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 | 66602 | 66474 | 62896 | 1.00 | 4.35 | 0.0062/0.0061/0.0043 | Yes | orig clean | ccd1:54739 ccd2:30967 ccd3:36916 ccd4:32004 ccd5:29364 ccd7:29471 |
filter=Medium date-obs=2010-03-29T12:16:33 object=PSR B1937+21 roll_angle=92.6506271362 |
|
mos2 | 66607 | 66541 | 63599 | 1.00 | 4.35 | 0.0051/0.005/0.0036 | Yes | orig clean | ccd1:48323 ccd2:27184 ccd3:26870 ccd4:22739 ccd5:24510 ccd6:31388 ccd7:27953 |
filter=Medium date-obs=2010-03-29T12:16:33 object=PSR B1937+21 roll_angle=92.6506271362 |
17 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 Sun Dec 18 01:51:04 2011
This data set was last accessed on Sun Dec 18 01:51:04 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0605370101
Position of field target = 19 39 38.56 21 34 59.1
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