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 | 27943 | 27943 | 27943 | 1.00 | 4.35 | 0.0019/0.0019/0.0019 | Yes | orig clean | ccd2:4071 ccd3:5275 ccd4:3864 ccd5:4057 ccd6:5306 ccd7:4097 |
filter=Thick date-obs=2001-01-26T20:20:58 object=lam Andromeda roll_angle=224.612091064 |
|
mos2 | 28548 | 28548 | 28544 | 1.00 | 4.35 | 0.0027/0.0027/0.0027 | Yes | orig clean | ccd1:191556 ccd2:4171 ccd3:5012 ccd4:3727 ccd5:4081 ccd6:5157 ccd7:4625 |
filter=Thick date-obs=2001-01-26T20:10:31 object=lam Andromeda roll_angle=224.612091064 |
|
pn | 28200 | 28200 | 28199 | 1.00 | 4.35 | 0.14/0.14/0.14 | Yes | orig clean | ccd4:528957 |
filter=Thick date-obs=2001-01-26T20:24:00 object=lam Andromeda timedel=0.00 roll_angle=224.612091064 |
16 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 Mon Dec 26 14:15:06 2011
This data set was last accessed on Mon Dec 26 14:15:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0099320101
Position of field target = 23 37 33.84 46 27 29.3
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