| 31 | | We will continue with GR as scheduled above, while working on the dark current model and outstanding photometry issues, including extended source photometry. (This does not include large galaxies, which are a special case for the next stage of development). When these are resolved (i.e "good enough") then the photometry analysis of the GR'd pixels will be redone. When this is complete we will do another deletion of what is in the PSPS and load the new results as Data Release 0.2. Ideally we would be ready to do this by the time the first 2hr slice of 5 band data is re-processed. Maybe this becomes Data Release 1.0, we hope so, but it may turn out to take more than one release before we "freeze" the IPP code |
| | 31 | We will continue with GR as scheduled above, while working on the dark current model and outstanding photometry issues, including extended source photometry. (This does not include large galaxies, which are a special case for the next stage of development). When these are resolved (i.e "good enough") then the photometry analysis of the GR'd pixels will be redone. When this is complete we will do another deletion of what is in the PSPS and load the new results as Data Release 0.2. Ideally we would be ready to do this by the time the first 2hr slice of 5 band data is re-processed. Maybe this becomes Data Release 1.0, we hope so, but it may turn out to take more than one release before we "freeze" the IPP code for the year. These steps will be done in consultation with the Data Reduction and Verification Group, or DRAVG, with members at every institution. |
