This module supports ISAPI Extensions within Apache for Windows. ... This module implements the Internet Server extension API. It allows Internet Server extensions ( e.g. ISAPI .dll modules) to be served by Apache for Windows, subject to the noted restrictions. ISAPI extension modules (.dll files) are written by third parties. ... Review the Additional Notes and the Programmer's Journal for additional details and clarification of the specific ISAPI support offered by mod_isapi. ...

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• Apache module mod_vhost_alias

Modules | ... Apache HTTP Server Version 2.2 . ... ISAPI Extensions within Apache for Windows . ... isapi_module . ... It allows Internet Server extensions ( e.g. ISAPI .dll modules) to be served by Apache for Windows, subject to the noted restrictions. ISAPI extension modules (.dll files) are written by third parties. ... In the server configuration file, use the AddHandler directive to associate ISAPI files with the isapi-handler handler, and map it to them with their file extensions. ...

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• Principal Components Analysis
• mod_vhost_alias - Apache HTTP Server
• mod_info - Apache HTTP Server

... Two additional extensions contain the polynomial coefficients describing the distortion for all the filters. FILTER-U . ... Each extension FILTER-FilterId holds a binary table sampling the detector distortion of a specific filter at a coarse resolution ( 1 datapoint every 25 subpixel). ... The filter element is found in the column FILTER_ID. The required binary table entry is identified by matching the value of the column FILTER_ID with the State Variable FilterID. ... not applicable . ...

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• List of CCF Components used:
• External SAS packages
• List of CCF Components used

Modules | ... Apache HTTP Server Version 2.2 . ... ISAPI Extensions within Apache for Windows . ... isapi_module . ... It allows Internet Server extensions ( e.g. ISAPI .dll modules) to be served by Apache for Windows, subject to the noted restrictions. ISAPI extension modules (.dll files) are written by third parties. ... In the server configuration file, use the AddHandler directive to associate ISAPI files with the isapi-handler handler, and map it to them with their file extensions. ...

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• mod_vhost_alias - Apache HTTP Server
• mod_info - Apache HTTP Server

. You have submitted a form or followed a link to a page that requires a web server and the FrontPage Server Extensions to function properly. This form or other FrontPage component will work correctly if you publish this web to a web server that has the FrontPage Server Extensions installed.

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• Inference of Coefficients for Use in Phase Correction
• Inference of Coefficients for Use in Phase Correction Bojan Nikolic web pages
• OptInt PmWiki : MROIFastTipTilt / Tech Meet 6

CIMA is more than just the observing tool - in fact, the observing tool is just a part of a bigger package called the CIMA software package. ... There is also a another package called the CIMA WAPP software which contains the WAPP software, the special Tcl/Tk interpreter used by CIMA and support libraries. ... All CIMA software components recognize the following general options that are part of the CIMA version selection system: . ... The select_cima script can be used to set up a default version. ...

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• Chapter 5. Listing of Installed Components
• Appendix D. GLX Support
• pdev_birdies_25jun07

Pipeline Code Internal Organization ######################################## Major software components and object classes ================================================ The GPI data pipeline is implemented in object-oriented fashion using IDL classes. ... Loops forever waiting for recipe files and processes them one at a time when they arrive. drf High level wrapper class for recipe files (aka DRFs). ... This class can be both an internal and a GUI, depending on how it's invoked.* ...

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• Pipeline Code Internal Organization GPI Data Pipeline 1.0 documentation
• CDBS Operations
• CSPICE Routines: VUPACK_C

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/computing/software/gipsy/sub/voigt.shl
• http://www.atnf.csiro.au/computing/software/gipsy/sub/gaussn.dc2
• cmodel (Model Image Generator) CentralProcessor 0.11 documentation

... Please note that throughout this exercise you need some patience since the PEARL procedures use the Direct Fourier Transform which is quite slow for the size of map we are trying to work with! . ... Initial chisq= 24.980139 . SVD: will edit 0 singular values! ... Click Update to add the selected number of CLEAN component to the current model (which was empty at the start), self-calibrate the phases, subtract the CLEAN components from the data, and re-display the updated residual and final maps. ...

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• DFS Commissioning: integration kick-off meeting
• Spectroscopy
• Astrometry

TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• Astrophysical Research Consortium - Apache Point Observatory
• Drawing and Part Configuration Management Directive and Procedures:
• Procedure for Part Numbering Convention: Larry Carey, 2005

.

