... In more detail, the task requires as main input a table in a data set which contains a column with times in XMM MET (Mission Elapsed Time) frame[1]. ... Parameter Mand Type Default Constraints withtable yes boolean true Whether to convert ta- ble in a dataset should be set to true if a table containing events to correct has been speci ed and to false otherwise. table yes string name of existing table a speci er which must point to a table in a data set. ...

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• http://xmm.vilspa.esa.es/sas/7.0.0/doc/earthbarycen.ps.gz
• Initialisation

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• The LWS Interactive Analysis (LIA) Package
• ADASS 2003 Conference Proceedings
• Data Analysis and Processing Techniques

The FITS archive & data processing pipelines . ... The archived data are broad band images (BBI) and long-slit spectra (LSS) plus their associated template and calibration files. The data in HFA can enter into the HyperLeda processing pipeline and the results can be freely downloaded. ... Definition of the file system (structure of the archive) . ... The coordinate systems must be updated when the data (pixel data, other keywords, related tables) are altered (eg. rebinning of the image). ...

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• Comparison of two stochastic processes
• HyperLeda: example of online pipeline processing
• HyperLEDA documentation: FITS archive

... System for maintaining reference files and tables used to calibrate HST observational datasets. ... COSTAR: Corrective Optics Space Telescope Axial Replacement. ... Used for archiving HST data. ... Basic tool used to retrieve files from a remote system. Ask your system manager for information about using FTP. ... STARCAT: System used for retrieving archived HST data. ... STEIS: Space Telescope Electronic Information System. ... STSDAS: Space Telescope Science Data Analysis System. ...

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• http://www.stsci.edu/~mperrin/software/gpidata/_sources/usage/overview.txt
• http://www.stsci.edu/documents/dhb/web/c26_stisdataanal.fm4.html
• Pipeline Conceptual Overview GPI Data Pipeline 1.0 documentation

... Astronomers have developed their ways of processing signals almost independent to but sometimes collaboratively with engineers, although the fundamental of signal processing is same: extracting information. ... 2007 Vol 24 Issue 4: Bootstrap methods in signal processing . ... Bootstrap for Empirical Multifractal Analysis (H. Wendt, P. Abry & S. Jaffard) explains block bootstrap methods for dependent data, bootstrap confidence limits, bootstrap hypothesis testing in addition to multifractal analysis....

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• The AstroStat Slog image processing
• The AstroStat Slog signal processing
• The AstroStat Slog bootstrap

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Introduction
• Solar System Data Archive Home Page
• (EHIPS) Content

Next: Interpolation/Extrapolation Tolerance Up: Calibration Strategies Previous: Information on planets . You should now have a program source dataset containing the appropriate calibration solutions. The antenna gain solutions have been derived from observations of a phase calibrator, near the program source, taken typically for 2 minutes every fifteen minutes or so. The program source antenna gains are derived by interpolating and extrapolating these gain solutions. ...

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• Pulsar Group Processing/Ut 1
• uvdump
• Package: panel

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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• East Siberian Center for the Earth's Ionosphere Research. Databases.

... PUL VLBI Analysis Center . ... Pulkovo EOP and Reference Systems Analysis Center (PERSAC) is located at the Pulkovo Observatory . ... Processing of VLBI , GPS, and optical observations aimed at analysis of the Earth rotation, station displacement, and celestial reference system. ... Celestial Pole Offset (CPO) and Free Core Nutation (FCN) . Four daily updated CPO and FCN series (models) are provided. ... File fcn1.dat contains the ZM1 FCN model with variable amplitude and phase. ...

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• The Canadian S2 Correlator - Principles of Radio Interferometry

... The association log contains a list of calibration products used to process a raw file (or a set of raw files). ... The header of the association log contains the name of the association block , a data type tag, a setup tag, and the flag COMPLETE or INCOMPLETE (in case of missing calibrations). ... FLAG: not relevant here (always REAL) . ... OK MCALIB REAL GI_PFEE_071012A_Medusa1_L543.1nm_o3.fits FF_EXTERRORS 0.458 OK MCALIB REAL GI_PDIS_071012A_Medusa1_L543.1nm_o3.fits DISPERSION_SOLUTION 0.462 . ...

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• ESO - HARPS Pipeline Processed Data Available through Phase 3
• ESO - Phase 2 Submission
• ESO - My OFFSET data are not processed.

