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相关论文: Atomic Transition Probabilities of Neutral Calcium

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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…

太阳与恒星天体物理 · 物理学 2014-03-28 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

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…

天体物理学 · 物理学 2009-11-13 Jennifer S. Sobeck , James E. Lawler , Christopher Sneden

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…

太阳与恒星天体物理 · 物理学 2018-10-10 J. E. Lawler , T. Feigenson , C. Sneden , J. J. Cowan , G. Nave

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$^{\rm o}_{1,2}$…

太阳与恒星天体物理 · 物理学 2023-03-29 E. A. Den Hartog , J. E. Lawler , C. Sneden , I. U. Roederer , 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…

太阳与恒星天体物理 · 物理学 2014-02-19 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

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…

太阳与恒星天体物理 · 物理学 2009-11-13 J. E. Lawler , C. Sneden , J. J. Cowan , I. I. Ivans , E. A. Den Hartog

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…

太阳与恒星天体物理 · 物理学 2015-05-14 J. Gurell , H. Nilsson , L. Engstrom , H. Lundberg , R. Blackwell-Whitehead , K. E. Nielsen , S. Mannervik

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…

天体物理学 · 物理学 2007-05-23 J. E. Lawler , E. A. Den Hartog , Z. E. Labby , C. Sneden , J. J. Cowan , I. I. Ivans

We tabulate spontaneous emission rates for all possible 811 electric-dipole-allowed transitions between the 75 lowest-energy states of Ca I. These involve the $4sns$ ($n=4-8$), $4snp$ ($n=4-7$), $4snd$ ($n=3-6$), $4snf$ ($n=4-6$), $4p^2$,…

原子物理 · 物理学 2017-11-22 Yanmei Yu , Andrei Derevianko

Accurate atomic data are essential for opacity calculations and for abundance analyses of the Sun and other stars. The aim of this work is to provide accurate and extensive results of energy levels and transition data for C I - IV. The…

原子物理 · 物理学 2021-02-03 W. Li , A. M. Amarsi , A. Papoulia , J. Ekman , P. Jönsson

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…

太阳与恒星天体物理 · 物理学 2025-03-31 G. T. Voith , E. A. Den Hartog , I. U. Roederer

Accurate transition probabilities for forbidden lines are important diagnostic parameters for low-density astrophysical plasmas. In this paper we present experimental atomic data for forbidden [FeII] transitions that are observed as strong…

太阳与恒星天体物理 · 物理学 2015-05-14 J. Gurell , H. Hartman , R. Blackwell-Whitehead , H. Nilsson , E. Backstrom , L. O. Norlin , P. Royen , 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…

天体物理学 · 物理学 2009-11-10 R. Schnabel , M. Schultz-Johanning , M. Kock

We present a comprehensive study of the electronic transitions in neutral cadmium (Cd I) with a focus on forbidden transitions, motivated by recent advances in laser technology and the growing relevance of cadmium in quantum gas research,…

原子物理 · 物理学 2025-10-07 P. J. Robert , S. Manzoor , M. Chiarotti , N. Poli

Quasar spectra reveal a rich array of important astrophysical information about galaxies which intersect the quasar line of sight. They also enable tests of the variability of fundamental constants over cosmological time and…

宇宙学与河外天体物理 · 物理学 2015-06-17 Michael T. Murphy , Julian C. Berengut

We report new branching fraction measurements for 224 ultraviolet (UV) and optical transitions of Tm II. These transitions range in wavelength (wavenumber) from 2350 - 6417 Angstroms (42532 - 15579 cm-1) and originate in 13 odd-parity and…

太阳与恒星天体物理 · 物理学 2024-07-24 E. A. Den Hartog , G. T. Voith , I. U. Roederer

In this critical compilation, all known to us experimental data on the spectrum of neutral carbon were methodically evaluated and supplemented by parametric calculations with Cowan's code. The sources of experimental data vary from…

原子物理 · 物理学 2017-11-23 K. Haris , A. Kramida

Recent radiative lifetime measurements accurate to +/- 5% (Stockett et al. 2007, J. Phys. B 40, 4529) using laser-induced fluorescence (LIF) on 8 even-parity and 62 odd-parity levels of Er II have been combined with new branching fractions…

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…

天体物理学 · 物理学 2007-05-23 J. E. Lawler , E. A. Den Hartog , C. Sneden , J. J. Cowan

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…

太阳与恒星天体物理 · 物理学 2021-05-05 E. A. Den Hartog , J. E. Lawler , I. U. Roederer
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