. XMM-Newton Science Analysis System . eposcorr (eposcorr-3.12.1) [xmmsas_20080701_1801-8.0.0] . Meta Index / Home Page / Description At the moment we have no rigurous mathematical method to handle the statistical errors of the offsets found. For the moment we use the square root of the second order moment in as a function of off-set divided by the number of optical counter parts. XMM-Newton SOC/SSC -- 2008-07-01

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• Description

... The analysis and reduction of the STIS flanking fields proceeded in similar fashion as for the imaging of the Main STIS Field. ... The DARK calibration reference file used in the CALSTIS data reduction steps was constructed using a 'delta-dark' image appropriate for the epoch of the flanking field observations. ... DRIZZLE drop-size used for the flanking fields was a "pixfrac" of 0.8. ... For information on the data reduction, please read first the technical information for the Main WFPC2 Field . ...

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• A Brief Description of the Instrument and Its Operation
• GHRS Instrument Science Report 073: A Description of the Phenomenon
• A Description of the Phenomenon

... 173Wall Peacock We catalogue the brightest extragalactic radio sources at 2.7 GHz. ... These data were originally presented in Wall and Peacock, MNRAS, 216, 173. The values in parenthesis include (units, datatype, example). 1 iauname Name of source in IAU convention (char7, example: '0320-37') . ... 3 ra_1950 rad Right ascension of source in radians (B1950) (real, example: 0.876068) . ... 9 alpha Spectral index of source between 2.7 and 5 GHz (real, example: 0.52) . ... Longair, 1975 . ...

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• A VLA Survey of the First Quadrant of the Galactic Plane at 1.5
• Instrument Description: CASPEC
• MIDAS utilities for time series analysis

Each file type known to SAOtng can have user-defined analysis commands associated with it. ... A help line describing the file types . ... For example, the default analysis file currently contains the following: # # Analysis command descriptions: # help # file templates # file types # analysis command line counts -- number of events in region (no background) *.qp *.imh QPOE IMH uiraf '${xraybin}'/x_xspatial.e imcnts source='${filename}' region=$sregion bkgd=0 table=NONE | ...

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• Topics in AstroStatistics
• Marker Analysis Routines in SAOtng
• Funtools and DS9 Image Display

... 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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• Yu. Burman: Publications

As the Universe expands, gravity pulls on the Universe, and slows the expansion down over time. As we look to great distances, we are looking back in time. If we can measure how fast the Universe is expanding in the past, and compare it to how fast it is expanding now, we can see the total gravitational effect of all matter in the Universe. Here we plot the distance between two galaxies as a function of time. ... Universes with lots of material . ...

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• GSAOI Instrument Description Page
• Gemini NIFS Brief Description.
• GSAOI Bulk Motions Science Page

... Up: Data Analysis Applications . Previous: Mixing IRAF and Starlink Applications - FIGARO under IRAF . ... An infrared-array reduction and analysis package which is written in the IRAF environment has been developed to handle the huge amount of data obtained at the Teide Observatory using the 1.5 m Carlos S?nchez Telescope with the new infrared Camera/Instituto de Astrof?sica de Canarias(IRCAM/IAC). ... One of the advantages of this package is that it can easily handle the large amount of data. ...

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• A Computer-Based Technique for Automatic Description and Classification of
• The SRON-HeaD Data Analysis System
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared

... Classes . ... casa::PrecTimer . ... Precision timer to measure elapsed times in a cumulative way. More... #include < PrecTimer.h > . ... The PrecTimer supplements the Timer class. ... Get the real time (in seconds). void casa::PrecTimer::print_time . ... Show real time on cout or a user supplied stream. void casa::PrecTimer::show . ... Show real time on cout or a user supplied stream preceeded by the string parameter. void casa::PrecTimer::start . ... long long casa::PrecTimer::total_time . ...

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• casacore: TableMeasures_module
• casacore: casa::SofaTest Class Reference
• casacore: Measures_module_internal_classes

Section I: Introduction to ALFA and GALFA . Section II: System Description . ... ALFA receives 7 beams, 2 polarizations per beam, each covering 1225-1525 MHz. The 14 IF signals cover nominally the 100 to 400 MHz band. ... A high-resolution, low-bandwidth spectrometer (8K channels covering a 7 MHz bandwidth) . ... Each spectrometer board handles two polarizations from one telescope beam.The baseband signals are to be digitized by four 8-bit ADCs at 100 Msamples/sec. ... Bandwidth: . ...

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• DATA ANALYSIS
• Project Description
• Some Useful Routines for On-Line Data Analysis

... IBIS Instrumental Characteristics . ... Usable Wavelength Range . ... 2.5 frames/second @ 1024 x 1024(full-resolution) . 4 frames/second @ 512 x 512 (2 x 2 binning) . 4 frames/second @ 1024 x 512 (full-resolution) . ... Maximum Radial Wavelength Shift . ... Wavelength Drift of Transmission Profile . ... Wavelength Tuning Time . ... IBIS Fabry-Perot Characteristics . Fabry-Perot #1 . ... Nominal . ... Measured . ... 0.002 . ...

