XMM-Newton Science Analysis System Page: 1 epnoisemap July 9, 2007 Abstract This task makes a model image of the background due to PN double events (this is greatest between 200 and 300 eV). ... 4 Parameters This section documents the parameters recognized by this task (if any). ... See the eexpchipmap task documentation for a descrip- tion of the format of this le. outputstyle no string sky sky|raw If `sky', the noise map is output in sky coordinates, to the le referred to by parameter noiseimageset. ...

Еще в разделе: (Показать все результаты (>35483) - xmm.vilspa.esa.es/ )

• http://xmm.vilspa.esa.es/sas/8.0.0/doc/epnoisemap.ps.gz
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/eregionanalyse.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/eregionanalyse.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. ...

Еще в разделе: (Показать все результаты (>1996) - www.adass.org/ )

• A Graphical User Interface for a Development Environment (GUIDE)
• A Computer-Based Technique for Automatic Description and Classification of
• A Spectroscopy Exposure Time Calculator for IRAF

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 . ...

Еще в разделе: (Показать все результаты (>2734) - www.sao.ru/ )

• Echelle Spectra
• Session Parameters
• MIDAS utilities for time series analysis

COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 8: Target Acquisitions > 8.9 Recommended Parameters for all COS TA Modes . ... Always follow the first ACQ/SEARCH with an ACQ/IMAGE , ACQ/PEAKXD+ACQ/PEAKD , or a second 2 в 2 ACQ/SEARCH which uses FLUX-WT weighting. ... Use NUM-POS=5 , STEP-SIZE=0.9 , and CENTER=FLUX-WT-FLR for most ACQ/PEAKD centerings. ... For ACQ/PEAKD , use of the special parameter CENTER=DEFAULT is recommended. ...

Еще в разделе: (Показать все результаты (>21483) - www.stsci.edu/ )

• WFPC2 TIR Abstract
• Index
• WFPC2 Drizzle Cookbooks

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. ...

Еще в разделе: (Показать все результаты (>66887) - www.eso.org/ )

• ESO - Release Description
• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)

... 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 . ...

Еще в разделе: (Показать все результаты (>15941) - www.atnf.csiro.au/ )

• casacore: casa::Projection Class Reference
• casacore: casa::GaussianConvert Class Reference
• 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 .

Еще в разделе: (Показать все результаты (>8229) - www.arcetri.astro.it/ )

• Program parameters
• Determination of the Detector Parameters
• Description of program searchdup

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: . ...

Еще в разделе: (Показать все результаты (>861) - www.iki.rssi.ru/ )

• INTERBALL-TAIL KP list
• Brief description of GRS

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 ...

Еще в разделе: (Показать все результаты (>3504) - www.mrao.cam.ac.uk/ )

• Abstract
• Paper I: Method Bojan Nikolic web pages (r. 329)
• DUST: dustiface.h File Reference

... 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. ...

Еще в разделе: (Показать все результаты (>711) - xray.sai.msu.ru/ )

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

Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...

Еще в разделе: (Показать все результаты (>1518) - astro.uni-altai.ru/ )

• Stellarium: SphereParams Struct Reference
• Stellarium: TextParams Struct Reference