Commit 23258d4d authored by bourgesl's avatar bourgesl
Browse files

updated EMAA config

parent 39bae9fb
......@@ -3,14 +3,24 @@ bin/*-local.sh
bin/application*.yml
bin/osug-doi.log
bin/*.jar
src/test/resources/staging/
conf/**/xl_convert/
conf/EMAA/sync/conf/
conf/EMAA/sync/vfs/
data/public/*/
data/staging/*/
nbactions.xml
nb-configuration.xml
nbproject/
osug-doi.log
target/
data/public/*/
data/staging/*/
tmp/*/
www/
src/test/resources/staging/
#DOI_suffix;data_access_url
EMAA_CN_20050501_Hyperfine;https://emaa.osug.fr/details/CN/2005-05-01/Hyperfine
EMAA_CH+_20100101_Rotation;https://emaa.osug.fr/details/CH+/2010-01-01/Rotation
EMAA_HCN_20070501_Hyperfine;https://emaa.osug.fr/details/HCN/2007-05-01/Hyperfine
EMAA_HCN_20070501_Rotation;https://emaa.osug.fr/details/HCN/2007-05-01/Rotation
EMAA_H[13C]N_20070501_Hyperfine;https://emaa.osug.fr/details/H[13C]N/2007-05-01/Hyperfine
EMAA_H[13C]N_20141101_Rotation;https://emaa.osug.fr/details/H[13C]N/2014-11-01/Rotation
EMAA_HC[15N]_20171201_Rotation;https://emaa.osug.fr/details/HC[15N]/2017-12-01/Rotation
EMAA_HCO+_20071001_Rotation;https://emaa.osug.fr/details/HCO+/2007-10-01/Rotation
EMAA_ortho-NH3_20100901_Rotation;https://emaa.osug.fr/details/ortho-NH3/2010-09-01/Rotation
EMAA_para-NH3_20100901_Rotation;https://emaa.osug.fr/details/para-NH3/2010-09-01/Rotation
EMAA_ortho-NHD2_20110501_Rotation;https://emaa.osug.fr/details/ortho-NHD2/2011-05-01/Rotation
EMAA_para-NHD2_20110501_Rotation;https://emaa.osug.fr/details/para-NHD2/2011-05-01/Rotation
EMAA_ortho-NHD2_20110501_Hyperfine;https://emaa.osug.fr/details/ortho-NHD2/2011-05-01/Hyperfine
EMAA_para-NHD2_20110501_Hyperfine;https://emaa.osug.fr/details/para-NHD2/2011-05-01/Hyperfine
EMAA_C[15N]_20050501_Hyperfine;https://emaa.osug.fr/details/C[15N]/2005-05-01/Hyperfine
EMAA_[13C]N_20050501_Hyperfine;https://emaa.osug.fr/details/[13C]N/2005-05-01/Hyperfine
EMAA_ortho-H2CO_20170201_Rotation;https://emaa.osug.fr/details/ortho-H2CO/2017-02-01/Rotation
EMAA_para-H2CO_20170201_Rotation;https://emaa.osug.fr/details/para-H2CO/2017-02-01/Rotation
EMAA_ortho-H2CO_20170201_Hyperfine;https://emaa.osug.fr/details/ortho-H2CO/2017-02-01/Hyperfine
EMAA_H2_Rovibration_5e046bb5;https://emaa.osug.fr/details/H2/5e046bb5/Rovibration
EMAA_HeH+_Rotation_2ccc89ee;https://emaa.osug.fr/details/HeH+/2ccc89ee/Rotation
EMAA_CH+_Rotation_47eb31e0;https://emaa.osug.fr/details/CH+/47eb31e0/Rotation
EMAA_[13C]H+_Rotation_4b641db0;https://emaa.osug.fr/details/[13C]H+/4b641db0/Rotation
EMAA_OH_Hyperfine_83ce026b;https://emaa.osug.fr/details/OH/83ce026b/Hyperfine
EMAA_CN_Hyperfine_d9a30dbd;https://emaa.osug.fr/details/CN/d9a30dbd/Hyperfine
EMAA_C[15N]_Hyperfine_a1b197e3;https://emaa.osug.fr/details/C[15N]/a1b197e3/Hyperfine
EMAA_[13C]N_Hyperfine_18ebf4d6;https://emaa.osug.fr/details/[13C]N/18ebf4d6/Hyperfine
EMAA_[36Ar]H+_Rotation_173ef621;https://emaa.osug.fr/details/[36Ar]H+/173ef621/Rotation
