[1] BERTI E,VOLONTERI M.Cosmological black hole spin evolution by mergers and accretion[J].The Astrophysical Journal,2008,684(2):822-828.
[2] WOLTER H.Mirror systems with grancing incidence as image-forming optics for X-rays[J].Annals of Physics,1952,10(6):94-114.
[3] RAMSEY B D.The development of focusing optics for the hard X-ray region[J].Advances in Space Research,2006,38(12):2985-2988.
[4] ASCHENBACH B.Realization of X-ray telescopes-from design to performance[J].Experimental Astronomy,2009,26(1-3):95-109.
[5] WEISSKOPF M C,TANANBAUM H D,SPEYBROECK L P,et al.Chandra X-ray observatory(CXO):Overview[C].SPIE,2000,4012:2-16.
[6] KUNIEDA H,ISHIDA M,ENDO T,et al.X-ray telescope onboard Astro-E:optical design and fabrication of thin foil mirrors[J].Applied Optics,2001,40(4):553-564.
[7] KOGLIN J E,CHEN C M H,CHONKO J C,et al.Hard X-ray Optics:from HEFT to NuSTAR[C].SPIE,2004,5488:856-867.
[8] ZHANG W W.Manufacture of mirror glass substrates for the NUSTAR mission[C].SPIE,2009,7437:74370N.
[9] ROMAINE S,RRUNI R,GORENSTEIN P,et al.Platinum as a release layer for thermally formed optics for IXO[C].SPIE,2010,7732:77323T-1-6.
[10] ZHANG W W,BOLOGNESE J,BYRON G,et al.Mirror technology development for the international X-ray observatory(IXO)mission[C].SPIE,2009,7360:73600J-1-10.
[11] PROSERPIO L.Development of the glass slumping technology for the production of the X-ray mirrors aboard the international X-ray observatory optical module[D].Como and Varese:University of Insubria,2011.
[13] GHIGO M,BASSO S,CITTERIO O,et al.Hot slumping glass technology for the grazing incidence optics of future missions,with particular reference to IXO[C].SPIE,2010,7732:77320C-1-12.
[14] CHEN Y.Thermal forming process for precision freeform optical mirrors and micro glass optics[D].Columbus:The Ohio State University,2010.
[15] GHIGO M,BASSO S,CANESTRARI R,et al.Hot slumping glass technology and integration process to manufacture a grazing incidence scaled prototype for the IXO telescope modules[C].SPIE,2009,7437:74370P-1-15.