References of "Biémont, Emile"
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See detailRadiative Lifetimes for the 4p Excited States of Phosphorus and the Oscillator Strengths of Solar Lines
Berzinsh, U.; Svanberg, S.; Biémont, Emile ULg

in Astronomy and Astrophysics (1997), 326

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See detailEffets lumineux et météores dans l'atmosphère terrestre
Biémont, Emile ULg

Book published by Presses Universitaires de France (1997)

Detailed reference viewed: 3 (1 ULg)
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See detailBeam-laser measurements and relativistic Hartree-Fock calculations of the lifetimes of the 4d95p levels in Ag II
Biémont, Emile ULg; Pinnington, E. H.; Kernahan, J. A. et al

in Journal of Physics : B Atomic Molecular & Optical Physics (1997), 30

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See detailMultipole Transitions in Nicke-like and Palladium-like Spectra
Biémont, Emile ULg

in Journal of Physics : B Atomic Molecular & Optical Physics (1997), 30

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See detailMeasurements of the ground state ionization energy and wavelengths for the 1snp1P1 - 1s2 1S0(n=4-10) lines of O VII
Bartnik, A.; Biémont, Emile ULg; Dyakin, V. M. et al

in Journal of Physics : B Atomic Molecular & Optical Physics (1997), 30

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See detailFourier Transform Spectroscopy in the Infrared Region
Biémont, Emile ULg

Conference (1997)

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See detailSpectroscopy of Ne IV in the wavelength Range 450–1100 Å
Bastin, Thierry ULg; Biémont, Emile ULg; Dumont, Paul-Dominique ULg et al

in Journal of the Optical Society of America. B, Optical Physics (1997), 14

An analysis of the Ne IV spectrum was undertaken in the 450–1100-Å spectral range. The spectra were produced by the beam–foil method with beam energies of 1.2 and 2.5 MeV, respectively. The resolution ... [more ▼]

An analysis of the Ne IV spectrum was undertaken in the 450–1100-Å spectral range. The spectra were produced by the beam–foil method with beam energies of 1.2 and 2.5 MeV, respectively. The resolution that was achieved, with a normal-incidence 2-m spectrometer, was sufficient to identify 53 new Ne IV lines and, consequently, to determine 18 new levels in the quartet and doublet systems and one sextet term. The energy values of 13 additional levels were also revised. The classification work was facilitated by the use of scaled relativistic Hartree–Fock calculations. [less ▲]

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See detailThe Spectrum of Ne V
Bastin, Thierry ULg; Biémont, Emile ULg; Dumont, Paul-Dominique ULg et al

in Physica Scripta (1997), 55

A new investigation of the Ne V spectrum is reported. The beam-foil method has been used to produce spectra at two different energies (1.2 MeV and 2.5 MeV) between 450 and 11OOA Sixty-five lines of Ne V ... [more ▼]

A new investigation of the Ne V spectrum is reported. The beam-foil method has been used to produce spectra at two different energies (1.2 MeV and 2.5 MeV) between 450 and 11OOA Sixty-five lines of Ne V have been newly identified. Fifty levels have been determined for the first time and energies have been revised for seven levels. [less ▲]

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See detailTheoretical Radiative Lifetimes of 3p3(4S°)4s5S° and 3S° States in S I
Biémont, Emile ULg; Storey, P. J.; Zeippen, C. J.

in Astronomy and Astrophysics (1996), 309

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See detailRadiative Lifetimes for States in Cu I
Biémont, Emile ULg; Fryczynski, F.; Palmeri, P. et al

in Journal of Quantitative Spectroscopy & Radiative Transfer (1996), 55

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See detailUV Lines of Astrophysical Interest in Mg II
Biémont, Emile ULg

Conference (1996)

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See detailHyperfine structure of Sc I by Infrared Fourier Transform Spectroscopy
Aboussaïd, A.; Carleer, M.; Hurtmans, D. et al

in Physica Scripta (1996), 53

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See detailForbidden Lines in 6pk (j=1-5) configurations
Biémont, Emile ULg; Quinet, Pascal ULg

in Physica Scripta (1996), 54

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See detailTerm analysis and Hyperfine Structure in Neutral Vanadium
Palmeri, P.; Biémont, Emile ULg

in Proceedings of the 5th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (1996)

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See detailTheoretical Radiative Lifetimes of 3p3(4S°)4s 5S° and 3S° States in S I
Biémont, Emile ULg; Storey, P. J.; Zeippen, C. J.

in Proceedings of the 5th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (1996)

Detailed reference viewed: 5 (0 ULg)
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See detailProbabilities for forbidden transitions in atoms and ions: 1989-1995. A commented bibliography
Biémont, Emile ULg; Zeippen, C. J.

in Physica Scripta (1996), T65

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See detailHyperfine structure of infrared Al II lines
Palmeri, P.; Biémont, Emile ULg

in Journal of Physics : B Atomic Molecular & Optical Physics (1996), 29

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See detailLa Lumière
Biémont, Emile ULg

Book published by Presses Universitaires de France (1996)

Detailed reference viewed: 5 (2 ULg)