A non-LTE study of neutral and singly-ionized iron line spectra in 1D models of the Sun and selected late-type stars

Inelastic Na+H collision data for non-LTE applications in stellar atmospheres

(2010) P. S. Barklem et al.   ASTRONOMY & ASTROPHYSICS

An absolutely calibratedTeffscale from the infrared flux method

(2010) L. Casagrande et al.   ASTRONOMY & ASTROPHYSICS

Cross sections for low-energy inelastic H+Na collisions

(2010) A. K. Belyaev et al.   PHYSICAL REVIEW A

Solar Chemical Abundances Determined with a CO5BOLD 3D Model Atmosphere

(2010) E. Caffau et al.   SOLAR PHYSICS

The Chemical Composition of the Sun

(2009) Martin Asplund et al.   Annual Review of Astronomy and Astrophysics

Both accurate and precise gf-values for Fe  II lines

(2009) J. Meléndez et al.   ASTRONOMY & ASTROPHYSICS

New extended atomic data in cool star model atmospheres

(2009) F. Grupp et al.   ASTRONOMY & ASTROPHYSICS

Oxygen lines in solar granulation

(2009) T. M. D. Pereira et al.   ASTRONOMY & ASTROPHYSICS

A new implementation of the infrared flux method using the 2MASS catalogue

(2009) J. I. González Hernández et al.   ASTRONOMY & ASTROPHYSICS

The radius and other fundamental parameters of the F9 V star β Virginis

(2009) J. R. North et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Atomic data necessary for the non-LTE analysis of stellar spectra

(2009) Lyudmila Mashonkina   PHYSICA SCRIPTA