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Bolometers are the most sensitive detectors for measuring millimeter and submillimeter wavelength astrophysical signals. Cameras comprised of arrays of bolometers have already made significant contrib...
Known bright S stars, recognized as such by their enhanced s-process abundances and C/O ratio, are typically members of the asymptotic giant branch (AGB) or the red giant branch (RGB). Few modern digi...
This paper proposes to use compression-based similarity measures to cluster spectral signatures on the basis of their similarities. Such universal distances estimate the shared information between tw...
A spectral atlas of Landolt stars for a reliable mid-IR spectrophotometric calibration for large telescopes。
STARK WIDTHS OF Fe I AND Ni I SPECTRAL LINES。
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 ...

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