... Meta Index / Home Page This section documents the parameters recognized by this task (if any). Parameter . ... tables . ... list of table specifiers . ... This is the list of input GTI tables to be merged. withgtitable . ... boolean . false . true false . Boolean parameter controlling whether or not the name of the resulting output table is to be explicitly given in parameter gtitable . In the latter case the resulting single GTI table will replace the first input table of tables . ...

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Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...

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... GOODS unites extremely deep observations from NASA's Great Observatories, Spitzer , Hubble , and Chandra , ESA's Herschel and XMM-Newton , and from the most powerful ground-based facilities, to survey the distant universe to the faintest flux limits across the electromagnetic spectrum. ... The space-based observations are complemented by ground-based imaging and spectroscopy, including extensive commitments of ESO and NOAO observing time. ... 2010-04-10: Deep VLA 1.4 GHz data for GOODS-North . ...

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• How precise are the parameters of my double star as measured in Transfer Mode?
• covar2ellipse.pro (JWST Pipeline routines in IDL)
• STScI Preprint #1200

... Posts tagged ?Bayes Theorem? ... As if great books about probability and information theory for statisticians and engineers exist, I believe there are great statistical physics books for physicists. ... In this regard, I thought the lecture note can be useful. [arxiv:physics.data-an:0808.0012] . ... Category: arXiv , Bayesian , Cross-Cultural , Data Processing , Fitting , Physics , Stat | ... Tags: Bayes Theorem , Bayesian , BEHR , prior , prior propagation , Tom Loredo . ... SAMSI AstroStat Prog. ...

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• The AstroStat Slog Tom Loredo
• The AstroStat Slog Blog Archive ab posteriori ad priori
• The AstroStat Slog prior propagation

Photometry of galaxies in U B V R and I . HyperLeda home | ... The present catalogue continues the compilations published by G. Longo & A. de Vaucouleurs (1983, 1988 Monographs of University of Austin). ... We have updated this catalogue by scanning the literature and extended it by adding aperture photometry derived from published surface photometry. ... We used the catalogue of aperture photometry to derive global photometric parameters from growth curve fitting. ... Photometric type . ...

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• HyperLEDA documentation: parameter: logd25
• Saving and Loading Session Parameters
• Session Parameters

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• casacore: scimath/Functionals/FunctionParam.h Source File
• Task parameter manipulation
• Unified Radio Catalog: results for Version 1.1

... 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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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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• Tunable Kernel Parameters?
• Determination of the Detector Parameters
• Where are the tunable parameters of the kernel?

... 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 . ...

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• Stellarium: RingParams Struct Reference
• Stellarium: core/StelSphereGeometry.hpp File Reference
• Stellarium: StelCircleArcRenderer Class Reference

Organisers: Philippe Lebacque (Laboratoire de Math matiques de Besan on ) , Michael Tsfasman (CNRS, Laboratoire Poncelet, Institute for Information Transmission Problems) , Alexey Zykin (Laboratoire Poncelet, State University Higher School of Economics, IITP) . ... General Information . ... The classical differential Galois theory studies symmetry groups of solutions of linear differential equations. ... Poncelet Laboratory web page . ...

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• Conference Global Fields

... 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 . ...

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• The 50" Great Melbourne Telescope, 1868-2003
• The Great Melbourne Telescope in Melbourne

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

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• Initial parameters of compact stars
• Other parameters of the evolutionary scenario
• Initial Distributions of Binary Parameters

... 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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• ADASS 2003 Conference Proceedings
• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• The SRON-HeaD Data Analysis System

... Impact of Covariance Information on the Orientation Parameters Between Radio Source Position Catalogs, IVS 2012 General Meeting Proceedings, p.339­341 http://ivscc.gsfc.nasa.gov/publications/gm2012/sokolova.pdf Impact of Covariance Information on the Orientation Parameters Between Radio Source ... IVS Analysis Centers provide these catalogs in a standard IERS format, where together with radio source positions and other relevant information, RA/DE correlations are reported. ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm09a.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/kurdubov.pdf

... N.V. Bystrova "Some comparisons of the Galactic HI disk and the Magellanic Stream", The Magellanic Clouds Newsletter, An electronic exchange on the Magellanic Clouds research, Edited by Eva K. Grebel You-Hua Chu, Chicago,IL., ... N.V. Bystrova "Some comparisons of the Galactic HI disk and the Magellanic Stream", JENAM-2000, Moscow, Russia, Abstracts, p.50. ... N.V. Bystrova "The great circle of the Magellanic Stream - the HI observations", JENAM-2000, Moscow, Russia Abstracts, p.103. ...

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• Results scientific researchs 8
• harak_e
• SCORPIO parameters

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• Vladimir Marsakov Abstracts
• Population of Galactic globular clusters, tabl

... 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: ...

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• Preparation of parameter file
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• Parameters

... The possibility to use the electrostatic approximation to calculate the polarizability allows one to consider practically any shape scatterers - from the regular ones (ellipsoid, cylinder, disc) [ 7 , 274 ] to those with an arbitrary shape, structure and anisotropy [ 308 , 309 , 313 , 405 ] (in the last case the polarizability tensor should be found numerically) - using the theory of the Rayleigh scattering. ...

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• Linear polarization: wavelength dependence
• AI SPbU library of scattering codes
• Database of Optical Properties -- Level: subpage

THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/Greg/Publications/ms38/ms090.pdf
• http://selena.sai.msu.ru/Pug/Publications/m44_70_pugacheva.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms084.pdf

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. ...

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• HSTPOLIMA (V1.00) --- April99 --- HSTPOLIMA (V1.00)
• HSTPOLPOINTS (V1.00) --- May99 --- HSTPOLPOINTS (V1.00)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)