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 | 54715 | 54702 | 49843 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:80468 ccd2:43979 ccd3:54336 ccd4:43328 ccd5:50459 ccd7:40613 |
filter=Medium date-obs=2010-08-20T23:04:57 object=Centaurus A roll_angle=306.160766602 |
|
mos2 | 54720 | 54699 | 50795 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:67149 ccd2:35141 ccd3:34955 ccd4:29983 ccd5:33405 ccd6:44475 ccd7:35097 |
filter=Medium date-obs=2010-08-20T23:04:56 object=Centaurus A roll_angle=306.160766602 |
|
pn | 52696 | 46056 | 27672 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:201088 ccd2:194852 ccd3:132498 ccd4:215855 ccd5:173759 ccd6:134700 ccd7:184832 ccd8:182643 ccd9:124934 ccd10:159408 ccd11:158905 ccd12:120125 |
filter=Medium date-obs=2010-08-20T23:27:18 object=Centaurus A timedel=0.07 roll_angle=306.160766602 |
62 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |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 Feb 14 20:41:01 2012
This data set was last accessed on Tue Feb 14 20:41:01 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0651710101
Position of field target = 13 27 48.75 -43 2 16.5
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