You are in: ATHENA TWG Workshop - Program
First day: Monday 14th March:: 2 p.m. to 6:30 p.m.
2:00 p.m.Welcome address G. Tagliaferri - OAB/INAF Director
2:05 p.m.Introduction: Scope of the meeting, Role of the TWG, Sharing of the activities, Organization G. Pareschi, R. Willingale
2:30 p.m. Athena Optics: general activities on the finalization of missions and optics:
  • Athena implementation Athena Development program and the optics implementation
  • ATHENA Mirrors: Technology consolidation program & production plan

  • Mark Ayre, ESA

  • Marcos Bavdaz
3:30 p.m.Possible contributions from international partners:
  • NASA
  • JAXA

  • R. Petre
  • H. Matsumoto (TBC)
4:00 p.m.Coffee Break
4:30 p.m.Implementation & Integration:
  • SPO Module opto-mechanical design & implementation
  • Alignment of mirror modules I
  • Alignment of mirror modules II

  • Max Collon/Cosine
  • D. Vernani, RUAG
  • G. Valsecchi, Media Lario
5:30 p.m.Scattering & Stray X-rays:
  • The baffling and stray - light issues and solutions
  • The baffling and stray - light issues and solutions
  • Baffling implementation after the activities performed for IXO
  • The scattering issue: models and experiments
  • The science point of view (I): diffuse sources
  • The science point of view (II): deep and extended surveys

  • R. Willingale, Leicester Univ.
  • G. Cusumano, INAF/IASF-Palermo
  • G. Vacanti, Cosine
  • Spiga/Ferreira TBC
  • S. Molendi, INAF/IASF-Milano
  • A. Comastri, INAF/OABologna
8:30 p.m. Social Dinner
Second day: Thuesday 15th March:: 9:30 a.m. to 4 p.m.
9:30 p.m.X-ray tests and calibrations:
  • Calibration products, responsibilities, resources
  • Mirror calibration plan within the ATHENA calibration plan
  • Current and future activities at Panter
  • A large area X-ray collimator for ATHENA
  • BeatriX as a testing, alignment and calibration facility at the industry premises

  • D. Lumb, ESA (TBC)
  • R. Willingale, Leicester Univ.
  • V. Burwitz, MPE
  • B. Menz, MPE
  • D. Spiga, OAB/INAF
10:30 a.m.Mirror performance modelling:
  • Error Budget
  • SW under development
  • High energy response. Specification and requirements

  • R. Willingale, Leicester Univ.
  • D. Spiga
  • D. Willingale
11:00 a.m.Coffee Break
11:30 a.m.Transmission of soft proton through the mirror system:
  • Introduction to the problem
  • Proposed implementation
  • Review on simulations and experimenta activities needed

  • R. Willingale, Leicester Univ.
  • ESA, Mark Ayre, TBC
  • D. Spiga, S. Molendi
12:30 a.m.Lunch (on site)
14:30 a.m.Contributed talks
15:30 a.m.Rapporteur talk
Discussion – Closing remarks, Track of actions
G. Pareschi
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