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Commit 7a121def authored by bourgesl's avatar bourgesl
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updated EMAA database (2023.12.07)

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with 1084 additions and 66 deletions
#DOI_suffix;data_access_url
EMAA_C-plus_Fine_0b142c87;https://emaa.osug.fr/details/C+/0b142c87/Fine
EMAA_O_Fine_5038a7a8;https://emaa.osug.fr/details/O/5038a7a8/Fine
EMAA_H2_Rovibration_5e046bb5;https://emaa.osug.fr/details/H2/5e046bb5/Rovibration
EMAA_HeH-plus_Rotation_2ccc89ee;https://emaa.osug.fr/details/HeH+/2ccc89ee/Rotation
EMAA_CH-plus_Rotation_47eb31e0;https://emaa.osug.fr/details/CH+/47eb31e0/Rotation
EMAA_(13C)H-plus_Rotation_4b641db0;https://emaa.osug.fr/details/[13C]H+/4b641db0/Rotation
EMAA_OH-plus_Hyperfine_1d30b9b4;https://emaa.osug.fr/details/OH+/1d30b9b4/Hyperfine
EMAA_OH_Fine_2e526008;https://emaa.osug.fr/details/OH/2e526008/Fine
EMAA_OH_Hyperfine_83ce026b;https://emaa.osug.fr/details/OH/83ce026b/Hyperfine
EMAA_HC3N_Hyperfine_f86a675e;https://emaa.osug.fr/details/HC3N/f86a675e/Hyperfine
EMAA_e-CH3(18O)H_Rotation_da227d5c;https://emaa.osug.fr/details/E-CH3[18O]H/da227d5c/Rotation
EMAA_(18O)H-plus_Hyperfine_1c669710;https://emaa.osug.fr/details/[18O]H+/1c669710/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_para-(15N)H2D_Rotation_e7374da5;https://emaa.osug.fr/details/para-[15N]H2D/e7374da5/Rotation
EMAA_ortho-H2O_Rotation_0d2ed16f;https://emaa.osug.fr/details/ortho-H2O/0d2ed16f/Rotation
EMAA_(13C)N_Hyperfine_18ebf4d6;https://emaa.osug.fr/details/[13C]N/18ebf4d6/Hyperfine
EMAA_HDS_Rotation_d3b568cc;https://emaa.osug.fr/details/HDS/d3b568cc/Rotation
EMAA_CH2NH_Hyperfine_9027c066;https://emaa.osug.fr/details/CH2NH/9027c066/Hyperfine
EMAA_ortho-H2(34S)_Rotation_2f37d6f0;https://emaa.osug.fr/details/ortho-H2[34S]/2f37d6f0/Rotation
EMAA_H(13C)O-plus_Rotation_326f961f;https://emaa.osug.fr/details/H[13C]O+/326f961f/Rotation
EMAA_C2H_Hyperfine_e0d01d58;https://emaa.osug.fr/details/C2H/e0d01d58/Hyperfine
EMAA_ortho-H2CO_Hyperfine_21889b23;https://emaa.osug.fr/details/ortho-H2CO/21889b23/Hyperfine
EMAA_(13C)(17O)_Hyperfine_164ecb70;https://emaa.osug.fr/details/[13C][17O]/164ecb70/Hyperfine
EMAA_SO_Fine_e3d652e7;https://emaa.osug.fr/details/SO/e3d652e7/Fine
EMAA_para-C3H2_Rotation_bcdd4e50;https://emaa.osug.fr/details/para-c-C3H2/bcdd4e50/Rotation
EMAA_ortho-D2S_Rotation_a6fd14e0;https://emaa.osug.fr/details/ortho-D2S/a6fd14e0/Rotation
EMAA_(40Ar)H-plus_Rotation_8c27af9a;https://emaa.osug.fr/details/[40Ar]H+/8c27af9a/Rotation
