Differences

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

--- tools [2022/01/14 15:30] – cjoblin
+++ tools [2026/11/06 16:39] (current) – pah
@@ Line 2: / Line 2: @@
 ===== * PAHTAT =====
-** Description ** \\
+**Description** \\
 The PAHTAT tool aims to analyze astronomical mid-infrared spectra containing PAH emission. It uses spectral templates that were derived from observations. [[https://doi.org/10.1051/0004-6361/201015915]]\\
-** Tool access **
+**Tool access**
 [[http://userpages.irap.omp.eu/~cjoblin/PAHTAT/Site/PAHTAT.html]]
 ===== *  mMass_updated =====
-** Description ** \\
+**Description** \\
 **mMass_updated** is a modified version of[[http://www.mmass.org/|mMass|]] with new functionalities such as double bond equivalent calculation and separation into families of compounds (compatible with 64-bit MacOS). [[tools:mmass_u|More]]\\
-** Tool access **
+**Tool access**
 //planned in 2022//
 ===== *  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)
 ===== *  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 a 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. \\
-** Tool access **
+**Tool access**
-//planned in 2022//
+//available// \\
+--> Additional information on description and access is available [[tools:mfit|Here]]
 ===== *  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]]\\