EMAA_[38Ar]H+_Rotation_4186bb1b;https://emaa.osug.fr/details/[38Ar]H+/4186bb1b/Rotation
EMAA_[40Ar]H+_Rotation_8c27af9a;https://emaa.osug.fr/details/[40Ar]H+/8c27af9a/Rotation
EMAA_HCN_Hyperfine_73e9d7ef;https://emaa.osug.fr/details/HCN/73e9d7ef/Hyperfine
EMAA_HCN_Rotation_a4d98833;https://emaa.osug.fr/details/HCN/a4d98833/Rotation
EMAA_H[13C]N_Hyperfine_9c162ef8;https://emaa.osug.fr/details/H[13C]N/9c162ef8/Hyperfine
EMAA_H[13C]N_Rotation_e05542a3;https://emaa.osug.fr/details/H[13C]N/e05542a3/Rotation
EMAA_HC[15N]_Rotation_0d5ef109;https://emaa.osug.fr/details/HC[15N]/0d5ef109/Rotation
EMAA_HCO+_Rotation_a861ef7a;https://emaa.osug.fr/details/HCO+/a861ef7a/Rotation
EMAA_H[13C]O+_Rotation_326f961f;https://emaa.osug.fr/details/H[13C]O+/326f961f/Rotation
EMAA_DCO+_Rotation_0e47c7b0;https://emaa.osug.fr/details/DCO+/0e47c7b0/Rotation
EMAA_N2H+_Rotation_5874615e;https://emaa.osug.fr/details/N2H+/5874615e/Rotation
EMAA_N2H+_Hyperfine_e9d3c782;https://emaa.osug.fr/details/N2H+/e9d3c782/Hyperfine
EMAA_N[15N]H+_Hyperfine_4f2d77ce;https://emaa.osug.fr/details/N[15N]H+/4f2d77ce/Hyperfine
EMAA_N2D+_Hyperfine_39813cf9;https://emaa.osug.fr/details/N2D+/39813cf9/Hyperfine
EMAA_para-NH3_Rotation_44e467bd;https://emaa.osug.fr/details/para-NH3/44e467bd/Rotation
EMAA_ortho-NH3_Rotation_7565c572;https://emaa.osug.fr/details/ortho-NH3/7565c572/Rotation
EMAA_para-NH2D_Rotation_bc5106bb;https://emaa.osug.fr/details/para-NH2D/bc5106bb/Rotation
EMAA_ortho-NH2D_Rotation_4f72e13c;https://emaa.osug.fr/details/ortho-NH2D/4f72e13c/Rotation
EMAA_para-NH2D_Hyperfine_f7886cfc;https://emaa.osug.fr/details/para-NH2D/f7886cfc/Hyperfine
EMAA_ortho-NH2D_Hyperfine_0ead32a0;https://emaa.osug.fr/details/ortho-NH2D/0ead32a0/Hyperfine
EMAA_para-[15N]H2D_Rotation_e7374da5;https://emaa.osug.fr/details/para-[15N]H2D/e7374da5/Rotation
EMAA_ortho-[15N]H2D_Rotation_018a251d;https://emaa.osug.fr/details/ortho-[15N]H2D/018a251d/Rotation
EMAA_para-NHD2_Rotation_8fdc530e;https://emaa.osug.fr/details/para-NHD2/8fdc530e/Rotation
EMAA_ortho-NHD2_Rotation_a29be09d;https://emaa.osug.fr/details/ortho-NHD2/a29be09d/Rotation
EMAA_para-NHD2_Hyperfine_3bc12b4c;https://emaa.osug.fr/details/para-NHD2/3bc12b4c/Hyperfine
EMAA_ortho-NHD2_Hyperfine_b4d17e14;https://emaa.osug.fr/details/ortho-NHD2/b4d17e14/Hyperfine
EMAA_para-ND3_Rotation_da7fd1bd;https://emaa.osug.fr/details/para-ND3/da7fd1bd/Rotation
EMAA_meta-ND3_Rotation_4181d476;https://emaa.osug.fr/details/meta-ND3/4181d476/Rotation
EMAA_ortho-ND3_Rotation_84ab10a1;https://emaa.osug.fr/details/ortho-ND3/84ab10a1/Rotation
EMAA_para-ND3_Hyperfine_416718be;https://emaa.osug.fr/details/para-ND3/416718be/Hyperfine
EMAA_meta-ND3_Hyperfine_b3e9eff8;https://emaa.osug.fr/details/meta-ND3/b3e9eff8/Hyperfine
EMAA_ortho-ND3_Hyperfine_56cd60b2;https://emaa.osug.fr/details/ortho-ND3/56cd60b2/Hyperfine
EMAA_para-H2CO_Rotation_0b3b04a6;https://emaa.osug.fr/details/para-H2CO/0b3b04a6/Rotation
