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 | 38044 | 38036 | 36691 | 1.00 | 4.35 | 0.0044/0.0044/0.0037 | Yes | orig clean | ccd1:22661 ccd2:12545 ccd3:15588 ccd4:12032 ccd5:13354 ccd6:14955 ccd7:12120 |
filter=Thin1 date-obs=2000-10-01T03:59:48 object=PSR J0751+18 roll_angle=101.480430603 |
|
mos2 | 38041 | 38041 | 36247 | 1.00 | 4.35 | 0.0045/0.0045/0.0036 | Yes | orig clean | ccd1:24212 ccd2:12624 ccd3:14557 ccd4:11695 ccd5:12664 ccd6:16811 ccd7:13646 |
filter=Thin1 date-obs=2000-10-01T03:59:51 object=PSR J0751+18 roll_angle=101.480430603 |
44 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 Wed Nov 30 19:18:17 2011
This data set was last accessed on Wed Nov 30 19:18:17 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111100301
Position of field target = 7 51 9.00 18 7 39.0
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