Direct hot slumping and accurate integration process to manufacture prototypal x-ray optical units made of glass

X-ray telescopes with very large collecting area, like the proposed International X-ray Observatory (IXO, with around 3 m2 at 1 keV), need to be composed of a large number high quality mirror segments, aiming at achieving an angular resolution better than 5 arcsec HEW (Half-Energy-Width). A possible technology to manufacture the modular elements that will compose the entire optical module, named X-ray Optical Units (XOUs), consists of stacking in Wolter-I configuration several layers of thin foils of borosilicate glass, previously formed by hot slumping. The XOUs are subsequently assembled to form complete multi-shell optics with Wolter-I geometry. The achievable global angular resolution of the optic relies on the required surface shape accuracy of slumped foils, on the smoothness of the mirror surfaces and on the correct integration and co-alignment of the mirror segments. The Brera Astronomical Observatory (INAF-OAB) is leading a study, supported by ESA, concerning the implementation of the IXO telescopes based on thin slumped glass foils. In addition to the opto-mechanical design, the study foresees the development of a direct hot slumping thin glass foils production technology. Moreover, an innovative assembly concept making use of Wolter-I counter-form moulds and glass reinforcing ribs is under development. The ribs connect pairs of consecutive foils in an XOU stack, playing a structural and a functional role. In fact, as the ribs constrain the foil profile to the correct shape during the bonding, they damp the low-frequency profile errors still present on the foil after slumping. A dedicated semirobotic Integration MAchine (IMA) has been realized to this scope and used to build a few integrated prototypes made of several layers of slumped plates. In this paper we provide an overview of the project, we report the results achieved so far, including full illumination intra-focus X-ray tests of the last integrated prototype that are compliant with a HEW of around 17’’.

[1]  Paolo Conconi,et al.  Development of high angular resolution x-ray telescopes based on slumped glass foils , 2012, Other Conferences.

[2]  Marcos Bavdaz,et al.  In focus measurements of IXO type optics using the new PANTER x-ray test facility extension , 2013, Optics & Photonics - Optical Engineering + Applications.

[3]  Daniele Spiga,et al.  Point spread function of real Wolter-I X-ray mirrors: computation by means of the Huygens-Fresnel principle , 2011, Optical Engineering + Applications.

[4]  Giovanni Pareschi,et al.  Cost-effective design and simulations for a prototypal x-ray optical unit for the IXO telescope , 2011, Optical Engineering + Applications.

[5]  Paolo Conconi,et al.  Accurate integration of segmented x-ray optics using interfacing ribs , 2013 .

[6]  Paolo Conconi,et al.  Design of the IXO optics based on thin glass plates connected by reinforcing ribs , 2011, Optical Engineering + Applications.

[7]  Manfred W. Grindel,et al.  Measurement of x‐ray telescope mirrors using a vertical scanning long trace profiler , 1996 .

[8]  Paolo Conconi,et al.  An integration machine for the assembly of the x-ray optic units based on thin slumped glass foils for the IXO mission , 2011, Optical Engineering + Applications.

[9]  K. Nandra,et al.  The International X‐ray Observatory , 2010, 1001.2843.

[10]  Paolo Conconi,et al.  IXO x-ray mirrors based on slumped glass segments with reinforcing ribs: optical and mechanical design, image error budget, and optics unit integration process , 2010, Astronomical Telescopes + Instrumentation.

[11]  Paolo Conconi,et al.  Evaluation by UV optical measurements of the imaging quality of grazing incidence x-ray optics , 1994, Optics & Photonics.

[12]  William W. Zhang,et al.  Development of lightweight x-ray mirrors for the Constellation-X mission , 2006, SPIE Astronomical Telescopes + Instrumentation.

[13]  Paolo Conconi,et al.  3D characterization of thin glass x-ray mirrors via optical profilometry , 2010, Optical Engineering + Applications.

[14]  Paolo Conconi,et al.  IXO glass mirrors development in Europe , 2011, Optical Engineering + Applications.

[15]  S. Basso,et al.  Hot slumping glass technology and integration process to manufacture a grazing incidence scaled prototype for the IXO telescope modules , 2009, Optical Engineering + Applications.

[16]  M. Bavdaz,et al.  Performance characterization of silicon pore optics , 2006, SPIE Astronomical Telescopes + Instrumentation.