What is WITS?The Web Infrared Tool Shed is a collection of web pages and programs ("tool boxes") for the analysis of astronomical objects that emit primarily in the wavelength range 2 µm to 1 mm. The goal of WITS is to provide the astronomical community with a uniform set of models over a large parameter space of source properties. WITS currently consists of:
- PDR Toolbox (PDRT) - plots of physical parameters (surface temperature, gas density, incident radiation field) as a function of observables (spectral line intensities and ratios) for standard model photodissociation regions (PDRs); and interactive fitting of observables to models.
April, 2007
- Faster web server.
- H2 line intensity maps
- Dust InfraRed Toolbox (DIRT) - a comprehensive Java applet for modelling astrophysical process in circumstellar dust shells around young and evolved stars.
And don't forget our motto:
"Reliable Astrophysics at Everyday Low, Low Prices!"®
The development of these tools was supported by NASA Applied Information Systems Research Program grant NAG 5-10751 under the direction of Drs. Mark Wolfire, Marc Pound, Peter Teuben, Lee Mundy, and Steve Lord. Previous support was from NASA Astrophysics Data Program grant NAG 5-675.
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