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 | 13351 | 13351 | 13351 | 1.00 | 4.35 | 0.0051/0.0051/0.0051 | Yes | orig clean | ccd2:5652 ccd3:8649 ccd4:4912 ccd5:4319 ccd7:5481 |
filter=Medium date-obs=2006-10-02T01:01:39 object=PSRB 0540-69 roll_angle=104.011039734 |
|
mos2 | 13354 | 13354 | 13353 | 1.00 | 4.35 | 0.005/0.005/0.005 | Yes | orig clean | ccd2:5637 ccd3:4929 ccd4:6344 ccd5:7450 ccd6:6127 ccd7:4158 |
filter=Medium date-obs=2006-10-02T01:01:39 object=PSRB 0540-69 roll_angle=104.011039734 |
31 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 Fri Nov 25 07:59:05 2011
This data set was last accessed on Fri Nov 25 07:59:05 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0413180201
Position of field target = 5 40 11.00 -69 19 58.0
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