Detector | Exposure (Original/High-E Flare Cleaned/Low-E Cleaned) | Image binning | Plate scale ("/pixel) | Bgd. level (orig/High-E flare cleaned/cleaned, counts/sq. arcmin/s) | GTI file | Bgd. light curves | Roll angle | CCD counts | Extra info |
---|---|---|---|---|---|---|---|---|---|
mos1 | 3861 | 3861 | 3797 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:5013 ccd2:1696 ccd3:2002 ccd4:1734 ccd5:1798 ccd7:1539 |
filter=Thin1 date-obs=2011-06-11T07:15:15 object=SN2011dh roll_angle=326.705230713 |
|
pn | 10148 | 3312 | 1696 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:155826 ccd2:151204 ccd3:101800 ccd4:174268 ccd5:132936 ccd6:98753 ccd7:140519 ccd8:141098 ccd9:94306 ccd10:116145 ccd11:114896 ccd12:87361 |
filter=Thin1 date-obs=2011-06-11T05:05:03 object=SN2011dh timedel=0.07 roll_angle=326.705230713 |
22 source(s) in memory Iteration: 2 Images: |mos1 |pn |
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Python version = 2.5.4 (r254:67916, Aug 14 2009, 18:07:15) [GCC 4.1.1 20070105 (Red Hat 4.1.1-52)]
Headas version = 6.11
XAssist version = 1.000
SAS version = xmmsas_20110223_1801-11.0.0
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Tue Apr 10 13:21:17 2012
This data set was last accessed on Tue Apr 10 13:21:16 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0677980801
Position of field target = 13 30 5.12 47 10 11.3
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = OK
Detection method = eboxdetect
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Log files: processing messages |error messages |all messages (very detailed) |source logs