XMM-Newton Science Analysis System Page: 1 epnoisemap July 2, 2008 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 (>35587) - xmm.vilspa.esa.es/ )

• http://xmm.vilspa.esa.es/sas/7.1.0/doc/epnoisemap.ps.gz
• Home Page

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 (>1995) - www.adass.org/ )

• A Graphical User Interface for a Development Environment (GUIDE)
• A Spectroscopy Exposure Time Calculator for IRAF
• ADASS 2003 Conference Proceedings

... ACQ-DIST Optional Parameter for FGS 1 , 2 . ACQTYPE Optional Parameter for STIS . Acquisition modes . ... ACCUM . ... AFTER date Special Requirement . ... BINAXIS1, BINAXIS2 Optional Parameters for STIS 1 , 2 . ... BUFFER-TIME Optional Parameter for STIS . ... CHECKBOX Optional Parameter for STIS . ... Calibration Targets . ... CR-SPLIT Optional Parameter for STIS . ... DIFFUSE-CENTER Optional Parameter for STIS . ... GAIN Optional Parameter for STIS . ... PCS MODE Fine Special Requirement . ...

Еще в разделе: (Показать все результаты (>22114) - www.stsci.edu/ )

• Chapter 5: Visits, Exposures and Exposure Groups
• GHRS Instrument Handbook
• STIS Reference Files

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 (>3465) - www.sao.ru/ )

• HyperLEDA documentation: parameter: t
• Radio data
• Echelle Spectra

Full-Text Search in PostgreSQL: A Gentle Introduction . ... COMMENT ON FULLTEXT -- define or change the comment of a full-text object . COMMENT ON FULLTEXT { CONFIGURATION | ... COMMENT ON FULLTEXT stores a comment about a full-text object (configuration, dictionary, parser). To modify a comment, issue a new COMMENT ON FULLTEXT command for the same full-text object. ... COMMENT ON FULLTEXT DICTIONARY intdict IS 'Dictionary for integers'; =# \dFd+ intdict List of fulltext dictionaries Schema | ...

Еще в разделе: (Показать все результаты (>2116) - www.sai.msu.su/ )

• Zen: sncat design
• ALTER FULLTEXT ... OWNER

... Apache HTTP Server Version 2.4 . ... Session encryption support . ... session_crypto_module . ... The session will be encrypted with the given key. Different servers can be configured to share sessions by ensuring the same encryption key is used on each server. ... The SessionCryptoPassphrase directive specifies the keys to be used to enable symmetrical encryption on the contents of the session before writing the session, or decrypting the contents of the session after reading the session. ...

Еще в разделе: (Показать все результаты (>9968) - www.arcetri.astro.it/ )

• Program parameters
• mod_authn_dbd - Apache HTTP Server
• mod_macro - Apache HTTP Server

Weaving together Astronomy+Statistics+Computer Science+Engineering+Intrumentation, far beyond the growing borders . ... Archives . ... Therefore, semiparametric is not exactly [MADS] but almost [MADS]. ... Besides, I wonder if Section 3.3, the cluster detection algorithm works similarly to a source detection algorithm in high energy astrophysics if tight photon clusters indicate sources. ... 123.1807G]: cut and enhance (CE) cluster detection method. ... Comment ( RSS ) | ... Chandra Blog . ...

Еще в разделе: (Показать все результаты (>4264) - hea-www.harvard.edu/ )

• Structure of the Spectral Package
• The AstroStat Slog Blog Archive [ArXiv] Recent bayesian studies from astro-ph
• The AstroStat Slog nuisance parameter

... Co-ordinate systems description . Directories structure . The file names' construction . The file set description . ... The orbital information for each month is presented in the separate directory. The INTERBALL orbital data are located on the STDA server, for each month in the separate subdirectory, which name consists from the year (YYYY) and month (MM) numbers. The Parent Directory of the Tail Probe orbital data is http://www.iki.rssi.ru/da/interball/tail/orbit/ . ...

Еще в разделе: (Показать все результаты (>1704) - www.cosmos.ru/ )

• STDA files
• Magnetic mapping file description
• BOKZ Star Trackers

... StelScriptMgr Class Reference . ... const QStringљ . ... Stops any running script. ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getDescription . ... If the file is not found or cannot be opened for some reason, an Empty string will be returned. const QString StelScriptMgr::getLicense . ... Get the rate at which the script is running as a multiple of the normal execution rate. void StelScriptMgr::pauseScript . ...

Еще в разделе: (Показать все результаты (>1704) - astro.uni-altai.ru/ )

• Stellarium: StelObjectModule Class Reference
• StelTexture::StelTextureParams Struct Reference
• Stellarium: TelescopeClient Class Reference

... There are compelling reasons for the pulsar community to utilise a standard data storage format. For example, standardisation of file formats significantly decreases the amount of effort required to integrate new instruments into the analysis chain. ... Accordingly, we have defined PSRFITS as a standard FITS-based format for pulsar data files. ... For example, the first line of Processing History HDU contains information about the data acquisition program and the initial structure of the file. ...

