... read input parameters find angles of the SIAM corresponding to current instrument STATT: calculate pointing of the star-tracker for ref attitude SRCinFOV: calculate FOV positions of 5 test sources intended FOV positions: add offsets (ry,rz) to FOV positions of 5 test sources minimize distance of "intended FOV positions" from SRCinFOV positions by of iteration SIAM angles and re-calculating STATT and SRCinFOV. print resulting angles . ...

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... Values have been scaled arbitrarily. High ratios are shown in blue, corresponding to blue colors, and low ratios are shown in red, corresponding to red colors. ... Noise combined with background subtraction difficulties in the lower left quadrant of the WISP1 data (see Fig. \ref{Fig:wisp_snr_mskd}) make colors in this area very unreliable. ... The values shown here are typically a factor of ~3 less than those calculated for the Schmidt data, shown in Figure \ref{Fig:bj_alpha}. ...

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• Details of Rotang
• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA

... The observed PSF is proportional to the power spectrum of the plane wave incident at the entrance pupil of the telescope (Goodman 1968). ... where is the phase of the plane wave incident on the entrance pupil of the telescope and is a proportionality constant. ... However, Eq. ( 1 ) expresses the PSF as a function of the wave front phase at the entrance pupil. ... Zernike polynomials and their variants are known for better modeling of different aberrations of the phase function ( Zernike 1935). ...

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• Update to the dark rates of the COS FUV segments and impact on ETC calculations
• CSPICE Routines: Q2M_C
• Approach for Calculating an Analytical PSF

... The file names' construction . The flight (m) stage's file set . ... the orbital data used for the flight operation monthly (m) long-term planning, . ... The orbital calculations are based on the initial orbital data determined by KIAM RAN using the orbital radio- measurement treatment. The determined initial orbital data are presented as a state vector (satellite position and velocity) in the J2000 reference. ... Accept the file with extension '.bgr', where the Moscow time (MT=UT+3h) is used. ...

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• Prediction technique
• Tail Probe | Matrix of Transformation Tail Probe | Matrix of Transformation
• Magnetic mapping

... Categories: calibration, map making SELFCAL is a MIRIAD task to perform self-calibration of visibility data. ... The input to SELCAL are a visibility data file, and model images. ... Key: vis Name of input visibility data file. ... Several models can be given, which can cover different channel ranges and different pointing and sources of the input visibility data. ... NOTE: When you give SELFCAL a model, it will, by default, select the data associated with this model from the visibility data- set. ...

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• hermes
• Angular separation of two sources

This is how a typical dispersion modeling result looks when shown as a map. ... Their numerical values are shown at the top. White normally means no data, but high values may be also shown as white if above the fixed high limit (that is, if no automatic normalization is used for colors). Note that calculations were done both for cell positions and for station positions, so both are colored. PO territories are filled by color corresponding to the average value of cells overlaying them. ...

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• Fortran subroutine attid1
• International Organizing Committee (IOC) of MSS-09
• How Orbital Motion is Calculated

Taking into account the result by Watanabe P=2.5 days in outburst, I reconstruct old set of photographic observations being partly lost, and add some new observations. ... The periodogram calculated with the method by Lafler and Kinman is shown. ... The last periodogram indicates peaks corresponding following possible periods with the double-wave light curve: 0.4236, 0.4650, 0.5379, 0.6064, 0.7365, 0.871, 1.168, 1.5437, 2.8173, and 6.89 days. ...

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• di_eks
• Description of algorithm

User has possibility to impose some restriction(s) on the Results of calculation. ... Possible set of restrictions depends on coordinates that were specified for planned run. ... The set of the quantities on which may be imposed restrictions in the next run are highlighted on marking Set restrictions . ... Dist. d(R.A.)/dt . ... Phase . ... To impose restriction on any quantity mark check box at the left of corresponding line and then click on the field where you want to introduce limitative value. ...

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• AY (preface)
• AY2006 (preface)
• AY2008 (preface)

The following figures show the behaviour of the efficiency factors Q ext , Q sca , Q abs as well as albedo and asymmetry parameter g for porous particles. ... These optical characteristics are compared with results of Lorenz-Mie calculations for corresponding n -layered spheres. ... factors . Qext(x) . Qsca(x) . ... Qabs (x) . ... albedo (x) . ... Henning, Modelling the optical properties of composite and porous interstellar grains, Astronomy and Astrophysics , 429 , 371-381, 2005. ...

