XMM-Newton Science Analysis System . ... This task constructs the PPS product, grism spectra, extracted from an Optical Monitor image obtained with one of the OM grism-filters. The image is previously undistorted by omgprep and rotated in order to align the spectra with the image columns. ... The output file contains tables with background subtracted spectrum rates & corresponding errors, background rates & error, spectrum flux & error. ... XMM-Newton SOC/SSC -- 2007-11-15 ...

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• Analysis options

... The Digitized Sky Survey is now available on CD-ROMs and will be on the ST ScI archive. ... ST ScI has digitized Schmidt plates of the entire Sky. ... The software then accesses the data, decompresses the scans and returns the data in a form of a photographic intensity as a function of x and y plate pixel coordinates. ... accesses the Digitized Sky Survey (DSS) CD ROMs and decompressed the data returning a photographic intensity as a function of x and y pixel coordinates. ...

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• An Infrared Camera Reduction/Analysis Package
• ADASS 2002 Conference Proceedings
• A Computer-Based Technique for Automatic Description and Classification of

... Calibrated STIS data have been processed through the STScI calstis pipeline. The pipeline unpacks the databits from individual exposures, combines them into files containing raw, uncalibrated data, and performs image and spectroscopic reduction on the data to produce output files which can be used directly for scientific analysis (see Chapter 21 for a more detailed description of the STIS pipeline). ... The nature of the individual files in your dataset, i.e., what data is stored in what file. ...

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• Installing Compiled Executables for use with the IDL Runtime GPI Data Pipeline
• Description of the Reconstruction Methods
• GPI Data Formats GPI Data Pipeline 1.0 documentation

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

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• delaysolver CentralProcessor 0.11 documentation
• Basic Structure
• ccontsubtract CentralProcessor 0.11 documentation

... A Hidden object is used for passing name/value pairs when a form submits. ... JavaScript 1.0 . JavaScript 1.1: added type property The HTML INPUT tag, with "hidden" as the value of the TYPE attribute. ... Property . ... The form contains a "Display hidden value" button that the user can click to display the value of the Hidden object in an Alert dialog box. ... P><INPUT TYPE="button" VALUE="Display hidden value" NAME="button2" . ... Form name:<INPUT TYPE="hidden" NAME="h1" VALUE="Beluga"> . ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/anchor.htm
• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/plugin.htm

Next: Order Definition Up: Echelle Reduction Method Previous: Retrieving demonstration and . ... That is the mapping between the space wavelength, spectral order and the space sample x , line y in the raw image. ... Sections and describe the solution of this mapping. The second step in the reduction, described in Section , is to estimate the image background. ... In the rest of this Section the algorithms used in each step of the reduction are described. ...

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• Echelle Spectra
• Wavelength calibration
• TRANSF/WAVE

... Bojan Nikolic web pages (r. 329) . Understanding Infrared emission from galaxies . This page contains a description and links for download of software that may be used for modelling various aspect of absorption and emission of radiation by interstellar dust. ... Also, some basic modelling of radiation fields and similar supporting code . ... dust-1.0.1 . ... Modelling absorption and emission of radiation by interstellar dust . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Description of the OOF software architecture Bojan Nikolic web pages (r. 329)
• How to create a new tool in CASA Bojan Nikolic web pages (r. 329)
• Accessing measurement set data Bojan Nikolic web pages (r. 329)

Next: Photometry Up: Regions and Source Parameters Previous: *imcnts* - Find counts . This task (developed for use with optical images, but also useful with x-ray data) will quickly compute location, size, ellipticity, and position angle of sources. ... User can generate contour plots of any portion of the image and count rates in slices through the image. The program is advertised as ``quick [optical] photometry''. input file: rp110590_im1.imh . output file: logfile . ... Photometry . ...

