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Related papers: Fe II lifetimes and transition probabilities

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The Fe II/Mg II emission line flux ratio in quasar spectra serves as a proxy for the relative Fe to alpha-element abundances in the broad line regions of quasars. Due to the expected different enrichment timescales of the two elements, they…

In this paper, energy levels, radiative rates and lifetimes are reported for 11 F-like ions with 12 $\le$ Z $\le$ 23. Up to 198 levels (depending on the ion) have been considered which include 113 of the 2s$^2$2p$^5$, 2s2p$^6$,…

Atomic Physics · Physics 2019-01-16 K M Aggarwal

With new astronomical infrared spectrographs the demands of accurate atomic data in the infrared have increased. In this region there is a large amount of parity-forbidden lines, which are of importance in diagnostics of low-density…

Astrophysics · Physics 2008-11-26 M. Aldenius , S. Johansson

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

We describe a method for determining the radiative decay properties of a molecule by studying the saturation of laser-induced fluorescence and the associated power broadening of spectral lines. The fluorescence saturates because the…

Atomic Physics · Physics 2008-12-23 T. E. Wall , J. F. Kanem , J. J. Hudson , B. E. Sauer , D. Cho , M. G. Boshier , E. A. Hinds , M. R. Tarbutt

We measure the lifetime of the 8s level on a magneto-optically trapped sample of ^{210}Fr atoms with time-correlated single-photon counting. The 7P_{1/2} state serves as the resonant intermediate level for two-photon excitation of the 8s…

Atomic Physics · Physics 2009-11-10 E. Gomez , L. A. Orozco , A. Perez Galvan , G. D. Sprouse

In this paper, we report on the gas-phase abundance of singly-ionized iron (Fe II) for 51 lines of sight, using data from the Far Ultraviolet Spectroscopic Explorer (FUSE). Fe II column densities are derived by measuring the equivalent…

Astrophysics · Physics 2010-11-05 Adam G. Jensen , Theodore P. Snow

In an effort to better calibrate the supernova rate of starburst galaxies as determined from near-IR [Fe II] features, we report on a [Fe II] 1.644 microns line-imaging survey of a sample of 42 optically-selected SNRs in M33. A wide range…

Astrophysics · Physics 2009-11-07 T. Morel , R. Doyon , N. St-Louis

Energy levels, lifetimes, and transition probabilities for transitions between computed levels of 3d^5 of Fe IV are reported. The E2 and M1 transition probabilities are compared with earlier theoretical results, often only the values…

Astrophysics · Physics 2007-05-23 Charlotte Froese Fischer , Robert H. Rubin

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 study the low-contrast Fe II emission blends in the ultraviolet (1250--2200A) and optical (4000--6000A) spectra of the Seyfert 1 galaxy NGC 5548 and show that these features vary in flux and that these variations are correlated with…

Astrophysics · Physics 2009-11-10 M. Vestergaard , B. M. Peterson

The time of life of fermionic quasiparticles, the distribution of which in the momentum-energy space can be measured by angle resolved photoemission (ARPES), is the first quantity to look for fingerprints of interaction responsible for the…

We present extensive calculations of radiative transition rates and electron impact collision strengths for Fe II. The data sets involve 52 levels from the $3d\,^7$, $3d\,^64s$, and $3d\,^54s^2$ configurations. Computations of $A$-values…

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

Transition frequencies of Fe II ion are known to be very sensitive to variation of the fine structure constant \alpha. The resonance absorption lines of Fe II from objects at cosmological distances are used in a search for the possible…

Atomic Physics · Physics 2009-11-13 S. G. Porsev , K. V. Koshelev , I. I. Tupitsyn , M. G. Kozlov , D. Reimers , S. A. Levshakov

Lifetime measurements using beam foil techniques for the $5s5p^{2}$ $^{2}D_{3/2,5/2}$ levels in Sn II are presented. The resulting oscillator strengths for transitions at 1699.4, 1831.8 and 1811.2 \AA{} are reported. We also studied these…

Atomic Physics · Physics 2016-10-19 N Heidarian , R E Irving , S R Federman , D G Ellis , S Cheng , L J Curtis

We estimate the range of the radiative lifetime and energy of the anomalous, low-energy $3/2^+(7.8 \pm 0.5$ eV) state in the $^{229}$Th nucleus. Our phenomenological calculations are based on the available experimental data for the…

Atomic Physics · Physics 2015-12-09 E. V. Tkalya , Christian Schneider , Justin Jeet , Eric R. Hudson

We present absolute frequency measurements of the ${}^{1}\text{P}_1 \leftarrow {}^{1}\text{S}_0$ ($229$nm) and ${}^{3}\text{P}_1 \leftarrow {}^{1}\text{S}_0$ ($326$nm) transitions for all naturally occurring isotopes of cadmium. The isotope…

We have recorded spectra of iron-neon and iron-argon hollow cathode lamps in the region 1700A -- 5um (59000 -- 2000cm-1), with Fourier transform (FT) spectrometers at the National Solar Observatory, Tucson, Arizona, U.S.A. and Imperial…

Astrophysics · Physics 2007-05-23 I. G. Nave , S. Johansson , R. C. M. Learner , A. P. Thorne , J. W. Brault

Calculations of energy levels, radiative rates and lifetimes are reported for eight ions of tungsten, i.e. S-like (W LIX) to F-like (W LXVI). A large number of levels has been considered for each ion and extensive configuration interaction…

Atomic Physics · Physics 2016-02-15 K M Aggarwal , F P Keenan