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 | 6316 | 6316 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:8305 ccd2:5842 ccd3:7756 ccd4:5918 ccd5:5604 ccd7:5584 |
filter=CalClosed date-obs=2012-05-18T16:33:47 object=XXLs070 roll_angle=53.8424301147 |
|
pn | 103737 | 94774 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:323402 ccd2:323297 ccd3:226242 ccd4:345572 ccd5:274356 ccd6:218821 ccd7:255149 ccd8:254371 ccd9:181440 ccd10:220141 ccd11:225034 ccd12:175282 |
filter=Thin1 date-obs=2012-05-17T09:15:45 object=XXLs070 timedel=0.07 roll_angle=53.8424301147 |
85 source(s) in memory Iteration: 1 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 Thu May 9 17:24:14 2013
This data set was last accessed on Thu May 9 17:24:14 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0677760101
Position of field target = 23 39 33.70 -55 54 58.0
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = detect did not complete
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