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 | 27407 | 27397 | 21167 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:70618 ccd2:42796 ccd3:52434 ccd4:40426 ccd5:41909 ccd7:40796 |
filter=Medium date-obs=2011-08-07T06:32:00 object=NLTT 7887 roll_angle=61.6951942444 |
|
pn | 18940 | 10906 | 5434 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:133781 ccd2:130536 ccd3:86830 ccd4:141482 ccd5:111141 ccd6:84264 ccd7:132444 ccd8:130159 ccd9:87574 ccd10:111583 ccd11:110348 ccd12:82750 |
filter=Medium date-obs=2011-08-07T06:54:21 object=NLTT 7887 timedel=0.07 roll_angle=61.6951942444 |
9 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 Tue May 21 09:06:24 2013
This data set was last accessed on Tue May 21 09:06:24 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0670650101
Position of field target = 2 24 40.83 40 8 23.0
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