... The call to OMDETECT is changed in accordance with the new interface of OMDETECT (a few parameters have been removed) PARAM- file is set to OMDETECT-4.1 Version 1.22.9 -2002-05-29 ( VNY ) (+doc/omfchain_description.tex) documentation has been updated Version 1.22.8 -2002-05-27 (+src/omfchain.pl) The code for extraction of the ... Changed dependancy file to omfastshift 1.4 Version 1.2: 9 Oct 1998 Updated 'event-frame' locating algorithm in omfasttest.f90 and omfastshift. ...

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• Change history

... News and . ... Press Releases . ... Description . Release Notes . ... PyRAF . ... Packages or tasks that have had minor enhancements of bug fixes include: analysis.isophote graphics.stplot.igi .skymap hst_calib.ghrs Parameter files that have changed ( new parameters or new default values, excluding prameters indicating version number changes): analysis/dither/acsdq.par (the following should all be considered new even though some have correspondences in the previous version of ...

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• WFPC2 Header Changes due to OPUS 10.0 Update
• Archive for February
• Changing Programs & Resolving Problems

... Archives . ... X-ray summer school is on going. ... Recently I went to JSM 2007 and tried to attend talks about (bayesian) change point problems, which frequently appears in time series models, often found in economics. ... Tags: ARCH , Bayesian Block , challenges , change point problem , GARCH , light curves , summer school , X-ray . ... I received another type of changing point problem, defining a peak precisely, from a x-ray school student, who tried bayesian block but said it didn?t work. ...

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• Possible Pitfalls
• Editing Files and Parameters
• The AstroStat Slog change point problem

Next: Equations of condition Up: Extinction and transformation Previous: Extinction and transformation . Bias can also be introduced by improper fitting procedures. For example, the reduction program known as SNOPY, used for many years at La Silla and also at La Palma, uses a simple iterative technique in which some subsets of the parameters are solved for, while others are held fixed; then the ones last solved for are held fixed, while the ones previously fixed are redetermined. ...

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• Saving and Loading Session Parameters
• Gain steps
• Installation

Current status of the source finding service: HALTED . ... Also fixing a bug preventing the sorting of output source lists. 13/6/2012 - v1.6, r15987 - Improved Gaussian fitting, performance improvements, use of casacore-1.4.0 and a few bug fixes. ... A major part of the ASKAP software development is to produce an effective source-finding tool to automatically process the images and cubes that come out of the pipeline imager. ... Please report any bugs or problems via the Redmine ticket system . ...

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• Changing the task context
• Package: panel
• Package: listw

I loaded my config file, but when i went to apply it, the data had changed' . ... I got a 'the correlator has failed to start' error from a WAPP - what is that? ... It happens occasionally that one or several WAPPs suddenly report a large number of serious chip count errors for a second or two, and then continue taking data without any problem. ... The problem does not require any special action (like a restart of the WAPPs) since the same WAPP will work perfectly immediately afterwards. ...

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• Arecibo Observatory L-Wide Band Receiver
• pulsedPwrIntoAlfa
• datataking_software

... UNIX commands . ... passwd command . ... changing . ... preventing prompt for . ... display to working directory . ... changing for access . ... accessing with the shift command . ... passing command arguments with . ... PostScript . files, printing . ... files . print queue . ... printer . ... printing . cancelling . ... PostScript files . ... prompt . ... display current directory in . display username in . display system name in . ...

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• Example of changing a password with the passwd command
• Index: C
• Changing your local directory

The problem of solar wind data correlation for the observations onboard several spacecraft is very important for three points of view: . ... This problem is studied now in detail by systematic determination of ion flux and ion velocity data correlations by INTERBALL-1 (IKI group), WIND and IMP 8 (both - MIT group). ... Solar wind plasma correlation lengths from IMP 8, WIND and INTERBALL-1. ... Correlation of solar wind observations onboard several spacecraft: INTERBALL-1, IMP 8 and WIND data. ...

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• IKI SSC, INTMINS APRIL99
• V.G. Petukhov (Khrunichev State Research and Production Space Center).

OptInt PmWiki . ... Edit Page | ... MROI Delay Line Design Contract . ... Changes From Pm Wiki 1 . This page is intended to describe features of PmWiki 1.0 that have been changed or eliminated in PmWiki 2.0. ... action=post no longer exists -- posting a new page is now performed by using ?action=edit with the post control set to a true value. ... PmWiki's ReadPage() function no longer supplies default text for non-existent pages -- this is now decided by whatever functions need the page. ...

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• OptInt PmWiki : PmWiki / Changes From Pm Wiki 1
• OptInt PmWiki : Trolley Software | History
• OptInt PmWiki : Design Documentation | History

AstroImageJ Release Notes . ... Daily Build Version db3.2.1 (with ImageJ 1.47i) (Last Updated: 02/04/2016) . Changes . Version 3.2.0 (with ImageJ 1.47i) (Release date: 02/01/2016) . ... Version 3.1.0 (with ImageJ 1.47i) . ... Known Problems . Feature Requests in Roadmap but not in this Version . ... Version 2.0.0 (with ImageJ 1.47a1) . ... Changes in this Version . ... Version 1.1 (with ImageJ 1.45l) . ...

