... applies to task version 0.1 and 1.0 . ... applies to task version 1.1: minor updates . ... applies to task version 1.4: improved flow-chart . ... applies to task version 2.0: new parameter names . ... applies to task version 2.1: new parameter names, some minor updates . ... minor updates for task version 3.0 . ... applies to task version 4.0: new command line parameter . ... applies to task version 5.0: another new command line parameter . ... applies to task version 6.3: new L A T E Xmacros . ...

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... 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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• STSDAS Version 3.10 Release Notes
• Changes Since the Previous Cycle
• WFPC2 Header Changes due to OPUS 10.0 Update

... eparam* - edit parameter files . ... Type ``<esc>-?'' within a parameter editor for more details on commands. *tupar* - Edit table headers . Table files (* .tab ) consist of a header including a variety of parameters and the table itself. It is possible to edit the header using tupar and the table with tedit provided you have write-access to the file. ... Works like emacs but uses <ctrl> D to exit. *hedit* - edit image file header . qphedit* - edit .qp file headers . ...

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• The ST-4
• Structure of the Spectral Package
• Possible Pitfalls

... B.1 New functionality . ... B.3 Semantic changes from CSS1 . ... CSS2 builds on CSS1 and all valid CSS1 style sheets are valid CSS2 style sheets. The changes between the CSS1 specification (see [CSS1] ) and this specification fall into three groups: new functionality, updated descriptions of CSS1 functionality, and changes to CSS1. ... Several internationalization features, including list numbering styles , support for bidirectional text , and support for language-sensitive quotation marks . ...

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... prjprm Struct Reference . ... intљ . ... It consists of certain members that must be set by the user ( given ) and others that are set by the WCSLIB routines ( returned ). ... This signals the initialization routine ( prjset() or ???set() ) to recompute the returned members of the prjprm struct. flag will then be reset to indicate that this has been done. ... If undefined (set to a magic value by prjini() ) the initialization routine will set this to a projection-specific default. int prjprm::bounds...

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• Release of 22 Feb 1996
• casacore: casa::Gaussian1D< T > Class Template Reference
• THE SCHED INPUT FILES (Includes parameter lists)

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Landscape Class Reference abstract . ... More... #include < Landscape.hpp > . ... Landscape (float _radius=2.f) . ... load (const QSettings &landscapeIni, const QString &landscapeId)=0 . ... setBrightness (const float b) . ... floatљ . ... const QStringљ . getTexturePath (const QString &basename, const QString &landscapeId) . ... const floatљ . ... Definition at line 42 of file Landscape.hpp . ... const QString Landscape::getTexturePath . ...

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• Stellarium: StelButton Class Reference
• Stellarium: StelScriptMgr Class Reference
• Stellarium: ScreenImageMgr Class Reference

The 2.6 kernel contains a long list of changes which affect device driver writers. As part of the task of porting the Linux Device Drivers sample code to 2.6, your humble LWN Kernel Page author is producing a set of articles describing the changes which must be made. ... November 25, 2003) The entire set of articles has been updated to reflect the 2.6.0-test10 kernel. ... Timekeeping changes (November, 2003; 2.6.0-test9); changes to how the kernel manages time and time-related events. ...

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• comedi_set_buffer_size
• comedi_dio_config
• Writing programs that use comedi and comedilib

OptInt PmWiki : Pm Wiki / 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. ... ThisGroup:SideBar&action=edit Edit menu]] . ... 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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• How to create a new tool in CASA Bojan Nikolic web pages (r. 329)
• OptInt PmWiki : Page List Templates
• DUST: dustiface.h File Reference

... 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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• List of currently available KP AZ.
• The Face on Mars
• INTERBALL-TAIL KP

... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...

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• Making backups with tar

ESO Phase 3 Data Release Description Please start from this template when preparing the documentation for your ESO Phase 3 data release. ... Finally, the release description will be published as submitted - without further editing by ESO - to support the user community in utilizing the data. ... Please indicate if this is a catalogue data release. ... Data Reduction and Calibration Please address the following questions for scientific catalogue data, particularly in case of source catalogues: . ...

