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 | 0 | 1.00 | 1.00 | 0/0 | Yes | orig clean |
date-obs=2001-12-05T18:42:25 object= roll_angle=247.901885986 |
||
mos2 | 30944 | 30939 | 21328 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:146585 ccd2:106745 ccd3:166948 ccd4:98647 ccd5:168943 ccd6:190484 ccd7:105681 |
filter=CalClosed date-obs=2001-12-05T18:42:34 object=AR Lacertae roll_angle=247.901885986 |
65 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 Mon May 27 10:10:13 2013
This data set was last accessed on Mon May 27 10:10:13 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111370101
Position of field target = 22 8 40.82 45 44 32.1
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