C. Reynolds, E. Kara, R. Mushotzky, A. Ptak, M. Koss, Brian J. Williams, Steven W. Allen, F. Bauer, Marshall W. Bautz, Arash Bogadhee, Kevin B. Burdge, N. Cappelluti, Brad Cenko, G. Chartas, Kai-wing Chan, Lía Corrales, T. Daylan, Abraham D. Falcone, A. Foord, Catherine E. Grant, M. Habouzit, D. Haggard, Sven Herrmann, Edmund Hodges-Kluck, O. Kargaltsev, George W. King, M. Kounkel, Laura A. Lopez, S. Marchesi, M. Mcdonald, Eileen Meyer, Eric D. Miller, M. Nynka, T. Okajima, F. Pacucci, H. Russell, S. Safi-Harb, Keivan G. Strassun, Anna Trindade Falcao, Stephen A. Walker, J. Wilms, M. Yukita, William W. Zhang
{"title":"Overview of the advanced x-ray imaging satellite (AXIS)","authors":"C. Reynolds, E. Kara, R. Mushotzky, A. Ptak, M. Koss, Brian J. Williams, Steven W. Allen, F. Bauer, Marshall W. Bautz, Arash Bogadhee, Kevin B. Burdge, N. Cappelluti, Brad Cenko, G. Chartas, Kai-wing Chan, Lía Corrales, T. Daylan, Abraham D. Falcone, A. Foord, Catherine E. Grant, M. Habouzit, D. Haggard, Sven Herrmann, Edmund Hodges-Kluck, O. Kargaltsev, George W. King, M. Kounkel, Laura A. Lopez, S. Marchesi, M. Mcdonald, Eileen Meyer, Eric D. Miller, M. Nynka, T. Okajima, F. Pacucci, H. Russell, S. Safi-Harb, Keivan G. Strassun, Anna Trindade Falcao, Stephen A. Walker, J. Wilms, M. Yukita, William W. Zhang","doi":"10.1117/12.2677468","DOIUrl":null,"url":null,"abstract":"The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra x-ray Observatory by providing low-background, arcsecond-resolution in the 0.3-10 keV band across a 450 arcminute2 field of view, with an order of magnitude improvement in sensitivity. AXIS utilizes breakthroughs in the construction of lightweight segmented x-ray optics using single-crystal silicon, and developments in the fabrication of large-format, small-pixel, high readout rate CCD detectors with good spectral resolution, allowing a robust and cost-effective design. Further, AXIS will be responsive to target-of-opportunity alerts and, with onboard transient detection, will be a powerful facility for studying the time-varying x-ray universe, following on from the legacy of the Neil Gehrels (Swift) x-ray observatory that revolutionized studies of the transient x-ray Universe. In this paper, we present an overview of AXIS, highlighting the prime science objectives driving the AXIS concept and how the observatory design will achieve these objectives.","PeriodicalId":434863,"journal":{"name":"Optical Engineering + Applications","volume":"142 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2023-10-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Optical Engineering + Applications","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2677468","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
The Advanced X-ray Imaging Satellite (AXIS) is a Probe-class concept that will build on the legacy of the Chandra x-ray Observatory by providing low-background, arcsecond-resolution in the 0.3-10 keV band across a 450 arcminute2 field of view, with an order of magnitude improvement in sensitivity. AXIS utilizes breakthroughs in the construction of lightweight segmented x-ray optics using single-crystal silicon, and developments in the fabrication of large-format, small-pixel, high readout rate CCD detectors with good spectral resolution, allowing a robust and cost-effective design. Further, AXIS will be responsive to target-of-opportunity alerts and, with onboard transient detection, will be a powerful facility for studying the time-varying x-ray universe, following on from the legacy of the Neil Gehrels (Swift) x-ray observatory that revolutionized studies of the transient x-ray Universe. In this paper, we present an overview of AXIS, highlighting the prime science objectives driving the AXIS concept and how the observatory design will achieve these objectives.