IPP Software Navigation Tools IPP Links Communication Pan-STARRS Links

Changes between Initial Version and Version 1 of IppDataProductsForWeakLensing


Ignore:
Timestamp:
Nov 6, 2009, 2:34:37 PM (17 years ago)
Author:
dravg.uk.edinburgh
Comment:

First version, copied from the ROE's internal tWiki

Legend:

Unmodified
Added
Removed
Modified
  • IppDataProductsForWeakLensing

    v1 v1  
     1= IPP Data Products we (ROE Weak Lensing Group) require for Weak Lensing analysis =
     2
     3== Pointings ==
     4
     5There are 10 pointings customised for high-redshift supernova searches. These are the Medium Deep Surveys. Each field has a footprint the size of the detector.
     6
     7There is also a deep pointing of Andromeda (MD00).
     8
     9The WL group will be using data from all 11 of these pointings.
     10
     11|| Field || Required || Available ||
     12|| MD01 || X || X ||
     13|| MD02 || X || X ||
     14|| MD03 || X ||   ||
     15|| MD04 || X ||   ||
     16|| MD05 || X ||   ||
     17|| MD06 || X ||   ||
     18|| MD07 || X ||   ||
     19|| MD08 || X || X ||
     20|| MD09 || X || X ||
     21|| MD10 || X || X ||
     22|| 11 (M31) ||  X || || 
     23
     24== Products for the Medium Deep (MD) surveys ==
     25
     26Imaging is done in 5 filters: g r i z y, with the highest integrated throughput in r & i.
     27
     28||        || g || r || i || z || y ||
     29|| raw    ||   ||   ||   ||   ||   ||
     30|| chip   ||   || f || f ||   ||   ||           
     31|| camera ||   || c || c ||   ||   ||
     32|| warp   ||   || f || f ||   ||   ||
     33|| stack  || f || f || f || f || f ||
     34
     35    * f => full
     36    * c => clean
     37
     38"Distribution bundles are built in either ''full'' or ''clean'' state. In the full state all of the associated data products are included. In the clean state the larger images are omitted. Once the dependent products are available at the mirror site, a run can be set to update state which causes the images to be re-created."
     39
     40-- http://svn.pan-starrs.ifa.hawaii.edu/trac/ipp/wiki/GPC1_DataDistribution_Overview
     41
     42All products for a later production stage can be generated from a full bundle. But though that implies all we really need is the full state of clean, the CPU time isn't worth it. Best to just grab the full warps, for example.
     43
     44== Data Storage Requirements ==
     45
     46    * 1.4e9 pixels
     47    * 10 bytes/pixel
     48    * 0.3 compression factor
     49    * 11 fields (10 MDS + M31)
     50    * ~100 images
     51
     52=> ~4 TB
     53
     54Since it's an approximation, budget for 8 TB
     55Medium Deep Survey pointings
     56
     57(sorry for the size, I don't know why tWiki doesn't scale images.)
     58
     59Also, the following image is WRONG. The background map needs to be flipped L-R. Hence the Andromeda (M31) pointing at the far right should really be over Andromeda, which in this map is at the far left, angled the wrong way.
     60
     61Pan-STARRS1_MDS.png
     62
     63-- EricTittley - 2009-11-06