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 | 4740 | 4735 | 4735 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:22852 ccd2:13308 ccd3:18950 ccd4:16659 ccd5:12954 ccd6:16103 ccd7:12664 |
filter=CalClosed date-obs=2004-07-04T07:02:40 object=MKN 590 roll_angle=65.7002716064 |
|
pn | 43906 | 43906 | 43906 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:188909 |
filter=Thin1 date-obs=2004-07-04T08:36:22 object=MKN 590 timedel=0.00 roll_angle=65.7002716064 |
11 source(s) in memory Iteration: 2 Images: |mos1 |pn |
|
|
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 23 07:00:04 2013
This data set was last accessed on Thu May 23 07:00:04 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0201020201
Position of field target = 2 14 33.56 -0 46 0.1
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