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• Parameters
• extractStat
• phoenixMonitor

Full-Text Search in PostgreSQL: A Gentle Introduction . ... Fast Backward . ... ALTER FULLTEXT DICTIONARY -- change a full-text dictionary . ALTER FULLTEXT DICTIONARY dictname RENAME TO newdictname ; ALTER FULLTEXT DICTIONARY dictname SET OPTION opt_text ; . ALTER FULLTEXT DICTIONARY change an existing full-text dictionary. dictname . The name (optionally schema-qualified) of the dictionary to rename. newdictname . The new name of the dictionary. ... CREATE FULLTEXT DICTIONARY . ...

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• ALTER FULLTEXT PARSER
• ALTER FULLTEXT CONFIGURATION
• ALTER FULLTEXT ... OWNER

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

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• Arecibo Observatory L-Wide Band Receiver
• fast2010_page2
• CIMA Configuration Files

... Tiny Tim has been used for generating Hubble Space Telescope ( HST ) point-spread functions (PSFs) for deconvolution, algorithm testing, proposal planning, and optical studies. ... Tiny Tim is a stand-alone program for simulating HST PSFs as viewed with the on-board imaging cameras (WF/PC-1, WFPC2, FOC, COSTAR/FOC). ... The measured aberrations for FOC f/96, WF/PC-1 PC6, WFPC2, and COSTAR/FOC are used by Tiny Tim . ... Figure: FOC f/96 observed and Tiny Tim model PSFs (pre-COSTAR) at 253 nm. ...

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• ETCs and Observations Simulation at the VLT
• ADASS 2003 Conference Proceedings
• A Spectroscopy Exposure Time Calculator for IRAF

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

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• AI SPbU library of scattering codes

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . ... include . tcc . telConst.h . ... 8 љ - Changed SCT_min_LCT's name and units; changed Elevation's units. R.O. 8/87 . ... 13 љ - Adapted to C++ and changed units of elevation from km to m. R.O. 2011-12 . ... 18 љ const double MeanLong = -105.820417; // longitude east, deg . 19 љ const double MeanLat = 32.780361; // latitude north, deg . 20 љ const double Elevation = 2788; // elevation above mean sea level, m . ... const double Elevation . ...

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• lsst.coordConv: coordConv::Coord Class Reference
• lsst.coordConv: coordConv::FK4CoordSys Class Reference
• Agile ICC Version History

fitshdr_edit - FITS-file headers interactive editor fitshdr_edit [options] FITSfile_name . fitshdr_edit utility allows to modify FITS headers' lines interactively (FITS MultiExtentionsFiles included). fitshdr_edit is just simple shell script around fitshdr utility. ... It means, that You can't remove line from header! ... 560:CRDELT2 = 21.0 / this is example 640: 720:HISTORY header No.0: 1st history line 123456789012345678901234567 880:COMMENT Sat Sep 25 21:17:34 CEST 2004 / by fitshdr_edit . ...

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• Manpage of FITSHDR

Next: Summary of reduction Up: Echelle Reduction Previous: Saving the Data . In the present version we will be concerned with the standard configuration of CASPEC, the Cassegrain Echelle Spectrograph which is in operation at the Cassegrain focus of the ESO 3.6 m telescope. ... In its standard configuration CASPEC uses a a 31.6 lines/mm echelle grating together with a 300 lines/mm grating cross disperser. ... The table shows the change in resolution with the order number. Table: Resolution . ...

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• mod_so - Apache HTTP Server
• Format of the table for atomic parameters (ABSP.TBL).
• Echelle Spectra

Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...

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• Magnetic mapping
• Multipoint correlations of the solar wind parameters observed by several
• BOKZ Star Trackers

Next: Mass change Up: Evolutionary Scenarios of Binary Previous: Stellar Winds From Normal . As mentioned earlier, the duration of the binary evolutionary stage (say, I+I) is determined by the faster evolving component , where is the time each component spends at the corresponding evolutionary stage. ... Next, we should calculate the mass change for the slower evolving companion, the orbital semi-major axis and the eccentricity. Mass change . Semi-major axis change . ...

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• Mass change
• Semi-major axis change
• Contents