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 | 10522 | 10129 | 2437 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:33556 ccd2:11296 ccd3:11517 ccd4:11512 ccd5:10395 ccd6:10029 ccd7:9583 |
filter=CalClosed date-obs=2003-10-28T10:59:24 object=0848+1119 roll_angle=104.850135803 |
|
pn | 9820 | 7104 | 5230 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:64287 ccd2:62080 ccd3:41688 ccd4:70887 ccd5:55959 ccd6:41854 ccd7:53950 ccd8:52270 ccd9:35695 ccd10:47948 ccd11:47041 ccd12:36337 |
filter=Medium date-obs=2003-10-28T07:52:58 object=0848+1119 timedel=0.07 roll_angle=104.850135803 |
19 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 Mon May 28 06:07:04 2012
This data set was last accessed on Mon May 28 06:07:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0148742501
Position of field target = 8 50 45.70 11 8 40.0
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