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 |
---|---|---|---|---|---|---|---|---|---|
mos2 | 20171 | 19982 | 15054 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:22538 ccd3:24535 ccd4:19816 ccd5:21674 ccd6:28692 ccd7:23913 |
filter=Thin1 date-obs=2003-05-20T11:19:18 object=HU Aqr roll_angle=70.5494232178 |
|
pn | 0 | 1.00 | 1.00 | 0/0 | Yes | orig clean |
date-obs=2003-05-20T10:32:29 object= roll_angle=70.5494232178 |
3 source(s) in memory Iteration: 2 Images: |mos2 |pn |
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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 Mar 4 03:52:05 2012
This data set was last accessed on Sun Mar 4 03:52:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153090101
Position of field target = 21 7 58.30 -5 17 39.4
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