J/A+A/542/A75ivo://CDS.VizieR/J/A+A/542/A75doi:10.26093/cds/vizier.35420075CDSLara N.Gonzalez M.A.Gigosos M.A.2017-06-27T06:37:51Z2012-06-12T10:29:41ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsThe tables contain the area normalized Stark broadened spectral profiles of the HeI 492.2nm line. Doppler effect has not been included in the profiles. The first column of each table is the wavelength detuning, measured in nanometers, from the unperturbed wavelength. The other columns give the spectral profiles for different cases of perturber mass and electron temperature. Each table contains the data for a fixed electron density, ranging from 10^20^m^-3^ to 10^24^m^-3^ in different tables. Data corresponding to four different reduced masses of the emitter perturber pair, {mu}, are given in each table. The values of {mu} given in the tables are {mu}=0.8, 2.0, 4.0 and 10.0, in units of the proton mass. For each case of {mu} the profiles for different electron temperatures are given in different columns. Each table has a head giving the electron density value, and the values of {mu} and temperature corresponding to each column.2012A&A...542A..75Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A75CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/503/293 : Stark broadening of He447.1nm line (Gigosos+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A75https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/542/A75http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/542/A75https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/542/A75https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/542/A75http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/542/A75GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/542/A75/part1Helium I 492.2nm Stark profiles (tables 4-13 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogNeElectron density (G1)log(m**-3)phys.density;phys.electronfloatDlambdaWavelength detuning, from the unperturbed wavelengthnmspect.line.broad.StarkdoubleIDL0.8/40Spectral profile for {mu}=0.8, T=40000K (G2)spect.line.broad.StarkdoubleIDL2/5? Spectral profile for {mu}=2, T=5000K (G2)spect.line.broad.StarkdoublenullableIDL2/10Spectral profile for {mu}=2, T=10000K (G2)spect.line.broad.StarkdoubleIDL2/20Spectral profile for {mu}=2, T=20000K (G2)spect.line.broad.StarkdoubleIDL2/40Spectral profile for {mu}=2, T=40000K (G2)spect.line.broad.StarkdoubleIDL4/5? Spectral profile for {mu}=4, T=5000K (G2)spect.line.broad.StarkdoublenullableIDL4/10Spectral profile for {mu}=4, T=10000K (G2)spect.line.broad.StarkdoubleIDL4/20Spectral profile for {mu}=4, T=20000K (G2)spect.line.broad.StarkdoubleIDL4/40Spectral profile for {mu}=4, T=40000K (G2)spect.line.broad.StarkdoubleIDL10/5? Spectral profile for {mu}=10, T=5000K (G2)spect.line.broad.StarkdoublenullableIDL10/10Spectral profile for {mu}=10, T=10000K (G2)spect.line.broad.StarkdoubleIDL10/20Spectral profile for {mu}=10, T=20000K (G2)spect.line.broad.StarkdoubleIDL10/40Spectral profile for {mu}=10, T=40000K (G2)spect.line.broad.StarkdoubleIDL0.8/5? Spectral profile for {mu}=0.8, T=5000K (G2)spect.line.broad.StarkdoublenullableIDL0.8/10Spectral profile for {mu}=0.8, T=10000K (G2)spect.line.broad.StarkdoubleIDL0.8/20Spectral profile for {mu}=0.8, T=20000K (G2)spect.line.broad.StarkdoubleJ/A+A/542/A75/part2Helium I 492.2nm Stark profiles (tables 14-16 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogNeElectron density (G1)log(m**-3)phys.density;phys.electronfloatDlambdaWavelength detuning, from the unperturbed wavelengthnmspect.line.broad.StarkdoubleIDL0.8/20? Spectral profile for {mu}=0.8, T=20000K (G2)spect.line.broad.StarkdoublenullableIDL0.8/30Spectral profile for {mu}=0.8, T=30000K (G2)spect.line.broad.StarkdoubleIDL0.8/40Spectral profile for {mu}=0.8, T=40000K (G2)spect.line.broad.StarkdoubleIDL2/20? Spectral profile for {mu}=2, T=20000K (G2)spect.line.broad.StarkdoublenullableIDL2/30Spectral profile for {mu}=2, T=30000K (G2)spect.line.broad.StarkdoubleIDL2/40Spectral profile for {mu}=2, T=40000K (G2)spect.line.broad.StarkdoubleIDL4/20? Spectral profile for {mu}=4, T=20000K (G2)spect.line.broad.StarkdoublenullableIDL4/30Spectral profile for {mu}=4, T=30000K (G2)spect.line.broad.StarkdoubleIDL4/40Spectral profile for {mu}=4, T=40000K (G2)spect.line.broad.StarkdoubleIDL10/20? Spectral profile for {mu}=10, T=20000K (G2)spect.line.broad.StarkdoublenullableIDL10/30Spectral profile for {mu}=10, T=30000K (G2)spect.line.broad.StarkdoubleIDL10/40Spectral profile for {mu}=10, T=40000K (G2)spect.line.broad.Starkdouble