/H], kpc -1 . ...

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• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
• Vladimir Marsakov Abstracts
• Vladimir Marsakov Publication List

Before calibrating the visibility data, we need to plot it and flag the blue channels 21 to 32 because of their low signal-to-noise ratio. Select VisSq, the uncalibrated raw (squared) visibility amplitude, and plot it versus channel. ... The data selection defines which data is to be used to compute the correlation parameters, with the exception that if the Option|Loop parameter is selected in the calibration widget, the channels are calibrated independently, doing every selected channel. ...

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• Loading configuration and logs
• OYSTER Lab
• The Hierarchical Stellar Systems Model Format