[PDF][PDF] Handbook of basic atomic spectroscopic data

JE Sansonetti, WC Martin - Journal of physical and chemical reference data, 2005 - nist.gov
This handbook is designed to provide a selection of the most important and frequently used
atomic spectroscopic data in an easily accessible compact format. The compilation includes …

Atomic Data for Resonance Absorption Lines. III. WavelengthsLongward of the Lyman Limit for the Elements Hydrogen toGallium

DC Morton - The Astrophysical Journal Supplement Series, 2003 - iopscience.iop.org
This compilation revises the 1991 listing of atomic data for the lighter elements from
hydrogen to gallium. The tabulation emphasizes resonance lines, ie, lines whose lower level …

The extremely metal-poor, neutron capture-rich star CS 22892-052: a comprehensive abundance analysis

C Sneden, JJ Cowan, JE Lawler, II Ivans… - The Astrophysical …, 2003 - iopscience.iop.org
High-resolution spectra obtained with three ground-based facilities and the Hubble Space
Telescope (HST) have been combined to produce a new abundance analysis of CS 22892 …

The impact of recent advances in laboratory astrophysics on our understanding of the cosmos

DW Savin, NS Brickhouse, JJ Cowan… - Reports on Progress …, 2012 - iopscience.iop.org
An emerging theme in modern astrophysics is the connection between astronomical
observations and the underlying physical phenomena that drive our cosmos. Both the …

Recent advances in the study of lanthanide atoms and ions

E Biémont, P Quinet - Physica Scripta, 2003 - iopscience.iop.org
We present an overview of the recent developments concerning the spectroscopic
properties of lanthanide atoms and ions (Z= 57–71). This review is focussed on the …

Improved Laboratory Transition Probabilities for NdII and Application to the Neodymium Abundances of the Sun andThree Metal-poor Stars

EA Den Hartog, JE Lawler, C Sneden… - The Astrophysical …, 2003 - iopscience.iop.org
Radiative lifetimes, accurate to±5%, have been measured for 168 odd-parity levels of Nd II
using laser-induced fluorescence. The lifetimes are combined with branching fractions …

Atomic data for the Gaia-ESO Survey

U Heiter, K Lind, M Bergemann, M Asplund… - Astronomy & …, 2021 - aanda.org
Context. We describe the atomic and molecular data that were used for the abundance
analyses of FGK-type stars carried out within the Gaia-ESO Public Spectroscopic Survey in …

New rare earth element abundance distributions for the Sun and five r-process-rich very metal-poor stars

C Sneden, JE Lawler, JJ Cowan, II Ivans… - The Astrophysical …, 2009 - iopscience.iop.org
We have derived new abundances of the rare earth elements Pr, Dy, Tm, Yb, and Lu for the
solar photosphere and for five very metal-poor, neutron-capture r-process-rich giant stars …

Near-ultraviolet observations of HD 221170: new insights into the nature of r-process-rich stars

II Ivans, J Simmerer, C Sneden, JE Lawler… - The Astrophysical …, 2006 - iopscience.iop.org
Employing high-resolution spectra obtained with the near-UV-sensitive detector on the Keck
I HIRES, supplemented by data obtained with the McDonald Observatory 2d-coudé, we …

The Hamburg/ESO R-process enhanced star survey (HERES)-III. HE 0338-3945 and the formation of the r+ s stars

K Jonsell, PS Barklem, B Gustafsson… - Astronomy & …, 2006 - aanda.org
We have derived abundances of 33 elements and upper limits for 6 additional elements for
the metal-poor () turn-off star HE 0338-3945 from high-quality VLT-UVES spectra. The star is …