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 |
---|---|---|---|---|---|---|---|---|---|
mos2 | 2077 | 2077 | 2077 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:7521 ccd2:468 ccd3:511 ccd4:424 ccd5:432 ccd6:580 ccd7:452 |
filter=Thin1 date-obs=2003-06-28T16:28:48 object=Abell 2597 roll_angle=69.2769012451 |
|
pn | 1880 | 1880 | 1880 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:7272 ccd2:7187 ccd3:4742 ccd4:8042 ccd5:6925 ccd6:6872 ccd7:6867 ccd8:8289 ccd9:5731 ccd10:4757 ccd11:3944 ccd12:2430 |
filter=CalClosed date-obs=2003-06-27T08:30:31 object=Abell 2597 timedel=0.19 roll_angle=69.2769012451 |
6 source(s) in memory Iteration: 2 Images: |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 = 6.13
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 Thu Jun 13 00:38:03 2013
This data set was last accessed on Thu Jun 13 00:38:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0147330101
Position of field target = 23 25 18.00 -12 6 30.0
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