LHAASO detection of the Gamma-ray Emission from the W43 Direction
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Pre-published on:
May 01, 2024
Published on:
September 27, 2024
Abstract
We report the very-high-energy to ultra-high-energy $\gamma$-ray emission, detected by the Large High Altitude Air Shower Observation (LHAASO), from the direction toward the young star forming region W43. The extended $\gamma$-ray source is detected with a significance of ${\sim}19\sigma$ with KM2A and a significance of ${\sim}17\sigma$ with WCDA.
DOI: https://doi.org/10.22323/1.444.0603
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.