title;Rotation excitation of CH+ by H and electron collisions
description:Abstract;"14 rotation energy levels / 13 radiative transitions / 76 collisional transitions for electron (12 temperatures in the range 10-3000K) / 91 collisional transitions for H (12 temperatures in the range 10-3000K) / 14 formation transitions for C+ + H2(v=2,J2=0) (12 temperatures in the range 10-3000K) / 14 destruction transitions for electron (12 temperatures in the range 10-3000K) / 14 destruction transitions for H (12 temperatures in the range 10-3000K)"
description:Abstract;14 rotation energy levels / 13 radiative transitions / 76 collisional transitions for electron (12 temperatures in the range 10-3000K) / 91 collisional transitions for H (12 temperatures in the range 10-3000K) / 14 formation transitions for C+ + H2(v=2,J2=0) (12 temperatures in the range 10-3000K) / 14 destruction transitions for electron (12 temperatures in the range 10-3000K) / 14 destruction transitions for H (12 temperatures in the range 10-3000K)
contributorName:Funder;"Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), UGA - CNRS"
contributorName:Funder;"Centre National de la Recherche Scientifique (France) - CNRS, Institut de Sciences de l'Univers (France) - INSU"
contributorName:Funder;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Funder;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (http://osug.emaa.fr and https://osug.fr/doi/10.26302/EMAA). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Hyperfine excitation of CN by electron and para-H2 collisions
description:Abstract;73 hyperfine energy levels / 218 radiative transitions / 2267 collisional transitions for electron (19 temperatures in the range 10-1000K) / 2628 collisional transitions for para-H2 (20 temperatures in the range 5-100K)
description:Abstract;121 hyperfine energy levels / 218 radiative transitions / 2267 collisional transitions for electron (19 temperatures in the range 10-1000K) / 2628 collisional transitions for para-H2 (20 temperatures in the range 5-100K)
contributorName:Funder;"Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), UGA - CNRS"
contributorName:Funder;"Centre National de la Recherche Scientifique (France) - CNRS, Institut de Sciences de l'Univers (France) - INSU"
contributorName:Funder;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Funder;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (http://osug.emaa.fr and https://osug.fr/doi/10.26302/EMAA). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Hyperfine excitation of C[15N] by para-H2 collisions
description:Abstract;34 hyperfine energy levels / 76 radiative transitions / 560 collisional transitions for para-H2 (25 temperatures in the range 5-150K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title:AlternativeTitle;Excitation of Molecules and Atoms for Astrophysics
title:Subtitle;
publicationYear;2021
date:Created;2020-10-19
date:Updated;2021-01-01
description:Abstract;The EMAA database contains collisional excitation rates data calculated for astrophysically-relevant atomic and molecular systems for a range of temperatures. It covers rotational, vibrational, rovibrational and reactive excitation. It provides different levels of data taking into account rotational levels, and fine and hyperfine levels, when relevant. The collisional data are distributed combined with the spectroscopic data (energy levels, radiative transitions) in the form of a RADEX file.
contributorName:ResearchGroup;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
contributorName:ResearchGroup;University College London (UK) - UCL
contributorName:ResearchGroup;Institut de Physique de Rennes, Université de Rennes 1 (France) - IPR
contributorName:ResearchGroup;Laboratoire Ondes et Milieux Complexes, Université du Havre (France) - LOMC
contributorName:ResearchGroup;The Cologne Database for Molecular Spectroscopy (Germany) - CDMS
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Hyperfine excitation of HCN by electron and para-H2 collisions
description:Abstract;25 hyperfine energy levels / 45 radiative transitions / 300 collisional transitions for para-H2 (6 temperatures in the range 5-30K) / 290 collisional transitions for electron (12 temperatures in the range 10-1000K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Rotation excitation of HCN by He, electron, ortho-H2 and para-H2 collisions
description:Abstract;22 rotation energy levels / 21 radiative transitions / 231 collisional transitions for para-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for ortho-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for He (25 temperatures in the range 5-500K) / 36 collisional transitions for electron (12 temperatures in the range 10-1000K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Rotation excitation of HCO+ by electron, ortho-H2 and para-H2 collisions
description:Abstract;22 rotation energy levels / 21 radiative transitions / 231 collisional transitions for para-H2 (9 temperatures in the range 10-200K) / 231 collisional transitions for ortho-H2 (9 temperatures in the range 10-200K) / 132 collisional transitions for electron (12 temperatures in the range 10-1000K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Rotation excitation of HC[15N] by He, electron, ortho-H2 and para-H2 collisions
description:Abstract;22 rotation energy levels / 21 radiative transitions / 231 collisional transitions for para-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for ortho-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for He (25 temperatures in the range 5-500K) / 36 collisional transitions for electron (12 temperatures in the range 10-1000K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
title;Hyperfine excitation of H[13C]N by electron and para-H2 collisions
description:Abstract;16 hyperfine energy levels / 27 radiative transitions / 120 collisional transitions for para-H2 (6 temperatures in the range 5-30K) / 115 collisional transitions for electron (12 temperatures in the range 10-1000K)
funderName;Institut de Planétologie et d’Astrophysique de Grenoble (France) - IPAG
funderName;Institut de Sciences de l'Univers (France) - INSU
funderName;Centre National de la Recherche Scientifique (France) - CNRS
funderName;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
funderName;Université Grenoble Alpes (France) - UGA
funderName;European Commission
rights;"Please acknowledge the use of EMAA Database by citing the original articles in which the data were published (BibTeX format available), and adding the following sentence in your publication:
This research has made use of spectroscopic and collisional data from the EMAA database (https://emaa.osug.fr). EMAA is supported by the Observatoire des Sciences de l'Univers de Grenoble (OSUG)"
rights;Licence: CC BY 4.0;rightsURI;https://creativecommons.org/licenses/by/4.0
rights;Data access and use are ruled by the EMAA data policy.;rightsURI;https://emaa.osug.fr
