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 | 35381 | 35381 | 31349 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:29665 ccd2:16575 ccd3:21490 ccd4:16013 ccd5:16308 ccd6:20370 ccd7:16112 |
filter=Medium date-obs=2002-06-19T08:35:55 object=PSR J0034-0534 roll_angle=65.5238113403 |
|
mos2 | 35386 | 35371 | 32042 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:28512 ccd2:15388 ccd3:16831 ccd4:14009 ccd5:15204 ccd6:18988 ccd7:15746 |
filter=Medium date-obs=2002-06-19T08:35:54 object=PSR J0034-0534 roll_angle=65.5238113403 |
39 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 = 6.13
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 24 02:52:04 2013
This data set was last accessed on Fri May 24 02:52:04 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0031740101
Position of field target = 0 34 21.82 -5 34 36.5
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