... 2:2448/1417.12 CREDITS : id - for the game which will last forever (even with Quake coming) DENIS MOELLER/TiC for NWT GREG LEWIS for Dehacked `SKYCLAD' and `DEINE LAKAIEN' without whose music I would not have survived the last week ;) the many people who tested the levels -=[ LEVEL INFORMATION ]=- ------------------------------------------------------------------------------- GAME : DooM II LEVEL #S : Maps 01-09 SINGLE PLAYER : ... The second is TTPDEATH.WAD, two DM levels for DooM...

... Version 2.11.4 - 2004-03-16 (IMS SSC/LUX) -------------------------- - Fixed SPR 3277. ... Version 2.11.1 - 2003-12-19 (IMS SSC/LUX) -------------------------- - Removed unnecessary prints (SPR 3190). ... Version 2.11 - 2003-12-08 (IMS SSC/LUX) -------------------------- - Added 'user' as a possible value of --radiusstyle and an associated parameter --userradius. ... Version 2.3 - 2002-08-12 (IMS SSC/LUX) -------------------------- - Fixed a few bugs to do with the format of text added to the image....

Next: Release of 18 September Up: Old Releases Previous: Version 6.01 Contents . This includes many items that were in the 4 Oct 2004 release made in the AOC. Add the Australian LBA to list of recognized correlators. 30 Sept 2003 RCW. ... Since the compiler is g77 and the underlying operating system is unix, the only changes needed to sched were a couple of library pointers in the makefile. ... Added complete set of 3mm VLBA frequencies to freq.dat. ... 3 Feb 2005 RCW . ... 2004 RCW. ...

Spectral jumps were seen in data taken back in 18mar08 . That data had the rms fixed at 15 and changed pshift as well as fixing pshift and changing the rms. ... Take 6 sets of data. At each set, take data with fftlens = 8192,4096,2048,1024, and 512. fftlengths with even, odd number of butterfly stages will have rms voltage levels that differ by sqrt(2) (since the butterfly down shift changes voltage by factor of 2 and it takes 2 butterfly stages to increase the rms by a factor of 2). ... rms . ...

Some radio clocks and related timekeeping gear have a pulse-per- second (PPS) signal that can be used to discipline the local clock oscillator to a high degree of precision, typically to the order less than 50 us in time and 0.1 PPM in frequency. ... Either way requires conversion of the PPS signal, usually at TTL levels, to RS232 levels, which can be done using a circuit such as described in the Gadget Box PPS Level Converter and CHU Modem page. ...

spaceweb@oulu.fi - last update: 28 May 1995, 0800 UT . Advanced plasma theories are extremely important when one tries to explain, for example, the various waves and instabilities found in the plasma environment. ... In the kinetic theory it is necessary to know only the distribution function for the system of particles. ... The dependence of the distribution function on the independent variables r , v , and t is governed by an equation known as the Boltzmann equation . ... Hot plasma theory . ...

... Context files provide a way to group commands which relate to a specific reduction sequence or application package. For example, the command SET/CONTEXT applic1 will execute the MIDAS procedure applic1.ctx , which would contain all the new command definitions for the application package applic1 as well as any new keyword definitions and default settings. Each enabled context has a corresponding context no. which links new commands to the context in which they were created. ...

A Test of Galaxy Evolutionary Models Via Angular Sizes M. Im S. Casertano, R. E. Griffiths, & K. U. Ratnatunga (The Johns Hopkins University) The relationship between angular size, magnitude, and redshift of faint galaxies is explored as a potential tool to distinguish between different galaxy evolutionary models. ... The mild lumi­ nosity evolution model predicts more luminous galaxies of large angular size at high redshift, as does a standard no evolution model. ... 25) with redshift higher than z ? ...

To change the Scaling Function (how pixel values are binned into color levels): . ... For example, the basic grey-scale color map specifies no intensity for any color at the lowest color level, full intensity for all colors at the highest color level, with the red, green and blue intensities varying linearly for intermediate levels. ... At low bias, low color levels (i.e., low pixel values) will have non-zero intensities, while at high bias only high pixel values will have non-zero intensity. ...

