J/A+AS/129/41 J/A+AS/129/41 Fe I line shifts in the Sun C Allende Prieto R J Garcia Lopez Astron. Astrophys. Suppl. Ser. 129 41 1998 1998A&AS..129...41A J/A+AS/102/269 : Lab. and solar Highly-excited levels of Fe I (Nave+ 1993) J/ApJS/94/221 : New multiplet table for FeI (Nave+, 1994) Atomic physics Sun atlases convection stars: atmospheres Sun: photosphere Central wavelengths measured in the FTS disc-centre spectrum, in the FTS flux spectrum, rest wavelengths, excitation potentials, transition probabilities (log(gfs)) and line equivalent widths at the centre of the disc when available (from Moore et al. 1966 (The Solar Spectrum 2935{AA} to 8770{AA}, National Bureau of Standards Monograph 61) and compiled by A. D. Wittmann, private communication). An asterisk in the equivalent width means that the line has a blend.

Int. Central Waveleng. in the disc-centre spectrum 0.1nm Flux Central Wavelengths in the flux spectrum 0.1nm Lab Central Wavelengths at rest (Nave et al., 1994, Cat. <J/ApJS/94/221>) 0.1nm EP Excitation potential (Thevenin, 1989A&AS...77..137T, 1990A&AS...82..179T) eV log(gf) Transition probabilities (Nave et al. 1994, Cat. <J/ApJS/94/221>) --- EW Equivalent widths (disc centre) mA n_EW Note on line number=1 *: The line is Known to be blended --- Patricia Bauer CDS 1997Sep18Carlos Allende Prieto <callende@ll.iac.es> J_A+AS_129_41.xml