Next: Generation from Ground Calibration Up: EMOS_REDIST Previous: EMOS_REDIST Contents . The redistribution parameters for the MOS cameras. ... Attributes: . None. Columns: . ... The central CCD of each MOS detector has developed a patch where the energy resolution is worse than the average. ... The energy bounds of PHA channels. ... The energy bounds of the PI channels, used to determine the equivalent energies of spectral channels in the redistribution matrix construction. ...

Еще в разделе: (Показать все результаты (>11359) - xmm.vilspa.esa.es/ )

• Generation from Ground Calibration Data
• SAS package check list
• Errors

The binary distribution kits for livedata and gridzilla should include everything required to run them on compatible Linux, Solaris, and/or Darwin systems. ... VERSION date this release was generated. livedata_root.tar.bz2 (required) contains top-level files. livedata_linux.tar.bz2 contains linux binaries. livedata_linux64.tar.bz2 binaries for 64-bit linux systems. livedata_darwin.tar.bz2 contains Darwin (Mac OS X) Intel binaries. livedata_sun4sol.tar.bz2 contains Sun Solaris binaries. ...

Еще в разделе: (Показать все результаты (>25638) - www.atnf.csiro.au/ )

• Tools - Random numbers
• casacore: casa::RNG Class Reference
• casacore: scimath/Fitting/FittingProxy.h File Reference

.

Еще в разделе: (Показать все результаты (>351) - zebu.uoregon.edu/ )

• Evidence for Dark Matter
• Energy From the Wind

... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

Еще в разделе: (Показать все результаты (>8399) - www.sai.msu.su/ )

• Monitoring Options
• Hints and Kinks
• APOD: November 27, 1995 - Too Close to a Black Hole

Next: The OaPd System for Web Access to Large Astronomical Catalogues . ... The IUE Newly Extracted Spectra System (INES), a complete astronomical archive and its associated data distribution system, was developed with the goal of delivering IUE data to the scientific community in a simple and efficient form. ... Taking advantage of the expertise gained with ULDA and the distribution system for IUE Final Archive data, the ESA-IUE Observatory began to develop INES in early 1997. ... 2000). ...

Еще в разделе: (Показать все результаты (>1869) - www.adass.org/ )

• Starlink's Software Distribution System
• The IUE Archive at Villafranca
• INES Version 3.0: Functionalities and Contents

Next: Simulations Up: Maximum Likelihood Estimation of Previous: Introduction . The properties of an ensemble of faint galaxies can be defined by the distribution of the parameters of the models that best fit each individual object. ... The model also includes instrumental parameters, such as the sky background (estimated locally) and amplitude of the noise. ... The probability of the observed value is then computed for each pixel using the adopted error distribution. ...

Еще в разделе: (Показать все результаты (>20173) - www.stsci.edu/ )

• THE BRUZUAL- CHARLOT ATLAS
• CALOBS
• Infrared Spectral Energy Distributions of Nearby Galaxies

Distribution of the analyzed SEPs with different >100 MeV proton fluxes ( J 100 ) at the microwave flux density plane ' S 9 vs. ... 1) General correspondence takes place between intensities of microwave bursts and proton fluxes - J 100 increases when S 9 and S 15 rise. ... 3) Powerful microwave bursts ( S 9 , S 15 >3000-10000 sfu ) with hard radio spectra ( S 9 < S 15 ) correspond to majority of powerful proton fluxes ( J 100 >10 pfu ). ...

Еще в разделе: (Показать все результаты (>311) - www.izmiran.rssi.ru/ )

• Ionospheric plasma-wave interaction

Monte Carlo Methods for Including Calibration Uncertainties in Model Fitting Analyses Jeremy J. Drakea , Peter Ratzlaffa , Vinay Kashyapa , Richard Edgara , Rima Izemb , Diab Jeriusa , Herman ... University, Cambridge, MA 02138 MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA 02139 b c SUMMARY · Instrument response uncertainties almost universally ignored in astrophysical X-ray ... Limiting accuracy of Chandra ACIS reached in spectra with 10 4 counts. ...

Еще в разделе: (Показать все результаты (>2430) - hea-www.harvard.edu/ )

• The AstroStat Slog Pareto distribution
• The AstroStat Slog Blog Archive Redistribution
• *ftpplot* - Distribution of FFT coefficient values

Introduction This catalogue contains mainly the atomic data needed in the astrophysical investigations of low-density plasma. It is a revised and extended version of the "Catalogue of Atomic Data for the Rarefied Astrophysical Plasma" (Golovatyj et al. ... Low-density plasma. ... In the present study we represent only the atomic data for computation of sp ectra of low-density astrophysical plasma (most known kinds of it are gaseous nebulae), their thermal and ionization structure. ...

