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 | 5161 | 5161 | 5161 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:53 ccd2:1033 ccd3:1234 ccd4:1205 ccd5:1254 ccd6:1260 ccd7:1050 |
filter=Thick date-obs=2005-03-04T16:31:52 object=HR 6299 roll_angle=95.6227416992 |
|
pn | 4970 | 4970 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:1241 |
filter=Thick date-obs=2005-03-04T16:37:05 object=HR 6299 timedel=0.00 roll_angle=95.6227416992 |
2 source(s) in memory Iteration: 1 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 Tue Sep 10 22:36:11 2013
This data set was last accessed on Tue Sep 10 22:36:11 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0201952101
Position of field target = 16 57 40.00 9 22 30.0
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