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A 0.9 m diameter f/1.8 paraboloidal mirror of moderate quality (s2 armit) has been produced by spinning an epoxy-coated spherical substrate. This mirror has been used to build a prototype flux collector for stellar seismology. The objective is to produce 2 m mirrors for this application.
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Paolo Conconi, Oberto Citterio, Mauro Ghigo, Francesco Mazzoleni, "Replicated metal mirrors for grazing-incidence x-ray optics," Proc. SPIE 1931, Metal Mirrors, (15 October 1993); https://doi.org/10.1117/12.158730