... Parameter Mand Type Default Constraints mandatoryparam yes type default value constraints description for mandatory parameter optionalparam no type default value constraints description for optional parameter xmmsas 20080701 1801-8.0.0 XMM-Newton Science Analysis System Page: 2 5 Errors This section documents warnings and errors generated by this task (if any). ... 8 Algorithm 9 Comments  References xmmsas 20080701 1801-8.0.0 ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/rudi5mosaic.ps.gz
• http://xmm.vilspa.esa.es/sas/7.0.0/doc/htrframes.ps.gz
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/rudi5mosaic.ps.gz

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 Graphical User Interface for a Development Environment (GUIDE)
• Using XML and Java for Astronomical Instrument Control
• A Computer-Based Technique for Automatic Description and Classification of

Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

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• Session Parameters
• Echelle Spectra
• Session parameters

... 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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• WFPC2 TIR Abstract
• COS Instrument Handbook
• STSDAS release notes

... The Miriad task uvgen can be used to simulate a variety of observing modes. ... Simulating a telescope approximately, let alone in some detail, requires a good many parameters. uvgen takes an appreciable number of parameters and input files to describe the telescope, correlator and source. Fortunately keyword and set-up files for some common situations exist ( e.g. simulating the ATCA and VLA). ... For example, to load typical parameters for the ATCA, use miriad% source $MIRCAT/uvgen.def.atca . ...

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• Central Processor Manager CentralProcessor 0.11 documentation
• ccontsubtract CentralProcessor 0.11 documentation
• User Parameters - Data Location & Beam Selection CentralProcessor 0.11

. The description of the instrument is divided into the following sections: . Optical Design . Cryogenics and Mechanics . Electronics and Software . Determination of Detector parameters . Some photos of the instrument . Other high resolution images .

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• Program parameters
• Determination of the Detector Parameters
• Program use

The VLTI Calibrator Selector Tool is a tool intended to assist in the selection of suitable interferometric calibrators for VLTI observations with MIDI and AMBER. It uses a model of the VLTI and its instruments to assess the fringe visibility, given the observed bandpass, the geometry, spectrum, and coordinates of the target and the time at which the observations are to be made. ... The tool offers an HTML/Java based interface and consists of two pages. ... The quality flag depends on LDD_chi2. ...

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• ESO - Release Description
• pyQC: script structure
• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)

... 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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• Sfit Control Language: Classified Listing
• SCL Sfit Genetic Commands
• FFIT - Command Syntax

... 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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• Topics in AstroStatistics
• Model Spectra for Spectral-Fitting Program
• IRAF/PROS

... Next . comedi_get_cmd_generic_timed -- streaming input/output capabilities . ... int comedi_get_cmd_generic_timed (comedi_t * device, unsigned int subdevice, comedi_cmd * command, unsigned int period_ns); . The command capabilities of the subdevice indicated by the parameters device and subdevice are probed, and the results placed in the command structure pointed to by the parameter command. ... The command measures samples at a rate that corresponds to the period period_ns. ...

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• Parameters of the 41 Dra system components
• comedi_get_cmd_src_mask
• проект SCORPIO-2: parameters

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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• Abstract
• Paper I: Method Bojan Nikolic web pages (r. 329)
• OptInt PmWiki : MROIDelayLineSW / Baseline Solution Software

... 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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• Parameters of the starburst
• The Model
• The Effect of Relativistic Wind on Accretion Flow Parameters

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

The MOD and IOPT parameters value depend of the external magnetic field model (MOD), used during magnetic mapping and IOPT version (IOPT = Kp + 1), see the table: . MOD . External model . IOPT range . ... N.A.Tsyganenko, Planet. Space Sci., ... N.A. Tsyganenko, A magnetospheric magnetic fields model with a warped Tail current sheet: Planet. Space SCI., ...

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• BOKZ Star Trackers
• PhSRM
• ASCII files description

... 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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hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

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

Rotang can either be run from the command line as described here or through the alfa_ang GUI . ... To run rotang at Arecibo: . Start IDL . ... rotang, Date , RA , Dec , Time , /choice . Here Date takes the format YYMMDD (e.g. 041128 for the 28 th of November, 2004). ... Rotang also calculates the Azimuth and Zenith Angle fir every source. If the Zenith Angle is greater than 20 degrees, then the program will return that the source is down and will not calculate an optimum ALFA angle. ...

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• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/parameter
• WAPP File Format Page
• GALFA System Description

... 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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• COMMENT ON FULLTEXT
• ALTER FULLTEXT CONFIGURATION
• CREATE FULLTEXT DICTIONARY

... 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/fb Es
• 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

Stellarium 0.12.3 . ... Classes . ... ClassљList . ClassљIndex . ... StelObjectModule Class Reference abstract . Specialization of StelModule which manages a collection of StelObject . ... virtual QList< StelObjectP >љ . searchAround (const Vec3d &v, double limitFov, const StelCore *core) const =0 . ... searchByNameI18n (const QString &nameI18n) const =0 . Find a StelObject by name. ... searchByName (const QString &name) const =0 . ... virtual QStringљ . ... const QString &љ . ...

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• Stellarium: SphereParams Struct Reference
• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: TextParams Struct Reference