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . IPAC exists to carry out large, data-intensive processing tasks of critical importance to NASA's infrared astronomy program, and to provide scientific expertise on those projects to the astronomical community. ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....

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... 4.4 Imbedding HTML in a Document . In the following discussion of SPECIAL processing
, I will assume that rtftohtml has not been customized. If it has, the text styles used to create special effects may be different. ... Normally, if your RTF document contained the text "<cite>hello</cite>", the translator would output this as: "&lt;cite&gt;hello&lt;/cite&gt;". ... If, however, you want the <cite></cite> to be interpreted as HTML markup, you must format the tags using Hidden and Shadow. ...

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• The IMG (Image) Element
• Processes
• Managing jobs and processes

... Class . ... SUMMARY: NESTED | FIELD | ... METHOD . DETAIL: FIELD | ... java.lang.Object ij.process.FloatPolygon . public class FloatPolygon . ... Used by the Roi classes to return float coordinate arrays and to determine if a point is inside or outside of spline fitted selections. ... float[] . ... Field Detail public int npoints . ... Constructor Detail public FloatPolygon (float[] xpoints, float[] ypoints, int npoints) . ... Method Detail public boolean contains (float x, float y) . ...

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• ij.process (ImageJ API)
• Uses of Package ij.process (ImageJ API)
• Alsvid - Python Programs for Processing FITS Astronomical Image Data

Russian Version [ MS-Win ] . ... Satellite data ] . ... The program is a powerful tool for multi-purpose image analysis and processing. It operates on files in main standard image storage formats: TIFF, BMP, GIF, PDF. The program contains a rich collection of operations for visual image quality improvement: linear and logarithmic normalization, equalization, brightness transformation by arbitrary look-up table, etc. ... ALMAZ-1 satellite data processing . NOAA satellites data processing . ...

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... Hook, R. N. Walsh, J. Pirzkal, N. Freudling, W. IRAF, polarimetry, image: analysis, image: restoration, spectroscopy, GRISM data analysis . We have collected together many of the astronomical applications developed as IRAF tasks at the Space Telescope European Coordinating Facility (ST-ECF) into a new IRAF layered package called ``stecf". ... stecf.nictools - NICMOS GRISM Tools . ... stecf.impol - an IRAF Imaging Polarimetry Reduction Package . ... stecf.impol - Package Tasks . ...

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• NICMOS Data Calibration and Analysis
• STScI NICMOS Software

... 1.7 GSC 084 Pulkovo Obs., 0.33 15 x 15' 1.0" 7 34 0.179 0.307 Normal Asgr. 3.0 UCAC 118 Slovakia, 0.57 14 x 10' 1.7" 3 12 0.090 0.145 Modra 3.3 USNO 127 Germany, 0.19 30 x 20' 2.4" 3 15 0.151 0.087 Bornheim 0.8 GSC 168 34 200 0.282 0.315 291 USA,Kitt Peak, 1.8 390 x 30' 1.0" 1 5 0.143 0.144 Spacewatch II 4.7 USNO 300 Japan, 0.5 78 x 78' 2.3" 7 36 0.420 0.447 Bisei Center 1.3 ACT 461 Hungary, JATE 0.60 28 x 19' 1.1" 6 22 0.124 0.153 Asteroid Surv. ... Polynesia 1.0 UCAC F85 Tiki Obs., ...

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Ultraviolet data (DUV) . ... The section "Original data" contains original information in analogue-digital and digital- analogue codes. The section "Data for analysis" contains pre-processed data for further analysis. Tatiana" program can be used for graph presentation of the experimental data, and "Orbitron" program - for geographical control of the data. Manual on how to use the programs and the data is in the HELP-file. ... Original data . Data for analysis . Tatiana program . ...

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... Display (spectra, total power). ... Using the data archive. ... entering cmds, editing cmd lines, input from files, batch, run. constants, variables,arrays, structures, operators, procedures, functions. programming in idl . ... A user would call arch_gettbl() to input the table (or a subset of it). corfindpat() can create subsets of the table. arch_getdata() or arch_getonoff() can be used to read in the spectra. ... input the data (spectra) for a subset of the archive table: arch_getdata () . ...

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• http://www.naic.edu/~phil/usrproj/a1552/a1552.html
• http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/lcu/pcr/c600/source/STARTUP/MSDOS.INC
• http://www.naic.edu/alfa/galfa/docs/gsrinit_whitebelt.ps.gz