========================================================================== J/A+AS/113/71 Lines in the infrared solar spectrum (Ramsauer+, 1995) The following files can be converted to FITS (extension .fit .fit.Z .fgz) table1 table3 table2 table4 ========================================================================== Query from: http://vizier.u-strasbg.fr/cgi-bin/VizieR?-source=J/A+AS/113/71 ==========================================================================
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Beginning of ReadMe : J/A+AS/113/71 Lines in the infrared solar spectrum (Ramsauer+, 1995) ================================================================================ Interesting lines in the infrared solar spectrum. II: Unblended lines between 1.0 and 1.8um RAMSAUER J., SOLANKI S.K., BIEMONT E. <Astron. Astrophys. Suppl. Ser. 113, 71 (1995)> =1995A&AS..113...71R (SIMBAD/NED BibCode) ================================================================================ ADC_Keywords: Sun; Spectra, infrared Keywords: lines: profiles - lines: identification - atomic data - Sun: infrared Description: We list 603 spectral lines between 1.0, 1.8um that are judged to be relatively unblended from a visual inspection of spectra of the quiet sun. Much of the atomic data of relevance to studies of solar and stellar magnetism, convection and atmospheric structure are also provided. Particular attention is paid to blending by telluric lines. We determine the level of blending both in the presence and the absence of telluric lines. We also describe how telluric blends may be removed from spectra with high spectral resolution.
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