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• IJEventListener (ImageJ API)

Full-Text Search in PostgreSQL: A Gentle Introduction . Prev . Fast Backward . Fast Forward . Next . ALTER FULLTEXT PARSER -- change a full-text parser . ALTER FULLTEXT PARSER prsname RENAME TO newprsname ; . ALTER FULLTEXT PARSER changes an existing full-text parser. prsname . The name (optionally schema-qualified) of the parser to rename. newprsname . The new name of the parser. ... CREATE FULLTEXT PARSER . ... DROP FULLTEXT PARSER . ... ALTER FULLTEXT .. ...

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• ALTER FULLTEXT DICTIONARY
• Zen: sncat design
• ALTER FULLTEXT CONFIGURATION

Download Izmccd (~2.7 MB). Solution of problems at identification of star field. ... 2) Scale is not correct. ... In this case algorithm of identification will revise all values of scale from twice smaller up to twice greater. ... There should be more than value of the field "Number of stars in frame". ... The star field is considered identified if number of the identified stars more or equally to this value. It is necessary to set value from 4 up to value of field "Number of stars in frame". ...

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In this chapter we will consider an example of visual expert system written on the Actor Prolog language. ... There are a lot of methods of oil field bed stimulation that increase output of the oil production: thermal, physical-chemical, gas, microbiological, and others. ... Fig. ... The Top-Most diagram consists of three blocks: the "Describe parameters of hydrocarbon field" block, the "Check adaptability of existed methods of oil production" block, and the "Display solution" block. ... Gas methods. ...

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• Laboratory of Cybernetics. IRE RAS.
• Research Activities of InformChaos Lab.

Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...

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• Solar Physics
• Spherical and Practical Astronomy
• Introduction to Astronomy

Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...

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• New Tools for the Analysis of ISOPHOT P32 Mapping Data in PIA
• Using a Data-Driven Model for Instrument Software Development
• Indexing and Searching Distributed Astronomical Data Archives

... Just to learn how to generate a system call, I created a simple system call that basically sets and resets the value of a global parameter "PREFETCH". SYSTEM CALL code ********************************** int PREFETCH = 0; /* this is a global variable */ . ... To execute the sys_prefetch system call, I wrote a prefetch.c file with the following code. ************************code to call sys_prefetch***************** #include <linux/unistd.h> _syscall2 (int, prefetch, int, mode, int, nr_hints) . ...

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• mod_charset_lite - Apache HTTP Server
• Where are the tunable parameters of the kernel?
• mod_session_crypto - Apache HTTP Server

... New version of magnetic field data (descriptor "itm") is now available with small corrections in offsets and attitude coverage. ... Full set of INTERBALL-TAIL AKR radiointensity KP for AKR instrument is now available (descriptor "ita"). ... KP data availability plots are created. ... Magnetic field data (descriptor "itm") after 1st January, 1998 are recomputed with corrected Bx_GSE offset (this was just 0.5 nT correction). ... CDF files for plasma wave KP are now available (descriptor "itw"). ...

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• INTERBALL-TAIL KP
• The Face on Mars
• Global change [Oulu]

Next: Scattering properties Up: Polarization properties (transmitted radiation) Previous: Linear polarization: wavelength dependence . Traditionally, the main problem considered in connection with circular interstellar polarization is the meaning of the wavelength where changes the sign . ... This is also demonstrated by Fig. 19 (lower panel) which shows the wavelength dependence of the factors of linear and circular polarization for particles of magnetite as was done by Shapiro ([ 1975 ]). ...

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• Linear polarization: wavelength dependence
• Polarization efficiency: size/shape/orientation effects
• Database of Optical Properties -- Level: subpage

Contact Russet McMillan (primary) or your Observing Specialists (secondary) for additional information. Contact Jack Dembicky for web page errors, corrections, ommisions, or additions. This page last updated: July 6, 2004 - JMD . This page last checked: September 14, 2003 - JMD . Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . Taking your Calibration lamps . ... Setting up multiple exposures . ... Stopping an exposure (discarding data) . ...

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• coordConv Version History
• TUI:Scripts:Built In Scripts:Telescope:Pointing Data
• lsst.tcc: tcc.cmd.showObject Namespace Reference

... enabled for phoenix v2, MCALIB production . ... supporting MASTER/SLAVE model (MUSE) . ... upload to qcweb (monitor/FINISHED); on SLAVE accounts, also scp to MASTER . ... The monthly output pages list only the SCIENCE ABs (if for IDPs) or only the processed CALIB ABs. ... YES . ... YES|NO (NO); if YES, the tool checks for the marker PROCESSED_SLAVE in $DFO_SCI_DIR and thereby recognizes data content as coming from the SLAVE account (which is then marked by dark square). ... PROC_INSTRUMENT . ... ABS...

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• DFS Problem Reporting rules and recommendations
• list of DFS Department documentation templates
• OYSTER Lab