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 | 70794 | 70258 | 67771 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1791867 ccd2:30063 ccd3:43474 ccd4:32188 ccd5:32106 ccd6:42284 ccd7:29159 |
filter=Thin1 date-obs=2002-12-01T23:00:08 object=Mkn 421 roll_angle=111.855979919 |
|
mos2 | 70791 | 70330 | 67520 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1738614 ccd2:31735 ccd3:36722 ccd4:27871 ccd5:32574 ccd6:40309 ccd7:34484 |
filter=Thin1 date-obs=2002-12-01T23:00:08 object=Mkn 421 roll_angle=111.855979919 |
171 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
|
|
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 Thu May 2 17:49:06 2013
This data set was last accessed on Thu May 2 17:49:06 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0136541001
Position of field target = 11 4 27.31 38 12 31.8
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