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 | 11074 | 7620 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:51026 ccd3:61765 ccd4:52404 ccd5:53710 ccd6:57801 ccd7:50212 |
filter=Thin1 date-obs=2003-09-02T13:01:17 object=BY Cam roll_angle=99.2660064697 |
|
mos2 | 10954 | 8144 | 2650 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:52130 ccd3:57313 ccd4:47099 ccd5:50261 ccd6:66523 ccd7:57273 |
filter=Thin1 date-obs=2003-09-02T13:01:17 object=BY Cam roll_angle=99.2660064697 |
1 source(s) in memory Iteration: 1 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 Fri May 3 14:14:01 2013
This data set was last accessed on Fri May 3 14:14:01 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0148590501
Position of field target = 5 42 48.90 60 51 31.8
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