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 | 16401 | 16337 | 13076 | 1.00 | 4.35 | 0.011/0.011/0.003 | Yes | orig clean | ccd2:14559 ccd3:18171 ccd4:14199 ccd5:14323 ccd6:16949 ccd7:13750 |
filter=Thin1 date-obs=2004-05-02T01:53:34 object=RX J0513.9-6951 roll_angle=322.878540039 |
|
mos2 | 16406 | 16406 | 13334 | 1.00 | 4.35 | 0.011/0.011/0.0031 | Yes | orig clean | ccd2:13754 ccd3:15144 ccd4:12612 ccd5:13963 ccd6:18056 ccd7:14876 |
filter=Thin1 date-obs=2004-05-02T01:53:33 object=RX J0513.9-6951 roll_angle=322.878540039 |
9 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 01:51:06 2011
This data set was last accessed on Sat Dec 17 01:51:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0151412101
Position of field target = 5 13 50.80 -69 51 47.0
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