EMAA_para-(13C)C2H2_Rotation_62296b37;https://emaa.osug.fr/details/para-c-[13C]C2H2/62296b37/Rotation
EMAA_DCN_Hyperfine_0b4f7ab6;https://emaa.osug.fr/details/DCN/0b4f7ab6/Hyperfine
EMAA_DCO-plus_Rotation_0e47c7b0;https://emaa.osug.fr/details/DCO+/0e47c7b0/Rotation
EMAA_HCO-plus_Rotation_a861ef7a;https://emaa.osug.fr/details/HCO+/a861ef7a/Rotation
EMAA_a-CH3OH_Rotation_aa19a665;https://emaa.osug.fr/details/A-CH3OH/aa19a665/Rotation
EMAA_C(15N)_Hyperfine_a1b197e3;https://emaa.osug.fr/details/C[15N]/a1b197e3/Hyperfine
EMAA_e-(13C)H3OH_Rotation_26e2c2d2;https://emaa.osug.fr/details/E-[13C]H3OH/26e2c2d2/Rotation
EMAA_ortho-H2CO_Rotation_b10653cc;https://emaa.osug.fr/details/ortho-H2CO/b10653cc/Rotation
EMAA_para-H2O_Rotation_18d206fb;https://emaa.osug.fr/details/para-H2O/18d206fb/Rotation
EMAA_ortho-(13C)C2H2_Rotation_a4239764;https://emaa.osug.fr/details/ortho-c-[13C]C2H2/a4239764/Rotation
EMAA_(13C)O_Rotation_922483ff;https://emaa.osug.fr/details/[13C]O/922483ff/Rotation
EMAA_CS_Rotation_d0c6405a;https://emaa.osug.fr/details/CS/d0c6405a/Rotation
EMAA_DCN_Rotation_0d1b1e03;https://emaa.osug.fr/details/DCN/0d1b1e03/Rotation
EMAA_(13C)H-plus_Rotation_4b641db0;https://emaa.osug.fr/details/[13C]H+/4b641db0/Rotation
EMAA_(13C)CH_Hyperfine_b78c5723;https://emaa.osug.fr/details/[13C]CH/b78c5723/Hyperfine
EMAA_CO_Rotation_e6542418;https://emaa.osug.fr/details/CO/e6542418/Rotation
EMAA_para-H2(34S)_Rotation_52d67276;https://emaa.osug.fr/details/para-H2[34S]/52d67276/Rotation
EMAA_ortho-H2C(18O)_Rotation_7963f75b;https://emaa.osug.fr/details/ortho-H2C[18O]/7963f75b/Rotation
EMAA_ortho-H2(13C)O_Rotation_e08b64e2;https://emaa.osug.fr/details/ortho-H2[13C]O/e08b64e2/Rotation
EMAA_CH-plus_Rotation_47eb31e0;https://emaa.osug.fr/details/CH+/47eb31e0/Rotation
EMAA_HC3N_Rotation_4ac6b479;https://emaa.osug.fr/details/HC3N/4ac6b479/Rotation
EMAA_SO2_Rotation_cdf6a320;https://emaa.osug.fr/details/SO2/cdf6a320/Rotation
EMAA_HNC3_Rotation_96dd18c8;https://emaa.osug.fr/details/HNC3/96dd18c8/Rotation
EMAA_(38Ar)H-plus_Rotation_4186bb1b;https://emaa.osug.fr/details/[38Ar]H+/4186bb1b/Rotation
EMAA_para-D2S_Rotation_1e071ded;https://emaa.osug.fr/details/para-D2S/1e071ded/Rotation
EMAA_CH2NH_Rotation_6a3d5ab2;https://emaa.osug.fr/details/CH2NH/6a3d5ab2/Rotation
EMAA_(13C)O_Rotation_30dfe01d;https://emaa.osug.fr/details/[13C]O/30dfe01d/Rotation
EMAA_HNC_Rotation_20269bc3;https://emaa.osug.fr/details/HNC/20269bc3/Rotation
EMAA_para-H2CO_Rotation_0b3b04a6;https://emaa.osug.fr/details/para-H2CO/0b3b04a6/Rotation
EMAA_C(18O)_Rotation_a61158dd;https://emaa.osug.fr/details/C[18O]/a61158dd/Rotation