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• Database of Optical Constants -- Level: welcome
• Model realization and some results
• Rayleigh-Debye-Gans approximation (RDG)

Algorithm for calculations of the Voigt function . ... алгоритма расчета профиля Фойгта ! ... функция Фойгта ! текст модуля на языке Паскаль (Delphi) для ее вычисления ! ... github.com...dawson.cpp процедура Хумличека для вычисления функции Фойгта ! ... Humlicek 1979 JQSRT v21 p309 ! ... 2005A+A___442___11F 2006 Tepper-Garcia, MNRAS, v369 p2025 ! 2006MNRAS_369_2025T 2007 Letchworth and Benner, JQSRT, v107 p173 ! ... 2009JQSRT_110__376A 2014 Abrarov and Quine, J. Math. ...

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... Bojan Nikolic web pages (r. 329) . Out-Of-Focus (OOF) Holography . The circle polynomials of Zernike, or Zernike polynomials, are an infinite set of polynomials orthonormal on the unit circle. ... The code used by the OOF system to calculate Zernike polynomials is available under the terms of the GPL. ... The first column in the table shows some of the labels that are used for the Zernike polynomial shown. ... The GBT= label is the label used by the GBT control software. ... Label . ...

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• Zernike Polynomials
• ALMA WVR phase correction algorithms and software Bojan Nikolic web pages (r.
• DUST: dustiface.h File Reference

My colleagues and I have recently completed a series of observations of SN1999an. ... The telescope is located at Martin Observatory in Blacksburg, VA, and is operated by the Physics Department of Virginia Tech. Our IAU Minor Planet Center Observatory Code is 841. ... Attached you will find a copy of one of our images (in .jpg format) with the supernova indicated. ... Virginia Tech Department of Physics . Back to Bright Supernovae . Back to Supernova 1999an . ...

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. First page Back Continue Last page Overview Graphics .

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• Abstract
• Armagh Observatory
• Astrodynamics 101

... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...

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Next: Pyramidal Algorithm Up: The discrete wavelet Previous: Multiresolution Analysis . ... One assumes that the sampled data are the scalar products at pixels k of the function with a scaling function which corresponds to a low pass filter. ... The signal difference contains the information between these two scales and is the discrete set associated with the wavelet transform corresponding to . ... The figure shows the wavelet associated to the scaling function. Figure: Wavelet . ...

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• Analysis in the time domain
• Introduction
• Echelle Spectra

Next: *upspecrdf, downspecrdf* - Transform Up: Spectral Analysis Previous: *grid_plot* - Plot Results . The conversion of count rate to flux depends on the intrinsic spectrum of the source, so xflux must be used in conjunction with fit . Fit generates a table of the best fit intrinsic spectrum ( _int.tab extension). xflux uses this table to calculate either the integrated flux between two energy limits or the flux density at a specific energy. ... This produces ``..._obs.tab'' file. ...

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• The Chandra Multiwavelength Project (ChaMP) - Spectra
• Data analysis and Spatial Corrections
• The AstroStat Slog Blog Archive a century ago

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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• Long description of example of cell background calculation
• The Chirplet Transform: Physical Considerations
• Notation

Fast algorithm of reconstruction of absolute conductivity distribution in a cross-section of human body by measurements of electrodes' potentials on the skin surface is described. ... This paper describes fast algorithm for absolute conductivity reconstruction and results of its application. ... The main problem under the absolute image reconstruction is obtaining of reference data, corresponding to the object with uniform conductivity and the same electrode positions. ...

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• Getting Started in Actor Prolog. 3D Web Site.
• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.A"
• Getting Started in Actor Prolog. Visual Expert Systems.

Next: Identification and Analysis of Binary Star Systems using Probability Theory . ... We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. ... In the case of slowly rotating stars one can use the zero-rotation approximation to describe stellar pulsations. Such a model was used already by Cugier, Dziembowski & Pamyatnykh (1994) to study nonadiabatic observables of Cephei stars. ...

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• A Computer-Based Technique for Automatic Description and Classification of
• A New PROS Task for Calculating HRI Source Intensities or Upper Limits
• Recreating Einstein Level One Processing Exposure Masks and Background Maps in

Next: Beam procedures and functions Up: Introduction Previous: Introduction Contents . A collection of procedures capable of imaging interferometric data. ... In the latter, a model (list of CLEAN components) is built-up incrementally between phase self-calibrations. ... PEARL will work with the complex visibilities, which have to be initialized with the observed visibility and closure phase data using the set_complexvis procedure. ...

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• Adding plot variables
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• DFS Department internal procedure for issue of documentation