The Feshbach Resonances Applied to the Calculation of Stark Broadening of Ionized Spectral Lines: An Example of Interdisciplinary Research by Sylvie Sahal-Bréchot, Haykel Elabidi

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Revisiting Near-infrared Features of Kilonovae: The Importance of Gadolinium by Salma Rahmouni, Masaomi Tanaka, Nanae Domoto, Daiji Kato, Kenta Hotokezaka, Wako Aoki, Teruyuki Hirano, Takayuki Kotani, Masayuki Kuzuhara, Motohide Tamura

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Line List for the A2Π−X2Σ+ and the B2Σ+−X2Σ+ Band Systems of CaF by Léo Lavy, Peter F Bernath, Adam Pastorek

Subjects: “…Spectral line lists…”
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Amplitude estimating algorithm for single channel mixing signals by RUI Guo-sheng 1, XU Bin 2, ZHANG Song2

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Optical-emission spectrometry method with inductively coupled plasma for determining the mass concentration of phosphorus in an oil-water emulsion by N. A. Zmeeva, O. Yu. Vinokurova

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Surface morphology, magnetic resonance and antistatic properties of fabric with carbon coating, modified by metal clusters by A. G. Anisovich, I. P. Akula, A. P. Laskovnev, M. I. Markevich, N. M. Chekan

“…The first line is a broad spectral line with an effective g-factor of 2.27 ± 0.01 and a width of 94.4 mT. …”
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Creation and research of antistatic carbon coatings on fabric 05С8-КВ, modified by metal clusters by A. G. Anisovich, I. P. Akula, A. P. Laskovnev, M. I. Markevich, N. M. Chekan

“…It was found that the EPR spectrum contains a spectral line 94.4 mt wide, which indicates a high concentration of magnetic resonance centers, the effective value of the g-factor is 2.26 ± 0.01. …”
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Detection of Dissolved Carbon Monoxide in Transformer Oil Using 1.567 μm Diode Laser-Based Photoacoustic Spectroscopy by Qu Zhou, Chao Tang, Shiping Zhu, Weigen Chen, Xiaojuan Peng

“…In this investigation, a tunable PAS experimental system based on a distributed-feedback (DFB) diode laser was proposed for recognizing dissolved CO in transformer oil. The molecular spectral line of CO gas detection was selected at 1.567 μm in the whole experiment. …”
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DIGITAL CONTACT POTENTIAL DIFFERENCE PROBE by K. U. Pantsialeyeu, A. I. Svistun, A. K. Tyavlovsky, A. L. Zharin

“…In this case is possible computation of the root mean square value or determination of the desired spectral line of the signal after fast Fourier transformation. …”
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Lessons from the High-resolution Spectroscopy of AW UMa and ϵ CrA: Is the Lucy Model Valid? by Slavek M. Rucinski

“…A complicating factor in detailed spectral analysis may be the occurrence of Enhanced Spectral-line Perturbations (ESPs) projected over the secondary profiles, appearing in different numbers in the two studied binaries. …”
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Photoreflectance Spectroscopy Characterization of Ge/Si0.16Ge0.84 Multiple Quantum Wells on Ge Virtual Substrate by Hung-Pin Hsu, Pong-Hong Yang, Jeng-Kuang Huang, Po-Hung Wu, Ying-Sheng Huang, Cheng Li, Shi-Hao Huang, Kwong-Kau Tiong

“…A detailed comparison of PR spectral line shape fits and theoretical calculation led to the identification of various quantum-confined interband transitions. …”
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3D Nonequilibrium Ionization and Spectroscopic Modeling of Coronal Mass Ejections. I. Comparison with Hinode/EIS Observations by E. M. Wraback, E. Landi, W. B. Manchester, J. Szente

“…For the first time, we combined self-consistent nonequilibrium charge state calculations in the EUV spectral line synthesis for a CME simulation to account for the plasma departures from ionization equilibrium everywhere in the CME. …”
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Technical review of radiative-property modeling approaches for gray and nongray radiation, and a recommended optimized WSGGM for CO2/H2O-enriched gases by Osama A. Marzouk

“…We compare the performance of these seven WSGGMs models to a reference solution obtained using the spectral line-based weighted-sum-of-gray-gases (SLW) approach in terms of predicted total emissivities and predicted radiative heat fluxes in a 3D enclosure with different temperatures and chemical compositions when either a gray radiation solution method (solving a single radiative transfer equation, “RTE”) or a nongray radiation solution method (solving multiple radiative transfer equations) is followed. …”
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The Arizona Molecular ISM Survey with the SMT: Variations in the CO(2–1)/CO(1–0) Line Ratio across the Galaxy Population by Ryan P. Keenan, Daniel P. Marrone, Garrett K. Keating

“…The J  = 1 → 0 spectral line of carbon monoxide (CO(1–0)) is the canonical tracer of molecular gas. …”
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ExoMolHR: A Relational Database of Empirical High-resolution Molecular Spectra by Jingxin Zhang, Christian Hill, Jonathan Tennyson, Sergei N. Yurchenko

“…The ExoMolHR database currently provides 24,307,135 spectral lines for 33 molecules and 58 isotopologues; these numbers will increase as the ExoMol database is updated.…”
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Discharge and Optical Emission Spectrum Characteristics of a Coaxial Dielectric Barrier Discharge Plasma-Assisted Combustion Actuator by Pengfei Liu, Liming He, Bingbing Zhao

“…The intensity of the spectral lines (297.54 nm, 315.76 nm, 336.96 nm, and 357.56 nm) first increased, then maintained, and then increased rapidly with the increased radius; however, the intensity of the spectral lines (380.34 nm, 405.80 nm, and 434.30 nm) basically remained unchanged, then increased, and finally decreased with the increased radius. …”
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Detection of Ammonia in Liquids Using Millimeter Wave Spectroscopy by Hilmi Ozturk, Hakki Nazli, Korkut Yegin, Mehmet Sezgin

“…The inversion of ammonia molecule results in split rotational spectral lines and transitions of these lines can be detected. …”
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Corroborating the magnetic easy axis of epitaxial (100) α-iron and (0001) BaFe12O19 thin films by 57Fe Mössbauer spectroscopy by Y. E. Li, J. Shine, C. Guguschev, M. Brützam, D. G. Schlom, N. Ravi

“…X-ray diffraction and RHEED data indicate that each film behaves as a single crystal material consistent with the relative intensity ratios of the spectral lines observed in the CEMS spectrum. Data further confirm that the easy axis of magnetization lies along the ⟨100⟩ family of directions of the cubic α-iron film. …”
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Detectability of Emission from Exoplanet Outflows Calculated by pyTPCI, a New 1D Radiation-hydrodynamic Code by Riley Rosener, Michael Zhang, Jacob L. Bean

“…We show that the most detectable spectral lines tend to be the 589 nm Na i doublet and the 1083 nm metastable helium triplet. …”
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Thermodynamics of the substantial universe by V. Yu. Stetsenko

“…The main reason for the redshift of spectral lines of light from distant stars and galaxies is not the expansion of the substantial Universe, but its clouds of gas and dust, which reduce the energy of photons.…”
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