VizieR Online Data Catalog: The solar gravitational redshift (Gonzalez Hernandez+, 2020)
Abstract
Line data and velocity shifts of the FeI and FeII lines, with laboratory wavelengths, λlab, from Nave et al. (1994ApJS...94..221N, 2013ApJS..204....1N) and excitation potentials, oscillator strengths from the VALD database (Piskunov et al. 1995A&AS..112..525P).
In Table A.1 we provide the mean line core shifts, vcoreobs, measured on the spectral lines from the observed HARPS-LFC spectra of the MOON and computed with respect to the original laboratory wavelengths (Nave et al. 1994ApJS...94..221N, 2013ApJS..204....1N). We also give the recalibrated wavelengths, lambda_nist, computed from recalibrated wavenumber measurements and Ritz wavelengths, lambda_ritz, computed from recalibrated energy levels, with their corresponding wavelengths uncertainties, extracted from the NIST database (Kramida et al. 2019APS..DMPN09004K). In Table A.2, we give the line core shifts measured on the observed spectral lines, vcoreobs_n, estimated using the recalibrated wavelengths, lambda_nist, as reference laboratory wavelengths, the 3D profiles, vcore,3D, and the global line shifts, vfit3Dn, from fitting the observed spectral lines using 3D profiles, and corrected using the recalibrated wavelengths lambda_nist as reference laboratory wavelengths. Wavelengths are given in Angstroms, wavelength uncertainties in miliAngstroems, excitation potentials in eV, equivalent widths (EW) in miliAngstroems, and velocity shifts in m/s. (2 data files).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- September 2020
- DOI:
- 10.26093/cds/vizier.36430146
- Bibcode:
- 2020yCat..36430146G
- Keywords:
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- Solar system;
- Sun;
- Equivalent widths;
- Line Profiles