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 | 9399 | 9399 | 9398 | 1.00 | 4.35 | 0.0018/0.0018/0.0018 | Yes | orig clean | ccd2:1289 ccd3:1595 ccd4:1289 ccd5:1264 ccd6:1460 ccd7:1329 |
filter=Thin1 date-obs=2003-11-09T22:33:00 object=RX J1914+24 roll_angle=242.216018677 |
|
mos2 | 9666 | 9666 | 9536 | 1.00 | 4.35 | 0.002/0.002/0.0017 | Yes | orig clean | ccd1:1996 ccd2:1537 ccd3:1642 ccd4:1420 ccd5:1326 ccd6:1749 ccd7:1507 |
filter=Medium date-obs=2003-11-09T22:33:06 object=RX J1914+24 roll_angle=242.216018677 |
|
pn | 9472 | 9472 | 9440 | 1.00 | 4.35 | 0.013/0.013/0.013 | Yes | orig clean | ccd4:9013 |
filter=Thin1 date-obs=2003-11-09T22:38:16 object=RX J1914+24 timedel=0.00 roll_angle=242.216018677 |
12 source(s) in memory Iteration: 2 Images: |mos1 |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 = 6.11
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 Thu Dec 1 05:15:16 2011
This data set was last accessed on Thu Dec 1 05:15:16 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0109500101
Position of field target = 19 14 26.10 24 56 43.6
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