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 | 43215 | 43197 | 43197 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:53451 ccd2:14258 ccd3:16730 ccd4:13528 ccd5:14070 ccd7:12697 |
filter=Medium date-obs=2011-03-17T11:43:36 object=AX J1754.2-2754 roll_angle=90.4510955811 |
|
mos2 | 43220 | 43210 | 43210 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:52023 ccd2:13080 ccd3:12976 ccd4:11848 ccd5:12479 ccd6:16025 ccd7:13461 |
filter=Medium date-obs=2011-03-17T11:43:36 object=AX J1754.2-2754 roll_angle=90.4510955811 |
31 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
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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 Thu Jun 21 07:02:01 2012
This data set was last accessed on Thu Jun 21 07:02:01 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0651450101
Position of field target = 17 54 14.50 -27 54 35.6
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