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  X-ray tests of the ATHENA mirror modules in BEaTriX: from design to reality

Salmaso, B., Basso, S., Ghigo, M., Spiga, D., Vecchi, G., Sironi, G., et al. (2022). X-ray tests of the ATHENA mirror modules in BEaTriX: from design to reality. In Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray. doi:10.1117/12.2628227.

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 Creators:
Salmaso, B., Author
Basso, S., Author
Ghigo, M., Author
Spiga, D., Author
Vecchi, G., Author
Sironi, G., Author
Cotroneo, V., Author
Conconi, P., Author
Redaelli, E., Author
Bianco, A., Author
Pareschi, G., Author
Tagliaferri, G., Author
Sisana, D., Author
Pelliciari, C., Author
Fiorini, M., Author
Incorvaia, S., Author
Uslenghi, M., Author
Paoletti, L., Author
Ferrari, C., Author
Lolli, R., Author
Zappettini, A., AuthorRio, M. Sanchez del, AuthorParodi, G., AuthorBurwitz, V.1, Author           Rukdee, S.2, Author           Hartner, G.1, Author           Müller, T.3, Author           Schmidt, T.1, Author           Langmeier, A.4, Author           Ferreira, D. D., AuthorMassahi, S., AuthorGellert, N. C., AuthorChristensen, F., AuthorBavdaz, M., AuthorFerreira, I., AuthorCollon, M., AuthorVacanti, G., AuthorBarrière, N., Author more..
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              
2Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159895              
3Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              
4MPI for Extraterrestrial Physics, Max Planck Society, ou_159888              

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 Abstract: The BEaTriX (Beam Expander Testing X-ray) facility is now operative at the INAF-Osservatorio Astronomico Brera (Merate, Italy). This facility has been specifically designed and built for the X-ray acceptance tests (PSF and Effective Area) of the ATHENA Silicon Pore Optics (SPO) Mirror Modules (MM). The unique setup creates a parallel, monochromatic, large X-ray beam, that fully illuminates the aperture of the MMs, generating an image at the ATHENA focal length of 12 m. This is made possible by a microfocus X-ray source followed by a chain of optical components (a paraboloidal mirror, 2 channel cut monochromators, and an asymmetric silicon crystal) able to expand the X-ray beam to a 6 cm × 17 cm size with a residual divergence of 1.5 arcsec (vertical) × 2.5 arcsec (horizontal). This paper reports the commissioning of the 4.5 keV beam line, and the first light obtained with a Mirror Module.

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Language(s): eng - English
 Dates: 2022-08-31
 Publication Status: Published online
 Pages: -
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 Rev. Type: -
 Identifiers: DOI: 10.1117/12.2628227
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Title: SPIE Astronomical Telescopes + Instrumentation,
Place of Event: Montréal, Québec, Canada
Start-/End Date: 2022-07-17 - 2022-07-23

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Title: Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray
Source Genre: Proceedings
 Creator(s):
Nakazawa, Kazuhiro, Author
Nikzad, Shouleh , Author
A. den Herder, Jan-Willem , Author
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Publ. Info: -
Pages: - Volume / Issue: 12181 Sequence Number: - Start / End Page: - Identifier: -

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Title: Proceedings of SPIE
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Publ. Info: Bellingham, WA, USA : Society of Photo-Optical Instrumentation Engineers
Pages: - Volume / Issue: - Sequence Number: 121810W Start / End Page: - Identifier: ISSN: 0277-786X