This task focuses on the process and tools used to do the initial plan window assignment for the visits of a new cycle in the operational LRP. May 25, 2000 Presentation by I. Jordan on Major steps in "Process for Constructing a New LRP. This document is an overview of the cycle-long process governing the construction of a new cycle's LRP. Related information can be found on the Procedure page for Merging Cycles. October 2000 Presentation by I. Jordan on "Building a New Cycle LRP" . ...

... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

... 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. ...

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

... Bojan Nikolic web pages (r. 329) . ... I have a bzr branch of the casa-core repository (sing the bzr-svn plugin), and I?ve made a branch off this branch with some small build improvements. ... Destination directory export CCINSTALLDIR=/home/bnikolic/p/casa-main #HDF5 wget http://www.hdfgroup.org/ftp/HDF5/current/src/hdf5-1.8.3.tar.gz tar xzvf hdf5-1.8.3.tar.gz cd hdf5-1.8.3 ./configure --enable-cxx --prefix=$CCINSTALLDIR make && make install && cd .. ... Building the casa-core libraries . ...

I'm glad you're interested in collaborating on the ConcepTests for Astronomy WWW database project! ... Paul . ... a) high luminosity, high temperature to low luminosity, low temperature . b) high luminosity, low temperature to low luminosity, low temperature . c) high luminosity, low temperature to low luminosity, high temperature . d) high luminosity, high temperature to low luminosity high temperature. ... Back to Paul Green's Peer Instruction page. ... Back to Paul Green's HomePage . ...

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

The AstroGuide . ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . The observatory consists of a dome containing a 17" f/15 classical Cassegrain reflector, a roll-off roof building containing a 12.5" f/6.5 Newtonian reflector, a classroom building with a darkroom, and two other buildings. ... Web Site . http://www.astrohbg.org/naylor_observatory.php . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . ...