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相关论文: Remarks on statistical errors in equivalent widths

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In a recent mathematical approach, Netzel (2018) proposes a method for determining the statistical error of spectral line equivalent widths. Using various approximations, he derives a determination equation that differs significantly from…

天体物理仪器与方法 · 物理学 2019-05-23 Thomas Eversberg

We present a new set of accurate formulae for the computation of random errors in the measurement of atomic and molecular indices. The new expressions are in excellent agreement with numerical simulations. We have found that, in some cases,…

天体物理学 · 物理学 2009-10-30 N. Cardiel , J. Gorgas , J. Cenarro , J. J. Gonzalez

We present a new automatic code (ARES) for determining equivalent widths of the absorption lines present in stellar spectra. We also describe its use for determining fundamental spectroscopic stellar parameters. The code is written in C++…

天体物理学 · 物理学 2009-11-13 S. G. Sousa , N. C. Santos , G. Israelian , M. Mayor , M. J. P. F. G. Monteiro

The zero-width approximation (ZWA) restricts the intermediate unstable particle state to the mass shell and, when combined with the decorrelation approximation, fully factorizes the production and decay of unstable particles. The ZWA…

高能物理 - 唯象学 · 物理学 2013-06-27 Nikolas Kauer

We point out an important source of error in measurements of extragalactic H-alpha emission and suggest ways to reduce it. The H-alpha line, used for estimating star formation rates, is commonly measured by imaging in a narrow band and a…

天体物理仪器与方法 · 物理学 2011-11-28 Oded Spector , Ido Finkelman , Noah Brosch

In this paper we present a measurement of the natural widths of $\Sigma_c^0$ and $\Sigma_c^{++}$. Using data from the FOCUS experiment, we find $\Gamma(\Sigma_c^0) = 1.55 +0.41/-0.37 \pm 0.38$ MeV/c^2 and $\Gamma(\Sigma_c^0) = 2.05…

高能物理 - 实验 · 物理学 2012-08-27 FOCUS Collaboration

We present the results of a long-term variability campaign of very broad-line AGNs with line widths broader than FWHM $>$ 5000 kms$^{-1}$. The main goal of our investigation was to study whether the widths of the optical broad emission…

天体物理学 · 物理学 2007-05-23 W. Kollatschny , M. Zetzl , M. Dietrich

High-accuracy dimensional measurements by laser interferometers require corrections because of diffraction, which makes the effective fringe-period different from the wavelength of a plane (or spherical) wave $\lambda_0$. By using a…

光学 · 物理学 2016-04-20 Carlo Paolo Sasso , Enrico Massa , Giovanni Mana

We present a tool for measuring the equivalent width (EW) in high-resolution spectra. The Tool for Automatic Measurement of Equivalent width (TAME)provides the EWs of spectral lines by profile fitting in the automatic or the interactive…

太阳与恒星天体物理 · 物理学 2015-06-05 Wonseok Kang , Sang-Gak Lee

A continuous atom laser will almost certainly have a linewidth dominated by the effect of the atomic interaction energy, which turns fluctuations in the condensate atom number into fluctuations in the condensate frequency. These correlated…

量子物理 · 物理学 2009-11-07 H. M. Wiseman , L. K. Thomsen

The experimentally predicted narrowing in the bandwidth of sodium is interpreted in terms of the non-local self-energy effect on quasi-particle energies of the electron liquid. The calculated self-energy correction is a monotonically…

材料科学 · 物理学 2009-10-31 H. Yasuhara , S. Yoshinaga , M. Higuchi

Spectral data is routinely broadened in order to improve appearance, approximate a higher sampling level or model experimental measurement effects. While there has been extensive work in the signal processing field to develop efficient…

材料科学 · 物理学 2023-09-22 Jessica Farmer , Adam J. Jackson

There are two aspects to the 1995 summer update of the combined preliminary electroweak data from LEP and SLC. On the one hand, agreement between experiments and the Standard Model (SM) has improved for the line-shape and the asymmetry…

高能物理 - 唯象学 · 物理学 2007-05-23 Kaoru Hagiwara

The electroweak corrections at the order of $O(\alpha_{ew}m_{t(b)}^2/m_W^2)$ to the partial widths of the $\tilde{t}_2 \to \tilde{g} + t$ and $\tilde{g} \to \tilde{t}_1 + \bar{t} $ decays (depending on the masses of the particles involved)…

高能物理 - 唯象学 · 物理学 2015-06-25 Hou Hong-Sheng , Ma Wen-Gan , Wan Lang-Hui , Zhang Ren-You

A new bandwidth selection rule that uses different bandwidths for the local linear regression estimators on the left and the right of the cut-off point is proposed for the sharp regression discontinuity estimator of the mean program impact…

统计方法学 · 统计学 2015-08-10 Yoichi Arai , Hidehiko Ichimura

We estimate $\dg/\Gamma_d$, including $1/m_b$ contributions and part of the next-to-leading order QCD corrections. We find that adding the latter corrections decreases the value of $\dg/\Gamma_d$ computed at the leading order by a factor of…

高能物理 - 唯象学 · 物理学 2007-05-23 Amol Dighe , Tobias Hurth , Choong Sun Kim , Tadashi Yoshikawa

We present a critical analysis of Pade-based methods for the unitarization of low energy amplitudes. We show that the use of certain Pade Approximants to describe the resonance region may lead to inaccurate determinations. In particular, we…

高能物理 - 唯象学 · 物理学 2008-11-26 Pere Masjuan , Juan Jose Sanz-Cillero , Javier Virto

Comparison of six high-redshift quasar spectra obtained with the Large Binocular Telescope with previous observations from the Sloan Digital Sky Survey shows that failure to correctly identify absorption and other problems with accurate…

A semiconductor quantum dot mimics a two-level atom. Performance as a single photon source is limited by decoherence and dephasing of the optical transition. Even with high quality material at low temperature, the optical linewidths are a…

The Voigt profile - a convolution of a Gaussian and a Lorentzian - accurately describes the absorption lines of atomic and molecular gases at low probe powers. Fitting such to experimental spectra yields both the Lorentzian natural…

原子物理 · 物理学 2015-06-04 Thomas M. Stace , Gar-Wing Truong , James Anstie , Eric F. May , Andre N. Luiten
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