EMAA_HeH-plus_Rotation_2ccc89ee;https://emaa.osug.fr/details/HeH+/2ccc89ee/Rotation
EMAA_N(15N)H-plus_Hyperfine_4f2d77ce;https://emaa.osug.fr/details/N[15N]H+/4f2d77ce/Hyperfine
EMAA_N2H-plus_Hyperfine_e9d3c782;https://emaa.osug.fr/details/N2H+/e9d3c782/Hyperfine
EMAA_H(13C)N_Rotation_e05542a3;https://emaa.osug.fr/details/H[13C]N/e05542a3/Rotation
EMAA_OH_Fine_73f2c321;https://emaa.osug.fr/details/OH/73f2c321/Fine
EMAA_para-NH3_Rotation_44e467bd;https://emaa.osug.fr/details/para-NH3/44e467bd/Rotation
EMAA_ortho-NH3_Rotation-hot_2c68197a;https://emaa.osug.fr/details/ortho-NH3/2c68197a/Rotation-hot
EMAA_DNC_Rotation_65a4bdbe;https://emaa.osug.fr/details/DNC/65a4bdbe/Rotation
EMAA_O_Fine_5038a7a8;https://emaa.osug.fr/details/O/5038a7a8/Fine
EMAA_C-plus_Fine_0b142c87;https://emaa.osug.fr/details/C+/0b142c87/Fine
EMAA_para-NH3_Rotation-hot_9da5b297;https://emaa.osug.fr/details/para-NH3/9da5b297/Rotation-hot
EMAA_ortho-NH2D_Hyperfine_0ead32a0;https://emaa.osug.fr/details/ortho-NH2D/0ead32a0/Hyperfine
EMAA_SH-plus_Hyperfine_da4d4f7a;https://emaa.osug.fr/details/SH+/da4d4f7a/Hyperfine
EMAA_(36Ar)H-plus_Rotation_173ef621;https://emaa.osug.fr/details/[36Ar]H+/173ef621/Rotation
EMAA_(38Ar)H-plus_Rotation_4186bb1b;https://emaa.osug.fr/details/[38Ar]H+/4186bb1b/Rotation
EMAA_(40Ar)H-plus_Rotation_8c27af9a;https://emaa.osug.fr/details/[40Ar]H+/8c27af9a/Rotation
EMAA_SiO_Rotation_424f5a89;https://emaa.osug.fr/details/SiO/424f5a89/Rotation
EMAA_CS_Rotation_d0c6405a;https://emaa.osug.fr/details/CS/d0c6405a/Rotation
EMAA_para-NH2_Hyperfine_0d542831;https://emaa.osug.fr/details/para-NH2/0d542831/Hyperfine
EMAA_ortho-C3H2_Rotation_caf26a12;https://emaa.osug.fr/details/ortho-c-C3H2/caf26a12/Rotation
EMAA_a-CH3(18O)H_Rotation_c65648f1;https://emaa.osug.fr/details/A-CH3[18O]H/c65648f1/Rotation
EMAA_N2D-plus_Hyperfine_39813cf9;https://emaa.osug.fr/details/N2D+/39813cf9/Hyperfine
EMAA_para-H2S_Rotation_f76b8b70;https://emaa.osug.fr/details/para-H2S/f76b8b70/Rotation
EMAA_para-ND3_Rotation_da7fd1bd;https://emaa.osug.fr/details/para-ND3/da7fd1bd/Rotation
EMAA_e-CH3OH_Rotation_b00fa82a;https://emaa.osug.fr/details/E-CH3OH/b00fa82a/Rotation
EMAA_para-NHD2_Hyperfine_3bc12b4c;https://emaa.osug.fr/details/para-NHD2/3bc12b4c/Hyperfine
EMAA_HD(34S)_Rotation_8a51ba80;https://emaa.osug.fr/details/HD[34S]/8a51ba80/Rotation
EMAA_C(18O)_Rotation_1175b5dd;https://emaa.osug.fr/details/C[18O]/1175b5dd/Rotation
EMAA_ortho-(15N)H2D_Rotation_018a251d;https://emaa.osug.fr/details/ortho-[15N]H2D/018a251d/Rotation
EMAA_ortho-NHD2_Hyperfine_b4d17e14;https://emaa.osug.fr/details/ortho-NHD2/b4d17e14/Hyperfine
