| 484 | | * 10/10/2012: to be replaced with [wiki:MD02.refstack.20120927] |
| 485 | | |
| 486 | | Started for OC144 (September 12, 2011) with a new reference stack and a small sample of reprocessed exposures released as nightly stacks. Due to a need of rebalancing the reprocessing load, only a minimal amount of processing required to make the reference stack was done. |
| 487 | | |
| 488 | | || MD02 does have some offset dither exposures illustrated in the sample g-band V3 plot, but many are single exposure coverage and won't typically be enough for a reference stack skycell. || [[Image(MD02_g_smf.png,200px)]] || |
| | 484 | * 10/5/2012: to be replaced with [wiki:MD02.refstack.20120927] -- diffims 20121001 onwards will use. |
| | 485 | |
| | 486 | Started for OC144 (September 12, 2011) with a new reference stack and a small sample of reprocessed exposures to release nightly stacks as well. Due to a need of rebalancing the reprocessing load, only a minimal amount of processing required to make the reference stack was done. |
| | 487 | |
| | 488 | || MD02 does have some offset dither exposures illustrated in the sample g-band V3 plot, but many are single exposure coverage and won't typically be enough for a reference stack skycell. While warps will extend to some of the outer skycells, the nightly stack distribution will define what is likely for the skycells released due to magic. 012-017, 21-28, 31-38, 41-48, 51-58, 61-68, 71-78, 82-87 || [[Image(MD02_g_smf.png,200px)]] || |