... This is the real fix of SSC-SPR-6458 (the previous version didn'n fix it). ... Version 2.15 - 2003-11-26 ( VNY ) ------------ Protected against inconsistency of the image size and DETSEC attribute +( src / ommodmap_mod.f90 ) Version 2.14 - 2003-11-18 (CB) ------------ DEPEND file ammended for ssclib 3.0 Version 2.13 - 2003-11-18 ( VNY ) +( src /Makefile) link to SASDAL added to the makefile in order to rectify the static build Version 2.12 - 2003-11-13 ( VNY ) +( src /Makefile) ...

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• http://xmm.vilspa.esa.es/sas/6.0.0/doc/inthist/ChangeLog
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/ommag/ChangeLog
• http://xmm.vilspa.esa.es/sas/5.4.1/doc/omprep/ChangeLog

... the dark tail just above the actual trap, which can be treated with wfixup or fixpix , . cases where real objects cross the bad column, such as the object just above 2-637 in Figure 5 , . ... The standard technique for removing the effects of traps (i.e., "bad columns") is to use the . ... c1h images. ... Note that trap 2-637 from Figure 1 and Figure 5 appears to be the only trap which leaks a small amount of charge in an "upstream" direction, thus we chose a more typical trap for this example.) ...

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• Archive for February
• Archive for December
• HST Program Implementation Cron Jobs

... Changed time to 08:00-14:00 (AT, HO, MP, SH, HH) V125a Nov 01 Cancel 3C380 (VLBA, GO) VS07u Nov 03 Changed observing times (KA, HO, HH) V053c3 Nov 05 Changed observing times (VLBA) VS09q Nov 20 Cancel (GB, AR) V019b Nov 25 Changed observing times (AT, HH, MP, UD) V001a Dec 02 Removed AT VS03j Dec 03 Cancel (KA, MP, UD) V029a Dec 10 Changed times (MK, TI, AT, HH, MP) V035a1 Dec 21 Changed stop time (VLBA, GO, RO) Modified on Sep 26: Most changes are related to VSOP survey source additions. ...

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• VLA Standard Bands.
• Pulsar Group Tasks/Change Priority
• Release of 22 Feb 1996

Changed FITS time keywords to observatory standard and TAI: . Changed DATE-OBS from UTC date (yy-mm-dd) to TAI date and time (yy-mm-ddthh:mm:ss.sss) . Removed UTC-OBS; it was UTC time (hh:mm:ss.sss) . Added TIMESYS=TAI . AVAILMIN and AVAILMAX are now in TAI instead of UTC . Added IMAGETYP to FITS headers. ... Changed "expose stop" to halt the exposure sequence after the current exposure is finished normally (instead of aborting immediately and discarding the current exposure). ...

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• Procedure to Install the 2.5m Secondary Truss
• DIS Keywords
• SDSS M1 Mechanical Collimation

Very important in the introduction of a new programming language standard is that old programs (at least those who obey the outgoing standard) can be used once again, with the new standard. When we went from Fortran 66 to Fortran 77 the extended DO -loop was removed (the extended DO -loop means that if you do not change any of the DO -loop parameters you can jump out of the loop and then jump in again (this is somewhat contrary to the concept of structured programming). ... 2, June 1993, page 1. ...

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• Use of program libraries
• Introduction

The vertex software has encoder corrections that can be interactively modified via the ocu or lcu interface. ... When adding a correction, the display position includes the correction. Preset mode works fine with the correction (eg. start at 270, add correction=1deg, display reads 271, preset to 270 moves the telescope be 1 degree). I think that program track mode works differently with the offsets.. mainly because we had an offset of 1 degree for 5 months and we could still see sources. ...

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• pulsedPwrIntoAlfa
• RF observing program
• system Performance

XmCCD Copyright 2007-2013 John Kielkopf ======================================= Development Log =============== March 9, 2002 Version 1.0.0 * Support for SBIG cameras using the first public SBIG library * Basic panel for operation with ds9 +--------------------------+ May 22, 2002 Version 1.1.0 * Updated to use libudrv 4.35 +--------------------------+ May 24, 2004 Version 1.2.0 * USB support +--------------------------+ March 1, 2005 ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/libcfitsio/libcfitsio-3.310/Makefile.in
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/libcfitsio/libcfitsio-3.310/Makefile
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/libcfitsio/libcfitsio-3.340/Makefile

Next: Interactive Editing of Up: Management of Tables Previous: Displaying Tables . Elements in a table can be inserted, changed , and deleted . These functions are all performed by the WRITE/TABLE or COPY commands (See Table 5.4). The element to be modified must be defined by giving its column and row location. ... Table: Commands to Modify a Table . ... All commands that do not change a table element will only use the subset selected. ... Table: Commands to Transfer Table Data . ...

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• Converting Modules from Apache 1.3 to Apache 2.0 - Apache HTTP Server
• Moving objects
• Standard values

Modules | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Developer Documentation . ... This is a first attempt at writing the lessons I learned when trying to convert the mod_mmap_static module to Apache 2.0. ... create per-server config structures */ . ... merge per-server config structures */ . ... Questions on how to manage the Apache HTTP Server should be directed at either our IRC channel, #httpd, on Freenode, or sent to our mailing lists . ...

