1020-compare different method pipeline-star

  1. Extract diffuse foreground power spectrum from partial sky (compare it with other component)

  2. Find out threshold in T maps

  3. Generate point sources simulation from previous threshold

  4. Do template fitting for pcfn simulations and n simulations

  5. Check goodness of fit.

  6. Produce template fitting after maps on QU

  7. Do inpainting (generate input by recycling method first)

  8. Power spectrum estimation

Diffuse fg configuration

  • 215GHz numerical error occur at 3500; calc at 3000; power spectrum estimation on 2500. finally use up to 2000. flux density error on T is 30.7mJy

  • 95GHz numerical error occur at 1600; calc at 1500; power spectrum estimation at 1000. finally use up to 720. flux density error on T is 154.2 mJy.

  • 30GHz numerical error occur at ?; calc at 500; power spectrum estimation at 500. finally use up to 300. flux density error on T is 145.6 mJy.

  • 270GHz numerical error occur at 4500; calc at 4000; power spectrum estimation on 3500. finally use up to 2400. flux density error on T is ?mJy

  • 155GHz numerical error occur at 2500; calc at 2000; power spectrum estimation on 1800. finally use up to 1270. flux density error on T is ?mJy

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