... I decided that I don't need another script to synch duplicates between ldap and Active Directory after looking at the records on both. ... I got a connector for Active Directory set up in Zope, got the COI over https problem resolved with Alex, and worked on fixing up the broken ldap reports. ... I updated the manager selection code in the photo gallery so it will work with active directory and started developing a fix for the problem with LDAPSearch that prevented the delivery. ... Archive for 2014...

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• Archive for February
• Archive for May
• Changing Programs & Resolving Problems

... Posts tagged ?change point problem? ... X-ray summer school is on going. ... Tags: ARCH , Bayesian Block , challenges , change point problem , GARCH , light curves , summer school , X-ray . ... 4 Comments . ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...

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• The AstroStat Slog Blog Archive Change Point Problem
• Comments on: Change Point Problem By: vlk By: vlk By: hlee By: vlk
• Apple Scrolling - Which Way is Up?

... The path of the dome will now follow a different track in focus. ... The dome was set to 19.6 degrees. ... Focus curves taken with sbn (.ps) ( more info ) show the offset (in inches) from the the platform reference position (1256.22 feet). ... Moving the ref ch position from 8.84 to 18 degrees will raise the platform corner by .7 inches.7 platform inches is 1.7*.7 is 1.2 tie down inches of stroke .7 platform inches is 3.5 degrees F. The path length will increase by .1 in (za=2) to .8 inches (za=20)....

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• td12_16jan08
• a2584
• telescope cycles by year

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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... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...

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• Phil Plait's Bad Astronomy: Mad Science
• Phil Plait's Bad Astronomy: Bitesize Astronomy

... Radio telescope interferometers exhibit chromatic aberration effects. ... Reduction packages such as AIPS and AIPS++ will produce a beam pattern image for each frequency channel. This allows these packages to compute a spectral-line cube which has a pixel size (cellsize) independent of frequency. ... Because of this, Miriad produces cubes where the pixel size changes with frequency. ... The correct approach is to produce a cube in Miriad which does not have a variable pixel size. ...

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• difx:troubleshooting [ATNF VLBI Wiki]
• Release of 18 September 2003.
• Archive of VLBI Observations Majordomo List

... Version 1.23.4 - 2001-05-01 ------------------------------- + ( src / omflatfield_mod.f90 ) array INDEX removed temporarily until ts size can be properly determined (fixes SPR -2360) Version 1.23.3 - 2001-03-29 ------------------------------- + (config/omflatfield.par) Parameter ppsflatset mode changed to optional ( SPR -2307) Version 1.23.2 - 2001-03-19 ------------------------------- + ( src / omflatfield_mod.f90 ) Further checks ... Added checks on input file types. ...

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• http://xmm.vilspa.esa.es/sas/5.4.1/doc/omfchain/ChangeLog
• http://xmm.vilspa.esa.es/sas/6.5.0/doc/ommodmap/ChangeLog
• http://xmm.vilspa.esa.es/sas/7.0.0/doc/omgsource/ChangeLog

... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...

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• Additional problems at the transition
• XFree86/OS2 project
• Appendix B: Changes from CSS1

... Example: Moving to a new database. ... Load the dump file into a new database. createdb ts_db_b; psql ts_db_b < ts_db_a.sql; . ... The oids pointing to tsearch functions are correct in database ts_db_a but do not exist in database ts_db_b. Try installing tsearch2.sql into the new database ts_db_b before loading dump file ts_db_a.sql. dropdb ts_db_b; createdb ts_db_b; psql ts_db_b < /usr/local/pgsql/share/contrib/tsearch2.sql; psql ts_db_b < ts_db_a.sql; . ... Does tsearch work though? ...

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• Zen: Search for: "count problem"
• Zen: Changes
• Zen: History of count problem

... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... Each such choice is known as a frame of reference . Some possible frames are -- the interior of the airliner, . ...

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• Parallax
• Principles of the Magnetic Trapping of Particles
• Space weather [Oulu]

.

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• Energy Storage
• Moving Towards Life
• Astronomy 123 Spring 1996

... 22.Reference Frames . ... To derive the motion of a penny dropped inside an airliner moving at 600 miles/hr (about 1000 km/hr)--should we calculate it with respect to the interior of the airliner, or with respect to the ground? ... And if a similar penny is let go inside an orbiting spaceship--should its motion be calculated relative to the interior of the spaceship, or relative to the Earth outside? ... How do observations differ in the two frames--the airliner cabin and the Earth? ...

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• Lagrangian Points
• Motion in a Circle
• Principles of the Magnetic Trapping of Particles

... 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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• LWN: Driver porting: Timekeeping changes
• LWN: Changes to the USB driver API for the 2.5 series kernel
• LWN: Driver porting: dealing with interrupts

... With the Moon's terminator moving almost 10 mph (16 km/h) across its equator, how long would it take for an observer using binoculars to notice a change in lunar features? ... The lunar terminator, the sunset/sunrise line that sweeps across the Moon s surface as the Moon orbits Earth, travels at a rate of 9.6 mph (15.4 km/h) along our satellite s equator. ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ...

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• With the Moon gradually moving away from Earth, what will happen to people and
• Problems posed by massive stars | Astronomy.com
• In what direction and at what speed is the solar system moving through the

Modules | ... Apache HTTP Server Version 2.4 . ... In order to assist folks upgrading, we maintain a document describing information critical to existing Apache HTTP Server users. ... This document describes changes in server behavior that might require you to change your configuration or how you use the server in order to continue using 2.4 as you are currently using 2.2. ... Many third-party modules designed for version 2.2 will otherwise work unchanged with the Apache HTTP Server version 2.4. ...

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• Educator's Guide to Moon Phases
• mod_charset_lite - Apache HTTP Server
• Problem Getting the Kernel small enough

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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• ESO-MIDAS Problem report Form
• Errors in Tired Light Cosmology
• Removal of particle hits

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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• 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-4.2.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/xmccd-4.2.1/libcfitsio/libcfitsio-3.340/Makefile

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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• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• ADASS 2003 Conference Proceedings
• An IRAF-Independent Interface for Spatial-Region Descriptors

... Bojan Nikolic web pages (r. 329) . ALMA . ... AATM is a re-packaging of the version of ATM as used by the ALMA online calibration software ?TelCal?. ... The main reason for AATM is to bring the version of ATM used by ALMA to an as wide an audience as possible. ... This version of AATM therefore corresponds exactly to version on ATM-0_3_0 branch of the CVS, and will (I believe) be the same as what is used in ALMA 7.1. ... Computing dispersive atmospheric delay with AATM . ... ATM and AATM . ...

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• OptInt PmWiki : MROIDelayLine / Trolley Software
• OptInt PmWiki : MROIFastTipTilt / Tech Meet 16
• OptInt PmWiki : Tech Meet 16 | History

Changing a World . What did the students learn from all this? ... The students found this unsatisfactory -- some of them would not be able to fit another astronomy class into their schedules, but they wanted to know about our planetary neighbors, and this project gave them the opportunity to find out without spending valuable class time on the subject. ... The students also learned to learn for themselves, perhaps one of the most important milestones during formal education. ...

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• ASP: An Ancient Universe - Changes in the Solar System
• ASP: Book Review
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