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 | 5257 | 5245 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:37198 ccd3:45639 ccd4:35721 ccd5:39169 ccd6:42315 ccd7:35201 |
filter=Medium date-obs=2002-03-27T01:19:45 object=Her X-1 roll_angle=75.9790420532 |
|
mos2 | 5437 | 5136 | 4882 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:83113 ccd2:37554 ccd3:39066 ccd4:33363 ccd5:37020 ccd6:44174 ccd7:39833 |
filter=Medium date-obs=2002-03-27T01:19:38 object=Her X-1 roll_angle=75.9790420532 |
5 source(s) in memory Iteration: 1 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 Wed May 1 07:36:08 2013
This data set was last accessed on Wed May 1 07:36:08 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153950401
Position of field target = 16 57 49.80 35 20 32.6
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = Warning, bgd. level not computed because source mask doesn't exist
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