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 | 29937 | 29937 | 29681 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:173329 ccd2:104061 ccd3:148629 ccd4:127332 ccd5:108498 ccd6:126141 ccd7:99626 |
filter=CalClosed date-obs=2003-11-19T04:15:56 object=AG Draconis roll_angle=186.482223511 |
|
pn | 10434 | 10432 | 10432 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:3975 ccd2:3594 ccd3:3203 ccd4:4417 ccd5:3219 ccd6:2942 ccd7:3637 ccd8:3936 ccd9:3114 ccd10:3286 ccd11:3073 ccd12:2968 |
filter=Thin1 date-obs=2003-11-19T01:06:47 object=AG Draconis timedel=0.05 roll_angle=186.482223511 |
52 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 Thu May 2 07:40:11 2013
This data set was last accessed on Thu May 2 07:40:11 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0147131101
Position of field target = 16 1 40.94 66 48 9.0
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