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• Extended IDL Help
• Upgrading to 2.2 from 2.0 - Apache HTTP Server
• mod_ext_filter - Apache HTTP Server

... Astrophysics Group . ... Optical Interferometry . OIFITS: A Data Exchange Standard for Optical (Visible/IR) Interferometry . ... OIFITS is a standard for exchanging calibrated, time-averaged data from astronomical optical interferometers , based on the FITS Standard (OIFITS is a registered FITS convention ). ... The OIFITS standard is used in the biennial optical interferometry Imaging Beauty Contests: . ... A data exchange standard for optical (visible/IR) interferometry. ...

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• OptInt PmWiki : Tech Meet 16 | History
• OptInt PmWiki : Recent Changes
• OptInt PmWiki : Tech Meet 16

... Dialog box. ... At this point you should explain briefly what happens when changes are made to the options in the dialog box. For example, the following lines explain what happens with the Sparkle Plug-In when the options have been modified by the user: . Changes to the options effect the current image. ... Changes to the various options do not have an immediate effect on the image. ... Here would be the description of what the first option does and how to make changes with it. ...

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• Zen: sncat README
• Release Notes
• Building and Installing the Distribution

The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...

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• Index of /~bessell/FTP/Tim
• Designated Observatory Registry
• Index of /~bessell/FTP/Spectrophotometry

... This article is part of the LWN Porting Drivers to 2.6 series . This article serves as a sort of final resting place for various small changes in the kernel programming API which do not fit elsewhere. The kdev_t type has been removed from the kernel; everything which works with device numbers should now use the dev_t type. ... Consider using these while fixing your code; the next time the type of i_rdev changes, you will be happier. ... Driver porting: miscellaneous changes, designated inits . ...

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• NEdit.org
• NEdit
• LWN: Changes to the USB driver API for the 2.5 series kernel

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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• IDL programs

DATE DESCRIPTION 1.0 2004-09-14 created from scratch 1.1 2004-09-20 removes entries in JOB_FILE_NAME for $DATE 1.1.1 2004-09-28 bug removed for RBS (2004-09-28) 1.1.2 2004-10-19 bug removed with PLUGIN (2004-10-19); the PLUGIN part is not backwards compatible! 1.2 2004-11-08 modified call of renameProducts 1.2.1 2004 ...

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• list of DFS Department documentation templates
• pet.py: the python plot engine for trendPlotter
• DFS To-Do list rules

Next: The root filesystem Up: Overview of the Directory Previous: Overview of the Directory . This chapter is loosely based on the Linux filesystem standard, FSSTND, version 1.2 (see the bibliography, [ Qui95 ]), which attempts to set a standard for how the directory tree in a Linux system is organized. ... This chapter does not explain all files in detail. ... The major parts are the root, /usr љ , /var љ , and /home љ filesystems (see figure 2.1 ). ... Figure 2.1: Parts of a Unix directory tree. ...

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• Spectrum v1 - Input Syntax
• Index of /highlights/2012/600/relativistic_beam/beam_velocity/standard
• Index of /highlights/2012/600/losscone/losscone_l=3_space/standard

... Up: Data Processing Systems . ... koda, P. & lechta, M. 2003, in ASP Conf. ... The reduction of raw echelle data is a straightforward, although quite complicated task, where the reliability of the final result strongly depends on precise accomplishment of each step. ... We used them for processing of raw CCD echellegram of early-type stars secured with HEROS fiber echelle spectrograph currently installed at Cassegrain focus of Ond ejov observatory 2m telescope. ... The fit is then done order by...

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• Automated Photometric Calibration Software For IRAF
• ADASS 2002 Conference Proceedings
• Bias-Free Parameter Estimation with Few Counts, by Iterative Chi-Squared

Stellarium 0.12.3 . ... Classes . ... ClassљList . ... SatellitesListModel Class Reference . A model encapsulating a satellite list. ... Tell the model that its internal data structure is about to be modified. ... Tell the model that its internal data has been modified. ... The model keeps a pointer to the satellite list, not a copy, so every time that list is modified outside the model (i.e. satellites are added or removed), you need to call beginSatellitesChange() and endSatellitesChange() . ...

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• Stellarium: core/modules/Landscape.hpp Source File

... Denmark: ftp://ftp.dmi.min.dk/pub/Data/WDCC1/indices/kp-ap/ . Germany: ftp://ftp.gfz-potsdam.de/pub/home/obs/kp-ap/ . ... we do not guarantee the correctness of the international sunspot number R; these values are published separately (Brussels, Belgium) The following scientific and format documentation is adapted from ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/kp_ap.fmt The subscript p means planetary and designates a global magnetic activity index. ...

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• Geomagnetic Indices Kp, ap, Ap, Cp and C9
• Geomagnetic Kp Index
• Format Documentation of kpyymm.tab Files

multi-rsh is a perl script which runs the same command on multiple machines, in parallel, and provides reasonable, adjustable timeouts for those machines which fail to answer. Both standard output and standard error are returned through the same channel, and all output has the hostname prepended to each line. Multi-rsh must be run as root (remote jobs can be set to run as any user, see Options below). ... Neither form allows you to directly pass input to the remote programs. ...

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• Changes for release 1.8
• How to get the ApJ look of your paper
• PoA Style Guide