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 | 33096 | 33080 | 30366 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:45216 ccd2:21256 ccd3:25304 ccd4:22327 ccd5:20795 ccd7:20053 |
filter=Medium date-obs=2007-07-09T08:46:35 object=The Antennae roll_angle=297.017272949 |
|
pn | 31349 | 26504 | 16050 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:154099 ccd2:149918 ccd3:100499 ccd4:185212 ccd5:129719 ccd6:97052 ccd7:134504 ccd8:132531 ccd9:89203 ccd10:84890 ccd11:86845 ccd12:64025 |
filter=Thin1 date-obs=2007-07-09T09:08:54 object=The Antennae timedel=0.07 roll_angle=297.017272949 |
44 source(s) in memory Iteration: 2 Images: |mos1 |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 = 6.11
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 Sun Mar 11 14:57:05 2012
This data set was last accessed on Sun Mar 11 14:57:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0500070501
Position of field target = 12 1 52.10 -18 51 33.6
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