... The ANU 2.3m telescope building, the Anglo-AuтАж . Sidebar Left . ... Title: The ANU 2.3m telescope building, the Anglo-Australian Telescope dome and the ANU 24-inch telescope dome. ... NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. No use may be made of any of the images without Dr Shobbrook's written permission. ... The ANU 2.3m telescope building, the Anglo-Australian Telescope dome and the ANU 24-inch telescope dome. ...

... Bojan Nikolic web pages (r. 329) . ... http://carma.astro.umd.edu/wiki/index.php/Installing_Developer_CASA . Building CCMTools as required by CASA . ... Building . ... Notes related to building CASA . A prototype build system for CASA using SCons . ... Generating IDL files . ... Notes on the classic CASA build . ... Writing the tool XML file . ... Automatically generated IDL files from the files describing each of the tools of CASA. ... Building CASA . ... Building the casa-core libraries . ...

... Main . ... Telescope . ... Diameter of the main mirror, mm . ... The length of the telescope tube, mm . ... Weight of the main mirror, kg . ... Weight of the main mirror in holder, kg . ... Weight of the telescope, kg . ... field of . ... 1:7.7, with corrector . ... 1:7.7, without corrector . ...

XMM-Newton Science Analysis System . ... The current version of omcomb combines the four image segments generated by the full-frame low resolution mode into a single image, which the OM imaging chain task, OMICHAIN, can then process. ... A requirement therefore arose for a task in the OM imaging-chain to recombine the four full-frame low-resolution mode image segments into a single image, and since at the present time the OM slew-chain task is disabled, omcomb has been modified to perform this task. ...

... The GHRS has the usual components of an astronomical spectrograph: entrance apertures, a collimator, dispersers, camera mirrors, and detectors. ... The collimator and camera mirrors are unexceptional and need no further description here (see ``The HST Focal Plane and the GHRS Apertures'' on page 73 for details). ... The first two first-order gratings, G140L and G140M, have their spectra imaged by mirror Cam-A onto detector D1, which is optimized for the shortest wavelengths. ...

Open Systems Handbook: A Guide to Building Open Systems . ... This book is designed to provide interested individuals and organizations with an overview of open systems and the work being done to achieve them. ... This section is organized using a descriptive model of an open systems environment developed by the IEEE PI 003.0 Working Group, which is developing the Guide to POSIX-based Open System Architecture. ... Standards for open systems 13 . Chapter 3: The open systems environment (OSE) 15 . ...

... ASAP data handling works on objects called scantables. ... For example Parkes multibeam data would contain many beams, one IF and 2-4 polarisations, while the new Mopra 8-GHz filterbank will eventually produce one beam, many IFs, and 2-4 polarisations. A collection of sequential integrations (rows) for one source is termed a scan (and each scan has a unique numeric identifier, the ScanID). A scantable is then a collection of one or more scans. ...

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