Skip navigation
  • INAF logo
  • Home
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects
  • Explore by
    • Research outputs
    • Researchers
    • Organization units
    • Projects
  • Login:
    • My DSpace
    • Receive email
      updates
    • Edit Account details
  • Italian
  • English

  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 4 ALTRI PRODOTTI SCIENTIFICI (Other scientific products)
  4. 4.03 Rapporti di progetto
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/33100
Title: Test results of the BEaTriX paraboloidal mirror at PANTER
Authors: SPIGA, Daniele 
SALMASO, Bianca 
BASSO, Stefano 
SIRONI, GIORGIA 
GHIGO, Mauro 
VECCHI, Gabriele 
COTRONEO, Vincenzo 
PARESCHI, Giovanni 
TAGLIAFERRI, Gianpiero 
Burwitz, Vadim
Hartner, Gisela
Rukdee, Surankana
Mueller, Thomas
Schmidt, Thomas
Langmeier, Andreas
Budau, Bernd
Issue Date: 2021
Number: INAF-OAB internal report 2021/03
Abstract: Scope of this technical note is to report on the X-ray tests of the BEaTriX collimating mirror that have been carried out at the PANTER X-ray facility, before (May 4th-17th 2021) and after the coating with a Cr+Pt reflective layer at DTU, in the framework of the joint activities on optics for the ATHENA X-ray telescope. The tests planned before the deposition of the coating were aimed at confirming the mirror’s imaging quality expectations from the metrology tests, performed along with the polishing and finishing processes. Post-coating tests are oriented to the final qualification of the mirror and to ascertain that the mirror has maintained the focusing properties. Prior to coating, only tests at 1.49 keV are possible on the mirror. At this energy, PANTER can test the mirror in either diverging beam setup or making the beam parallel by means of a dedicated zone plate, canceling in this way the focus aberrations due to the finite distance of the source. After coating, in addition to the same tests at 1.49 keV, a test in diverging beam will be performed at 4.51 keV. The ZP cannot be used to collimate the 4.51 keV beam, but a comparison of the best focus at 1.49 keV and 4.51 keV will allow us to estimate the X-ray scattering that can be expected in the operation of the BEaTriX parabolic mirror. Simulations carried out from metrology on the uncoated mirror currently demonstrate a very low impact of the roughness on the mirror focusing performance.
URI: http://hdl.handle.net/20.500.12386/33100
Fulltext: open
Appears in Collections:4.03 Rapporti di progetto

Files in This Item:
File Description SizeFormat
IR_OAB_2021_03 part 1.pdfFULL TEXT part 1 of 34.18 MBAdobe PDFView/Open
IR_OAB_2021_03 part 2.pdfFULL TEXT part 2 of 39.7 MBAdobe PDFView/Open
IR_OAB_2021_03 part 3.pdfFULL TEXT part 3 of 35.83 MBAdobe PDFView/Open
Show full item record

Page view(s)

19
checked on Mar 21, 2023

Download(s)

8
checked on Mar 21, 2023

Google ScholarTM

Check


Items in DSpace are published in Open Access, unless otherwise indicated.


Explore by
  • Communities
    & Collections
  • Research outputs
  • Researchers
  • Organization units
  • Projects

Informazioni e guide per autori

https://openaccess-info.inaf.it: tutte le informazioni sull'accesso aperto in INAF

Come si inserisce un prodotto: le guide a OA@INAF

La Policy INAF sull'accesso aperto

Documenti e modelli scaricabili

Feedback
Built with DSpace-CRIS - Extension maintained and optimized by Logo 4SCIENCE