EMAA_ortho-NH3_Hyperfine_22b1dfb7;https://emaa.osug.fr/details/ortho-NH3/22b1dfb7/Hyperfine
EMAA_ortho-NH2_Hyperfine_6c2e5783;https://emaa.osug.fr/details/ortho-NH2/6c2e5783/Hyperfine
EMAA_para-H2O_Rotation_18d206fb;https://emaa.osug.fr/details/para-H2O/18d206fb/Rotation
EMAA_ortho-H2O_Rotation_0d2ed16f;https://emaa.osug.fr/details/ortho-H2O/0d2ed16f/Rotation
EMAA_HCN_Rotation_a4d98833;https://emaa.osug.fr/details/HCN/a4d98833/Rotation
EMAA_HC(15N)_Rotation_0d5ef109;https://emaa.osug.fr/details/HC[15N]/0d5ef109/Rotation
EMAA_para-H2(18O)_Rotation_4ebe92f7;https://emaa.osug.fr/details/para-H2[18O]/4ebe92f7/Rotation
EMAA_C(13C)H_Hyperfine_2bb79b69;https://emaa.osug.fr/details/C[13C]H/2bb79b69/Hyperfine
EMAA_ortho-ND3_Hyperfine_56cd60b2;https://emaa.osug.fr/details/ortho-ND3/56cd60b2/Hyperfine
EMAA_para-NH2D_Hyperfine_f7886cfc;https://emaa.osug.fr/details/para-NH2D/f7886cfc/Hyperfine
EMAA_meta-ND3_Rotation_4181d476;https://emaa.osug.fr/details/meta-ND3/4181d476/Rotation
EMAA_H2_Rovibration_5e046bb5;https://emaa.osug.fr/details/H2/5e046bb5/Rovibration
EMAA_HD_Rovibration_805a7aa5;https://emaa.osug.fr/details/HD/805a7aa5/Rovibration
EMAA_ortho-NH3_Rotation_331d9739;https://emaa.osug.fr/details/ortho-NH3/331d9739/Rotation
EMAA_ortho-NHD2_Rotation_a29be09d;https://emaa.osug.fr/details/ortho-NHD2/a29be09d/Rotation
EMAA_ortho-H2(18O)_Rotation_1ee1c3c9;https://emaa.osug.fr/details/ortho-H2[18O]/1ee1c3c9/Rotation
EMAA_HCN_Rotation_a4d98833;https://emaa.osug.fr/details/HCN/a4d98833/Rotation
EMAA_para-H2C(18O)_Rotation_8f130c2d;https://emaa.osug.fr/details/para-H2C[18O]/8f130c2d/Rotation
EMAA_HCN_Hyperfine_73e9d7ef;https://emaa.osug.fr/details/HCN/73e9d7ef/Hyperfine
EMAA_HNC_Rotation_20269bc3;https://emaa.osug.fr/details/HNC/20269bc3/Rotation
EMAA_HC(15N)_Rotation_0d5ef109;https://emaa.osug.fr/details/HC[15N]/0d5ef109/Rotation
EMAA_H(13C)N_Rotation_e05542a3;https://emaa.osug.fr/details/H[13C]N/e05542a3/Rotation
EMAA_para-H2(13C)O_Rotation_903f6446;https://emaa.osug.fr/details/para-H2[13C]O/903f6446/Rotation
EMAA_a-(13C)H3OH_Rotation_6b79e149;https://emaa.osug.fr/details/A-[13C]H3OH/6b79e149/Rotation
EMAA_meta-ND3_Hyperfine_b3e9eff8;https://emaa.osug.fr/details/meta-ND3/b3e9eff8/Hyperfine
EMAA_para-NH2D_Rotation_bc5106bb;https://emaa.osug.fr/details/para-NH2D/bc5106bb/Rotation
EMAA_ortho-ND3_Rotation_84ab10a1;https://emaa.osug.fr/details/ortho-ND3/84ab10a1/Rotation
EMAA_OH_Hyperfine_72d6c3c5;https://emaa.osug.fr/details/OH/72d6c3c5/Hyperfine
EMAA_ortho-H2S_Rotation_3f29e6c3;https://emaa.osug.fr/details/ortho-H2S/3f29e6c3/Rotation