EMAA_ortho-H2CO_Rotation_b10653cc;https://emaa.osug.fr/details/ortho-H2CO/b10653cc/Rotation
EMAA_ortho-H2CO_Hyperfine_4628f093;https://emaa.osug.fr/details/ortho-H2CO/4628f093/Hyperfine
EMAA_para-H2[13C]O_Rotation_903f6446;https://emaa.osug.fr/details/para-H2[13C]O/903f6446/Rotation
EMAA_ortho-H2[13C]O_Rotation_e08b64e2;https://emaa.osug.fr/details/ortho-H2[13C]O/e08b64e2/Rotation
EMAA_HC3N_Rotation_4ac6b479;https://emaa.osug.fr/details/HC3N/4ac6b479/Rotation
EMAA_HC3N_Hyperfine_f86a675e;https://emaa.osug.fr/details/HC3N/f86a675e/Hyperfine
EMAA_HNC3_Rotation_96dd18c8;https://emaa.osug.fr/details/HNC3/96dd18c8/Rotation
EMAA_HC3[15N]_Rotation_4dcd1291;https://emaa.osug.fr/details/HC3[15N]/4dcd1291/Rotation
EMAA_C+_Fine_0b142c87;https://emaa.osug.fr/details/C+/0b142c87/Fine
EMAA_O_Fine_5038a7a8;https://emaa.osug.fr/details/O/5038a7a8/Fine
#key;value
identifier:DOI;10.5072/EMAA_C+_Fine_0b142c87
resourceType:Dataset;EMAA File
publicationYear;2010
date:Collected;2010-08-01
title;Fine excitation of C+ by ortho-H2 and para-H2 collisions
description:Abstract;2 fine energy levels / 1 radiative transitions / 1 collisional transitions for para-H2 (10 temperatures in the range 5-500K) / 1 collisional transitions for ortho-H2 (10 temperatures in the range 5-500K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnrasl/slaa192
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C+
subject:main;excitationType Fine
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_CH+_20100101_Rotation
identifier:DOI;10.5072/EMAA_CH+_Rotation_47eb31e0
resourceType:Dataset;EMAA File
publicationYear;2010
date:Collected;2010-01-01
date:Collected;2010-04-01
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 / 91 collisional transitions for H (12 temperatures in the range 10-3000K) / 76 collisional transitions for electron (12 temperatures in the range 10-3000K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stx892
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target CH+
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 electron
subject:var;collider.1 H
subject:var;collider.0 H
subject:var;collider.1 electron
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
......
#key;value
identifier:DOI;10.5072/EMAA_CN_20050501_Hyperfine
identifier:DOI;10.5072/EMAA_CN_Hyperfine_d9a30dbd
resourceType:Dataset;EMAA File
publicationYear;2005
date:Collected;2005-05-01
title;Hyperfine excitation of CN by electron and para-H2 collisions
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)
description:Abstract;121 hyperfine energy levels / 337 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)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stt1544
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2012.20660.x
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target CN
subject:main;excitationType Hyperfine
subject:main;collisional excitation
......
