The far-infrared spectroscopic surveyor (FIRSS)
The far-infrared spectroscopic surveyor (FIRSS)
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DOI：
10.1007/s10686-021-09716-w
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发表时间：
2021-05
影响因子：
3
通讯作者：
D. Rigopoulou;Chris Pearson;B. Ellison;M. Wiedner;V. O. Okada;B. Tan;I. García-Bernete;M. Gerin;G. Yassin;E. Caux;S. Molinari;J. Goicoechea;Giorgio Savini;L. Hunt;D. Lis;P. Goldsmith;S. Aalto;G. Magdis;Carsten Kramer
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文献类型：
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作者：
D. Rigopoulou;Chris Pearson;B. Ellison;M. Wiedner;V. O. Okada;B. Tan;I. García-Bernete;M. Gerin;G. Yassin;E. Caux;S. Molinari;J. Goicoechea;Giorgio Savini;L. Hunt;D. Lis;P. Goldsmith;S. Aalto;G. Magdis;Carsten Kramer
我们正站在未来十年在地面和太空出现的强大新设施的十字路口，如ELT、SKA、JWST和Athena。将星系的星星形成潜力的叙述转化为定量理论将为天体物理学中许多悬而未决的问题提供答案，从行星的形成到星系的演化和重元素的起源。为了实现这一目标，迫切需要一个专门的空间，远红外光谱设施能够提供，第一次，大规模，高光谱分辨率（速度分辨）多波长的化学和动力学的ISM我们自己的银河系和附近的星系的研究。远红外光谱测量仪（FIRSS）满足了这些要求，并通过利用最近的光度测量的遗产，它抓住机会阐明我们宇宙的基本构建过程。
We are standing at the crossroads of powerful new facilities emerging in the next decade on the ground and in space like ELT, SKA, JWST, and Athena. Turning the narrative of the star formation potential of galaxies into a quantitative theory will provide answers to many outstanding questions in astrophysics, from the formation of planets to the evolution of galaxies and the origin of heavy elements. To achieve this goal, there is an urgent need for a dedicated space-borne, far-infrared spectroscopic facility capable of delivering, for the first time, large scale, high spectral resolution (velocity resolved) multiwavelength studies of the chemistry and dynamics of the ISM of our own Milky Way and nearby galaxies. The Far Infrared Spectroscopic Surveyor (FIRSS) fulfills these requirements and by exploiting the legacy of recent photometric surveys it seizes the opportunity to shed light on the fundamental building processes of our Universe.