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 | 4996 | 4996 | 4992 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:170 ccd2:1405 ccd3:4527 ccd4:2310 ccd5:2689 ccd6:2753 ccd7:1487 |
filter=Medium date-obs=2000-02-05T13:16:29 object=PSR0540 roll_angle=228.513809204 |
|
mos2 | 3598 | 3598 | 3598 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:120 ccd2:1878 ccd3:1060 ccd4:1867 ccd5:3826 ccd6:2210 ccd7:2073 |
filter=Medium date-obs=2000-02-05T15:44:17 object=PSR0540 roll_angle=228.513809204 |
28 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 Fri May 25 16:15:04 2012
This data set was last accessed on Fri May 25 16:15:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0116690801
Position of field target = 5 39 43.30 -69 19 60.0
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