Search Results - "QUINET, P"
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Opacity calculations in four to nine times ionized Pr, Nd, and Pm atoms for the spectral analysis of kilonovae
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…New atomic data for radiative transitions in Pr V–X, Nd V–X, and Pm V–X were determined by means of large-scale calculations involving three independent…”
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Atomic data and opacity calculations in La v–x ions for the investigation of kilonova emission spectra
Published in Monthly notices of the Royal Astronomical Society (05-05-2022)“…ABSTRACT A new set of radiative parameters for spectral lines in La v–x ions is reported in this paper. These data were determined through the use of a…”
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Large-scale atomic data calculations in Ce V – X ions for application to early kilonova emission from neutron star mergers
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT New radiative parameters (wavelengths, transition probabilities, and oscillator strengths) are reported in the present paper for a large number of…”
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Multiconfiguration Dirac–Hartree–Fock radiative parameters for emission lines in Ce ii–iv ions and cerium opacity calculations for kilonovae
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT Large-scale calculations of atomic structures and radiative properties have been carried out for singly, doubly, and trebly ionized cerium. For this…”
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Expansion and line-binned opacities of samarium ions for the analysis of early kilonova emission from neutron star mergers
Published in Monthly notices of the Royal Astronomical Society (13-04-2023)“…ABSTRACT Opacity calculations performed within the expansion and the line-binned formalisms are reported for Sm V–X ions in this paper. These were determined…”
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Opacities of singly and doubly ionized neodymium and uranium for kilonova emission modeling
Published in Monthly notices of the Royal Astronomical Society (12-07-2023)“…ABSTRACT Even though the electromagnetic counterpart AT2017gfo to the binary neutron star merger GW170817 is powered by the radioactive decay of r-process…”
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Calculated oscillator strengths for the strongest lines of cosmochronological interest in the visible spectrum of singly ionized uranium (U II)
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)Get full text
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Spectral line list of potential cosmochronological interest deduced from new calculations of radiative transition rates in singly ionized thorium (Th ii)
Published in Monthly notices of the Royal Astronomical Society (01-08-2020)“…ABSTRACT In this work, we report a list of 91 strong Th ii spectral lines in the visible wavelength region that could be used as cosmochronometers in future…”
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Photoionization Models for High-density Gas
Published in The Astrophysical journal (01-02-2021)“…Relativistically broadened and redshifted 6.4-6.9 keV iron K lines are observed from many accretion powered objects, including X-ray binaries and active…”
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First discovery of trans-iron elements in a DAO-type white dwarf (BD−22°3467)
Published in Monthly notices of the Royal Astronomical Society (01-02-2020)“…We have identified 484 lines of the trans-iron elements (TIEs) Zn, Ga, Ge, Se, Br, Kr, Sr, Zr, Mo, In, Te, I, Xe, and Ba, for the first time in the ultraviolet…”
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11
MCDHF calculations of isotope shifts of even-parity fine-structure levels in neutral osmium
Published in Journal of quantitative spectroscopy & radiative transfer (01-12-2016)“…Ab initio multiconfiguration Dirac–Hartree–Fock (MCDHF) calculations have been carried out in order to determine the isotope shifts of all the fine-structure…”
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Transcriptome analysis in venom gland of the predatory giant ant Dinoponera quadriceps: insights into the polypeptide toxin arsenal of hymenopterans
Published in PloS one (31-01-2014)“…Dinoponera quadriceps is a predatory giant ant that inhabits the Neotropical region and subdues its prey (insects) with stings that deliver a toxic cocktail of…”
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PHOTOIONIZATION MODELING OF OXYGEN K ABSORPTION IN THE INTERSTELLAR MEDIUM: THE CHANDRA GRATING SPECTRA OF XTE J1817-330
Published in The Astrophysical journal (01-05-2013)“…We present detailed analysis of oxygen K absorption in the interstellar medium (ISM) using four high-resolution Chandra spectra toward the X-ray low-mass…”
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Oscillator strengths for high-excitation Ti ii from laboratory measurements and calculations
Published in Monthly notices of the Royal Astronomical Society (21-07-2016)“…This work reports new experimental radiative lifetimes of six 3d2(3F)5s levels in singly ionized titanium, with an energy around 63 000 cm−1 and four 3d2(3F)4p…”
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Lifetime measurements and oscillator strengths in singly ionized scandium and the solar abundance of scandium
Published in Monthly notices of the Royal Astronomical Society (2017)“…Abstract The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s and 4p2) in the region 57 743–77 837 cm−1 of singly ionized scandium (Sc ii) were measured by…”
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Lifetime measurements and calculations in Y+ and Y2+ ions
Published in Monthly notices of the Royal Astronomical Society (2011)“…We report a new set oftheoretical transition probabilities in Y ii, obtained using a multiconfiguration relativistic Hartree-Fock method including core…”
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Experimental radiative lifetimes for highly excited states and calculated oscillator strengths for lines of astrophysical interest in singly ionized cobalt (Co ii)
Published in Monthly notices of the Royal Astronomical Society (11-11-2016)“…This work reports new experimental radiative lifetimes and calculated oscillator strengths for transitions of astrophysical interest in singly ionized cobalt…”
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Atomic data for radiative transitions in the third spectra of rhodium (Rh III), palladium (Pd III) and silver (Ag III)
Published in Physica scripta (01-12-2013)“…A new set of radiative decay rates in doubly ionized rhodium (Rh III), palladium (Pd III) and silver (Ag III) has been computed by means of the…”
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Recovery of precious metals from electronic scrap by hydrometallurgical processing routes
Published in Mining, metallurgy & exploration (01-02-2005)Get full text
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UNCERTAINTIES IN ATOMIC DATA AND THEIR PROPAGATION THROUGH SPECTRAL MODELS. I
Published in The Astrophysical journal (10-06-2013)“…We present a method for computing uncertainties in spectral models, i.e., level populations, line emissivities, and emission line ratios, based upon the…”
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