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We present lifetime measurements using beam-foil techniques for radiative transitions from the 3$p^4$($^1S$)4$s$ $^2S_{1/2}$, 3$p^4$($^3P$)5$s$ $^2P_{1/2,3/2}$, and 3$p^4$($^3P$)3$d$ $^2F_{5/2}$ levels in Cl I and the corresponding results…

Atomic Physics · Physics 2020-01-08 R. B. Alkhayat , R. E. Irving , S. R. Federman , D. G. Ellis , S. Cheng

We report lifetimes, branching fractions, and the resulting oscillator strengths for transitions within the P II multiplet (3s^23p^2 ^3P - 3s^23p4s ^3P^o) at 1154 A. These beam-foil measurements represent the most comprehensive and precise…

Astrophysics · Physics 2010-11-11 S. R. Federman , M. Brown , S. Torok , S. Cheng , R. E. Irving , R. M. Schectman , L. J. Curtis

We present the results of lifetime measurements made using beam-foil techniques on levels of astrophysical interest in Pb II producing lines at 1203.6 A ($6s6p^{2}$ $^{2}D_{3/2}$) and 1433.9 A ($6s^{2}6d$ $^{2}D_{3/2}$). We also report the…

Instrumentation and Methods for Astrophysics · Physics 2015-07-29 Negar Heidarian , Richard E. Irving , Adam. M. Ritchey , Steven R. Federman , David. G. Ellis , Song Cheng , Larry J. Curtis , Walter A. Furman

We report lifetimes, branching fractions, and the resulting oscillator strengths for transitions within the P II multiplet (3s23p2 3P - 3s3p3 3Po) at 1308 {\AA}. These comprehensive beam-foil measurements, which are the most precise set…

This work reports new experimental radiative lifetimes and calculated oscillator strengths for transitions from 3d8 4d levels of astrophysical interest in singly ionized nickel. Radiative lifetimes of seven high-lying levels of even parity…

Solar and Stellar Astrophysics · Physics 2017-04-12 H. Hartman , L. Engstrom , H. Lundberg , H. Nilsson , P. Quinet , V. Fivet , P. Palmeri , G. Malcheva , K. Blagoev

This work reports new experimental radiative lifetimes and calculated oscillator strengths for transitions of astrophysical interest in singly ionized cobalt. More precisely, nineteen radiative lifetimes in Co+ have been measured with the…

Solar and Stellar Astrophysics · Physics 2016-10-02 P. Quinet , V. Fivet , P. Palmeri , L. Engstrom , H. Hartman , H. Lundberg , H. Nilsson

Energies of ns[1/2] (n= 6-9), np[j] (n = 6-8), nd[j] (n= 6-7), and 5f[j] states in neutral Au and Au-like ions with nuclear charges Z = 80 - 83 are calculated using relativistic many-body perturbation theory. Reduced matrix elements,…

Atomic Physics · Physics 2009-11-10 U. I. Safronova , W. R. Johnson

The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s, and 4p$^2$) in the region 57743-77837 cm$^{-1}$ of singly ionised scandium (\ion{Sc}{ii}) were measured by two-step time-resolved laser induced fluorescence spectroscopy. Oscillator…

Solar and Stellar Astrophysics · Physics 2017-08-23 A. Pehlivan Rhodin , M. T. Belmonte , L. Engstrom , H. Lundberg , H. Nilsson , H. Hartman , J. C. Pickering , C. Clear , P. Quinet , V. Fivet , P. Palmeri

We report experimental oscillator strengths for 88 Ti I transitions covering the wavelength range 465 to 3892 nm, 67 of which had no previous experimental values. Radiative lifetimes for thirteen energy levels, including the low energy…

We present experimental atomic lifetimes for 12 levels in Sb I, out of which seven are reported for the first time. The levels belong to the 5p$^2$($^3$P)6s $^{2}$P, $^{4}$P and 5p$^2$($^3$P)5d $^{4}$P, $^{4}$F and $^{2}$F terms. The…

The electronic structure of singly ionized tin (SnII) is partly a one-electron and partly a three-electron system with ground configuration 5s25p. The excited configurations are of the type 5s2nl in the one-electron part, and 5s5p2, 5p3 and…

Atomic Physics · Physics 2014-12-08 K. Haris , A. Kramida , A. Tauheed

We report new experimental Fe I oscillator strengths obtained by combining measurements of branching fractions measured with a Fourier Transform spectrometer and time-resolved laser-induced fluorescence lifetimes. The study covers the…

Solar and Stellar Astrophysics · Physics 2017-11-01 M. T. Belmonte , J. C. Pickering , M. P. Ruffoni , E . A. Den Hartog , J. E. Lawler , A. Guzman , U. Heiter

The oscillator strengths of the $H^+_2$ molecular ion, $1s\sigma_{g}-2p\sigma_{u}$, $1s\sigma_{g}-2p\pi_{u}$ are calculated within the Born-Oppenheimer approximation. The variational expansion with randomly chosen exponents has been used…

Atomic Physics · Physics 2010-07-27 Ts. Tsogbayar , Ts. Banzragch

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

New radiative lifetimes, measured to $\pm$ 5 % accuracy, are reported for 31 even-parity levels of Fe I ranging from 45061 cm$^{-1}$ to 56842 cm$^{-1}$. These lifetimes have been measured using single-step and two-step time-resolved…

Solar and Stellar Astrophysics · Physics 2015-06-23 E. A. Den Hartog , M. P. Ruffoni , J. E. Lawler , J. C. Pickering , K. Lind , N. R. Brewer

We report calculations of energy levels and oscillator strengths for transitions in W XL, undertaken with the general-purpose relativistic atomic structure package ({\sc grasp}) and flexible atomic code ({\sc fac}). Comparisons are made…

Atomic Physics · Physics 2015-06-17 K. M. Aggarwal , F. P. Keenan

We report on calculations of energy levels, radiative rates, oscillator strengths, and line strengths for transitions among the lowest 253 levels of the (1s$^2$2s$^2$2p$^6$) 3s$^2$3p$^5$, 3s3p$^6$, 3s$^2$3p$^4$3d, 3s3p$^5$3d,…

Atomic Physics · Physics 2013-07-10 KM Aggarwal , FP Keenan , AZ Msezane

Energy levels, radiative rates (A-values) and lifetimes, calculated with the GRASP code, are reported for an astrophysically important O-like ion Mg~V. Results are presented for transitions among the lowest 86 levels belonging to the…

Atomic Physics · Physics 2016-09-28 K M Aggarwal , F P Keenan

We report empirical determinations of atomic oscillator strengths, or f-values, for 11 ground-state transitions of Fe II in the wavelength range 1050 to 1150 Ang. We use ultraviolet absorption line observations of interstellar material…

Astrophysics · Physics 2009-10-31 J. Christopher Howk , Kenneth R. Sembach , Katherine C. Roth , Jeffrey W. Kruk

Accurate and comprehensive atomic data are essential for the modelling of stellar spectra. Uncertainties in the oscillator strengths of specific lines used for abundance analyses directly translate into uncertainties in the derived…

Atomic Physics · Physics 2026-02-03 W. Li , A. M. Amarsi , P. Jönsson
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