EMAA_HC3(15N)_Rotation_4dcd1291;https://emaa.osug.fr/details/HC3[15N]/4dcd1291/Rotation
EMAA_CN_Hyperfine_d9a30dbd;https://emaa.osug.fr/details/CN/d9a30dbd/Hyperfine
EMAA_para-NH3_Hyperfine_1be97812;https://emaa.osug.fr/details/para-NH3/1be97812/Hyperfine
EMAA_H(13C)N_Hyperfine_9c162ef8;https://emaa.osug.fr/details/H[13C]N/9c162ef8/Hyperfine
EMAA_DCN_Rotation_0d1b1e03;https://emaa.osug.fr/details/DCN/0d1b1e03/Rotation
EMAA_DCN_Hyperfine_0b4f7ab6;https://emaa.osug.fr/details/DCN/0b4f7ab6/Hyperfine
EMAA_DNC_Rotation_65a4bdbe;https://emaa.osug.fr/details/DNC/65a4bdbe/Rotation
EMAA_HCO-plus_Rotation_a861ef7a;https://emaa.osug.fr/details/HCO+/a861ef7a/Rotation
EMAA_H(13C)O-plus_Rotation_326f961f;https://emaa.osug.fr/details/H[13C]O+/326f961f/Rotation
EMAA_DCO-plus_Rotation_0e47c7b0;https://emaa.osug.fr/details/DCO+/0e47c7b0/Rotation
EMAA_N2H-plus_Rotation_5874615e;https://emaa.osug.fr/details/N2H+/5874615e/Rotation
EMAA_N2H-plus_Hyperfine_e9d3c782;https://emaa.osug.fr/details/N2H+/e9d3c782/Hyperfine
EMAA_N(15N)H-plus_Hyperfine_4f2d77ce;https://emaa.osug.fr/details/N[15N]H+/4f2d77ce/Hyperfine
EMAA_N2D-plus_Hyperfine_39813cf9;https://emaa.osug.fr/details/N2D+/39813cf9/Hyperfine
EMAA_SO2_Rotation_cdf6a320;https://emaa.osug.fr/details/SO2/cdf6a320/Rotation
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_SiO_Rotation_424f5a89;https://emaa.osug.fr/details/SiO/424f5a89/Rotation
EMAA_(36Ar)H-plus_Rotation_173ef621;https://emaa.osug.fr/details/[36Ar]H+/173ef621/Rotation
EMAA_CO_Rotation_3d0e1a5c;https://emaa.osug.fr/details/CO/3d0e1a5c/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-NH2_Hyperfine_0d542831;https://emaa.osug.fr/details/para-NH2/0d542831/Hyperfine
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_para-H2C(18O)_Rotation_8f130c2d;https://emaa.osug.fr/details/para-H2C[18O]/8f130c2d/Rotation
EMAA_ortho-H2C(18O)_Rotation_7963f75b;https://emaa.osug.fr/details/ortho-H2C[18O]/7963f75b/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(17O)_Hyperfine_0ecc62b5;https://emaa.osug.fr/details/C[17O]/0ecc62b5/Hyperfine
EMAA_OH-plus_Hyperfine_1d30b9b4;https://emaa.osug.fr/details/OH+/1d30b9b4/Hyperfine
EMAA_para-NHD2_Rotation_8fdc530e;https://emaa.osug.fr/details/para-NHD2/8fdc530e/Rotation
#key;value
identifier:DOI;10.5072/EMAA_(13C)(17O)_Hyperfine_164ecb70
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-21
title;Hyperfine excitation of [13C][17O] by ortho-H2 and para-H2 collisions
description:Abstract;75 hyperfine energy levels / 176 radiative transitions / 2775 collisional transitions for para-H2 (11 temperatures in the range 5-400K) / 2775 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stac1430
