... epicproc (epicproc-2.9.18) [?? ... The SAS package epicproc contains the two tasks epproc and emproc , that can be used to process the data from the EPIC MOS and PN instruments. The two tasks are structured in the same manner, and actually share most of the code and parameters. ... For the instrument specific details, and the complete list of task parameters refer to the description of epproc and emproc . ... Exposure selection . Explicit exposure selection . ... CCD selection . ...

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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. ...

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• Automatic Detection of Linear Features in Astronomical Images
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• FTOOLS: A FITS Data Processing and Analysis Software Package

... CentralProcessor 0.11 documentation . ... Only continuum source-finding is done at this point - spectral-line source-finding will be added in the future. The source-finding applies a spatially-varying signal-to-noise threshold, and fits 2D Gaussians to detected islands to create a component catalogue. At this point, only a limited set of Selavy?s possible parameters are made available through these scripts. ... nsubx ( Selavy Basics ) . ... User Parameters - Mosaicking Continuum images . ...

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• User Parameters - Data Location & Beam Selection CentralProcessor 0.11
• User Parameters - Pipeline & job control CentralProcessor 0.11 documentation
• User Parameters - Preparation of the Science field data CentralProcessor 0.11

... The analysis of NICMOS polarization images is aimed at determining the Stokes' Parameters, and from those the polarization angle and degree for each pixel. NICMOS Camera 1 and Camera 2 each contain three polarizers, whose principal axes of transmission are separated by 120 degrees. ... The images in the three filters need to be compared, in order to produce the Stokes' parameters. ... The Stokes parameters can then be combined to yield the polarized intensity, I p: . ...

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• STSDAS release notes
• HDF-S Flanking Fields Data Reduction / Technical Issues
• Obsolescent Acquisition Parameters

... Публикации и издания Публикации профессорско-преподавательского состава СГАУ Издания проф. Сосниной Т.Н. Biosphere: Analysis of Value Parameters . ... Besides, the ways of saving the use value and value properties of biosphere are analyzed. The expediency of transformation of two-criterion theory of value into the three- criterion theory of the balance of value, where the ecologic component performs the function of the key criterion has been founded. ... BIOSPHERE USE VALUE OF THE PRODUCT: MAIN . ...

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... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/tsyba.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/perepelkin.pdf

Next: Algorithm Up: Description of program searchdup Previous: Program parameters . Program is started by the command searchdup with no parameters. The graphic user interface appears, with all parameters to their default value. After parameter entry, the button START starts data processing. ... It is possible to stop the program clicking button BREAK! ... It is then possible to change some parameters, or to exit the program, by clicking on the EXIT button. ... 2000-06-30 ...

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• Determination of the Detector Parameters
• Program parameters
• mod_session_crypto - Apache HTTP Server

Next: CCD Reductions Up: Analysis of Results Previous: Statistical Tests . ... Multivariate statistical methods can be applied in such a situation to give an objective description of the data. ... Grosb?l, P. : 1979, Image Processing in Astronomy , Eds. G. Sedmark, M. Capaccioli, R.J. Allen, Osservatorio Astronomico di Trieste, p. 371. ... Martin, R., Lutz,R.K. : 1979, Image Processing in Astronomy , Eds. G. Sedmark, M. Capaccioli, R.J. Allen, Osservatorio Astronomico di Trieste, p. 211. ...

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• The Fitting Process.
• HyperLeda: example of online pipeline processing
• Back-Illumination Paper-Optimize

... overview of pyQC . ... output used by . ... All pyQC scripts and modules share a similar structure. Python offers to group functions, classes, etc. into modules which can be imported by different scripts. ... In order to avoid confusion if names are used by different (especially external) modules, the QC scripts use the 'from' statement only for pyQC modules, i.e.: . ... For other modules, the simple 'import' statement is used: . ... Python modules are also used for keeping script configuration. ...

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• AB structure
• Association Blocks
• Quality Control and Data Processing: Home page

Next: DETAILED LIST OF ROSAT Up: PROS USERS GUIDE Previous: List of Related Documents . This section lists all PROS tasks (some of which are not described in this guide) and some useful IRAF tasks which are included. ... converts FITS to images and/or tables . ... delete a list of images . ... convert an Einstein FITS file into an IRAF/PROS QPOE file . ... convert a list of IRAF/PROS IMAGE files into RDF compatible format . ... convert a list of IRAF/PROS QPOE files into RDF compatible format . ...

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• The AstroStat Slog parameter estimation
• Model Spectra for Spectral-Fitting Program
• Topics in AstroStatistics

... 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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• Other parameters of the evolutionary scenario
• The Effect of Relativistic Wind on Accretion Flow Parameters
• Initial Distributions of Binary Parameters

... The procedure of radiometer signal integration can be considered as a sort of reducing dimension of the initial sampling space, where the samples are the result of analog-to-digital conversion. ... The probability distribution of the signal and spikes is completely known. ... The quality of the considered algorithm could be also illustrated by Figure 2 . ... One could see the considered adaptive algorithm is preferable even by low degree of compression, because all spikes have been depressed. ...

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• Determination of atmospheric parameters and calculation of chemical composition
• проект SCORPIO-2: parameters
• Access via e-mail

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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asncombine -- Process and combine images in one or two NICMOS associations asncombine association . ... set to yes to include error planes in co-added images error. background . ... This is useful to use different background subtractions for different images. fheader . set to yes in order to multiply the background by the value of keyword "factor" in the image header. ... Set to yes to use quadrants statistics save in the image header from previous runs of asncombine. regquad1 . ...

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• MAKEFLAT (Sep99) --- nictools --- MAKEFLAT (Sep99)
• ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)

Description and Technical Details . In 1980s two medium-size horizontal solar telescopes 50/35000 cm with large spectrographs Czerny-Turner made by Carl Zeiss Jena were installed in the Ond?ejov observatory. The Czerny-Turner-spectrographs in the Ond?ejov observatory called HSFA1 and HSFA2 according to the German name Horizontal-Sonnen-Forschungs-Anlage ("horizontal device for solar research") have been explored for more than two decades. ... Diffraction grating - Richardson, Spectra-Physics . ...

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• Data bases of Natural Satellites. Documentation. Structure

... 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: CLIProcessor Class Reference
• Stellarium: SphericalRegion::DrawParams Struct Reference
• Stellarium: StelObjectModule Class Reference

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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• Some Useful Routines for On-Line Data Analysis
• WAPP File Format Page
• WAPP Signal Processing Page

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• C.J. Butler, Research Astronomer
• Formatting
• Homepage of "Jorick Vink"

There are some variables which are set internally by the shell and which are available to the user: Name Description . ... 0 the name of the command currently being executed. $# the number of positional arguments given to this invocation of the shell. $? the exit status of the last command executed is given as a decimal string. ... For example '1 2' 3 becomes "1 2 3" . is identical to the arguments received by the shell, the resulting list of words completely match what was given to the shell. ...

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• Index: C
• Running processes in the foreground
• Killing processes

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

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