本文介绍了韦布空间望远镜上中红外(mid-infrared)仪器 MIRI 的独特科学价值及其在观测能力上的显著提升。作者阐述了在任务运行四年之际,通过持续的运行优化来增强该仪器科学产出的相关举措。
arXiv:2608.13873v1 Announce Type: new Abstract: MIRI, the Mid-Infrared Instrument on the James Webb Space Telescope, is the only instrument sensitive to wavelengths longward of 5 um on the observatory. In this regime, MIRI brings order-of-magnitude improvements over past instruments and missions in a wavelength range that is challenging or impossible to access from the ground. As such, MIRI occupies a unique parameter space, offering unparalleled capabilities in all areas of astrophysics, from the Solar System to the most distant galaxies in the Universe. We continue to make operational improvements to MIRI, four years into its operational lifetime, to create new observing opportunities, improve performance, and enhance its scientific return. In this paper we will describe several such improvements, and their anticipated impact on MIRI and JWST science.
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本站仅展示标题与摘要,正文版权归原作者及原发布机构所有。 原作者:S. Kendrew, M. Engesser, K. Rowlands, A. Noriega-Crespo, M. Decleir, H. Diamond-Lowe, M. Regan, J. Aguilar, S. Alberts, T. Bell, M. Cracraft, A. Dyrek, K. Gordon, D. Hines, B. J. Holler, K. Larson, D. Law, K. Murray, B. Nickson, B. O'Sullivan, A. Petric, B. Sargent, S. Shenoy, G. C. Sloan, B. Trahin, I. Wong。 原始页面