综述：未来十年的远红外仪器与技术发展
天体物理仪器与方法
2019-04-09 v2 仪器与探测器
摘要
自20世纪50年代末诞生以来，远红外天文学在成熟的技术基础和不断扩大的研究人员群体的推动下迅速发展。这一进展表明，远红外波长的观测在几乎全部天体物理领域都十分重要，从宜居行星与生命起源的搜寻，到宇宙历史最初几亿年星系组装的最早阶段。技术组合（尤其在探测器领域）仍在发展，以及可部署这些技术的平台集合不断扩大，意味着远红外天文学在未来十年具有实现范式转变进展的潜力。在本综述中，我们考察了当前与未来的远红外观测平台，包括地基、亚轨道和天基设施，并讨论了将使能并增强这些平台以最佳应对21世纪远红外天文学面临挑战的技术发展路径。
引用
@article{arxiv.1709.02389,
title = {Review: Far-Infrared Instrumentation and Technology Development for the Next Decade},
author = {Duncan Farrah and Kimberly Ennico Smith and David Ardila and Charles M. Bradford and Michael Dipirro and Carl Ferkinhoff and Jason Glenn and Paul Goldsmith and David Leisawitz and Thomas Nikola and Naseem Rangwala and Stephen A. Rinehart and Johannes Staguhn and Michael Zemcov and Jonas Zmuidzinas and James Bartlett and Sean Carey and William J. Fischer and Julia Kamenetzky and Jeyhan Kartaltepe and Mark Lacy and Dariusz C. Lis and Lisa Locke and Enrique Lopez-Rodriguez and Meredith MacGregor and Elisabeth Mills and S. Harvey Moseley and Eric J. Murphy and Alan Rhodes and Matt Richter and Dimitra Rigopoulou and David Sanders and Ravi Sankrit and Giorgio Savini and John-David Smith and Sabrina Stierwalt},
journal= {arXiv preprint arXiv:1709.02389},
year = {2019}
}
备注
Invited review article, submitted to the Journal of Astronomical Telescopes, Instruments, and Systems. Updated in light of referee reports