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 | 44115 | 43134 | 36054 | 1.00 | 4.35 | 0.033/0.031/0.021 | Yes | orig clean | ccd1:1128996 ccd2:44771 ccd3:56691 ccd4:44777 ccd5:48162 ccd7:42999 |
filter=Medium date-obs=2011-04-02T10:12:08 object=MAXI J0556-332 roll_angle=265.711303711 |
|
mos2 | 43855 | 43383 | 35522 | 1.00 | 4.35 | 0.012/0.012/0.0046 | Yes | orig clean | ccd2:43212 ccd3:45855 ccd4:38936 ccd5:44664 ccd6:52872 ccd7:44737 |
filter=Medium date-obs=2011-04-02T10:12:13 object=MAXI J0556-332 roll_angle=265.711303711 |
54 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
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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 Dec 17 01:51:03 2011
This data set was last accessed on Sat Dec 17 01:51:03 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0656781101
Position of field target = 5 56 46.30 -33 10 28.2
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