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target [13C][17O]
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_(13C)CH_Hyperfine_b78c5723
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-13
title;Hyperfine excitation of [13C]CH by para-H2 collisions
description:Abstract;98 hyperfine energy levels / 128 radiative transitions / 4752 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/stad1646
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target [13C]CH
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-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
......@@ -4,7 +4,7 @@ resourceType:Dataset;EMAA File
publicationYear;2021
date:Collected;2021-09-18
title;Rotation excitation of [13C]H+ by H and electron collisions
description:Abstract;12 rotation energy levels / 11 radiative transitions / 66 collisional transitions for H (12 temperatures in the range 10-3000K) / 60 collisional transitions for electron (12 temperatures in the range 10-3000K)
description:Abstract;12 rotation energy levels / 11 radiative transitions / 91 collisional transitions for H (12 temperatures in the range 10-3000K) / 60 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:References:DOI;10.1093/mnras/stv2429
......
......@@ -4,17 +4,17 @@ resourceType:Dataset;EMAA File
publicationYear;2021
date:Collected;2021-12-21
title;Rotation excitation of [13C]O by ortho-H2O, para-H2 and para-H2O collisions
description:Abstract;11 rotation energy levels / 10 radiative transitions / 10 collisional transitions for para-H2 (9 temperatures in the range 2-40K) / 55 collisional transitions for para-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for ortho-H2O (20 temperatures in the range 5-100K)
description:Abstract;14 rotation energy levels / 13 radiative transitions / 55 collisional transitions for para-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for ortho-H2O (20 temperatures in the range 5-100K) / 10 collisional transitions for para-H2 (9 temperatures in the range 2-40K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1088/2041-8205/799/1/L9
relatedIdentifier:References:DOI;10.1093/mnras/staa242
relatedIdentifier:References:DOI;10.1088/2041-8205/799/1/L9
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target [13C]O
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 para-H2O
subject:var;collider.2 ortho-H2O
subject:var;collider.0 para-H2O
subject:var;collider.1 ortho-H2O
subject:var;collider.2 para-H2
subject:var;astrophysics
subject:var;interstellar medium
subject:var;comets
......
