Aalto Susanne, Battersby Cara, Chin Gordon, Hunt Leslie K, Rigopoulou Dimitra, Stark Antony A, Viti Serena, Walker Christopher K
Department of Space, Earth and Environment, Onsala Space Observatory, Chalmers University of Technology, Onsala, Sweden.
Department of Physics, University of Connecticut, Storrs, 06269 CT USA.
Space Sci Rev. 2023;219(1):9. doi: 10.1007/s11214-023-00948-0. Epub 2023 Feb 2.
The , a proposed Astrophysics MIDEX-class mission concept, has an innovative 14-meter diameter inflatable primary mirror that will provide the sensitivity to study far-infrared continuum and line emission from galaxies at all redshifts with high spectral resolution heterodyne receivers. will have the sensitivity to follow the water trail from galaxies to the comets that create oceans. It will bring an understanding of the role of water in galaxy evolution and its part of the oxygen budget, by measuring water emission from local to intermediate redshift galaxies, observations that have not been possible from the ground. Observation of the ground-state HD line will accurately measure gas mass in a wide variety of astrophysical objects. Thanks to its exquisite spatial resolution and sensitivity, will, during its one-year baseline mission, detect water in galaxies with unprecedented statistical significance. This paper reviews the extragalactic science achievable and planned with .
这是一个拟议中的中等规模天体物理学任务概念,它有一个创新的14米直径可充气主镜,将通过高光谱分辨率外差接收器提供灵敏度,以研究所有红移星系的远红外连续谱和线发射。它将有能力追踪从星系到形成海洋的彗星的水迹。通过测量从本地到中等红移星系的水发射,这是地面无法进行的观测,它将带来对水在星系演化中的作用及其在氧预算中的作用的理解。对基态HD线的观测将准确测量各种天体物理对象中的气体质量。由于其出色的空间分辨率和灵敏度,在其一年的基线任务期间,它将以前所未有的统计显著性探测星系中的水。本文回顾了利用该任务可实现和计划进行的河外科学研究。