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 | 31767 | 31752 | 30792 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:545976 ccd2:112140 ccd3:163393 ccd4:130458 ccd5:120544 ccd7:119226 |
filter=CalMedium date-obs=2006-04-28T13:42:51 object=PSR B0833-45 roll_angle=295.344421387 |
|
mos2 | 31757 | 31754 | 31562 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:661628 ccd2:183857 ccd3:253242 ccd4:213548 ccd5:281722 ccd6:283719 ccd7:178387 |
filter=CalMedium date-obs=2006-04-28T13:42:56 object=PSR B0833-45 roll_angle=295.344421387 |
|
pn | 120821 | 120789 | 120484 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:3303344 |
filter=Medium date-obs=2006-04-27T13:00:19 object=PSR B0833-45 timedel=0.00 roll_angle=295.344421387 |
102 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 Sun Jun 24 20:39:02 2012
This data set was last accessed on Sun Jun 24 20:39:02 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153951401
Position of field target = 8 35 22.00 -45 10 48.0
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