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 | 16224 | 16224 | 16224 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:19374 ccd3:37333 ccd4:27431 ccd5:27981 ccd6:35793 ccd7:20502 |
filter=Thick date-obs=2004-03-22T16:39:59 object=Serpens X-1 roll_angle=89.4338989258 |
|
mos2 | 16227 | 16227 | 16227 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:24092 ccd3:31781 ccd4:21708 ccd5:25556 ccd6:37411 ccd7:28663 |
filter=Thick date-obs=2004-03-22T16:40:01 object=Serpens X-1 roll_angle=89.4338989258 |
65 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 = 6.13
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 May 3 08:14:05 2013
This data set was last accessed on Fri May 3 08:14:05 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0084020401
Position of field target = 18 39 57.00 5 2 6.0
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