tools:aibsim
Differences
This shows you the differences between two versions of the page.
| Both sides previous revisionPrevious revision | |||
| tools:aibsim [2022/01/14 15:33] – cjoblin | tools:aibsim [2022/01/14 15:34] (current) – cjoblin | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| + | ===== AIBsimulator ===== | ||
| + | ==== Detailed description ==== | ||
| - | ====== AIBsimulator ====== | ||
| - | |||
| - | |||
| - | ** Description ** \\ | ||
| Aromatic Infrared Bands (AIBs) observed in astronomical environments are generally attributed to emission from PAHs excited by UV photons from stars. The AIBsimulator is a simulator for a fast calculation of the emission of a given PAH in a given radiation field. The simulator will provide a library of synthetic AIB spectra based on theoretical and experimental molecular data, at the accuracy and sensitivity level required to match coming James Webb Space Telescope observations. | Aromatic Infrared Bands (AIBs) observed in astronomical environments are generally attributed to emission from PAHs excited by UV photons from stars. The AIBsimulator is a simulator for a fast calculation of the emission of a given PAH in a given radiation field. The simulator will provide a library of synthetic AIB spectra based on theoretical and experimental molecular data, at the accuracy and sensitivity level required to match coming James Webb Space Telescope observations. | ||
tools/aibsim.1642174415.txt.gz · Last modified: (external edit)