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Items for improvement for when we are next on-site:

Items for the photo-diode system:

  • Automate the data taking with scripts
  • Develop/install infrastructure needed for long term installation
  • Figure out effective A-Omega for the diode, so we can calibrate in mags per square arc sec.
  • Obtain 3 full sets of grizy (LSST preferred or SLOAN) 1-inch diameter filters for sky monitors

List of things left in Chile, in La Serena in green Pelican case:

  • keyboard, mouse and monitor for Mac Mini sys admin, with associated cables
  • cordless drill/screwdriver for mechanical installation
  • misc wood screws and 1/4-20 bolts for mechanical installation
  • Cat 5 network cables, various lengths
  • USB cables
  • 1 pr safety glasses
  • drill bit and driver set
  • mounting brackets (Newport type L brackets), 2 large and 1 small for mech mounting
  • cross-bar for mech mounting

 



Notes from Feb 6 meeting in Tucson:

make spectrograph that can catch OH emission

buy second lens for existing camera

Get NCSA accounts for Cws, Michael and anyone else

environmental monitoring of camera temp

Kem points out that sky is a slippery thing- we should define "LSST Sky" as what DM fits around point sources, for a 15 sec image on a 6.5m equivalent aperture telescope. Our pixels are really big and include lots of stars. This isn't such a big deal for scheduler and where-to-point decisions, but it does matter for making a model of sky background. In particular the Milky Way is a problem, in that stellar density is varying but not sky brightness. We should consider fitting out the stellar density dependence. 

So we should go to Magellan and take 15 images in grizy. 

 

 



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