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• The Galaxy Gallery Page VII: Infrared Imaging

Follow-up astrometry and recoveries are made with the ANU 40 inch (1.0-m) f/8 reflector at Siding Spring Observatory (IAU code 413). ... A routine follow-up of 2003 WY153 on 2003 Dec 15 became much more than routine when a faint object with unusual motion vector was found close to the target asteroid. ... During routine astrometry with the 1.0-m to improve the orbit of the Apollo asteroid 2004 CB, the asteroid was found on March 30 to have a short tail! ... Siding Spring Survey Main Page . ...

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• Marc White - Astrophysicist - The Australian National University
• Gemini NIFS August 2004 Update.
• Richard Woolley and Jim Banham inspecting optical and mechanical components,

... Team . ... All the results we present were obtained with the SCORPIO instrument mounted at the 6-m telescope of SAO RAS. TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1090 SUBJECT: GRB001109, Host Galaxy Spectroscopic Observations DATE: 01/09/08 07:28:47 GMT FROM: Vladimir Sokolov at SAO RAS <sokolov@sao.ru> . ... TITLE: GCN GRB OBSERVATION REPORT NUMBER: 1092 SUBJECT: GRB001109, Host Galaxy Astrometry DATE: 01/09/11 08:19:24 GMT FROM: Vladimir Sokolov at SAO RAS <sokolov@sao.ru> . ...

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• Fabry-Perot Interferometer: Gallery Old

Contents] [Prev page] [Next page] [Index] . Navigator 4 from Netscape, which is part of the Communicator product suite, includes three new areas of functionality that taken together give you Dynamic HTML. The three components of Dynamic HTML are style sheets, content positioning, and downloadable fonts. Used together, these three components give you greater control over the appearance, layout, and behavior of your web pages. ... Introducing Downloadable Fonts . ...

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• Additional problems at the transition
• Checking Compatibility of Video Hardware
• A Simple Example With a Single Chirp Component

Magnetic field measurements onboard the INTERBALL AURORAL spacecraft. Magnetic field measurements onboard the INTERBALL-2 (Auroral Probe) is carried out by the IMAP-3 instrument. ... The IMAP-3 instrument is designed to measure three components of the DC magnetic field in two ranges: +/- 6800 nT with resolution 1 nT and +/- 68000 nT with resolution 10 nT. ... We cannot calculate now By and Bz components separately due to absence of the spacecraft attitude data. ...

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• Vectors
• Wave complex KEM-3
• Vectors--Lesson Plan #23

TH setINDI 1 .SH NAME setINDI \- set one or more writable INDI property values .SH SYNOPSIS \fBsetINDI [options] device.property.e1[;e2...]=v1[;v2...] ... \fP .SH DESCRIPTION .na .nh .PP setINDI connects to an indiserver and sends commands to set new values for specified properties. ... TP -p <p> connect using alternate port p; the default is 7624. ... SH EXIT STATUS The setINDI program exits with a status of 0 if it suceeded in setting the new value for each specified property. ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/indiutil/getINDI.1
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/optec/INSTALL

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Lightcurve of HW Vir from images obtained using the Faulkes Telescope South, operated by Las Cumbres Observatory . The blue triangles show the difference between two stars whose brightness is constant. ... This shows the value of the Faulkes Telescopes in the follow-up observations of eclipsing binaries with the aim to detect and characterise additional circumbinary companions. ...

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• R-N Expression of Risk
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• Follow up from the Second Cross-Border Schools Science Conference |

... Archives . ... The PCA and ICA is used for separating mixed components with some assumptions. ... The need of source separation methods in astronomy has led various adaptations of decomposition methods available. ... I rarely come up with a paper which gathered and summarized component separation methods applicable to astronomical data. In that regards, the following paper seems useful to overview methods of reducing dimensionality for astronomers. [arxiv:0805.0269] . ... Chandra Blog . ...

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• Chandra Images for SNR J0519.5-6902
• The AstroStat Slog component separation
• Additional Tools

... To avoid extensive numerical calculations in the statistical simulations, we treat the continuous evolution of each binary component as a sequence of a finite number of basic evolutionary states (for example, main sequence, red (super)giant, helium (Wolf-Rayet) star,     hot WD), in which stellar parameters significantly differ from each other. ... Figure 2: Schematic representation of the typical evolutionary track of a massive binary system with normal and compact star stages indicated. ...

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• Massive X-ray Binaries
• Initial Distributions of Binary Parameters
• Observational Data

The idea of component-oriented programming is that in the course of implementation of various software projects a programmer (or a programmers team) accumulates a library of reused software fragments that are used in different projects. ... To solve such problems there are some special syntax means in Actor Prolog that support component-oriented programming. ... A package in Actor Prolog is a set of classes linked by implication. ... Actor Prolog supports visual component-oriented programming. ...

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