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 | 58103 | 54047 | 25647 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:187872 ccd2:104514 ccd3:113971 ccd4:93353 ccd5:99234 ccd6:131915 ccd7:113578 |
filter=Thin1 date-obs=2003-07-27T10:07:16 object=SN 1995N roll_angle=288.0362854 |
|
pn | 1880 | 1880 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:6608 ccd2:6488 ccd3:4085 ccd4:7225 ccd5:6414 ccd6:6256 ccd7:6086 ccd8:7333 ccd9:5153 ccd10:4043 ccd11:3154 ccd12:1692 |
filter=CalClosed date-obs=2003-07-27T06:30:32 object=SN 1995N timedel=0.19 roll_angle=288.0362854 |
15 source(s) in memory Iteration: 1 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 = 6.13
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 Thu May 30 08:44:04 2013
This data set was last accessed on Thu May 30 08:44:04 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0149620201
Position of field target = 14 49 28.27 -10 10 15.4
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