Еще в разделе: (Показать все результаты (>256) - www.astro.spbu.ru/ )

• Hydrogenated amorphous carbon
• Examples of data contained in the JPDOC

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

Еще в разделе: (Показать все результаты (>564) - xray.sai.msu.ru/ )

• Dependence on the Scenario Parameters and Initial Distributions
• Number of accreting X-ray binaries of selected types
• Test of the Initial Mass-Ratio Distribution

Next: Jets Up: M.D. Smith Previous: High-Mass Star Formation Contents . By contrast, stars of low mass like our Sun are formed within molecular clumps. Michael Smith has been investigating the clumps and the individual cores they contain within one nearby cloud near the star Rho Ophiuchi. With Stanke (Hawaii), Khanzadyan (Heidelberg) and Gredel (Calar Alto), he has determined the masses of over 100 protostellar cores and compared this to the distribution of masses for stars. ...

Еще в разделе: (Показать все результаты (>1898) - star.arm.ac.uk/ )

• Galactic distribution and absolute magnitudes
• Armagh Observatory
• Armagh Observatory: Chris Winter [ lte-codes ]

Programs to generate color spectra ================================== These programs were developed to produce realistic color spectra from digital data. ... The distribution here contains the original source code for colorspec and solar in C, and a version of solar written in Fortran. ... It will produce a color spectrum of any digital spectrum. ... The 800x50 image solarflux.ppm was generated by colorspec and the file fluxatlas.dat, a reformatted NSO Solar Flux Atlas in the data directory. ...

Еще в разделе: (Показать все результаты (>461) - www.astro.louisville.edu/ )

• Distribution (ImageJ API)

Below is a list of all of the modules that come as part of the Apache distribution. ... mod_setenvif Apache 1.3 and up . ... mod_unique_id Apache 1.3 and up . ... Determining document types using file extensions . ... mod_rewrite Apache 1.2 and up . ... User authentication using text files . ... User authentication using DBM files . ... User authentication using Berkeley DB files . mod_auth_anon Apache 1.1 and up . ... User-configurable logging replacement for mod_log_common . ...

Еще в разделе: (Показать все результаты (>107) - neptun.sai.msu.ru/ )

... Using the central limit theorem, the total noise can be approximated by a Gaussian or normal distribution which has the frequency function : . ... where is the mean intensity of the source. ... In the statistical analysis of the probability distribution of data several estimators based on moments are used. ... For a normal distribution, these moments are and while for a Poisson distribution are and . Besides these moments other estimators are used to describe a distribution e.g. median and mode . ...

Еще в разделе: (Показать все результаты (>1905) - www.sao.ru/ )

• Direct electron imaging-model
• Corrections to the probability distribution
• Table Formats

. On the plot the days are shown along X axis and Universal time along Y axis. The regions in the first satellite positions are shown by the regions symbols and colour. The time intervals of the conjugation between considered couple of the satellites during day are shown as a 'wide boxes'. The corresponding numerical file contains the coordinates of both satellites during magnetic conjugations. Dr. Victoria Prokhorenko . Modified 17 June 1999

Еще в разделе: (Показать все результаты (>980) - www.cosmos.ru/ )

• Nonequilibrium distributions
• Space Research Institute (IKI) Seminar
• The summary plot of time distribution of the multisatellites magnetic

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

Еще в разделе: (Показать все результаты (>73) - ip.rsu.ru/ )

• Vladimir Marsakov Abstracts

... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...

Еще в разделе: (Показать все результаты (>266) - www.gao.spb.ru/ )

• http://www.gao.spb.ru/english/as/j2014/presentations/kudryashova.pdf
• http://www.gao.spb.ru/english/personal/malkin/publ/zm08g.pdf
• Страница Е.В.Милецкого / Page of Eugen Miletsky

T his page contains synthetic Hertzsprung-Russell Diagrams (HRDs) for a simulated Star Forming Region, assuming different scenarios and timescales for the history of star formation. ... In the paper we only presented the best fits to the HRD of the CMa R1 Star Forming Region. ... Download movie (1.90 MB) . Scenario II: Constant rate of star formation during a time interval delta t . delta t = 0.1 Myr . ... Scenario IV: Linearly decreasing rate of star formation during a time interval delta t . ...

Еще в разделе: (Показать все результаты (>11767) - www.eso.org/ )

• Marina Rejkuba's Web Site
• ESO - Thesis Topic: Next generation Fornax Cluster surveys
• ESO - ESO-MIDAS Releases and Distribution

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

Еще в разделе: (Показать все результаты (>35) - sed.sao.ru/ )

• Description of SED models

... The essence of the solution is to generate a virtual PC on your desktop PC and install an old Linux distribution, circa 2006, in that. ... There are two major free virtual machines available for Linux, these are VirtualBox and KVM. ... Boot the virtual machine. ... Install a Linux 2.6 kernel if it isn't installed by default (you'll need to reboot the virtual machine after this step): . ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIDelayLine/TrolleySoftware) ...

Еще в разделе: (Показать все результаты (>1510) - www.mrao.cam.ac.uk/ )

• OptInt PmWiki : Trolley Software | History
• Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA
• DUST: Dust::CarbSD Class Reference