... The context ASTROMET can be enabled by the command SET/CONTEXT ASTROMET . ... These commands take care of the following: . read the measurements and standard stars, and compute the transformation parameters (this step is performed by the command ASTROMET/TRANSFORM ); . edit the standard star table to remove/restore some stars (this step is performed by the command ASTROMET/EDIT ); . actually compute the converted coordinates (this step is performed by the command ASTROMET/COMPUTE ). ...

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C#> gaussn.dc2 C CFunction: GAUSSN C CPurpose: GAUSSN computes the value of an N-component Gaussian C CFiles: gaussn.dc2,gaussn.shl C CAuthor: Peter Roelfsema C CCategory: UTILITY C CCall: C C GX=GAUSSN(X,PAR,NPAR) C C Input parameters: C X -R -running coordinate. C PAR -R -array defined as follows: PAR(0:NPAR*3) that C contains the parameters for the Gaussian in the following C order: C C PAR(0) -zerolevel C PAR(1) -PAR(3) -int, pos. of peak, fwhm cmp. ...

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• http://www.atnf.csiro.au/research/LVmeeting/magsys_pres/ruzicka.pdf
• Pulsar Group PmWiki/Available Actions
• Initial ``fixes'' to millimetre data

... sas (gui-1.37.5) [?? Meta Index / Home Page / Developer's notes / Layout file . It is recommended that the following guidelines are followed when developing tasks for use with the GUI: . Use the special parameter types which are available (see documentation of the param package), so that the GUI can use appropriate widgets. ... Use tab cards to organize a complex dialog into a set of pages. ... Use labeled frames to group together a set of related parameters, with a label. ...

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• Description

Your Phase II Proposal and Using RPS2 . ... 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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• Introduction
• Photometric Analysis
• Introduction to STIS

... 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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• mod_session_crypto - Apache HTTP Server
• Program parameters
• mod_macro - 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. ...

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• A New Entropy Measure Based on Multiple Resolution and Noise Modeling
• ASC Coordinate Transformation-The Pixlib Library
• Indexing and Searching Distributed Astronomical Data Archives

... This function can also be used for particular types of subtypes or kinds: KIND (0) integer KIND (0.0) floating point number KIND (.FALSE.) logical variable KIND ("A") string of characters There is an intrinsic function SELECTED_REAL_KIND , which returns the kind of the type REAL that has a representation with (at least) the precision and the exponential range requested. ... With the choice SELECTED_INT_KIND (5) all integers between (but not including the limits) -100 000 and +100 000 are permitted. ...

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• Notation
• NAG's Fortran 90
• Overview

... The package AMPLE (Adaptable Minor Planet Ephemerides) is dedicated to solving a number of problems concerning minor planets with the aid of IBM-type personal computer. ... Obtaining selection of orbital elements and/ or photometric parameters of minor planets in conformity with imposed restrictions. ... The orbital elements of all minor planets used in AMPLE for 2015 have been determined in IAA on the ground of available observations in the catalogue of observations of the Minor Planet Center. ...

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• ENGAMPLE
• IAA GPS Analysis Center

Next: Coherent integration Up: Astrometry data reduction Previous: Introduction Contents . ... In order to increase the SNR for these data, we coherently integrate the complex visibility for typically 200 ms. The coherent integration is done using the COBRA procedure cohstrictor . In order to provide the necessary input file for this step, the following CONSTRICTOR parameters should be used. ... The .coh extension is standard for coherent integration. ... NumAv = 100. ... Pass on metrology data . ...

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• The Hierarchical Stellar Systems Model Format
• Quality Control: Image flats
• ESO - Common Pipeline Library

Next: *tvimcontour* - Overlay contours Up: Celestial Coordinates from Image Previous: *wcscoord* all . To produce a high-quality black-and-white figure of a source with a coordinate grid overlaid, use the following recipe: . ... display.xcenter=0.55 . ... display ``rp110590n00.qp[bl=15][249:679,409:839]'' 1 . ... Packages ``images'' and ``tv'' must be loaded to run wlpars and wcslab . ... Run wcslab (overlays a world coordiante system). wcslab ``rp110590n00.qp[bl=15][249:670,409:839]'' 1 . ...

