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Changes between Version 3 and Version 4 of TestSN2009kf


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Timestamp:
Oct 29, 2009, 2:58:51 AM (17 years ago)
Author:
kpat.belfast
Comment:

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  • TestSN2009kf

    v3 v4  
    11= DRAVG test on SN 2009kf photometry (MT Botticella) =
    22We are working on photometry of the the SN PS1-0609001 (2009kf)
    3 and we have been looking at the newly released MD08 images (stacks for each epoch).
     3and we have been looking at the newly released MD08 images (stacks for each epoch)
     4and also are comparing them with the new, seasonal stack of the good images
     5released by Heather.
    46
    5 Several  immediate problems :
     7The main problem is the masking in the nightly stacks that Paul has given us,
     8compared what seems possible given Heather's new stacks. Example comparison is :
     9
     10Left : the seasonal stack made by Heather (MD08.skycell.102.stk.29916.fits) with 41 input images.
     11All NaN pixels are set to red. This looks good, brightest stars have saturated cores as expected. Virtually no other pixels are masked as NaN in these images. In fact apart from the butterfly
     12effect these stacks look very good. On the right is an example from one of Paul's nightly
     13stacks (MD08.skycell.102.stk.25151.fits) with 9 input images.
     14Many more stars are masked, and also bad chip areas are still visible, despite there being 9
     15input images. This is a similar problem to that noted by Durham in their ([wiki:Durham_MDS_Testing3])
     16
     17
     18[[Image(MD08-Heather-Paul-comp.jpg)]]
     19
     20
     21Some more severe masking is seen below :
    622
    723-'''masked areas'''