... This task takes as input a housekeeping file from any of the instruments, and removes from it any `columns' whose data is determined to not be useful for subsequent data processing. ... The TIME column of ODF compliant house keeping files will be a string in the format yyyy-mm-ddThh:mm:ss . In order for the HK data to be in a useful format for plotting, producing GTI files, etc., hkstrip will convert the TIME column of ODF files to seconds since the XMM reference time. ...

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... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

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• STDA files

... CentralProcessor 0.11 documentation . ... The following parameters determine where the measurement sets are that hold the data to be processed. The default behaviour is to read the MS from the given Scheduling Block (SB) directory. ... Location (on galaxy) of the scheduling blocks. This is used when specifying SB numbers - the default is the standard location for BETA operation. ... These parameters determine which beams in the data to process. ... User Parameters - Pipeline & job control . ...

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• Casda Upload Utility CentralProcessor 0.11 documentation
• casacore: casa::FunctionWrapper< T > Class Template Reference
• casacore: casa::GaussianConvert Class Reference

... Data . ... WFPC2 Home . ... WFPC2 History . ... LRF Data . ... Warm Pixels . ... STEP 3: DRIZZLE SEPARATE IMAGES (driz_separat = yes ) Drizzle onto separate output images? (driz_sep_out = ) Size of separate output frame's X-axis ( pixels ) (driz_sep_out = ) Size of separate output frame's Y-axis ( pixels ) (driz_sep_ker = turbo ) Shape of kernel function (driz_sep_wt_ = exptime ) Weighting factor for input data image (driz_sep_sca = INDEF) Absolute size of output ...

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• STSDAS release notes
• HDF-S Filename Legend
• stsci_python 2.8 Release Notes

... 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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• Using the PROS software
• Model Spectra for Spectral-Fitting Program
• Possible Pitfalls

... 18-Jan-2010 17:22 . ... Apache/2.2.3 (CentOS) Server at www.wdcb.ru Port 80 ...

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• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/f min
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/fo Es
• Index of /stp/data/Images_of_f-plots/TABL/Tables of different Parameters/Type...

. Name . Last modified . Size . Description . Parent Directory . - . parameter_controllergains.ini . 14-May-2004 16:11 . 214 . parameter_encoderreferencepositions.ini . 14-May-2004 17:03 . 111 . parameter_jackpositionoffsets.ini . 14-May-2004 16:49 . 66 . Apache/2.2.3 (CentOS) Server at www.naic.edu Port 80

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• Alfacal
• WAPP File Format Page
• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/defaultminmax

The determination of the detector parameters is based on sets of images of a spatially uniform-illumination scene (flatfield frames) and without any illumination (dark frames), putting a plug in place of the filter, taken at a series of exposure times. ... We interleave before and after each exposure time in the series of flatfield frames a set of reference images at an exposure time of 1 sec to determine the possible temporal variation of the illumination level. ...

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• mod_macro - Apache HTTP Server
• mod_session_crypto - Apache HTTP Server
• mod_authz_dbd - Apache HTTP Server

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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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)

Next: Buffer Manipulation Up: Programming in C Previous: Compiler Options . Listed below are nearly all the ANSI C standard library functions. The header file where related definitions are stored are given. These may vary on some systems so check local reference manuals. ... More info can be obtained from online man calls or reference manuals. Buffer Manipulation . Character Classification and Conversion . ... File Manipulation . ... Wed Sep 14 10:06:31 BST 1994 ...

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• comedi_from_phys
• comedi_to_phys
• проект SCORPIO-2: parameters

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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• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared
• A Computer-Based Technique for Automatic Description and Classification of
• Indexing and Searching Distributed Astronomical Data Archives

Next: Running CONSTRICTOR Up: How to use CONSTRICTOR Previous: Parameters Contents . ... OutputBeam.BiasMod(07:12) = 1, 7, 10, 8, 3, 5 OutputBeam.StationID(01:04) = 1, 3, 4, 6 OutputBeam.StationID(05:08) = 1, 2, 4, 5 OutputBeam.Wavelength (01:04) = 849.4e-9, 820.9e-9, 793.9e-9, 768.3e-9 OutputBeam.Wavelength (05:08) = 744.2e-9, 722.9e-9, 701.5e-9, 683.1e-9 OutputBeam.Wavelength (09:12) = 664.6e-9, 648.9e-9, 617.7e-9, 603.5e-9 OutputBeam.Wavelength (13:16) = 590.7e-9, 577.9e-9, 566.5e-9, 556.6e-9 ...

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• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)
• fitsreport
• Preparation of parameter file

... Apache HTTP Server Version 2.2 . ... For example, the following configuration will map /cgi-bin/script.pl to /usr/local/apache2/cgi-bin/script.pl in all cases: . ... A request for http://www.example.com/directory/file.html will be satisfied by the file /usr/local/apache/vhosts/www.example.com/directory/file.html . ... A request for http://www.domain.example.com/directory/file.html will be satisfied by the file /usr/local/apache/vhosts/example.com/d/o/m/domain/directory/file.html . ...

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• Multivariate Statistical Methods
• HyperLEDA documentation: parameter: t
• Mean astrophysical parameters from LEDA

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

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• Database of Optical Constants -- Misc: n-Mie code(s)
• Database of Optical Properties -- Level: subpage

Next: The /dev directory Up: The root filesystem Previous: The root filesystem . The /etc љ directory contains a lot of files. ... See the chapter on init љ for further information. /etc/passwd љ . ... Lists the filesystems mounted automatically at startup by the mount -a command (in /etc/rc љ or equivalent startup file). ... etc/issue љ . ... See the magic љ and file љ manual pages for more information. /etc/motd љ . ... Files executed at login or startup time by the Bourne or C shells. ...

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• lte-codes: sterne model atmospheres
• sfit help file
• Index of /archives/ArmaghObservatory/Huggins-Spectrum-Analysis M41

... 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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... Home All Namespaces All Classes Functions Coding Style Scripting Plugins File Structure . ... Manage textures loading. ... createTexture (const QString &filename, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams ()) . Load an image from a file and create a new texture from it. ... createTextureThread (const QString &url, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams (), const QString &fileExtension=QString(), bool lazyLoading=true) . ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: StelScriptMgr Class Reference
• Stellarium: Landscape Class Reference

Orbital data : INTERBALL AZ GSE and GSM cartesian coordinates, GSE cartesian velocity (once per 10 minutes). ... Magnetic field data from IMAP experiment. Magnetic fileld absolute value and magnetic field index (the difference between absolute value and model value), status flag. ... Counts of H+ and O+ ions are accumulated during one spin period by detectors D6 (antisunward looking), D8 (spin plane), D10 (sunward looking) of TRICS2 subsystem (1.0-30 keV). ... TRICS1, TRICS2, TRICS3 subsystems: . ...

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• Site Navigator
• Brief description of GRS
• INTERBALL-TAIL KP DESCRIPTION

... Exploring the physics of Type Ia supernovae through spectral analysis . ... Their progenitor scenario as well as the details of the explosion mechanism remain a mystery. ... It produces a supernova spectrum for a given luminosity, photospheric velocity, time since explosion and several elemental abundances. Tweaking these parameters to produce a spectrum that fits an observed spectrum is a complex, as of yet, manual task. ... The search space is large and complex. ...

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• Index of /~bessell/FTP/Bohlin2013
• Index of /~akarakas/stellar_yields

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 ...

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• NVSS Image ftp service Documentation Help for NVSS Image ftp service
• OptInt PmWiki : PmWiki / Page Directives
• Astrophysics Group MADCOW