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 | 9391 | 9391 | 8751 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:51568 ccd3:118827 ccd4:81696 ccd5:71668 ccd6:101596 ccd7:57250 |
filter=Thick date-obs=2002-03-08T06:37:18 object=Crab roll_angle=267.338409424 |
|
mos2 | 11848 | 11825 | 9963 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:76352 ccd3:99137 ccd4:70663 ccd5:84628 ccd6:117244 ccd7:87951 |
filter=Thick date-obs=2002-03-08T06:37:22 object=Crab roll_angle=267.338409424 |
226 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
|
|
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 = 6.13
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 May 11 10:54:28 2013
This data set was last accessed on Sat May 11 10:54:28 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153750301
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