#key;value
identifier:DOI;10.5072/EMAA_(13C)O_Rotation_922483ff
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-06-30
title;Rotation excitation of [13C]O by CO, ortho-H2, ortho-H2O, para-H2 and para-H2O collisions
description:Abstract;14 rotation energy levels / 13 radiative transitions / 91 collisional transitions for para-H2 (11 temperatures in the range 5-400K) / 91 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K) / 55 collisional transitions for para-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for ortho-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for CO (15 temperatures in the range 10-150K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stac1430
relatedIdentifier:References:DOI;10.1093/mnras/staa242
relatedIdentifier:References:DOI;10.1093/mnras/stad268
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target [13C]O
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 para-H2O
subject:var;collider.3 ortho-H2O
subject:var;collider.4 CO
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_C(13C)H_Hyperfine_2bb79b69
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-13
title;Hyperfine excitation of C[13C]H by para-H2 collisions
description:Abstract;98 hyperfine energy levels / 119 radiative transitions / 4752 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/stad1646
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C[13C]H
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-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_C(17O)_Hyperfine_0ecc62b5
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-03
title;Hyperfine excitation of C[17O] by ortho-H2 and para-H2 collisions
description:Abstract;75 hyperfine energy levels / 176 radiative transitions / 2775 collisional transitions for para-H2 (11 temperatures in the range 5-400K) / 2775 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stac1430
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C[17O]
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_C(18O)_Rotation_1175b5dd
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-03
title;Rotation excitation of C[18O] by CO, ortho-H2, ortho-H2O, para-H2 and para-H2O collisions
description:Abstract;11 rotation energy levels / 10 radiative transitions / 55 collisional transitions for para-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for ortho-H2O (20 temperatures in the range 5-100K) / 91 collisional transitions for para-H2 (11 temperatures in the range 5-400K) / 91 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K) / 55 collisional transitions for CO (15 temperatures in the range 10-150K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/staa242
relatedIdentifier:References:DOI;10.1093/mnras/stac1430
relatedIdentifier:References:DOI;10.1093/mnras/stad268
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C[18O]
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2O
subject:var;collider.1 ortho-H2O
subject:var;collider.2 para-H2
subject:var;collider.3 ortho-H2
subject:var;collider.4 CO
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_C2H_Hyperfine_e0d01d58
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-13
title;Hyperfine excitation of C2H by ortho-H2 and para-H2 collisions
description:Abstract;38 hyperfine energy levels / 94 radiative transitions / 702 collisional transitions for para-H2 (30 temperatures in the range 10-300K) / 703 collisional transitions for ortho-H2 (30 temperatures in the range 10-300K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/sty1568
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target C2H
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_CH2NH_Hyperfine_9027c066
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-02-28
title;Hyperfine excitation of CH2NH by para-H2 collisions
description:Abstract;43 hyperfine energy levels / 180 radiative transitions / 861 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;10.1021/acs.jpclett.8b01431
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target CH2NH
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-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_CH2NH_Rotation_6a3d5ab2
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-02-28
title;Rotation excitation of CH2NH by para-H2 collisions
description:Abstract;15 rotation energy levels / 31 radiative transitions / 105 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;10.1021/acs.jpclett.8b01431
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target CH2NH
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-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_CO_Rotation_3d0e1a5c
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-03-25
title;Rotation excitation of CO by CO, ortho-H2, ortho-H2O, para-H2 and para-H2O collisions
description:Abstract;14 rotation energy levels / 13 radiative transitions / 55 collisional transitions for para-H2O (20 temperatures in the range 5-100K) / 55 collisional transitions for ortho-H2O (20 temperatures in the range 5-100K) / 91 collisional transitions for para-H2 (11 temperatures in the range 5-400K) / 91 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K) / 55 collisional transitions for CO (15 temperatures in the range 10-150K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/staa242
relatedIdentifier:References:DOI;10.1093/mnras/stac1430
relatedIdentifier:References:DOI;10.1093/mnras/stad268