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• Doug Burke's Perl/S-Lang pages: CIAO examples
• Regions and Source Parameters
• Fixing and Freeing Region Markers

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 IDL routines
• AZ Key parameters, 1998
• AZ Key parameters, 1997

... The predicted MIR's ground tracks, which pass near INSPIRE net, are available in this home page. The track consists from magnetic footprints calculated by magnetic mapping from MIR positions with 30 s step. ... For each time some of the INSPIRE net place are selected as soon as its coordinates are close to the MIR magnetic footprint (the geocentric angular distance between SP and footprint is less then 2.1 deg) . Back to the Top . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• IKI SSC, INTMINS APRIL99
• Tail Probe | Matrix of Transformation Tail Probe | Matrix of Transformation
• The simulative geophysical regions cross-sections coordinates

... All the parameters provided in this database have been obtained using the the MIRIAD ( Sault et al. 1995 ) task MBSPECT . MBSPECT makes a spectrum of the velocity (or frequency) axis of a cube. The spectrum is beam-weighted, over the width specified, for the other image axes. ... Robust parameters are calculated by using an algorithm which minimises the mean absolute deviation of the flux-weighted velocities. mask= This specifies the x-axis ranges to be excluded from any continuum fit. ...

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• INTRODUCTION to Spectral Line Observing at AO
• Arecibo Observatory L-Wide Band Receiver
• The Mock Spectrometer

OptInt PmWiki : Pm Wiki / Debug Variables . Basic Variables | Variables | ... EnableDiag . The following actions are available only if you set $EnableDiag = 1; in your configuration file. They can be used for debugging and should not be set in a production environment. ?action= ruleset . ... If you have a wiki that composes a HTML page from multiple pages, such as a normal layout with a sidebar, you'll get separate timings for each subpage and for the total page.) ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• Simple logging of scripts and their parameters Bojan Nikolic web pages (r. 329)
• OptInt PmWiki : Available Actions

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... Refraction Class Reference . ... virtual voidљ . forward ( Vec3d &altAzPos) const . ... backward ( Vec3d &altAzPos) const . Remove refraction from position ("reduce"). ... forward ( Vec3f &altAzPos) const . ... setupGLSLTransform ( StelGLSLShader *shader) . ... virtual void Refraction::backward . ... virtual void Refraction::disableGLSLTransform . ... virtual void Refraction::forward . ... virtual void Refraction::setGLSLUniforms . ...

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• Stellarium: SphericalRegion::DrawParams Struct Reference
• Stellarium: StelToneReproducer Class Reference
• Stellarium: StelGeometryBuilder Class Reference

... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...

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• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)
• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Initial parameters of compact stars
• Page contents
• The Effect of Relativistic Wind on Accretion Flow Parameters

Russian page . The 6th International Astronomy Olympiad will be organized on September 26 - October 3, 2001 in the scientific town of Nauchnyj, Republic of Crimea. ... Weather in Crimea . ... Those who were interested to get further information about the VI International Astronomy Olympiad (including official invitations for teams and observers: Ukrainian visa and visa support was necessary for citizens of some countries!) were welcome to contact Coordinating Council in English or Russian . ...

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• VII International Astronomy Olympiad: information available before
• Bismuth chalcogenides (Bi2Se3, Bi2Te3)
• VIII International Astronomy Olympiad: information available before

... Flight 1) 2) 3) Flight 1) 2) 3) model FM1 has the following parts: LNA MY-18, serial number PN 01-0252, factory number FM1; receiver box KRT-18, serial number PN 17660-01, factory number FM-001; DC-DC converters IVEP1 and IVEP2, factory number 05. model FM2 has the following parts: LNA MY-18, serial number PN 01-0252, factory number FM2; Receiver box KRT-18 serial number PN 17660-01, factory number FM-002; DC-DC converters IVEP1 and IVEP2 factory number 06. ... See Appendix 1. ... 2003. ... 2004 . ...

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• Parameters of the Moon-perturbed orbit
• GOCG Pre-Observation Products
• MILLIMETRON

... There are a lot of computer codes simulating this scattering and freely available in the Internet (see e.g. links on our JPDOC page ). ... The code and input file are available in the directory . ... A slightly modified code of Barber Hill with a C-shell and input files is available in the directory . ... The code, input and test output files are available in the directory . ... See also readme file. file. ... The code, input file and their description (a TeX file) are available in the directory . ...

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