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 | 7600 | 7600 | 7408 | 1.00 | 4.35 | 0.0053/0.0053/0.0048 | Yes | orig clean | ccd1:7221 ccd2:3085 ccd3:3665 ccd4:2811 ccd5:3069 ccd6:3296 ccd7:3312 |
filter=Medium date-obs=2001-09-19T10:40:04 object=Mrk 3 roll_angle=97.7058029175 |
|
mos2 | 7602 | 7602 | 7346 | 1.00 | 4.35 | 0.0051/0.0051/0.0045 | Yes | orig clean | ccd1:7077 ccd2:2759 ccd3:3590 ccd4:2529 ccd5:2846 ccd6:3543 ccd7:2903 |
filter=Medium date-obs=2001-09-19T10:40:02 object=Mrk 3 roll_angle=97.7058029175 |
11 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 Sun Dec 25 09:55:07 2011
This data set was last accessed on Sun Dec 25 09:55:07 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0009221001
Position of field target = 6 15 36.30 71 2 15.0
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