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 | 48428 | 48428 | 46449 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:626468 ccd2:44282 ccd3:60253 ccd4:49213 ccd5:44970 ccd7:42776 |
filter=Thick date-obs=2010-05-03T07:20:20 object=Mkn 421 roll_angle=296.364868164 |
|
pn | 7169 | 7169 | 7169 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:9972 ccd2:2981 ccd3:2147 ccd4:1069147 ccd5:10290 ccd6:3448 ccd7:58146 ccd8:9341 ccd9:3284 ccd10:4937 ccd11:2428 ccd12:2040 |
filter=Thick date-obs=2010-05-03T07:48:37 object=Mkn 421 timedel=0.05 roll_angle=296.364868164 |
19 source(s) in memory Iteration: 2 Images: |mos1 |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 Fri May 17 08:56:13 2013
This data set was last accessed on Fri May 17 08:56:13 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0656380101
Position of field target = 11 4 27.31 38 12 31.8
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = extract did not complete
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