... The use of the parameters for the source and background extraction areas requires some care. ... In order to avoid these variations and to obtain a uniform combined light curve, it is better to use a fixed radius for the source extraction area for all the exposures in the ODF. ... Changing srcradius parameter one should also properly esablish the background extraction area setting bkginner and bkgouter parameters (see description of the parameters). ...

Еще в разделе: (Показать все результаты (>32712) - xmm.vilspa.esa.es/ )

• Parameters

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 (>2873) - www.sai.msu.su/ )

• Zen: sncat design
• CREATE FULLTEXT CONFIGURATION

Table 5.1: Special External Target Names . ... The Visit and Exposure Specifications are used to define the proposed exposures for all the Scientific Instruments. ... The rest of the exposure keywords are used to define parameters that usually change from one exposure to the next, such as filters, exposure times, and special scheduling requirements. ... An exposure consists of the events and data corresponding to a unique Exposure_Number within a given visit. ... Science exposure(s) . ...

Еще в разделе: (Показать все результаты (>22052) - www.stsci.edu/ )

• Index
• STSDAS release notes
• Solar System Targets

... 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 (>740) - xray.sai.msu.ru/ )

• Initial Distributions of Binary Parameters
• The Effect of Relativistic Wind on Accretion Flow Parameters

... Apache HTTP Server Version 2.4 . ... macro_module . ... These macros have parameters. ... macro definition within a <Macro> section, following the apache style. user defined names for the macro and its parameters. macro names are case-insensitive, like apache directives. macro parameter names are case sensitive. macro parameters must have distinct names. error on empty parameter names. redefining a macro generates a warning. macro definitions can be nested... (but what for?) . ... Use of a macro: . ...

Еще в разделе: (Показать все результаты (>9863) - www.arcetri.astro.it/ )

• Program parameters
• Determination of the Detector Parameters
• mod_session_crypto - Apache HTTP Server

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 Computer-Based Technique for Automatic Description and Classification of
• A Spectroscopy Exposure Time Calculator for IRAF
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared

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 (>3838) - www.mrao.cam.ac.uk/ )

• PPEUC Programme - Cosmic Microwave Background Workshop
• Astrophysics Group VSA
• Astrophysics Group MADCOW

... Archives . ... P Values: What They Are and How to Use Them . ... That is, if we derive a posterior probability distribution function for a parameter using one dataset, we can apply that as the prior when a new dataset comes along, and thereby improve our estimates of the parameter and shrink the error bars. ... Suppose you have two data sets, D1 and D2, hypotheses H, and background info (model, etc.) ... Comment ( RSS ) | ... Entries RSS . ... Chandra Blog . ... Entries (RSS) and Comments (RSS) . ...

Еще в разделе: (Показать все результаты (>4730) - hea-www.harvard.edu/ )

• The AstroStat Slog BEHR
• The AstroStat Slog prior propagation
• The AstroStat Slog Tom Loredo

... 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 (>1066) - astro.uni-altai.ru/ )

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

... IFP#1-LO 6300 - 6316 MHz USB LCP . ... IFP#2-LO 6642 - 6658 MHz USB LCP . ... IFP#2-HI 6658 - 6674 MHz USB LCP . ... Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v255/v255e . ... The 4 x 16 MHz bandpass setup will require feeding two separate LOs into IFP#1 and #2 on the DAS/frequency translator and splitting the LCP signal so that is feed into both sides. For Hobart the LOs should be set to 468 MHz (IFP#1) and 810 MHz (IFP#2) for the 4 x 16 MHz setup and 810 MHz for the 2 x 16 MHz setup. ...

Еще в разделе: (Показать все результаты (>19256) - www.atnf.csiro.au/ )

• VLBI Wiki | LBAMar2008 / V255A
• VLBI Wiki | LBAFeb2009 / V255D
• uvplanet

... 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 (>1547) - www.cosmos.ru/ )

• IKI SSC, INTMINS APRIL99
• IKI SSC INTMIN