The Ultraviolet Extinction Map and Dust Property at High Galactic Latitude
Mingxu Sun, Biwei Jiang, Haibo Yuan, and Jun Li

TL;DR
This study creates a detailed ultraviolet extinction map of high Galactic latitude regions using data from LAMOST, GALAH, and GALEX, revealing dust properties and extinction ratios crucial for understanding the extragalactic sky.
Contribution
It provides the first high-resolution ultraviolet extinction map at high Galactic latitudes, combining stellar spectroscopy and GALEX photometry to analyze dust properties and extinction ratios.
Findings
Mapped UV extinction over a third of the sky at high Galactic latitudes.
Derived mean color excess ratios consistent with previous studies.
Discussed how extinction ratios vary with Galactic latitude and extinction levels.
Abstract
Extinction in ultraviolet is much more significant than in optical or infrared, which can be very informative to precisely measure the extinction and understand the dust properties in the low extinction areas. The high Galactic latitude sky is such an area, important for studying the extragalactic sky and the universe. Based on the stellar parameters measured by the LAMOST and GALAH spectroscopy and the ultraviolet photomery by the \emph{GALEX} space telescope, the extinction of 1,244,504 stars in the \emph{GALEX}/NUV band and 56,123 stars in the \emph{GALEX}/FUV band are calculated precisely. \textbf{The error of color excess is 0.009, 0.128 and 0.454 mag for , and respectively.} They delineates the \emph{GALEX}/NUV extinction map of about a third of the sky mainly at the high Galactic latitude area with an angular…
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