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• The LongSp Description
• IBIS: Technical Description
• Description of program searchdup

... It consists of two energy-angle analyzers EA-2 and EA-3 for low energy particles, and two identical oppositely directed time-of-flight (TOF) analyzers EM-1-1 and EM-1-2 for high energies. ... Analyzers of low energy charged particles (EA-2 and EA-3). ... The instruments allow to measure simultaneously in eight angular sectors evenly distributed in the angle 2 perpendicular to the satellite rotation axis, and sequentially in 7 energy intervals for each angular sector. ... Interval . ...

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• Space physics cordinate systems
• PhSRM
• ASCII files description

Multi-Frequency Synthesis in K-band . The Multi-Frequency Synthesis (MFS) permits to realize a good quality imaging of the continuum radio sources in short time. ... The RadioAstron mission will operate one K-band circular polarized channel at fixed frequency 22,232 GHz. ... In general one K-band RadioAstron channel with fixed frequency will be unchanging and compatible with all the ground radio telescopes. ... Progress of the RadioAstron Project in Pictures . ...

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• Description of the RadioAstron project, russion version

... Bojan Nikolic web pages (r. 329) . Out-Of-Focus (OOF) Holography . ... The architecture of the OOF data reduction software can be summarised in following points: . ... A well defined set of external libraries is used and generally newer versions of these libraries are adopted quickly after release . ... Routines for simulating OOF data-sets . ... OOF ? ... Description of the OOF software architecture . ... OOF Reduction Software . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• OptInt PmWiki : Site / Page List Templates
• OptInt PmWiki : Page List Templates
• OptInt PmWiki : Production Software PDR To Do List | History

... The low energy plasma composition spectrometer AMEI-2 is built to be able to find in the low energy range of the phase space (E, q, j) and separate the fluxes of the major ion species in the magnetotail - H+, He++, He+ and O+, and analyse their energy and angular distributions. ... Electrostatic angular scanning in one direction and the use of the spin of the satellite to sample the other angle give the ability to measure 2-D distributions for each ion specie several times per spin. ...

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• INTERBALL/ELECTRON EXPERIMENT
• List of currently available KP AZ.
• Format Documentation of *.wdc Files

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Midas

. Comedi Documentation . Prev . Next . comedi_sv_measure -- slowly-varying inputs . #include <comedilib.h> . int comedi_sv_measure (comedi_sv_t * sv, double * data); . The function comedi_sv_measure() uses the slowly varying Comedi structure sv to measure a slowly varying signal. If sucessful, the result (in physical units) is stored in the location pointed to by data, and the number of samples is returned. On error, -1 is returned. Prev . Home . Next . comedi_sv_update . Up . comedi_get_cmd_src_mask

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• comedi_do_insn
• comedi_sv_init
• Format of data description

GENERAL DESCRIPTION OF DATABASE . It is a matter of common knoledge, that solar magnetic fields and, in particular, magnetic fields of sunspots, play important role in many solar events. In Pulkovo observatory the long-term data set of daily observations of magnetic fields of solar sunspots was accumulated, which contains great potential for further researches in solar physics. ... Second section includes files containing sum data about magnetic fields for every observational day. ...

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• General description of the database
• Structure of the database files
• Datafile structure

... Download . Description . ... Utilities for building libraries and applications . ... f77 . Global COMMON referenced with f77 INCLUDE statement . ... f77/f90 . ... Tools for building a spectral atlas . ... f77/f90/make . ... Obtaining the software . ... Building subroutine libraries . ... Building spectrum . ... Detailed reports describing bugs in the download/installation procedure or in the software itself will be welcome and should be addressed to Simon Jeffery at the address below. ...

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• Index of /archives/ArmaghObservatory/Huggins-Spectrum-Analysis M41
• Armagh Observatory: Chris Winter [ Documents ]
• Index of /archives/collections/Huggins

MATHEMATICAL MODELING: . ... This model is developed on the base of the probabilistic description of the collisional aeronomical processes and is realized on a computer as the numerical system (stochastic model). ... Shematovich, V.I., Bisikalo , D.V. ??????????? Nonequilibrium processes in the planetary and cometary atmospheres. ... In Russian) . ... Piarnpuu , A. A.; and Shematovich, V. I. ????? Construction of structural stochastic models of collision processes in rarefied gas media (abstract) . ...

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... Recent Topics . ... Forum . MAO main . Flame . The "Flame" description . ... The English description is not quite correct, I suggest something like: . ... Just testing forum . The administrator has disabled public write access. sekanato . ... Description changed. ... The administrator has disabled public write access. Board Categories MAO main - Info - MAO - news - Flame Technical - Technical Support(Forum)(Техподдержка(Форум)) . ... Powered by Kunena Forum . ...

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• Traffic Analysis for UARNET -- ursa
• Traffic Analysis for ursa (UARNET)