... The moonlit ANU 2.3m telescope building, theтАж . Sidebar Left . ... Title: The moonlit ANU 2.3m telescope building, the Anglo-Australian Telescope dome in the distance . Description: The ANU 24-inch telescope dome on the right. ... NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. ... The moonlit ANU 2.3m telescope building, the Anglo-Australian Telescope dome in the distance The ANU 24-inch telescope dome on the right. ...

... 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. ...

.