#key;value
identifier:DOI;10.5072/EMAA_C[15N]_20050501_Hyperfine
identifier:DOI;10.5072/EMAA_C[15N]_Hyperfine_a1b197e3
resourceType:Dataset;EMAA File
publicationYear;2005
date:Collected;2005-05-01
......@@ -7,6 +7,7 @@ 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)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stu2231
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C[15N]
subject:main;excitationType Hyperfine
subject:main;collisional excitation
......
#key;value
identifier:DOI;10.5072/EMAA_DCO+_Rotation_0e47c7b0
resourceType:Dataset;EMAA File
publicationYear;2009
date:Collected;2009-09-01
title;Rotation excitation of DCO+ by electron 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) / 132 collisional transitions for electron (12 temperatures in the range 10-1000K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/staa2308
relatedIdentifier:References:DOI;10.1051/0004-6361:200810571
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target DCO+
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 electron
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_H2_Rovibration_5e046bb5
resourceType:Dataset;EMAA File
publicationYear;2019
date:Collected;2019-09-24
title;Rovibration excitation of H2 by H and H+ collisions
description:Abstract;54 rovibration energy levels / 226 radiative transitions / 1431 collisional transitions for H (50 temperatures in the range 100-5000K) / 325 collisional transitions for H+ (26 temperatures in the range 5-3000K)
relatedIdentifier:References:DOI;10.1051/0004-6361/201936249
relatedIdentifier:References:DOI;10.1093/mnras/stv1683
relatedIdentifier:References:DOI;10.1063/5.0039629
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target H2
subject:main;excitationType Rovibration
subject:main;collisional excitation
subject:var;collider.0 H
subject:var;collider.1 H+
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_HC3N_Hyperfine_f86a675e
resourceType:Dataset;EMAA File
publicationYear;2000
date:Collected;2000-10-01
title;Hyperfine excitation of HC3N by ortho-H2 and para-H2 collisions
description:Abstract;61 hyperfine energy levels / 108 radiative transitions / 1810 collisional transitions for para-H2 (10 temperatures in the range 10-100K) / 1810 collisional transitions for ortho-H2 (10 temperatures in the range 10-100K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stw1156
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HC3N
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_HC3N_Rotation_4ac6b479
resourceType:Dataset;EMAA File
publicationYear;2000
date:Collected;2000-10-01
title;Rotation excitation of HC3N by electron, ortho-H2 and para-H2 collisions
description:Abstract;38 rotation energy levels / 37 radiative transitions / 564 collisional transitions for para-H2 (20 temperatures in the range 10-300K) / 564 collisional transitions for ortho-H2 (20 temperatures in the range 10-300K) / 37 collisional transitions for electron (5 temperatures in the range 10-1000K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stw1156
relatedIdentifier:References:DOI;10.1051/0004-6361/201321031
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HC3N
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 electron
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_HC3[15N]_Rotation_4dcd1291
resourceType:Dataset;EMAA File
publicationYear;2004
date:Collected;2004-12-01
title;Rotation excitation of HC3[15N] by electron, ortho-H2 and para-H2 collisions
description:Abstract;38 rotation energy levels / 37 radiative transitions / 564 collisional transitions for para-H2 (20 temperatures in the range 10-300K) / 564 collisional transitions for ortho-H2 (20 temperatures in the range 10-300K) / 37 collisional transitions for electron (5 temperatures in the range 10-1000K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stw1156
relatedIdentifier:References:DOI;10.1051/0004-6361/201321031
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HC3[15N]
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 electron
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
subject:var;circumstellar medium
subject:var;gas
subject:var;microwave spectroscopy
subject:var;infrared spectroscopy
subject:var;rotational excitation
subject:var;rovibrational excitation
subject:var;vibrational excitation
subject:var;electronic excitation
subject:var;collisional rate coefficients
subject:var;fine structure
subject:var;hyperfine structure
format;Radex
publisher;UGA, CNRS, CNRS-INSU, OSUG
creatorName;EMAA
language;en
contributorName:ContactPerson;contact@emaa.osug.fr
contributorName:Distributor;Institut de Planétologie et d'Astrophysique de Grenoble (France) - IPAG
contributorName:Distributor;Observatoire des Sciences de l'Univers de Grenoble (France) - OSUG
contributorName:Distributor;OSUG Data Center (France)
contributorName:HostingInstitution;Université Grenoble Alpes (France) - UGA
