... If your workstation can run any of the standard data reduction systems, it can run Draco. ... The Draco source files and executable will require about 20Mb of disk space. Draco is written in Common Lisp, specifically Allegro Common Lisp 4.2 beta by Franz, Inc. The distribution includes an executable image, so you don't need a Lisp system at your site. We chose Lisp since it offered a powerful, high-level development environment that is available on many different machines. ...

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• Software Conditions
• STScI Electronic Leave System

... 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. ...

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Next: Calibration with the ISOPHOT Interactive Analysis (PIA) . ... ISO P HOT I nteractive A nalysis, PIA , is a scientific and calibration data analysis tool for ISOPHOT data reduction. The PIA software was designed both as a tool for use by the instrument team for calibration of the PHT instrument during and after the ISO mission, and as an interactive tool for ISOPHOT data analysis by general observers. ... PIA is entirely based on the Interactive Data Language IDL (IDL92). ...

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• Distributed Software for Observations in the Near Infrared
• WIP -- An Interactive Graphics Software Package
• Starlink's Software Distribution System

... Posts tagged ?Pareto distribution? ... Posted by hlee . ... Tags: Classification , covariance , FARIMA , Fisher information , GL , GRB , Levy , light curve , limb darkening , ML , Pareto distribution , quasars , solar flare , standard candle , tessellation , time series , VO , void . ... 1 Comment . ... ArXiv] Pareto Distribution? ... 4 Comments . ... From arxiv/astro-ph, arXiv:0706.2590v1 Extreme Value Theory and the Solar Cycle by Ramos, A. This paper might drag a large attention from CHASC...

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• The AstroStat Slog Blog Archive [ArXiv] Pareto Distribution
• The AstroStat Slog VO
• The AstroStat Slog mixture

... The MIDAS system is built along lines which should allow easy integration of complex analysis algorithms as well as allowing greater flexibility in interactive use and in the creation of user specific procedures from the basic building blocks. ... The present version which became available in 1984 follows a similar philosophy in its application program interfaces, but has been expanded to the new Standard Interfaces which have a broader base than previously. ...

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• Distribution Policy
• Noise distributions
• Developer Documentation for Apache 2.0 - Apache HTTP Server

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. ...

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• SciSim 4.0 Installation
• SAS Developer's Documentation
• External SAS packages

XmTel is intended for interactive remote telescope operation. It is not primarily a robotic telescope control system, but rather a "hands-on" remote telescope interface with a server that permits remote operation and robotic control by making use of INDI for command line, scripted, and and interactive operation. ... We have adapted this telescope to the Galil controllers, and the Galil driver included here will operate a wide class of telescopes with that modification. ...

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• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.2/TELESCOPES
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.0/README
• http://www.astro.louisville.edu/software/xmtel/archive/xmtel-5.1/TELESCOPES

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 ). ...

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DEVCON for LAN Systems!! ... PSP LAN Systems develops products that provide network operating system services (such as file, print, transaction, security and directory) for multiple operating systems (OS/2, DOS, Windows and AIX). ... PSP LAN Systems has identified an API (or development tools) strategy that provides an application development environment with industry standard APIs for application portability and object frameworks to assist developers with code reuse. ...

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• XFree86/OS2 Available Ported Software
• XFree86/OS2 Available Ported Software - Games
• Energy distribution

... After a brief leave in Bangalore to work on astronomy (and holiday in Nepal), Dave will be continuing in management positions within the ATNF. ... We have also hosted an observing project visit from a contingent of ATNF and CTIP vacation scholars, who observed h Carina with the new 12-mm system (see article elsewhere in this issue), observed new HIPASS galaxies, and studied interference from microwave ovens. ... Currently we are testing this system with a single antenna. ...

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• The IR Spectral Energy Distribution
• Finding the Bivariate Brightness Distribution of galaxies from an HI selected
• WCSLIB: FITS-WCS and related software

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. ...

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• Description of SED models

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. ...