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 | 127246 | 127199 | 126050 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:35494 ccd2:18115 ccd3:22248 ccd4:17425 ccd5:18591 ccd6:21527 ccd7:17384 |
filter=Thick date-obs=2003-11-27T23:07:17 object=JUPITER roll_angle=114.350814819 |
|
mos2 | 127238 | 127204 | 126314 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:35974 ccd2:18379 ccd3:19800 ccd4:16577 ccd5:17192 ccd6:22927 ccd7:19284 |
filter=Thick date-obs=2003-11-27T23:07:19 object=JUPITER roll_angle=114.350814819 |
|
pn | 126072 | 125670 | 122113 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:29652 ccd2:27271 ccd3:23427 ccd4:41504 ccd5:24339 ccd6:24435 ccd7:28141 ccd8:29750 ccd9:25622 ccd10:22152 ccd11:23394 ccd12:23489 |
filter=Thick date-obs=2003-11-27T23:26:57 object=JUPITER timedel=0.05 roll_angle=114.350814819 |
206 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 Sun Feb 12 09:55:03 2012
This data set was last accessed on Sun Feb 12 09:55:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0200080701
Position of field target = 11 12 58.20 6 11 42.4
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