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 | 38626 | 38621 | 38621 | 1.00 | 4.35 | 0.025/0.025/0.025 | Yes | orig clean | ccd2:68312 ccd3:131715 ccd4:94040 ccd5:83649 ccd6:131501 ccd7:73161 |
filter=Thick date-obs=2001-10-09T09:18:30 object=4U1820-30 roll_angle=270.125061035 |
|
mos2 | 39003 | 31998 | 31998 | 1.00 | 4.35 | 0.087/0.082/0.082 | Yes | orig clean | ccd1:4015447 ccd2:90298 ccd3:118432 ccd4:80171 ccd5:85294 ccd6:129798 ccd7:101738 |
filter=Thick date-obs=2001-10-09T09:18:23 object=4U1820-30 roll_angle=270.125061035 |
205 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 Tue Nov 29 09:59:03 2011
This data set was last accessed on Tue Nov 29 09:59:03 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0084110201
Position of field target = 18 23 40.60 -30 21 41.0
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