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.