Take One:
---------

*) Introduce data
   - Dates
   - Instrument modes
   - Any 'incidents'
   - Other stars
     - HD5XXXX
     - is sigma Ori D one of the targets?

*) Analysis
   - Lomb-Scargle periodogram
   - Schwarzenberg-Czerny periodogram
   - Raw data vs. stray-light subtracted data
   - Pre-whitening using known period
     (save coefficients to get smoothed light curve; publish params)
   - Remaining stray light artifacts
   - Any remaining signals?
   - Monte-Carlo significance testing
   - Secular changes in eclipse depths
     - define eclipse windows
     - calculate equivalent width relative to smooth curve
     - look for secular change
   - Compare phasing of minimum to predicted phase
     (not the same, due to color-time effect)

*) Discussion
   - phase lag due to color-time effect -> bound-free opacity
   - Eclipse depth -> magnetosphere mass
   - mass -> fill time or fill limit? (RFHD)
   - Lack of flaring -> companion (again, RFHD)

Take 2
------

*) Intro
  - one of magnetic stars in Orion OB1
  - archetype
  - variability
  - photometric history
  - MOST campaign

*) Observations
  - Dates
  - Gaps
  - Reduction

*) Results
  - Light curves
  - Fourier analysis
  - Harmonics
  - Repeatability
  - Other star

*) Discussion
  - Eclipse depths
  - Magnetospheric mass
  - Hump - surface or CS?
  - No flares
  - Long-term period
