... Meta Index / Home Page / The task window . Source list table Stores information about each source in the current source-list. ... This table is cleared when a source is selected. average magnitude table This table stores the running average magnitudes computed from the logger table- each time the apply button is clicked an average magnitude is computed from all the entries in the logger table and added to the table. ...

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• Parameters

Next: The Schedule File Up: THE SCHED USER MANUAL Version Previous: Satellite Tracking Contents . This chapter covers the main input files that SCHED reads. ... See the SCHED Input and Output Files section of this manual for brief descriptions of the files and pointers to the standard versions. ... Summary List of SCHED Parameters . ... List of Frequency File Parameters . Setup Files . Standard Setup Files . ... Summary List of Setup File Parameters . Details of Setup File Parameters . ...

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• DOVEX
• Graphical User Interface Example (3)
• STATions

... 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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• Simulation of HST PSFs using Tiny Tim
• Interactive Fitting of EUVE Emission Line Spectra
• TwoFitlines: An Spectrum and Line Analysis Tool

... A photometric analysis was made of the simulated images using two of the widely available reduction programs, ROMAFOT (Buonanno et al. 1983) and DAOPHOT (Stetson 1987). ... The rebinned and expanded image gave better results (Fig. 7b), with the smallest errors in the order of = 0.04. ... Similarly to ROMAFOT, the image with the Moffat PSF gave significantly better results than the image generated with the Tiny Tim PSF; the errors in the magnitudes of the brighter stars were around = 0.02. ...

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• Model Fitting
• Prescription Retrieval
• Starburst99 - Chronology

Next: Individual data Up: Final results Previous: Residual plots . After the last residual plot, the final parameter values (and their errors) are printed, including the magnitudes and colors of the individual stars in the extinction solution. ... This is followed by a table of the individual residuals, which includes the symbols used to identify different stars in the residual plots. ... Tue Mar 28 16:52:29 MET DST 1995 ...

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• HyperLEDA documentation: parameter: celpos
• ASTROMET/TRANSFORM
• Line parameter measurements

... Several of the tasks in the spectral package share a common set of parameters. ... Each task in the spectral package has a hidden parameter which points to the pkgpars parameter file. The parameters stored here include the observed data sets and the model descriptor, and instrument-specific parameters. ... The observed counts and error data set contained in the table file ( *_obs.tab ) produced by qpspec will be the input data for subsequent spectral tasks. ...

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• The AstroStat Slog Blog Archive [ArXiv] Recent bayesian studies from astro-ph
• Editing Files and Parameters
• What are the popular words from #AAS221?

Next: About this guide Up: General information Previous: General information Contents . is the original interactive data reduction package developed for the Navy Precision Optical Interferometer at Lowell (NPOI). is an endeavor to combine all aspects of data reduction, modeling, astrometry, and imaging, including a stellar database, with an interactive data language in one package. ... Next: About this guide Up: General information Previous: General information Contents Christian Hummel 2015-04-28 ...

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• OYSTER Lab
• Include detmon as a generic pipeline
• Parameters

... Links given for particles of different shapes allow 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 . ... Q ext , Q sca , Q abs , Q bk , albedo, g, Q pr vs x for different m core , m mantle , V core /V total . ... Q ext , Q sca , Q abs , albedo, Q pol vs x for different m, alpha . ...

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• AI SPbU library of scattering codes
• Linear polarization: wavelength dependence

... The value of tile-size, NW , may be thought of as a sixth coordinate axis in the chirplet transform parameter space - TF-area. Including this sixth coordinate axis provides us with a hierarchical (multi-resolution) CCT. ... Various 2- D slices through the multiresolution CCT may correspond to useful tilings of the TF plane with true parallelograms (true to the extent that the DPSS define a truly rectangular region in the TF plane). ...

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• Introduction
• NAG's Fortran 90
• The Chirplet Transform: Physical Considerations

... Chapter 15. 15.0 Introduction Modeling of Data Given a set of observations, one often wants to condense and summarize the data by fitting it to a "model" that depends on adjustable parameters. Sometimes the model is simply a convenient class of functions, such as polynomials or Gaussians, and the fit supplies the appropriate coefficients. ... The parameters of the model are then adjusted to achieve a minimum in the merit function, yielding best-fit parameters. ... Data are generally not exact. ...

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• http://www.arcetri.astro.it/irlab/doc/library/nr/f15-0.pdf
• http://www.arcetri.astro.it/irlab/doc/library/recipes/bookcpdf/c14-0.pdf
• http://www.arcetri.astro.it/irlab/doc/library/nr/f14-0.pdf

... This program will be a part of AATM-0.06 examples when this version is released. ... Comments regarding this example welcome at: // Bojan Nikolic b.nikolic@mrao.cam.ac.uk // # include string # include vector # include iostream # include fstream // Unfortunately the using statement below is required because of poor // desgin of the header files using namespace std ; # include ATMRefractiveIndexProfile.h # include ATMPercent.h # include ATMPressure.h # ...

