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 | 69530 | 68960 | 64148 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:66236 ccd2:35933 ccd3:55746 ccd4:35731 ccd5:34536 ccd6:42354 ccd7:35223 |
filter=Medium date-obs=2002-04-14T21:58:44 object=PSR J2124-3358 roll_angle=76.7437515259 |
|
mos2 | 69517 | 69243 | 64388 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:66833 ccd2:34528 ccd3:38868 ccd4:31059 ccd5:42712 ccd6:43641 ccd7:36782 |
filter=Medium date-obs=2002-04-14T21:58:42 object=PSR J2124-3358 roll_angle=76.7437515259 |
68 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 Jun 16 06:59:09 2012
This data set was last accessed on Sat Jun 16 06:59:09 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0112320601
Position of field target = 21 24 44.00 -33 58 44.0
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