Еще в разделе: (Показать все результаты (>15912) - www.atnf.csiro.au/ )

• The Schedule File
• casacore: casa::FunctionOrder< T > Class Template Reference
• Making a Fake Observation

... Natalya V. Raguzova and Sergei B. Popov . ... We present a compilative catalogue of Be/X-ray binaries and candidates in the Galaxy and in the Large and Small Magellanic Clouds. This catalogue contains 160 sources and provides information on names and spectral types of optical components, distances, on spin characteristics of neutron stars, and on orbital and X-ray properties of binary systems. ... Be/X-Ray Binaries and candidates in the Galaxy . Galactic sources: comments to the Table 1 . ...

Еще в разделе: (Показать все результаты (>791) - xray.sai.msu.ru/ )

• Parameters of binary compact star evolution
• The Effect of Relativistic Wind on Accretion Flow Parameters
• Page contents

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 (>67142) - www.eso.org/ )

• ESO - Paranal Science Operations: End of Missions Report
• ESO - Release Description
• webCMS

From XEphem running the Soft03Cmt database of 20121002, for the date and time of the observation: RA: 08:16:04.25 Dec: 27:48:13 2012-09-30 UT 09:45 UTC Measured: RA: 08:16:04.4 Dec: 27:48:12.9 Header listing for HDU #1: SIMPLE = T / This is a FITS file BITPIX = -32 / NAXIS = 2 / NAXIS1 = 4341 / NUMBER OF ELEMENTS ALONG THIS AXIS NAXIS2 = 4355 / NUMBER OF ELEMENTS ALONG THIS AXIS EXTEND = T / This file may contain ...

Еще в разделе: (Показать все результаты (>1662) - www.astro.louisville.edu/ )

• http://www.astro.louisville.edu/shared_skies/archive/select/messier/m67/20110406/tmp/m67_4s_12800iso_1302145416.axy
• API Help (ImageJ API)
• Uses of Class ij.io.FileInfo (ImageJ API)

... This is the MS-DOS general help file. ... Type FASTHELP with no arguments to display the text in this file. ... APPEND Allows programs to open data files in specified directories as if they were in the current directory. ... COPY Copies one or more files to another location. ... FC Compares two files or sets of files, and displays the differences between them. ... PATH Displays or sets a search path for executable files. ... SYS Copies MS-DOS system files and command interpreter to a disk you...

Еще в разделе: (Показать все результаты (>5789) - www.naic.edu/ )

• Rotang - IDL procedure for calculating the optimum rotation angle for ALFA
• Index of /~phil/hardware/vertex/hagenDocmemos/klaus/ATA1A/parameter
• How to Propose

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 (>857) - www.iki.rssi.ru/ )

• INTERBALL-TAIL KP
• SPICE System Overview .
• INTERBALL-AURORAL KP plots

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

Еще в разделе: (Показать все результаты (>294) - www.stecf.org/ )

• MAKEASN (Nov98) --- nictools --- MAKEASN (Nov98)
• HSTPOLSIM (V1.00) --- April99 --- HSTPOLSIM (V1.00)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

Еще в разделе: (Показать все результаты (>4) - scan.sai.msu.ru/ )

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

Еще в разделе: (Показать все результаты (>647) - www.cplire.ru/ )

• Getting Started in Actor Prolog. Visual Expert Systems.
• SYNCHRONIZATION OF DRIVE-RESPONSE SYSTEMS ON CONDITION OF A LARGE MISMATCH OF
• Getting Started in Actor Prolog. Oil Production.

Light scattering by axisymmetric particles within a new approach to the T-matrix method The code AXISYM0.FOR realises the new approach to the solution of the light scattering problem suggested by Farafonov (Opt. ... Below them one finds also the description of the input and output parameters, and a list of some used subroutines. The comments given through the code's text allow one to follow its general structure. The file IN contains the input parameter values for a test run. ...

Еще в разделе: (Показать все результаты (>406) - www.astro.spbu.ru/ )

• Database of Optical Properties -- Level: subpage
• Database of Optical Constants -- Level: welcome
• Database of Optical Properties -- Level: subsubpage

Cambridge . ... Bojan Nikolic web pages home . ... Previous: Talk at the ALMA EU FP6 Enhancement.. I gave the following talk here at the University of Cambridge: . ... Observed broad-band radio spectra of both galactic and extra-galactic . ... parameters in these models which are only approximately a-priori . ... I will describe a computer program for straightforward Bayesian analysis . ... Please enable JavaScript to view the comments powered by Disqus. blog comments powered by Disqus . ...

Еще в разделе: (Показать все результаты (>3723) - www.mrao.cam.ac.uk/ )

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