DRAVG members, please give here a summary of mirroring requirements at your institution, with a link to a more detailed page if necessary.

• MPIA/MPE
  • Andromeda, Milky Way, brown dwarfs and quasars at MPIA (M31, 3pi): cmf files and/or dvo catalogs and corresponding postage stamps images ASAP.
  • For brown dwarfs & quasars: initially, the high-galactic-latitude sky will be enough; the brown dwarfs want the entire sky once proper-motions can be determined.
  • For quasars (and maybe brown dwarfs, too?):
    • izy stacks as soon as possible after data are taken
    • forced photometry in all other bands at the locations of all z and y-band detections
  • Pan-Planets:
• Belfast
  • 3pi survey from MHPCC: cmf files, postage stamp images,
  • from Garching: some detrend and difference images;
  • MDS from Garching: detrend images
• Edinburgh
• Durham
• CfA Full catalogs. 50-100% of Medium Deep Survey; detrending images only. Rapid-response postage stamp images.
• JHU
• LCOGT/UCSB
• NCU/TW Full catalogs; Medium Deep Survey; detrending images only; Rapid-response postage stamp images; cmf files.