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... Protected Member Functions | ... StelSkyPolygon Class Reference . ... StelSkyPolygon (const QString &url, StelSkyPolygon *parent=NULL) . ... StelSkyPolygon (const QVariantMap &map, StelSkyPolygon *parent) . ... voidљ . ... initFromUrl (const QString &url) . ... initFromQVariantMap (const QVariantMap &map) . ... loadFromQVariantMap (const QVariantMap &map) . ... Definition at line 31 of file StelSkyPolygon.hpp . ... const QString &љ . ...

... Briefly, the count rate at the detector from a source at a redshift z is . ... Another possible way that could lead to arising diverse peculiarities in the - distribution induced by the sources evolution is connected with a possible non-monotonic character of the star formation rate in galaxies. ... The most prominent feature of the obtained theoretical - is a notable sharp increase at low count rates due to evolutionary effects. ...

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... LX600 Series . ... LX200 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... LX200/LX600 Level/North Sensor Array. ...

... The fitting package in STSDAS (Space Telescope Science Data Analysis System) relies on two basic techniques (one linear and one non-linear) for fitting functions to data. ... Results show that both methods may generate biased coefficients (at the ~few percent level), and over or under-estimate error bars (at the ~10 percent level), in particular from low signal-to-noise data. ... Function coefficient errors are computed directly from the covariance matrix. ... Abscissa is signal-to-noise. ...

... Basic Living Allowance (cost living index 100) Team members Categories Type Employment contract 1 (#/year) Type Fixed ­ amount fellowship 2 (#/year) Early stage researchers years experience ) 550 275 Experienced researchers (4­10 years experience ) 000 500 Experienced researchers ( 10 years experience ) 500 250 Team leaders Categories Type Employment contract 1 (#/year) Type Fixed ­ amount 2 Fixed­amount fellowships minimum social security coverage are employment contracts. ...

... This page will present thoroughly checked optical properties in tabular form: . Fixed orientation, single particle . Data tables classified by shapes, m, a/b, orientation, etc. quantities . ... Q ext , Q sca , Q bk , g, some F ij . ... Q ext , Q sca , Q bk , g, ind (TE/TM) . inf.cyl. 20*x, 4*alpha, 10*m . ... fin.cyl. 10*x, 7*L/D, 4*alpha, 5*m . ... 10*x, 9*a/b, 4*alpha, 5*m . ... Chebyshev p. 10*x, 4*n, 6*eps, 4*alpha, 5*m . ... Random orientation, single particle . ...

... The results of long-term monitoring of Gigahertz-Peaked Spectrum sources were found the statistically significant differences (0.05 significance level) in the high-frequency spectral index distribution between subgroups of galaxies and quasars. ... This can mean that the electron energy distribution for GPS galaxies is steeper than for GPS quasars. ... The first area corresponds to GPS-quasars that have statistically larger value of redfhift, second area corresponds to GPS-galaxies. ...

Chair of solid state physics . ... Physics of Semiconductors . ... The electron mean free time. ... The dispersion of electrons and holes. ... The mean values of the velocity and acceleration of the electron, the electrons and holes in a magnetic field (the classical theory), the diamagnetic resonance. ... The energy spectrum of electrons and holes in a magnetic field (quantum theory), the energy spectrum of electrons and holes in a constant electric field (quantum theory), shallow impurity levels. ...

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

... From the uvby photometry and proper motions for about 5500 nearby F stars we have found the following: (i) F stars , taken in narrow ranges of metallicity , show at [fe/H] 0 rather distinct cut-off in their distribution along the Main Sequence (MS) at the blue side, which is suggested to be an indication for the MS turn-off in stellar groups of fixed metallicity ; (ii) the corresponding turn-off age from theoretical isohrones strongly correlates with the ...

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...