. XMM-Newton Science Analysis System . hkgtigen (hkgtigen-1.14.2) [xmmsas_20050815_1803-6.5.0] . Meta Index . HouseKeeping parameter driven Good-Time-Interval data set GENeration . Instruments/Modes . Use . Description . Motivation . Detailed Description . Examples . Long and short HK parameter names . Diagnostic mode . Comments . Parameters . Errors . Input Files . Output Files . Algorithm . Future developments . Bibliography . Index . XMM-Newton SOC/SSC -- 2005-08-16

Еще в разделе: (Показать все результаты (>35613) - xmm.vilspa.esa.es/ )

... Instruments . ... Exposure_Number: 1 Target_Name: HD12345 Config: HRS Opmode: ACQ Aperture: 2.0 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: BRIGHT=RETURN, ! ... Number_of_Iterations: 1 Time_Per_Exposure: 13.5S Special_Requirements: ONBOARD ACQ FOR 2 Comments: STEP-TIME = 1.5 sec Exposure_Number: 2 Target_Name: HD12345 Config: HRS Opmode: ACQ/PEAKUP Aperture: 0.25 Sp_Element: MIRROR-N1 Wavelength: Optional_Parameters: SEARCH-SIZE=5 ! ...

Еще в разделе: (Показать все результаты (>22538) - www.stsci.edu/ )

• Chapter 5: Visits, Exposures and Exposure Groups
• STIS Reference Files
• WFPC2 TIR Abstract

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/ )

• ADASS 2003 Conference Proceedings
• 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 (>3291) - www.sao.ru/ )

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

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 (>2225) - www.sai.msu.su/ )

• Zen: sncat design

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 (>67038) - www.eso.org/ )

• ESO - Paranal Science Operations: End of Missions Report
• pyQC: script structure
• HAWK-I Exposure Time Calculator

... 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 (>10647) - www.arcetri.astro.it/ )

• Program parameters
• The LongSp Description
• Determination of the Detector Parameters

... 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 (>826) - xray.sai.msu.ru/ )

• Be/X-ray binaries and candidates
• Initial Distributions of Binary Parameters
• The Model

... 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 (>1716) - astro.uni-altai.ru/ )

• Stellarium: gTime Class Reference
• Stellarium: StelObjectModule Class Reference
• Stellarium: SphereParams Struct Reference

... In the past month, I?ve noticed relatively frequent paper appearance in arxiv/astro-ph whose title includes Bayesian or Markov Chain Monte Carlo (MCMC) . ... astro-ph:0708.2340v1] Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm by L. Miller et. al. [astro-ph:0708.1871v1] Dark energy and cosmic curvature: Monte-Carlo Markov Chain approach by Y. Gong et. al. in addition to the previous posting in this slog, [ArXiv] Bayesian Star Formation Study. ...

Еще в разделе: (Показать все результаты (>4271) - hea-www.harvard.edu/ )

• The AstroStat Slog nuisance parameter
• The AstroStat Slog Blog Archive [MADS] Semiparametric
• The AstroStat Slog Blog Archive ab posteriori ad priori

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

Еще в разделе: (Показать все результаты (>2668) - star.arm.ac.uk/ )

• Armagh Observatory
• Sfit Control Language: Classified Listing

... Co-ordinate sy