J/A+A/561/A21       Line list for solar-type stars           (Sousa+, 2014)

A new procedure to defining a homogenous line list for solar-type stars. Sousa S.G., Santos N.C., Adibekyan V., Delgado-Mena E., Tabernero H.M., Gonzalez Hernandez J.I., Montes D., Smiljanic R., Korn A.J., Bergemann M., Soubiran C., Mikolatis S. <Astron. Astrophys. 561, A21 (2014)> =2014A&A...561A..21S 2014A&A...561A..21S
ADC_Keywords: Stars, fundamental ; Abundances, [Fe/H] ; Atomic physics Keywords: stars: fundamental parameters - stars: abundances - stars: statistics - methods: data analysis Abstract: The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it because of the diversity of the spectroscopic analysis methods used within a survey, such as spectrum synthesis and the equivalent width method. To solve this problem, constraints to the spectroscopic analysis can be set, such as the use of a common line-list. We present a procedure for selecting the best spectral lines from a given input line-list, which then allows us to derive accurate stellar parameters with the equivalent width method. Description: Table 2 presents the atomic data for the final line list derived from the procedure presented in the work. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 24 151 Atomic parameters of the spectral lines -------------------------------------------------------------------------------- See also: J/A+A/458/873 : Metal-rich solar-type stars stellar parameters (Sousa+, 2006) J/A+A/497/563 : Chemical abundances of 451 stars (Neves+, 2009) J/A+A/512/A13 : EW-Teff calibration for solar-type stars (Sousa+, 2010) J/A+A/526/A99 : Metal-poor solar-type stars spectroscopy & masses (Sousa+, 2011) J/A+A/544/A106 : p-mode frequencies of the solar twin 18 Sco (Bazot+, 2012) J/A+A/555/A150 : Cool solar-type stars precise parameters (Tsantaki+, 2013) J/ApJ/720/1592 : Abundances of solar analogs with planets (Hernandez+, 2010) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.2 0.1nm lambda [4808/6610] Central wavelength λ (Å) 9- 12 F4.2 eV EP Excitation potential 14- 19 F6.3 [-] loggf Oscilator strength 21- 24 A4 --- El Element and ionisation (FeI or FeII) -------------------------------------------------------------------------------- Acknowledgements: Sergio G. Sousa, sousasag(at)astro.up.pt
(End) Sergio Sousa [CAUP-Porto, Portugal], Patricia Vannier [CDS] 22-Nov-2013
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line