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target CO
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 para-H2O
subject:var;collider.1 ortho-H2O
subject:var;collider.2 para-H2
subject:var;collider.3 ortho-H2
subject:var;collider.4 CO
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_HD(34S)_Rotation_8a51ba80
resourceType:Dataset;EMAA File
publicationYear;2022
date:Collected;2022-05-12
title;Rotation excitation of HD[34S] by ortho-H2 and para-H2 collisions
description:Abstract;36 rotation energy levels / 151 radiative transitions / 630 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K) / 630 collisional transitions for para-H2 (11 temperatures in the range 5-400K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stac216
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HD[34S]
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 ortho-H2
subject:var;collider.1 para-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_HD_Rovibration_805a7aa5
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-03
title;Rovibration excitation of HD by H and H+ collisions
description:Abstract;52 rovibration energy levels / 368 radiative transitions / 1326 collisional transitions for H (15 temperatures in the range 5-5000K) / 171 collisional transitions for H+ (25 temperatures in the range 5-3005K)
relatedIdentifier:References:DOI;10.1016/j.jqsrt.2021.107949
relatedIdentifier:References:DOI;10.1093/mnras/stac911
relatedIdentifier:References:DOI;10.1063/5.0128598
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HD
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_HDS_Rotation_d3b568cc
resourceType:Dataset;EMAA File
publicationYear;2022
date:Collected;2022-05-12
title;Rotation excitation of HDS by ortho-H2 and para-H2 collisions
description:Abstract;36 rotation energy levels / 155 radiative transitions / 630 collisional transitions for ortho-H2 (11 temperatures in the range 5-400K) / 630 collisional transitions for para-H2 (11 temperatures in the range 5-400K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1093/mnras/stac216
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target HDS
subject:main;excitationType Rotation
subject:main;collisional excitation
subject:var;collider.0 ortho-H2
subject:var;collider.1 para-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_OH_Fine_73f2c321
resourceType:Dataset;EMAA File
publicationYear;2022
date:Collected;2022-12-15
title;Fine excitation of OH by H, ortho-H2 and para-H2 collisions
description:Abstract;20 fine energy levels / 50 radiative transitions / 190 collisional transitions for para-H2 (7 temperatures in the range 10-150K) / 190 collisional transitions for ortho-H2 (7 temperatures in the range 10-150K) / 66 collisional transitions for H (11 temperatures in the range 5-500K)
relatedIdentifier:References:DOI;10.1016/j.jqsrt.2019.106687
relatedIdentifier:References:DOI;10.1093/mnras/stx1968
relatedIdentifier:References:DOI;10.1063/5.0110724
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target OH
subject:main;excitationType Fine
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 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_OH_Hyperfine_72d6c3c5
resourceType:Dataset;EMAA File
publicationYear;2022
date:Collected;2022-12-15
title;Hyperfine excitation of OH by H, ortho-H2 and para-H2 collisions
description:Abstract;24 hyperfine energy levels / 95 radiative transitions / 264 collisional transitions for para-H2 (7 temperatures in the range 10-150K) / 264 collisional transitions for ortho-H2 (7 temperatures in the range 10-150K) / 276 collisional transitions for H (11 temperatures in the range 5-500K)
relatedIdentifier:References:DOI;10.1016/S0022-4073(98)00091-0
relatedIdentifier:References:DOI;10.1093/mnras/staa530
relatedIdentifier:References:DOI;10.1093/mnras/stac3458
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target OH
subject:main;excitationType Hyperfine
subject:main;collisional excitation
subject:var;collider.0 para-H2
subject:var;collider.1 ortho-H2
subject:var;collider.2 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_SO_Fine_e3d652e7
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-10-14
title;Fine excitation of SO by para-H2 collisions
description:Abstract;31 fine energy levels / 101 radiative transitions / 465 collisional transitions for para-H2 (10 temperatures in the range 5-50K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1063/1.2723733
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target SO
subject:main;excitationType Fine
subject:main;collisional excitation
subject:var;collider.0 para-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_a-(13C)H3OH_Rotation_6b79e149
resourceType:Dataset;EMAA File
publicationYear;2023
date:Collected;2023-07-10
title;Rotation excitation of A-[13C]H3OH by ortho-H2 and para-H2 collisions
description:Abstract;19 rotation energy levels / 40 radiative transitions / 165 collisional transitions for para-H2 (20 temperatures in the range 10-200K) / 171 collisional transitions for ortho-H2 (20 temperatures in the range 10-200K)
relatedIdentifier:References:DOI;10.1016/j.molstruc.2005.01.027
relatedIdentifier:References:DOI;10.1111/j.1365-2966.2010.16671.x
relatedIdentifier:IsPartOf:DOI;10.5072/EMAA
subject:main;target A-[13C]H3OH
subject:main;excitationType Rotation
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
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