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 | 22092 | 22092 | 18124 | 1.00 | 4.35 | 0.022/0.022/0.012 | Yes | orig clean | ccd1:191717 ccd2:34633 ccd3:42528 ccd4:33921 ccd5:34986 ccd7:32504 |
filter=Thin1 date-obs=2009-04-18T11:57:27 object=4U 1907+09 roll_angle=77.2489700317 |
|
mos2 | 21843 | 21827 | 18499 | 1.00 | 4.35 | 0.016/0.016/0.0094 | Yes | orig clean | ccd2:28376 ccd3:28224 ccd4:23977 ccd5:26972 ccd6:35062 ccd7:27110 |
filter=Thin1 date-obs=2009-04-18T11:57:22 object=4U 1907+09 roll_angle=77.2489700317 |
2 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 Wed Nov 30 20:25:07 2011
This data set was last accessed on Wed Nov 30 20:25:07 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0555410101
Position of field target = 19 9 37.90 9 49 49.0
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