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 | 3617 | 3617 | 3617 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:59840 ccd2:29300 ccd3:45570 ccd4:28127 ccd5:48230 ccd6:52033 ccd7:28536 |
filter=CalClosed date-obs=2003-04-04T13:12:44 object=SS433 roll_angle=67.7258148193 |
|
pn | 1998 | 1998 | 1998 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:8000 ccd2:8257 ccd3:4969 ccd4:8867 ccd5:7921 ccd6:7684 ccd7:7521 ccd8:8977 ccd9:6262 ccd10:5064 ccd11:3951 ccd12:2293 |
filter=CalClosed date-obs=2003-04-04T13:34:54 object=SS433 timedel=0.07 roll_angle=67.7258148193 |
26 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 = 6.11
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 Sat Jul 14 09:55:04 2012
This data set was last accessed on Sat Jul 14 09:55:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0137150301
Position of field target = 19 11 49.60 4 58 58.0
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