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| Format: | Preprint |
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2025
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| Online-Zugang: | https://arxiv.org/abs/2508.13600 |
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| author | Shipman, Russell F. Kitamoto, Shunji Wolfs, Rob Costantini, Elisa Eckart, Megan E. Ferrigno, Carlo Genolet, Ludovic Gorter, Nathalie Grim, Martin Herder, Jan Willem den Kilbourne, Caroline A. Leutenegger, Maurice A. van der Meer, Erik Mizumoto, Misaki Porter, F. Scott Paltani, Stéphane Sawada, Makoto Strotmann, Simon Tsujimoto, Masahiro de Vries, Cor P. |
| author_facet | Shipman, Russell F. Kitamoto, Shunji Wolfs, Rob Costantini, Elisa Eckart, Megan E. Ferrigno, Carlo Genolet, Ludovic Gorter, Nathalie Grim, Martin Herder, Jan Willem den Kilbourne, Caroline A. Leutenegger, Maurice A. van der Meer, Erik Mizumoto, Misaki Porter, F. Scott Paltani, Stéphane Sawada, Makoto Strotmann, Simon Tsujimoto, Masahiro de Vries, Cor P. |
| contents | The Resolve soft X-ray spectrometer is the high spectral resolution microcalorimeter spectrometer for the XRISM mission. In the beam of Resolve there is a filter wheel containing \xray{} filters. In the beam also is an active calibration source (the modulated X-ray source (MXS) that can provide pulsed \xray s to facilitate gain calibration.
The filter wheel consists of six filter positions. Two open positions, one $^{55}$Fe source to aid in spectrometer characterization during the commissioning phase, and three transmission filters: a neutral density filter, an optical blocking filter, and a beryllium filter.
The X-ray intensity, pulse period, and pulse separation of a MXS are highly configurable. Furthermore, the switch--on time is synchronized with the spacecraft's internal clock to give accurate start and end times of the pulses.
One of the issues raised during ground testing was the susceptibility of a MXS at high voltage to ambient light. Although measures were taken to mitigate the light leak, the efficacy of those measures must be verified in orbit. Along with an overview of issues raised during ground testing, this article will discuss the calibration source and the filter performance in--flight and compare with the transmission curves present in the Resolve calibration database. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_13600 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | In orbit operation of Resolve Filter Wheel and MXS Shipman, Russell F. Kitamoto, Shunji Wolfs, Rob Costantini, Elisa Eckart, Megan E. Ferrigno, Carlo Genolet, Ludovic Gorter, Nathalie Grim, Martin Herder, Jan Willem den Kilbourne, Caroline A. Leutenegger, Maurice A. van der Meer, Erik Mizumoto, Misaki Porter, F. Scott Paltani, Stéphane Sawada, Makoto Strotmann, Simon Tsujimoto, Masahiro de Vries, Cor P. Instrumentation and Methods for Astrophysics The Resolve soft X-ray spectrometer is the high spectral resolution microcalorimeter spectrometer for the XRISM mission. In the beam of Resolve there is a filter wheel containing \xray{} filters. In the beam also is an active calibration source (the modulated X-ray source (MXS) that can provide pulsed \xray s to facilitate gain calibration. The filter wheel consists of six filter positions. Two open positions, one $^{55}$Fe source to aid in spectrometer characterization during the commissioning phase, and three transmission filters: a neutral density filter, an optical blocking filter, and a beryllium filter. The X-ray intensity, pulse period, and pulse separation of a MXS are highly configurable. Furthermore, the switch--on time is synchronized with the spacecraft's internal clock to give accurate start and end times of the pulses. One of the issues raised during ground testing was the susceptibility of a MXS at high voltage to ambient light. Although measures were taken to mitigate the light leak, the efficacy of those measures must be verified in orbit. Along with an overview of issues raised during ground testing, this article will discuss the calibration source and the filter performance in--flight and compare with the transmission curves present in the Resolve calibration database. |
| title | In orbit operation of Resolve Filter Wheel and MXS |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2508.13600 |