... elcplot (elcplot-2.5) [xmmsas_20080701_1801-8.0.0] . Meta Index . elcplot produces plots of the net source and background time series for a single EPIC time series FITS file (the output of lccorr ), along with either the Good Time Intervals (GTIs) or the background flare time series and Fraction Exposure, on a single page. ... Input Files . Output Files . ... Index . ...

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... 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 ! ...

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• NICMOS Proposing Example - 5
• Index
• NICMOS Proposing Example - 1

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 | ...

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

Next: Echelle Reduction Method Up: No Title Previous: Example . This Chapter provides the basic information necessary to understand the echelle љ package implemented in MIDAS . ... Tutorial examples are available in the system (command TUTORIAL/ECHELLE ) and are also included in the Appendix so that users without previous experience in MIDAS could become familiar with the calibration procedures. ... Reduction steps which are not specific to echelle spectra are described in more detail in Chapter . ...

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• Instrument Description: CASPEC
• Contents
• Session Parameters

... Up: Iraf Packages . ... IRAF Group, NOAO 1 , PO Box 26732, Tucson, AZ 85726 . This paper describes a new IRAF spectroscopy exposure time calculator. ... SPTIME takes an input source spectrum, either a reference blackbody, power law, or a user spectrum, a background ``sky'', observing parameters such as exposure time, central wavelength, seeing, airmass, and moon phase, instrument parameters such as aperture sizes and detector binning, a description of the spectrograph, and desired output. ...

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• Using XML and Java for Astronomical Instrument Control
• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• On the Need for Input Data Control in Pipeline Reductions

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. ...

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• pyQC: overview
• HSTPOLSIM (V2.00) --- November00 --- HSTPOLSIM (V2.00)
• POLIMPLOT (V2.00) --- November00 --- POLIMPLOT (V2.00)

... The Boolean object is an object wrapper for a boolean value. ... JavaScript 1.3: added toSource method . ... If value is omitted or is 0, -0, null, false, NaN , undefined, or the empty string ( "" ), the object has an initial value of false. All other values, including any object or the string "false" , create an object with an initial value of true. ... For Boolean objects and values, the built-in toString method returns the string "true" or "false" depending on the value of the boolean object. ...

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• http://www.arcetri.astro.it/irlab/doc/library/javascript/clientreference/fileup.htm
• mod_authn_dbd - Apache HTTP Server
• mod_macro - Apache HTTP Server

... 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) . ...

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• lte-codes: sterne model atmospheres

... Posted by aneta . ... probability plotting involves a physical plot of the data on specially constructed probability plotting paper . ... 5 Comments . ... Any comments? ... The chi2 bias can affect the results of the X-ray spectral fitting and it . ... This spectrum is then fit with the absorbed power law model to get . ... I simulate 1000 spectra and fit each of them using different statistics: chi2 data variance, . ... three different statistics: chi2 with the model variance, chi2 with . ...

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• The AstroStat Slog Blog Archive [MADS] Semiparametric
• The AstroStat Slog 2007 November
• The AstroStat Slog Blog Archive [ArXiv] Recent bayesian studies from astro-ph

... 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. ...

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• casacore: casa::FunctionWrapper< T > Class Template Reference
• Making a Fake Observation
• casacore: casa::CompoundFunction< T > Class Template Reference

hstpolsim -- Produce simulated polarization input data frames for HST instruments . ... inint = "" [name] . ... Name of the HST instrument for which simulated polarization images are to be produced. ... Name of the instrument specific polarizing filter for simulated images (ignored for SPECIAL instrument). filtname = "" [name] . Name of the instrument specific colour filter for simulated images. ... The header parameter FILTER provides the filter name and POLANG the polarizer angle. ...

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• APOMASK (V1.0) --- Mar00 --- APOMASK (V1.0)
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• POLIMPLOT (V1.00) --- April99 --- POLIMPLOT (V1.00)

... 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. ...

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This diagram shows the six superimposed "layers" of the CSS table model. This diagram illustrates the algorithm for calculating a cell's final background. ... The diagram shows how, looking down on the six rectangles, one may compute the background color of each cell. ... A cell without a background color in the top layer is depicted as a "window" onto the lower layers, which give its final background color. ...

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• Long description of example illustrating background calculation
• Warbling Chirplet: Analysis of Signals of Oscillating Frequency
• Long description for background pattern

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 ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• Abstract
• Paper I: Method Bojan Nikolic web pages (r. 329)

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

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... 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/ . ...

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• STDA files
• Magnetic mapping file description
• Multipoint correlations of the solar wind parameters observed by several

... 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 . ...

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• Stellarium: StelGeometryBuilder Class Reference
• Stellarium: StelObjectModule Class Reference
• Stellarium: TextUserInterface Class Reference

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. ...

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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). ...

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

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: . ...

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• INTERBALL-TAIL KP
• OMNIDIRECTIONAL PLASMA SENSOR VDP
• ENERGETIC PARTICLE EXPERIMENT DOK-2