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  First light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission

Basso, S., Salmaso, B., Spiga, D., Ghigo, M., Vecchi, G., Sironi, G., et al. (2022). First light of BEaTriX, the new testing facility for the modular X-ray optics of the ATHENA mission. Astronomy and Astrophysics, 664: A173. doi:10.1051/0004-6361/202244028.

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Basso, S., Author
Salmaso, B., Author
Spiga, D., Author
Ghigo, M., 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. Della Monica, AuthorMassahi, S., AuthorGellert, N. C., AuthorChristensen, F., AuthorBavdaz, M., AuthorFerreira, I., AuthorCollon, M., AuthorVacanti, G., AuthorBarrière, N. M., 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              
3Center for Astrochemical Studies at MPE, MPI for Extraterrestrial Physics, Max Planck Society, ou_1950287              
4MPI for Extraterrestrial Physics, Max Planck Society, ou_159888              

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 Abstract: Aims. The Beam Expander Testing X-ray facility (BEaTriX) is a unique X-ray apparatus now operated at the Istituto Nazionale di Astrofisica (INAF), Osservatorio Astronomico di Brera (OAB), in Merate, Italy. It has been specifically designed to measure the point spread function (PSF) and the effective area (EA) of the X-ray mirror modules (MMs) of the Advanced Telescope for High-ENergy Astrophysics (ATHENA), based on silicon pore optics (SPO) technology, for verification before integration into the mirror assembly. To this end, BEaTriX generates a broad, uniform, monochromatic, and collimated X-ray beam at 4.51 keV. The beam collimation is better than a few arcseconds, ensuring reliable tests of the ATHENA MMs, in their focus at a 12 m distance.
Methods. In BEaTriX, a micro-focus X-ray source with a titanium anode is placed in the focus of a paraboloidal mirror, which generates a parallel beam. A crystal monochromator selects the 4.51 keV line, which is expanded to the final size by a crystal asymmetrically cut with respect to the crystalline planes. An in-house-built Hartmann plate was used to characterize the X-ray beam divergence, observing the deviation of X-ray beams from the nominal positions, on a 12-m-distant CCD camera. After characterization, the BEaTriX beam has the nominal dimensions of 170 mm × 60 mm, with a vertical divergence of 1.65 arcsec and a horizontal divergence varying between 2.7 and 3.45 arcsec, depending on the monochromator setting: either high collimation or high intensity. The flux per area unit varies from 10 to 50 photons s−1 cm−2 from one configuration to the other.
Results. The BEaTriX beam performance was tested using an SPO MM, whose entrance pupil was fully illuminated by the expanded beam, and its focus was directly imaged onto the camera. The first light test returned a PSF and an EA in full agreement with expectations. As of today, the 4.51 keV beamline of BEaTriX is operational and can characterize modular X-ray optics, measuring their PSF and EA with a typical exposure of 30 min. Another beamline at 1.49 keV is under development and will be integrated into the current equipment. We expect BEaTriX to be a crucial facility for the functional test of modular X-ray optics, such as the SPO MMs for ATHENA.

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Language(s): eng - English
 Dates: 2022-08-30
 Publication Status: Published online
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 Identifiers: DOI: 10.1051/0004-6361/202244028
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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: France : EDP Sciences S A
Pages: - Volume / Issue: 664 Sequence Number: A173 Start / End Page: - Identifier: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1