Observing programme: Drivers

1
Observing programme Drivers

• Cluster physics
• 1.1 selected sample (12) 12x1Ms 12Ms
• 1.2 Outer fields 12 x1Ms 12 Ms
• WHIM in emission
• 2.1 Deep pointings 10 x 1 Ms 10Ms with 1.2,
  DT3Ms
• 2.2 Larger area TBD
• WHIM in Absorption
• 3.1 150 GRB x 70 ks 10 M
• Cluster evolution
• 4.1 Deep survey 10 x 1 Ms 10 Ms with 1.2,
  DT3Ms
• 4.2 Shallower survey TBD with 2.2
• GRB as cosmological probes
• 5.1 200 GRB x 70 ksec 14 Ms with 3.1, DT4Ms
• Note observing efficiency 0.9 (smart pointing,
  equatorial orbit)
• overlap observing program
• Total 44Ms/0.9 49Ms 1.6 years

2
Observing programme CV related

• EOS NS
• 30 (20 per year in full sky0.53yrs) x 20ksec
  0.6Ms
• Pointed TBD
• GRB physics
• Late time afterglow evolution for 20 events
  20x100 ksec 2Ms
• 3. Compact objects fast ourbursts follow up TBD