contributorName:Sponsor;Programme National de Physique et Chimie du Milieu Interstellaire - INSU/CNRS (PCMI)
contributorName:Sponsor;Institut National des Sciences de l'Univers - INSU
contributorName:DataManager;Raphaël Jacquot;affiliation;IR/OSUG;nameIdentifier:ORCID;0000-0001-6345-2774
contributorName:DataCurator;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:DataCurator;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Alexandre Faure;affiliation;DR/IPAG;nameIdentifier:ORCID;0000-0001-7199-2535
contributorName:ProjectLeader;Aurore Bacmann;affiliation;Astron/IPAG;nameIdentifier:ORCID;0000-0003-1263-4986
contributorName:ProjectLeader;Bernard Boutherin;affiliation;CNRS/IPAG;nameIdentifier:ORCID;0000-0002-0860-0698
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
relatedIdentifier:Cites:URL;https://emaa.osug.fr
#key;value
identifier:DOI;10.5072/EMAA_HCN_20070501_Hyperfine
identifier:DOI;10.5072/EMAA_HCN_Hyperfine_73e9d7ef
resourceType:Dataset;EMAA File
publicationYear;2007
date:Collected;2007-05-01
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)
description:Abstract;25 hyperfine energy levels / 45 radiative transitions / 290 collisional transitions for electron (12 temperatures in the range 10-1000K) / 300 collisional transitions for para-H2 (6 temperatures in the range 5-30K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1051/0004-6361/201832622
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2007.12416.x
relatedIdentifier:References:DOI;10.1051/0004-6361/201832622
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HCN
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 electron
subject:var;collider.0 electron
subject:var;collider.1 para-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
......
#key;value
identifier:DOI;10.5072/EMAA_HCN_20070501_Rotation
identifier:DOI;10.5072/EMAA_HCN_Rotation_a4d98833
resourceType:Dataset;EMAA File
publicationYear;2007
date:Collected;2007-05-01
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)
description:Abstract;22 rotation energy levels / 21 radiative transitions / 36 collisional transitions for electron (12 temperatures in the range 10-1000K) / 231 collisional transitions for He (25 temperatures in the range 5-500K) / 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)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stx422
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2010.16826.x
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2007.12416.x
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2010.16826.x
relatedIdentifier:References:DOI;10.1093/mnras/stx422
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HCN
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 He
subject:var;collider.3 electron
subject:var;collider.0 electron
subject:var;collider.1 He
subject:var;collider.2 para-H2
subject:var;collider.3 ortho-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
......
#key;value
identifier:DOI;10.5072/EMAA_HCO+_20071001_Rotation
identifier:DOI;10.5072/EMAA_HCO+_Rotation_a861ef7a
resourceType:Dataset;EMAA File
publicationYear;2007
date:Collected;2007-10-01
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)
description:Abstract;22 rotation energy levels / 21 radiative transitions / 132 collisional transitions for electron (12 temperatures in the range 10-1000K) / 231 collisional transitions for ortho-H2 (9 temperatures in the range 10-200K) / 231 collisional transitions for para-H2 (9 temperatures in the range 10-200K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/staa2308
relatedIdentifier:References:DOI;10.1051/0004-6361:200810571
relatedIdentifier:References:DOI;10.1093/mnras/staa2308
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HCO+
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.0 electron
subject:var;collider.1 ortho-H2
subject:var;collider.2 electron
subject:var;collider.2 para-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
......
#key;value
identifier:DOI;10.5072/EMAA_HC[15N]_20171201_Rotation
identifier:DOI;10.5072/EMAA_HC[15N]_Rotation_0d5ef109
resourceType:Dataset;EMAA File
publicationYear;2017
date:Collected;2017-12-01
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)
description:Abstract;22 rotation energy levels / 21 radiative transitions / 36 collisional transitions for electron (12 temperatures in the range 10-1000K) / 231 collisional transitions for ortho-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for para-H2 (12 temperatures in the range 5-500K) / 231 collisional transitions for He (25 temperatures in the range 5-500K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2007.12416.x
relatedIdentifier:References:DOI;10.1093/mnras/stx422
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2010.16826.x
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2007.12416.x
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HC[15N]