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 | 69106 | 68989 | 68221 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:109221 ccd2:15833 ccd3:17999 ccd4:13724 ccd5:13823 ccd6:17886 ccd7:13971 |
filter=Thin1 date-obs=2002-10-09T03:33:16 object=PSR J0437-4715 roll_angle=138.7006073 |
|
mos2 | 69104 | 69088 | 68384 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:117357 ccd2:14188 ccd3:15314 ccd4:14303 ccd5:14405 ccd6:18154 ccd7:15163 |
filter=Thin1 date-obs=2002-10-09T03:33:16 object=PSR J0437-4715 roll_angle=138.7006073 |
72 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 2 23:09:04 2012
This data set was last accessed on Sat Jun 2 23:09:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0112320201
Position of field target = 4 37 16.00 -47 15 8.0
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