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 | 70367 | 67798 | 57155 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:252484 ccd2:127621 ccd3:143748 ccd4:119574 ccd5:119573 ccd7:113147 |
filter=Medium date-obs=2011-08-14T17:48:53 object=HD101088 roll_angle=330.539520264 |
|
pn | 62097 | 48301 | 31014 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:423359 ccd2:413311 ccd3:277898 ccd4:568199 ccd5:350637 ccd6:264826 ccd7:381969 ccd8:375220 ccd9:255064 ccd10:334503 ccd11:335642 ccd12:254307 |
filter=Medium date-obs=2011-08-14T17:54:54 object=HD101088 timedel=0.07 roll_angle=330.539520264 |
47 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 Mon Jun 3 07:38:05 2013
This data set was last accessed on Mon Jun 3 07:38:05 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0672080101
Position of field target = 11 37 14.70 -69 40 27.2
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