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 | 15990 | 15980 | 15980 | 1.00 | 4.35 | 0.0044/0.0044/0.0044 | Yes | orig clean | ccd2:4599 ccd3:7596 ccd4:5665 ccd5:6545 ccd6:7068 ccd7:4603 |
filter=Thick date-obs=2001-01-22T15:32:27 object=XB1254-69 roll_angle=117.845314026 |
|
mos2 | 16752 | 16752 | 16751 | 1.00 | 4.35 | 0.0097/0.0097/0.0097 | Yes | orig clean | ccd1:582730 ccd2:5562 ccd3:6746 ccd4:5569 ccd5:5335 ccd6:8751 ccd7:6184 |
filter=Thick date-obs=2001-01-22T15:22:00 object=XB1254-69 roll_angle=117.845314026 |
13 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 08:01:10 2011
This data set was last accessed on Fri Nov 25 08:01:10 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0060740101
Position of field target = 12 57 37.20 -69 17 21.1
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