The wide-field x-ray monitor (WFXM) on the HiZ-GUNDAM mission

The HiZ-GUNDAM mission is one of the candidates for the JAXA’s competitive M-class missions. HiZ-GUNDAM revolutionizes our understanding of the high redshift universe and promotes multi-messenger astronomy. Combining a highly sensitive wide-field X-ray monitor, a near-infrared telescope, and autonomous spacecraft slew capability makes a powerful machine to hunt interesting X-ray transients and immediately identify their counterparts in near-infrared. The Wide Field X-ray Monitor (WFXM) is the main instrument to search for the transients in the soft X-ray band. WFXM comprises lobster-eye optics (LEO) and pnCCD as an X-ray imager. LEO has a size of 40 mm x 40 mm and a radius of curvature of 600 mm. We are planning to use the LEO manufactured by Photonis Inc. One WFXM module has three by three LEOs, which cover a field of view of 12 deg x 12 deg. The current baseline design is composed of 16 modules to cover 0.7 sr sky. The candidate focal imager is the pnCCD detector by PNSensor Inc. We will present the current status and prospects of the WFXM.

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Publication Details

Published
2024-08-21
DOI
https://doi.org/10.1117/12.3018771
Citations
3
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.99
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article

The wide-field x-ray monitor (WFXM) on the HiZ-GUNDAM mission

Junko S. Hiraga, Akihiro Doi, Daisuke Yonetoku, T. Sakamoto et al.
3 citations
Astrophysical Phenomena and Observations
0.99
article

The wide-field x-ray monitor (WFXM) on the HiZ-GUNDAM mission

Junko S. Hiraga, Akihiro Doi, Daisuke Yonetoku, T. Sakamoto, Hideo Matsuhara, Tatsuya Sawano, M. Arimoto, T. Mihara, S. Gunji
article en
3 citations

Abstract

The HiZ-GUNDAM mission is one of the candidates for the JAXA’s competitive M-class missions. HiZ-GUNDAM revolutionizes our understanding of the high redshift universe and promotes multi-messenger astronomy. Combining a highly sensitive wide-field X-ray monitor, a near-infrared telescope, and autonomous spacecraft slew capability makes a powerful machine to hunt interesting X-ray transients and immediately identify their counterparts in near-infrared. The Wide Field X-ray Monitor (WFXM) is the main instrument to search for the transients in the soft X-ray band. WFXM comprises lobster-eye optics (LEO) and pnCCD as an X-ray imager. LEO has a size of 40 mm x 40 mm and a radius of curvature of 600 mm. We are planning to use the LEO manufactured by Photonis Inc. One WFXM module has three by three LEOs, which cover a field of view of 12 deg x 12 deg. The current baseline design is composed of 16 modules to cover 0.7 sr sky. The candidate focal imager is the pnCCD detector by PNSensor Inc. We will present the current status and prospects of the WFXM.

Kanazawa University (JP), Yamagata University (JP), Aoyama Gakuin University (JP), Kwansei Gakuin University (JP), Japan Aerospace Exploration Agency (JP), Institute of Space and Astronautical Science (JP), Nitto RIKEN (Japan) (JP)
Openalex Percentile: Top 24%
Astrophysical Phenomena and Observations
0.99
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