Mapping Diffuse Emission in Lyman UV band
Li Ji (1, 12), Zheng Lou (1), Jinlong Zhang (2), Keqiang Qiu (3),, Shuangying Li (2), Wei Sun (1, 12), Shuping Yan (1, 12), Shuinai Zhang, (1, 12), Yuan Qian (1), Sen Wang (4), Klaus Werner (5), Taotao Fang (6),, Tinggui Wang (7), J\"urgen Barnstedt (5), Sebastian Buntrock (5)

TL;DR
This paper discusses two proposed Chinese space missions, CAFE and LyRIC, aimed at mapping diffuse Lyman UV emissions from the interstellar and circum-galactic medium to better understand galaxy environments.
Contribution
It introduces the science objectives, mission concepts, and technological approaches of CAFE and LyRIC, advancing the study of diffuse UV emissions in space.
Findings
Proposed missions target mapping of Lyman UV emissions.
Technologies enable detection of ionized oxygen and Lyman series.
Current status of mission development is presented.
Abstract
The CAFE (Census of warm-hot intergalactic medium, Accretion, and Feedback Explorer) and LyRIC (Lyman UV Radiation from Interstellar medium and Circum-galactic medium) have been proposed to the space agencies in China respectively. CAFE was first proposed in 2015 as a joint scientific CAS-ESA small space mission. LyRIC was proposed in 2019 as an independent external payload operating on the Chinese Space Station. Both missions are dedicated to mapping the Lyman UV emission (ionized oxygen (O VI) resonance lines at 103.2 and 103.8 nm, and Lyman series) for the diffuse sources in our Galaxy and the circum-galactic mediums of the nearby galaxies. We present the primary science objectives, mission concepts, the enabling technologies, as well as the current status.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Calibration and Measurement Techniques · Photocathodes and Microchannel Plates
