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 | 16960 | 16266 | 847 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:856 ccd2:432 ccd3:496 ccd5:499 |
filter=Medium date-obs=2012-03-07T05:17:14 object=HESS J1804-216-NE roll_angle=89.900604248 |
|
pn | 13392 | 13102 | 12974 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:17017 ccd2:17538 ccd3:12492 ccd4:19313 ccd5:15241 ccd6:13727 ccd7:11170 ccd8:11160 ccd9:8674 ccd10:9756 ccd11:10279 ccd12:8337 |
filter=Medium date-obs=2012-03-07T05:39:28 object=HESS J1804-216-NE timedel=0.07 roll_angle=89.900604248 |
22 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 = 6.13
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 Sun May 5 20:26:28 2013
This data set was last accessed on Sun May 5 20:26:28 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0673690101
Position of field target = 18 6 16.40 -21 25 11.0
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