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Prediction of stellar atmospheric parameters from spectra, spectral indices and spectral lines using machine learning
stellar atmospheric parameters spectra spectral lines
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2009/6/8
Prediction of stellar atmospheric parameters from spectra, spectral indices and spectral lines using machine learning。
EXPERIMENTAL STARK SHIFT OF SEVERAL N II AND O II SPECTRAL LINES
EXPERIMENTAL STARK SHIFT N II O II
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2009/4/16
EXPERIMENTAL STARK SHIFT OF SEVERAL N II AND O II SPECTRAL LINES。
STARK WIDTHS OF Fe I AND Ni I SPECTRAL LINES
Fe I Ni I SPECTRAL LINES
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2009/4/8
STARK WIDTHS OF Fe I AND Ni I SPECTRAL LINES。
STARK BROADENING DATA TABLES FOR SOME ANALOGOUS SPECTRAL LINES ALONG Li AND Be ISOELECTRONIC SEQUENCES
STARK BROADENING DATA TABLES ISOELECTRONIC SEQUENCES ANALOGOUS SPECTRAL LINES
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2009/3/19
By using the semiclassical perturbation approach, Stark broadening
parameters due to the interaction with a selection of perturbers of interest for
recently published experimental results for Li - l...
STARK BROADENING PARAMETER TABLES FOR NEUTRAL CALCIUM SPECTRAL LINES. I
STARK BROADENING PARAMETER TABLES NEUTRAL CALCIUM SPECTRAL LINES
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2009/3/19
Using a semiclassical approach, we have calculated electron−, proton−,
He II−, Mg II-, Si II- and Fe II-impact line widths and shifts for 189 Ca
I multiplets as a function of tempe...
STARK BROADENING PARAMETER TABLES FOR NEUTRAL ZINC SPECTRAL LINES
NEUTRAL ZINC SPECTRAL LINES STARK BROADENING PARAMETER TABLES
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2009/3/19
Using a semiclassical approach, we have calculated electron−, proton−
and He II−impact line widths and shifts for 32 Zn I multiplets as a function
of temperature and perturber dens...
STARK BROADENING PARAMETER TABLES FOR NEUTRAL CALCIUM SPECTRAL LINES. II
STARK BROADENING PARAMETER TABLES NEUTRAL CALCIUM SPECTRAL LINES
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2009/3/18
Electron-, proton-, and ionized helium-impact broadening parameter
tables for neutral calcium spectral lines, have been presented as a function of the
temperature and the perturber density. Calculat...
MEASURED, CALCULATED AND PREDICTED STARK WIDTHS OF THE SINGLY IONIZED C, N, O, F, Ne, Si, P, S, Cl AND Ar SPECTRAL LINES
plasma spectroscopy ionized emitters Ar SPECTRAL LINES
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2009/3/18
In order to find reliable Stark width data, needed in plasma spectroscopy,
comparision between the existing measured, calculated and predicted
Stark width values was performed for ten singly ionized...
STARK BROADENING PARAMETER TABLES FOR Ne II AND Ne III SPECTRAL LINES
STARK BROADENING PARAMETER TABLES Ne II Ne III SPECTRAL LINES
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2009/3/13
Using a semiclassical approach, we have calculated electron−, proton−,
He II−, Mg II-, Si II- and Fe II-impact line widths and shifts for 10 Ne II
and 6 Ne III multiplets as a func...
ON THE MODIFICATIONS OF OSCILLATOR STRENGTHS AND DAMPING CONSTANTS OF Fe I SPECTRAL LINES FROM 500 nm TO 510 nm
Atomic data - Line profiles - Techniques spectroscopic
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2009/3/6
We modified oscillator strengths and enhancement factors of van
der Waals damping constants for 84 moderately strong and weak neutral iron spec-
tral lines between 500 nm and 510 nm, by fitting the ...
IDENTIFICATION OF PHASE-INDEPENDENT SPECTRAL LINES IN CLOSE BINARY V455 CYG：I. TELLURIC
Line identi¯ cation binaries spectroscopic-Stars individual V455 Cyg
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2009/2/17
Spectroscopic observations of close binary star V455 Cygni reveal
many lines that originate in interstellar and circumstellar medium and the atmo-
sphere of the Earth; we found over two hundred such...