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Changes between Version 26 and Version 27 of staticsky.20120706


Ignore:
Timestamp:
Dec 19, 2012, 2:48:08 PM (14 years ago)
Author:
bills
Comment:

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  • staticsky.20120706

    v26 v27  
    44
    55== Current Status ==
    6 Staticsky processing was stopped during the week ending 2012-12-07 to allow the stack construction up to RA 2H to complete. It was restarted on 2012-11-11
    7 with the area with RA < 15 DEC < 10 queued first.
    86
    9 As this region was nearing completion on 2102-12-14 we discovered that an error was made when setting the configuration parameters
    10 for the cuts to fix the excess y band detection problem discussed below. The data processed between 2012-12-11 and 2012-12-14 am had
    11 to be abandoned.
     7The following plot shows the skycells that have completed static sky processing as of 2012-12-19 22:30 UTC
    128
    13 The following plot shows the current status
    14 
    15 The stripe containing the Kepler field is on the left side of the plot 18 < RA < 20. The current area of interest RA < 15 and DEC < 10.
     9The stripe containing the Kepler field is on the left side of the plot 18 < RA < 20. The system is currently
     10working on the rest of that stripe in 18h < RA < 20h. Since this contains the galactic center progress has
     11slowed significantly.
    1612
    1713Other areas that have been processed were queued during several changes of direction described below.
    1814
    19 [[Image(ssky.20121214.png)]]
     15[[Image(ssky.20121219.png)]]
    2016
    2117== Sky calibration status 2012-12-10 ==
    2218
    23 The plot below shows the number of detections (matched and real) per skycell (log scale) for the region 267 < RA < 303 DEC > 10.
     19The plot below shows the number of sources detected per skycell in the r band.
    2420
    2521[[Image(logdetections.jpg)]]
     
    5854This effect is seen in 3% of the skycells north of 30 degrees declination.
    5955[[Image(mdr_cut.jpg)]]
     56
     57
     58After testing a more conservative cut was chosen. It is based on the ratio of the number of sources in y
     59to the number of sources detected in r, i, and z.
     60
     61Automatic forced photometry for sources detected in y band but not any other is disabled for skycells where
     62
     63{{{
     64   (NDetected_y / NDetected_r) > 1.7 && (NDetected_y / NDetected_i > 1.6) &&  && (NDetectected_z > 1.65)
     65}}}
     66
     67About 1 percent of skycells is affected by this feature.
    6068
    6169== Archival Notes ==