Abstract
Monitor of All-sky X-ray Image (MAXI) is the X-ray all-sky monitor on the International Space Station (ISS).
It has been continuously scanning almost the entire sky in every ISS orbit (92 minutes) since August, 2009.
MAXI has two instruments; Gas Slit Camera (GSC) and Solid-state Slit Camera (SSC).
Both utilize slit-camera optics.
For the one-dimensional position sensitive X-ray detector, GSC uses gas proportional counters while SSC uses CCDs.
The 3-σ detection limit in 3-10 keV for one GSC scan and for one day are 60-100 mCrab and 12–15 mCrab, respectively.
The MAXI/GSC Nova-Alert System is used for the automated nova search.
MAXI detected X-ray time variabilities from a variety of objects from flaring stars to extragalactic objects.
As of September, 2022, MAXI has discovered 31 new X-ray objects including 14 black-hole binaries, 13 neutron-star binaries, and one white-dwarf binary.
The 7-year GSC catalog (3MAXI), 4-year SSC catalog (1MAXIS) and CCD diffuse X-ray map were compiled.
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Mihara, T., Tsunemi, H., Negoro, H. (2022). MAXI: Monitor of All-Sky X-Ray Image. In: Bambi, C., Santangelo, A. (eds) Handbook of X-ray and Gamma-ray Astrophysics. Springer, Singapore. https://doi.org/10.1007/978-981-16-4544-0_38-1
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