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• *imcalc* - Obtain a background subtracted image for ROSAT PSPC Data
• Background Corrections
• Additional Tools

... 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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• Principles of organization
• Format of data description
• Access via e-mail

Next: NICMOS Science Up: NICMOS Data Calibration and Previous: NICMOS Software at the . ... Reference File Tools . Image Analysis and Reduction . ... These include the tasks used in the STScI pipeline, tools to generate the reference files used by the calibration pipeline tasks, and general image analysis, manipulation, and arithmetic tasks. ... Calnica is used to apply instrumental calibrations to individual datasets, while calnicb is used to process associated sets of NICMOS images. ...

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• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
• NICMOS Data Calibration and Analysis

This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...

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• Lunar Orbiter 1
• Lunar Orbiter 4
• Lunar Orbiter 5

Next: Observing the Old-Fashioned Way (Gui-Free Observations) Up: Spectral Line Appendices Previous: OLD Basic Analyz Routines For use with data taken BEFORE March 6, 2000 . This appendix contains example analyz sequences used to look at HI spectra. ... Additionally, if you have not run analyz before, instruction (2) should read: If you have not, instruction (3) should read: . ... 7) redln < rec < n : This first stores the individual ON/OFF - 1 data dumps into registers 100 - 100+ - 1. ...

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• Some Useful Routines for On-Line Data Analysis
• DATA ANALYSIS
• satellite prediction routines

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

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... For completeness' sake, we include here a description of the raw data averaging software, called CONSTRICTOR, which produces the input files for . ... CONSTRICTOR reads NPOI raw data files and observation logs, and decodes and integrates data such as visibilities, delays, photon rates, etc. ... Packet directories for the individual raw files are stored on disk (working directory), and can be read later for a faster restart on CONSTRICTOR should that become necessary. ...

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• Average
• API Help
• ESO - Phase 3 Release Validator

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

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• Amorphous magnesium silicate
• Silicate minerals
• Examples of data contained in the JPDOC

... Class Index . ... StelRendererStatistics Class Reference . Stores and provides access to statistics about a StelRenderer backend. ... getNext (const char *&name, double &value) . Get next statistic name and value. ... Access statistic with specified index to modify it. ... while (statistics.getNext(name, value)) . ... Name of the statistic will be stored here (only a pointer to it). value . ... A clean way to do this is to use an enum with name corresponding to the name of the statistic. ...

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• Stellarium: SphericalRegion::DrawParams Struct Reference
• Stellarium: TuiNode Class Reference

... On-line Data . ... The program enables to find out the exact present Earth coordinates of the international space station and "Shuttle". ... J-Track - this program is similar to the previous one, however it knows how to display images and orbits of space vehicles. ... NASA SkyWatch - a program for those, who are fond of watching artificial space objects through the telescope, field - glass or with the unaided eye. ... Info: Industry news On-line Data Company ATLAS news Events We in press Contact . ...

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... Early on, our interest in chirping analysis functions was motivated by a different kind of chirping phenomenon: chirping due to perspective. ... Our interest in radar, however, drew us toward processes that are more accurately analyzed by linear-FM chirplets. ... We have also constructed other chirplet transforms, such as a three-parameter Doppler chirplet representation that models a source producing a sinusoidal wave, while moving along a straight line (e.g. a train whistle). ...

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• Appendix B: Changes from CSS1
• Warbling Chirplet: Analysis of Signals of Oscillating Frequency
• Index of the HTML 4.0 Elements

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

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• Description of database

Next: The root filesystem Up: Overview of the Directory Previous: Overview of the Directory . This chapter is loosely based on the Linux filesystem standard, FSSTND, version 1.2 (see the bibliography, [ Qui95 ]), which attempts to set a standard for how the directory tree in a Linux system is organized. ... This chapter does not explain all files in detail. ... The major parts are the root, /usr   , /var   , and /home   filesystems (see figure 2.1 ). ... Figure 2.1: Parts of a Unix directory tree. ...

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• M.D. Smith, Research Astronomer
• The root filesystem
• The /etc directory