... Meta Index / Home Page / Description / Exposure selection . You can select the exposures to process explicitly via the parameters withinstexpid and instexpids . ... epicproc -withinstexpids=yes -instexpids="IIFnnn ..." . ... Note that the IIFnnn matches the analogous string found in the ODF file names. You may also want to look at the contents of the ODF with the odfbrowser , from which individual exposures can be selected, and the epicproc tasks can be configured and launched. ...

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• Detailed Description

... 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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• The Schedule File
• Parameters Specific to the VLA
• Central Processor Manager CentralProcessor 0.11 documentation

Next: Simulated Results with Up: Assessment of Methods Used Previous: Introduction . ... Then one has to use regularized inversion methods in order to obtain approximate and sensible solutions. ... All these methods contain a free parameter which is the so-called regularization parameter; in the case of method ( ) this is a smoothing of the higher spatial frequencies; for the methods ( ) - ( ), it is the number of iterations. ... In the case of method ( ) the iteration scheme is given by . ...

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• STSDAS release notes
• Obsolescent Acquisition Parameters
• UDF/ACS Parameters: . Pointing, Filters, Depth, and Status

This session will provide a forum for a discussion of variety of topics in Astrostatistics following the Special Session "Lectures on Astrostatistics" held on Wednesday morning. It will also anticipate the "Time-Domain and Applicable Methodologies" session scheduled for Thursday morning. ... 111.02 - Andreas Hans Wilhelm Kupper -- Exploding Satellites - The Tidal Debris of the Ultra-Faint Dwarf Galaxy Hercules . ... Moderators: Aneta Siemiginowska (CfA) and Vinay Kashyap (CfA) . ...

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• Parameters
• Using the PROS software
• Model Spectra for Spectral-Fitting Program

The numerical code for the revised (de Vaucouleurs) morphological type is defined in RC2. The correspondance with the Hubble type is: . The morphological type is also coded as the Hubble type: type , and other information about the morphology are contained in the bar and ring parameters and to some extend in the compactness and multiple parameters. This parameter is derived from the compilation of morphological description . ... HyperLeda . ...

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• Session parameters
• Mean astrophysical parameters from LEDA
• Parameters

gmtset - To change individual GMT default parameters gmtset PARAMETER1 value1 PARAMETER2 value2 PARAMETER3 value3 ... gmtset will adjust individual GMT defaults settings in the current directory's .gmtdefaults file. If no such file exists one will be created. ... To change the dpi to 600, set anotation font to Helvetica, and select grid-crosses of size 0.1 inch, try gmtset DOTS_PR_INCH 600 ANOT_FONT Helvetica GRID_CROSS_SIZE 0.1i gmt , gmtdefaults . ...

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• Parameters of binary compact star evolution

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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• Program parameters
• mod_session_crypto - Apache HTTP Server

Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• Magnetic mapping file description
• IKI SSC INTMINS APRIL98
• ASCII files description

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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• fitsreport
• pyQC: script structure
• VLTI Calibrator Selection Help Page

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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• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• WCS2DR (V1.0) --- Jan00 --- WCS2DR (V1.0)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

... comedi_dio_config -- change input/output properties of channel . ... int comedi_dio_config (comedi_t * device, unsigned int subdevice, unsigned int channel, unsigned int direction); . The function comedi_dio_config() configures individual channels in a digital I/O subdevice to be either input or output, depending on the value of parameter direction. ... Depending on the capabilities of the hardware device, multiple channels may be grouped together to determine direction. ...

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• проект SCORPIO-2: parameters
• comedi_get_cmd_generic_timed
• SCORPIO-2 project: description

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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• Brief description of GRS
• INTERBALL-TAIL KP
• INTERBALL-TAIL KP list

... 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/M3000

... 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: StelGeometryBuilder Class Reference
• Stellarium: TextParams Struct Reference
• Stellarium: RingParams Struct Reference

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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• A Computer-Based Technique for Automatic Description and Classification of
• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• A Spectroscopy Exposure Time Calculator for IRAF

. 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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• WAPP File Format Page
• ALFA Performance
• Untitled Document

... CREATE FULLTEXT CONFIGURATION -- create full-text configuration . CREATE FULLTEXT CONFIGURATION cfgname PARSER prsname [ LOCALE localename ] [ AS DEFAULT ]; CREATE FULLTEXT CONFIGURATION cfgname [ { PARSER prsname | ... PARSER . ... LOCALE . ... Create new configuration test with default parser and ru_RU.UTF-8 locale. CREATE FULLTEXT CONFIGURATION test PARSER default LOCALE 'ru_RU.UTF-8'; =# \dF+ test Configuration "public.test" Parser name: "pg_catalog.default" Locale: 'ru_RU.UTF-8' Token | ...

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• ALTER FULLTEXT CONFIGURATION
• CREATE FULLTEXT DICTIONARY
• CREATE FULLTEXT PARSER

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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• DUST: dustiface.h File Reference
• DUST: dust_silsdpars Struct Reference
• DUST: dust_sdpars Struct Reference

... 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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• lte-codes: sterne model atmospheres
• Homepage of "Jorick Vink"
• SCL Sfit Genetic Commands

... Space flight . ... Zero Gravity . ... Characteristics of a Complex Flight: . ... Characteristics of the Reduced Gravity (Lunar Gravitation): . ... Characteristics of the Reduced Gravity (Martian Gravitation): . ... Services / Zero Gravity: General description Technical description Flight parameters Photo gallery Price . ...

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• Baikonur cosmodrome. Space vehicle launch schedule
• Photo gallery: pictures of cosmonauts and participants in zero gravity flights.