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Changes between Version 6 and Version 7 of PS1_GR_psps


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Timestamp:
Jun 29, 2011, 10:44:58 PM (15 years ago)
Author:
chambers
Comment:

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  • PS1_GR_psps

    v6 v7  
    3131We 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.
    3232
     33=== Small Area Surveys ===
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     35We hope to get the "Footprint" and "Small Area Surveys" observations soon as the weather improves. Processing these will become a priority as they become available, but this will take the place of the nightly ongoing processing, and won't impact GR or PSPS. We should be able to deliver Footprint and SAS stacks quickly after the observations are complete.
     36The footprint survey is a single footprint with no dither of 3 years (60 total exposures) of 3pi data. The SAS is a 9x9 or 81 square degree survey to 3pi depth. Both are centered on MD09, and overlap SDSS Stripe 82.
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