XMM-Newton Science Analysis System . ... rgsframes creates the intermediate event lists and adds to them the PIXELS and EXPOSURE tables, and an internally generated GTI table called STDGTI . ... The GTI table created here sets the most relaxed standard for what time intervals may be included in the data products, and subsequent stages can only act to further restrict these intervals. XMM-Newton SOC/SSC -- 2004-11-22 ...

... Up: Future Instruments and Telescopes, Tools . ... New Generation Astronomical Telescopes (NGAT), a class of telescopes designed to be operated remotely and robotically, require efficient methods for communicating images over heterogeneous and low-bandwidth data networks such as the Internet. ... Methods researched thus far involve the classification of astronomical images based on object parameterisation, progressive image transmission, and evaluation of existing image compression schemes. ...

Next: Time Series Analysis Up: No Title Previous: Command Syntax Summary . This manual is intended as a guide to the use of the digital stellar photometry reduction program DAOPHOT II: The Next Generation. ... In DAOPHOT II: The Next Generation all of the major algorithms and actual FORTRAN coding are done by Stetson, with the exception of those Figaro, IRAF, or MIDAS routines which are used for the image input and output. Stetson is solely responsible for bugs and algorithm-related problems. ...

... Classes . ... casa::MVFrequency . ... MVFrequency (const MVFrequency &other) . ... MVFrequency (const Quantum < Vector < Double > > &other) . MVFrequency (const Vector < Double > &other) . ... Set the value from internal units (set 0 for empty vector). virtual Vector < Quantum < Double > > . ... Get the wave characteristics in (recognised) specified units. virtual Vector < Quantum < Double > > casa::MVFrequency::getRecordValue . ... virtual Vector < Double > casa::MVFrequency::getVector . ...

... 1.1.2 Spectral Filters . 1.1.3 Quantum Efficiency and Exposure Limits . ... 1.2 Which Instrument to Use: WFPC2, ACS, NICMOS, or STIS? 1.2.1 Comparison of WFPC2 and ACS . 1.2.2 Comparison of WFPC2 and NICMOS . 1.2.3 Comparison of WFPC2 and STIS . ... WFPC2 . ... 1.6 What's New in Version 6.0 for Cycle 11 . ... 2.9 Calibration Channel . ... 3.3.3 LRF Photometric Calibration . ... 4.8.1 Sources of Dark Current . ... 8.10 Calibration Plan Summary . 8.11 Cycle 4 Calibration Plan . ...

. This diagram illustrates the boxes generated by a UL list with two LI list items. There are two parts to the illustration. The first shows the actual rendering of the boxes generated by the list elements. Background colors and border styles vary to delimit the box areas. The second shows the same rendering, but the content, padding, border, and margin edges of each box are shown explicitly. In particular, the illustration shows how vertical margins between the LI boxes collapse. Return to image.

. md5 [ -0123456789 ] [ -h] file . This program generates the message digest of the given file using the RSA Message Digest 5 (MD5) and other selected algorithms. If file is not given, the program uses the standard input. -0123456789 . Select algorithm from the following list . -0 null . -1 MD5 . -2 SNEFRU . -3 CRC32 . -4 CRC16 . -5 MD4 . -6 MD2 . -7 SHA . -8 HAVAL . -9 null . -h . Display the result in hex; the default is base-64 . David L. Mills (mills@udel.edu)

Describes how funtools can be integrated into the ds9 Analysis menu. SAOImage/DS9 is an astronomical imaging and data visualization application used by astronomers around the world. DS9 can display standard astronomical FITS images and binary tables, but also has support for displaying raw array files, shared memory files, and data files automatically retrieved via FTP and HTTP. ... It can be manually loaded into DS9 from the Load Analysis Commands ... option of the Analysis menu. ...

... GSAOI Home . Instrument . ... The Gemini South Adaptive Optics Imager (GSAOI) is a near-infrared adaptive optics camera that will be used with the Multi-Conjugate Adaptive Optics (MCAO) system on the Gemini South 8-m telescope . ... Gemini's major instrumentation goal is to develop its Multi-Conjugate Adaptive Optics (MCAO) system for scientific use on Gemini South. ... Existing adaptive optics systems use a single natural guide star or artifical laser guide star to measure this image blur. ...

... Directives | ... Apache HTTP Server Version 2.2 . ... Generation of Expires and Cache-Control HTTP headers according to user-specified criteria . ... This module controls the setting of the Expires HTTP header and the max-age directive of the Cache-Control HTTP header in server responses. ... ExpiresByType . ... This directive defines the value of the Expires header and the max-age directive of the Cache-Control header generated for documents of the specified type ( e.g. , text/html ). ...

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...