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 | 30327 | 30309 | 30308 | 1.00 | 4.35 | 0.0022/0.0022/0.0022 | Yes | orig clean | ccd2:4823 ccd3:6543 ccd4:5691 ccd5:5492 ccd6:6332 ccd7:4962 |
filter=Thick date-obs=2001-02-20T18:01:51 object=1700-37 roll_angle=92.6015167236 |
|
mos2 | 30974 | 30974 | 30966 | 1.00 | 4.35 | 0.0025/0.0025/0.0025 | Yes | orig clean | ccd1:75245 ccd2:5582 ccd3:6221 ccd4:4706 ccd5:5464 ccd6:7539 ccd7:5874 |
filter=Thick date-obs=2001-02-20T17:52:24 object=1700-37 roll_angle=92.6015167236 |
23 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 Sat Dec 24 09:55:06 2011
This data set was last accessed on Sat Dec 24 09:55:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0083280401
Position of field target = 17 3 56.80 -37 50 39.1
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