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 | 19919 | 17579 | 13813 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:82960 ccd2:50735 ccd3:50866 ccd4:48996 ccd5:38883 ccd7:47917 |
filter=Thin1 date-obs=2012-06-29T09:04:35 object=2PIGG_1799 roll_angle=53.7376823425 |
|
pn | 14461 | 7880 | 6216 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:259642 ccd2:250498 ccd3:170467 ccd4:270521 ccd5:212409 ccd6:161448 ccd7:254639 ccd8:224242 ccd9:152272 ccd10:162975 ccd11:161732 ccd12:123231 |
filter=Thin1 date-obs=2012-06-29T09:26:50 object=2PIGG_1799 timedel=0.07 roll_angle=53.7376823425 |
15 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 Fri Jul 26 09:14:11 2013
This data set was last accessed on Fri Jul 26 09:14:11 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0693741001
Position of field target = 1 14 34.43 -33 56 9.8
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