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1. Home Page
. XMM-Newton Science Analysis System . hkgtigen (hkgtigen-1.14.2) [xmmsas_20070708_1801-7.1.0] . Meta Index . HouseKeeping parameter driven Good-Time-Interval data set GENeration . Instruments/Modes . Use . Description . Motivation . Detailed Description . Examples . Long and short HK parameter names . Diagnostic mode . Comments . Parameters . Errors . Input Files . Output Files . Algorithm . Future developments . Bibliography . Index . XMM-Newton SOC/SSC -- 2007-07-09
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/hkgtigen/hkgtigen.html -- 4.1 Кб -- 09.07.2007
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2. The SRON-HeaD Data Analysis System
Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/devriesc.html -- 9.7 Кб -- 23.06.1998
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3. STSDAS release notes
... News and . ... Press Releases . ... Description . Release Notes . ... PyRAF . ... Packages or tasks that have had minor enhancements of bug fixes include: analysis.isophote graphics.stplot.igi .skymap hst_calib.ghrs Parameter files that have changed ( new parameters or new default values, excluding prameters indicating version number changes): analysis/dither/acsdq.par (the following should all be considered new even though some have correspondences in the previous version of ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/software_hardware/stsdas/relnotes/stsdas33_summary -- 24.5 Кб -- 11.04.2016
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4. Program parameters
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 . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/Radio/red/searchdup/node2.html -- 8.0 Кб -- 30.06.2000
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5. http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/jg_mksp.pdf
Applying Bayesian analysis to polarisation data J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR MKSP Workshop 1 / 15 Outline 1 2 3 4 Polarisation simulations @ radio wavebands Bayesian analysis Analysis of polarisation data Conclusions J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/jg_mksp.pdf -- 784.2 Кб -- 09.04.2009
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6. Parameters of binary compact star evolution
... 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. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~lipunov/kionewht/node9.html -- 7.2 Кб -- 16.06.2000