Possible pipeline improvements for 6x processing.
6x observations status. (inactive link)
| Field | Hours | Format | Start Date | PI's. |
| LMC (inactive link)
New Standards (inactive link) |
350 | 450 square degrees Deep integration mode 28 x 18 degrees Centered on LMC Southern Observatory Original Survey Tiles |
August 2000 | Weinberg Cole |
| Virgo Cluster | 30 | 36 square degrees Deep integration mode 6 x 6 degrees Centered on Virgo Northern Observatory Special Tile Specifications |
April 2000 | Schneider |
| Galactic Plane Rescans |
80 | 40 square degrees Standard integration mode 16 fields along Galactic plane 2x6 degrees Both observatories Original Tile Specifications |
April 2000 | Skrutskie |
| Young Cluster Survey |
40 | 50 square degrees Deep integration mode Calibration format 50 young cluster fields 1x1 degree Both observatories Special Tile Specifications |
April 2000 | Carpenter/Skrutskie |
| Low Latitude Cluster Survey | 30 | 40 square degrees Deep integration mode Calibration format 40 Abell-type clusters Low Galactic Latitude 1x1 degree Both observatories Special Tile Specifications |
April 2000 | Huchra |
| High Latitude Survey | 75 | 90 square degrees Deep integration mode 3 Low-cirrus fields 5x6 degrees Both observatories Special Tile Specifications |
Lockman Hole April 2000 - North AXAF South September 2000 - South Groth Strip June 2000 - North |
Beichman |
| Young Cluster Variability
|
80 | 20 square degrees Standard integration mode 3 Young Clusters Nightly repeated photometry 1x6 degree South observatory Special Tile Specifications |
April 2000 | Carpenter Skrutskie |
| Common Proper Motion Survey | 50 | 70 square degrees Standard integration mode 50 stars within 10 parsecs 1x6 degree Both observatories Special Tile Specifications |
April 2000 | Cutri Kirkpatrick |