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 | 33386 | 33382 | 33190 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:10224 ccd2:20780 ccd3:25218 ccd4:19219 ccd5:21469 ccd7:19335 |
filter=Medium date-obs=2008-08-25T05:03:43 object=IGR J00291+5934 roll_angle=33.9355735779 |
|
mos2 | 33391 | 33381 | 33381 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:8235 ccd2:16238 ccd3:16915 ccd4:14199 ccd5:17885 ccd6:20503 ccd7:16526 |
filter=Medium date-obs=2008-08-25T05:03:38 object=IGR J00291+5934 roll_angle=33.9355735779 |
22 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 = 6.11
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 Wed Mar 7 18:25:07 2012
This data set was last accessed on Wed Mar 7 18:25:07 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0560180201
Position of field target = 0 29 3.10 59 34 19.2
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