The high-speed X-ray camera on AXIS: design and performance updates
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| Format: | Preprint |
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2025
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| author | Miller, Eric D. Grant, Catherine E. Goeke, Robert Bautz, Marshall W. Leitz, Christopher Donlon, Kevan Allen, Steven W. Herrmann, Sven Falcone, Abraham D. Angile, F. Elio Chattopadhyay, Tanmoy Cooper, Michael Jensen, Mallory A. Juneau, Jill LaMarr, Beverly Malonis, Andrew Morris, R. Glenn Orel, Peter Pan, Abigail Y. Persyn, Steven Poliszczuk, Artem Prigozhin, Gregory Y. Prigozhin, Ilya Ptak, Andrew Reynolds, Christopher Stueber, Haley R. Warner, Keith Wilkins, Daniel R. |
| author_facet | Miller, Eric D. Grant, Catherine E. Goeke, Robert Bautz, Marshall W. Leitz, Christopher Donlon, Kevan Allen, Steven W. Herrmann, Sven Falcone, Abraham D. Angile, F. Elio Chattopadhyay, Tanmoy Cooper, Michael Jensen, Mallory A. Juneau, Jill LaMarr, Beverly Malonis, Andrew Morris, R. Glenn Orel, Peter Pan, Abigail Y. Persyn, Steven Poliszczuk, Artem Prigozhin, Gregory Y. Prigozhin, Ilya Ptak, Andrew Reynolds, Christopher Stueber, Haley R. Warner, Keith Wilkins, Daniel R. |
| contents | AXIS, a Probe mission concept now in a Phase A study, will provide transformative studies of high-energy astrophysical phenomena thanks to its high-resolution X-ray spectral imaging. These capabilities are enabled by improvements to the mirror design that greatly increase the X-ray throughput per unit mass; and to the detector system, which operates more than an order of magnitude faster than heritage instruments while maintaining excellent spectral performance. We present updates to the design of the AXIS High-Speed Camera, a collaborative effort by MIT, Stanford University, the Pennsylvania State University, and the Southwest Research Institute. The camera employs large-format MIT Lincoln Laboratory CCDs that feature multiple high-speed, low-noise output amplifiers and an advanced single-layer polysilicon gate structure for fast, low-power clock transfers. A first lot of prototype CCID100 CCDs has completed fabrication and will soon begin X-ray performance testing. The CCDs are paired with high-speed, low-noise ASIC readout chips designed by Stanford to provide better performance than conventional discrete solutions at a fraction of the power consumption and footprint. Complementary Front-End Electronics employ state-of-the-art digital video waveform capture and advanced signal processing to further deliver low noise at high speed. The Back-End Electronics provide high-speed identification of candidate X-ray events and transient monitoring that relays fast alerts of changing sources to the community. We highlight updates to our parallel X-ray performance test facilities at MIT and Stanford, and review the current performance of the CCD and ASIC technology from testing of prototype devices. These measurements achieve excellent spectral response at the required readout rate, demonstrating that we will meet mission requirements and enable AXIS to achieve world-class science. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2508_14157 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The high-speed X-ray camera on AXIS: design and performance updates Miller, Eric D. Grant, Catherine E. Goeke, Robert Bautz, Marshall W. Leitz, Christopher Donlon, Kevan Allen, Steven W. Herrmann, Sven Falcone, Abraham D. Angile, F. Elio Chattopadhyay, Tanmoy Cooper, Michael Jensen, Mallory A. Juneau, Jill LaMarr, Beverly Malonis, Andrew Morris, R. Glenn Orel, Peter Pan, Abigail Y. Persyn, Steven Poliszczuk, Artem Prigozhin, Gregory Y. Prigozhin, Ilya Ptak, Andrew Reynolds, Christopher Stueber, Haley R. Warner, Keith Wilkins, Daniel R. Instrumentation and Methods for Astrophysics AXIS, a Probe mission concept now in a Phase A study, will provide transformative studies of high-energy astrophysical phenomena thanks to its high-resolution X-ray spectral imaging. These capabilities are enabled by improvements to the mirror design that greatly increase the X-ray throughput per unit mass; and to the detector system, which operates more than an order of magnitude faster than heritage instruments while maintaining excellent spectral performance. We present updates to the design of the AXIS High-Speed Camera, a collaborative effort by MIT, Stanford University, the Pennsylvania State University, and the Southwest Research Institute. The camera employs large-format MIT Lincoln Laboratory CCDs that feature multiple high-speed, low-noise output amplifiers and an advanced single-layer polysilicon gate structure for fast, low-power clock transfers. A first lot of prototype CCID100 CCDs has completed fabrication and will soon begin X-ray performance testing. The CCDs are paired with high-speed, low-noise ASIC readout chips designed by Stanford to provide better performance than conventional discrete solutions at a fraction of the power consumption and footprint. Complementary Front-End Electronics employ state-of-the-art digital video waveform capture and advanced signal processing to further deliver low noise at high speed. The Back-End Electronics provide high-speed identification of candidate X-ray events and transient monitoring that relays fast alerts of changing sources to the community. We highlight updates to our parallel X-ray performance test facilities at MIT and Stanford, and review the current performance of the CCD and ASIC technology from testing of prototype devices. These measurements achieve excellent spectral response at the required readout rate, demonstrating that we will meet mission requirements and enable AXIS to achieve world-class science. |
| title | The high-speed X-ray camera on AXIS: design and performance updates |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2508.14157 |