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 | 8198 | 8156 | 8156 | 1.00 | 4.35 | 0.088/0.088/0.088 | Yes | orig clean | ccd2:50343 ccd3:103307 ccd4:66948 ccd5:66272 ccd7:55548 |
filter=Thick date-obs=2011-09-06T08:42:53 object=Crab roll_angle=87.2057647705 |
|
mos2 | 8188 | 8175 | 8174 | 1.00 | 4.35 | 0.092/0.092/0.092 | Yes | orig clean | ccd2:71725 ccd3:88952 ccd4:62961 ccd5:60033 ccd6:90648 ccd7:71975 |
filter=Thick date-obs=2011-09-06T08:42:53 object=Crab roll_angle=87.2057647705 |
148 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
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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 Sat Nov 26 09:55:05 2011
This data set was last accessed on Sat Nov 26 09:55:05 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0611181201
Position of field target = 5 34 32.00 22 0 52.0
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