User Tools

Site Tools


tools

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
tools [2022/01/14 15:30]
cjoblin
tools [2022/01/14 15:55] (current)
pah [* Qchitool]
Line 16: Line 16:
 ===== *  Qchitool ===== ===== *  Qchitool =====
 ** Description ** \\ ** Description ** \\
-QChITool is a web application for easy extraction of information from the log files of some quantum chemistry calculations,​ and import in the theoretical PAH database. [[tools:pahtat|More]]\\+QChITool is a web application for easy extraction of information from the log files of some quantum chemistry calculations,​ and import in the theoretical PAH database. [[tools:qchitool|More]]\\
 ** Tool access **  ** Tool access ** 
 [[https://​qchitool-pah.oa-cagliari.inaf.it]] ​ (restricted use of the tool to add data to the PAH database) [[https://​qchitool-pah.oa-cagliari.inaf.it]] ​ (restricted use of the tool to add data to the PAH database)
Line 22: Line 22:
 ===== *  cosmicPAHmfit ===== ===== *  cosmicPAHmfit =====
 ** Description ** \\ ** Description ** \\
-cosmicPAHmfit ​is a python fitting tool. It performs ​a multi-component fit of the selected spectral feature using pseudo-Voigt functions (linear combination of a Gaussian curve and of Lorentzian curve modified by an asymmetry factor). It computes the area-weighed peak position and width of the feature. It has a graphical interface to select the spectral feature of interest as well as the number of components to be included in the fit. [[tools:mmass_u|More]]\\+cosmicPAHmfit ​provides ​a multi-component ​spectral ​fit and a graphical interface to derive ​area-weighed peak position and width of selected infrared features. [[tools:mfit|More]]\\
 ** Tool access **  ** Tool access ** 
 //planned in 2022// //planned in 2022//
Line 28: Line 28:
 ===== *  AIBsimulator ===== ===== *  AIBsimulator =====
 ** Description ** \\ ** 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 +The AIBsimulator is a simulator for a fast calculation of the emission of a given PAH in a given radiation field. The synthetic spectra ​are based on theoretical and experimental molecular data. [[tools:​aibsim|More]]\\ ​
  
  
tools.1642174229.txt.gz · Last modified: 2022/01/14 15:30 by cjoblin