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• OptInt PmWiki : PmWiki / Include Other Pages
• DUST: dustiface.h File Reference
• OptInt PmWiki : PmWiki / Page Directives

Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... Skybright Class Reference . Compute the luminance of the sky according to some parameters like sun moon position or time or altitude etc.. ... setDate (int year, int month, float moonPhase) . ... Set the moon and sun zenith angular distance (cosin given) and precompute what can be This function has to be called once before any call to getLuminance() More... љ . ... cos(angular distance between moon and the position) . ...

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• Stellarium: core/StelSphereGeometry.hpp File Reference
• Stellarium: gSatTEME Class Reference
• Stellarium: SphereParams Struct Reference

National Aeronautics and Space Administration . ... Gregory Errol Chamitoff (Ph.D.) . NASA Astronaut (Former) . ... NASA EXPERIENCE: In 1995, Dr. Chamitoff joined Mission Operations at the Johnson Space Center, where worked as a Guidance and Control Flight Controller. ... SPACE FLIGHT EXPERIENCE: Expedition 17/18 - In 2008, Dr. Chamitoff served as the flight engineer and science officer for a 6-month mission aboard the International Space Station during Expeditions 17 and 18. ... OCTOBER 2013 . ...

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• Astronaut Bio: Bruce McCandless II

... MAXLEN parameter specifies maximum length of the number considered as a 'good' integer. ... If REJECTLONG = FALSE (default), than dictionary returns prefixed part of integer number with length MAXLEN . ... This is a dict_tmpl.c file. # include postgres.h # include utils/builtins.h # include fmgr.h #ifdef PG_MODULE_MAGIC PG_MODULE_MAGIC; #endif # include utils/ts_locale.h # include utils/ts_public.h # include utils/ts_utils.h typedef struct { int maxlen ; bool rejectlong ; } ...

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• Further Information and Bibliography
• Zen: Gendict
• Zen: GiST internals

... IAA VLBI Analysis Center . ... First IAA SLR EOP submission to IERS Annual Report . ... Beginning of operational processing of SLR observations . ... We use several program packages for analysis mostly developed at the IAA: GROSS for processing of the SLR observations and analysis of EOP and coordinates time series, OCCAM/GROSS for computation of EOP, station coordinates, and troposphere parameters time series from the VLBI observations, GRAPE for processing of GPS observations. ...

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• NAA-2
• (Untitled)
• Annotation_26

last updated 03dec01 gain,tsys,sefd,pntErrs,beamwidth,coma,beam efficiency . Coma versus pitch and roll errors. ... Figure 1 is the gain (K/Jy) versus zenith angle (top plot) and versus azimuth angle (bottom). ... Their gains . Figure 2 plots the gain versus azimuth and zenith angle. ... The bottom plot is the pointing error (az,za error added in quadrature) versus zenith angle. ... Figure 2 bottom plots the pitch +roll errors (combined in quadrature) versus the coma parameter. ...

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• WAPP File Format Page
• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA
• Your NED Search Results

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... include . tcc . tcsShim.h . ... 51 љ double const FL = 1.0; . ... 97 љ std::ostream & operator<< (std::ostream &os, ASTROM const &astrom); . ... 99 љ std::ostream & operator<< (std::ostream &os, FLDOR const &fldor); . ... 101 љ std::ostream & operator<< (std::ostream &os, PORIG const &porig); . ... 103 љ std::ostream & operator<< (std::ostream &os, SITE const &site); . ... 105 љ std::ostream & operator<< (std::ostream &os, TARG const &targ); . ...

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• lsst.coordConv: coordConv::PVTCoord Class Reference
• lsst.coordConv: coordConv::Coord Class Reference
• lsst.coordConv: include/coordConv/site.h Source File

Enter the model parameters in the left (control) frame and press the "Compute" button. ... To save the parameters, press the "Save locally" button in the control frame. Your browser will be asked to save the parameters of your model into a local file on your computer. After the file is saved, you may close your browser and have a cup of tea, then open this file it by your browser to continue working with the saved parameters. ...

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• World Wide Web version
• Be/X-ray binaries and candidates
• Initial Distributions of Binary Parameters

The magnetic mapping is fulfilled by the magnetic field line tracing from the satellite position up to the Ionosphere (stop trace at the altitude 110 km). ... As a rule the Tsyganenko [1987] external magnetic field model and IOPT = 3 (Kp = 2) are used. ... The output file includes the following information: . ... For example the file with name aa9610d1.geo contains the information corresponding to the aposteriory magnetic mapping for INTERBALL Auroral Probe for the first decade of October 1996. ...

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• WAVE EXPERIMENTS ON TAIL PROBE
• INTERBALL MAGION 5 SITUATION ANALYSIS
• INTERBALL TAIL PROBE SITUATION ANALYSIS

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

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