English
Related papers

Related papers: Atomic Transition Probabilities for UV and Optical…

200 papers

We report new branching fraction measurements for 156 ultraviolet and optical transitions of Gd II. These transitions range in wavelength (wavenumber) from 2574 to 6766 Angstroms (38838 - 14777 cm-1) and originate in one odd-parity and 11…

Solar and Stellar Astrophysics · Physics 2025-03-31 G. T. Voith , E. A. Den Hartog , I. U. Roederer

We report new branching fraction measurements for 199 UV and optical transitions of Hf II. These transitions range in wavelength (wavenumber) from 2068- 6584 A (48322-15183 cm-1) and originate in 17 odd-parity upper levels ranging in energy…

Solar and Stellar Astrophysics · Physics 2021-05-05 E. A. Den Hartog , J. E. Lawler , I. U. Roederer

We report new measurements of branching fractions for 20 UV and blue lines in the spectrum of neutral silicon (Si I) originating in the 3$s^{2}$3$p$4$s$ $^{3}$P$^{\rm o}_{1,2}$, $^{1}$P$^{\rm o}_{1}$ and 3$s$3$p^{3}$ $^{1}$D$^{\rm o}_{1,2}$…

Solar and Stellar Astrophysics · Physics 2023-03-29 E. A. Den Hartog , J. E. Lawler , C. Sneden , I. U. Roederer , J. J. Cowan

We report new branching fractions for 121 UV lines from the low-lying odd-parity levels of Fe II belonging to the z6Do, z6Fo, z6Po, z4Fo, z4Do and z4Po terms of the 3d6(5D)4p configuration. These lines range in wavelength from 2250 - 3280…

Solar and Stellar Astrophysics · Physics 2019-08-21 E. A. Den Hartog , J. E. Lawler , C. Sneden , J. J. Cowan , A. Brukhovesky

New branching fraction measurements based primarily on data from a cross dispersed echelle spectrometer are reported for 84 lines of Co II. The branching fractions for 82 lines are converted to absolute atomic transition probabilities using…

Solar and Stellar Astrophysics · Physics 2018-10-10 J. E. Lawler , T. Feigenson , C. Sneden , J. J. Cowan , G. Nave

New experimental absolute atomic transition probabilities are reported for 203 lines of V II. Branching fractions are measured from spectra recorded using a Fourier transform spectrometer and an echelle spectrometer. The branching fractions…

Solar and Stellar Astrophysics · Physics 2015-06-22 M. P. Wood , J. E. Lawler , E. A. Den Hartog , C. Sneden , J. J. Cowan

Atomic transition probability measurements for 364 lines of Ti II in the UV through near IR are reported. Branching fractions from data recorded using a Fourier transform spectrometer and a new echelle spectrometer are combined with…

Solar and Stellar Astrophysics · Physics 2014-02-19 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

Radiative lifetimes from laser-induced fluorescence measurements, accurate to about +/- 5 percent, are reported for 41 odd-parity levels of Hf II. The lifetimes are combined with branching fractions measured using Fourier transform…

Astrophysics · Physics 2007-05-23 J. E. Lawler , E. A. Den Hartog , Z. E. Labby , C. Sneden , J. J. Cowan , I. I. Ivans

Radiative lifetimes, accurate to +/- 5%, have been measured for 212 odd-parity levels of Sm II using laser-induced fluorescence. The lifetimes are combined with branching fractions measured using Fourier-transform spectrometry to determine…

Astrophysics · Physics 2007-05-23 J. E. Lawler , E. A. Den Hartog , C. Sneden , J. J. Cowan

Aims: We measure transition probabilities for Cr II transitions from the z ^4H_J, z ^2D_J, y ^4F_J, and y ^4G_J levels in the energy range 63000 to 68000 cm^{-1}. Methods: Radiative lifetimes were measured using time-resolved laser-induced…

Solar and Stellar Astrophysics · Physics 2015-05-14 J. Gurell , H. Nilsson , L. Engstrom , H. Lundberg , R. Blackwell-Whitehead , K. E. Nielsen , S. Mannervik

Fe II radiative lifetimes were measured applying the time-resolved nonlinear laser-induced fluoresence technique. We investigated 21 levels of up to 47000 1/cm. The uncertainties are typically 2-3%. The lifetimes provide an improved…

Astrophysics · Physics 2009-11-10 R. Schnabel , M. Schultz-Johanning , M. Kock

Branching fraction measurements from Fourier transform spectra in conjunction with published radiative lifetimes are used to determine transition probabilities for 263 lines of neutral chromium. These laboratory values are employed to…

Astrophysics · Physics 2009-11-13 Jennifer S. Sobeck , James E. Lawler , Christopher Sneden

Atomic transition probability measurements for 371 Ni I lines in the UV through near IR are reported. Branching fractions from data recorded using a Fourier transform spectrometer and a new echelle spectrograph are combined with published…

Solar and Stellar Astrophysics · Physics 2014-03-28 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

Branching fractions were measured for electric dipole transitions from the 5p upper levels to the 5s levels in neutral krypton atoms. The measurements were made with a wall-stabilized electric arc and a 2m monochromator for the spectral…

Atomic Physics · Physics 2009-11-06 Krzysztof Dzierzega , Udo Volz , Gillian Nave , Ulf Griesmann

The goals of this study are 1) to test the best theoretical transition probabilities for Ca I (a relatively light alkaline earth spectrum) from a modern ab initio calculation using configuration interaction plus many body perturbation…

Solar and Stellar Astrophysics · Physics 2021-08-18 E. A. Den Hartog , J. E. Lawler , C. Sneden , J. J. Cowan , I. U. Roederer , J. Sobeck

Recent radiative lifetime measurements accurate to +/- 5% using laser-induced fluorescence (LIF) on 43 even-parity and 15 odd-parity levels of Ce II have been combined with new branching fractions measured using a Fourier transform…

Solar and Stellar Astrophysics · Physics 2009-11-13 J. E. Lawler , C. Sneden , J. J. Cowan , I. I. Ivans , E. A. Den Hartog

Optical transitions of highly charged ions can be very sensitive to hypothetical beyond-the-Standard-Model phenomena. Those near the $5s-4f$ level crossing, where the $5s$ and $4f$ are degenerate are especially promising. We present…

Radiative lifetimes, accurate to +/- 5%, have been measured for 49 even-parity and 14 odd-parity levels of Gd II using laser-induced fluorescence. The lifetimes are combined with branching fractions measured using Fourier transform…

Astrophysics · Physics 2007-05-23 E. A. Den Hartog , J. E. Lawler , C. Sneden , J. J. Cowan

We study the branching ratios of the allowed and forbidden radiative transitions among the first few (9) fine structure levels of O VI using relativistic coupled cluster theory. We find irregular patterns for a number of transitions with in…

Atomic Physics · Physics 2009-11-13 Chiranjib Sur , Rajat K Chaudhuri

The spectrum of the Fe I atom is critical to many areas of astrophysics and beyond. Measurements of the energies of its high-lying levels remain woefully incomplete, however, despite extensive analysis of ultraviolet laboratory iron…

Solar and Stellar Astrophysics · Physics 2015-06-19 Ruth C. Peterson , Robert L. Kurucz
‹ Prev 1 2 3 10 Next ›