https://cosmic-pah.irap.omp.eu/ 2026-04-26T21:59:33+0000 https://cosmic-pah.irap.omp.eu/ https://cosmic-pah.irap.omp.eu/lib/tpl/20conesCosmicPAH/images/favicon.ico text/html 2024-10-28T15:53:50+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=activities&rev=1730130830&do=diff The main part of the activities are related to laboratory astrophysics in order to provide molecular data on polycyclic aromatic hydrocarbons (PAHs) and related species of astrophysical interest, as well as tools to analyze astronomical data. More specifically, we cover the following topics: text/html 2026-01-08T09:04:32+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=databases&rev=1767863072&do=diff DATABASES ✔ AROMA database This is a mass spectrometry database providing information on the molecular content of meteorites, stardust analogues and soot samples. Targeted molecules include polycyclic aromatic hydrocarbons, carbon clusters, fullerenes and various hydrocarbons. text/html 2024-10-28T15:48:57+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=home&rev=1730130537&do=diff COSMIC PAH portal Description Polycyclic aromatic hydrocarbons (PAHs) and related molecular species (e.g. fullerenes) are key species in astrophysical environments. The primary objective of the Cosmic PAH portal is to ease access to databases and tools in order to: text/html 2024-10-28T15:52:18+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=news&rev=1730130738&do=diff - 10/2024: The public version of the CosmicPAH-IRDB database as well as the fitting tool CosmicPAHmfit will be released by the beginning of 2025. - 08/2021: The portal is now publicly available but still in the development phase. New information will be added on a regular basis. text/html 2024-10-28T15:56:15+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=platforms&rev=1730130975&do=diff The experimental information that we gather comes mainly from the following experimental setups: - PIRENEA, 'Piège à Ions pour la Recherche et l’Étude de Nouvelles Espèces Astrochimiques', is a cryogenic Fourier Transform Mass Spectrometer dedicated to astrochemistry. text/html 2024-10-28T16:12:27+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=production&rev=1730131947&do=diff Some recent relevant publications * Infrared Spectroscopy - Chakraborty, S., Mulas, G., Rapacioli, M., Joblin, C., “Modeling Anharmonic Infrared Spectra of Thermally Excited Pyrene (C16H10): the combined view of DFT AnharmonicCaOs and approximate DFT molecular dynamics”, J. Mol. Spec. 378 (2021), 111466, DOI: 10.1016/j.jms.2021.111466 text/html 2024-10-29T07:27:37+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=teams&rev=1730186857&do=diff Scientific team IRAP, Université Toulouse 3 / CNRS / CNES: C. Joblin, K. Demyk, H. Sabbah, O. Berné -- OAC, INAF, Cagliari, Italy: G. Mulas -- LCPQ, Université Toulouse 3 / CNRS: A. Simon, M. Rapacioli -- LCAR, Université Toulouse 3 / CNRS: D. Toublanc text/html 2025-07-17T11:14:21+0000 Anonymous (anonymous@undisclosed.example.com) https://cosmic-pah.irap.omp.eu/doku.php?id=tools&rev=1752750861&do=diff TOOLS * PAHTAT 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 <http://userpages.irap.omp.eu/~cjoblin/PAHTAT/Site/PAHTAT.html> * mMass_updated Description mMass_updated