Summary
This conference paper describes the Hitomi (ASTRO-H) x-ray astronomy satellite, a sixth-generation Japanese mission developed through international collaboration (Japan, USA, Canada, Europe). The mission was designed to achieve unprecedented energy resolution above 2 keV and cover four decades of energy range. Although the spacecraft ceased functioning on 26 March 2016, the brief commissioning phase yielded valuable performance data and early astrophysical observations that are documented here.
UK applicability
This paper is not applicable to UK farming systems, soil health, nutrient density, or food systems research. It is a space astronomy mission technical report with no bearing on agricultural or nutritional science.
Key measures
Energy resolution at E > 2 keV using microcalorimeter instrumentation; energy range coverage from soft X-rays to gamma-rays; spacecraft and instrument performance metrics during commissioning
Outcomes reported
The paper reported on the Hitomi (ASTRO-H) x-ray astronomy satellite's capabilities, initial operations, and instrument/spacecraft performance during a one-month commissioning phase following launch in February 2016.
Topic tags
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