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 | 66478 | 66436 | 64521 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:137503 ccd2:32346 ccd3:40332 ccd4:30417 ccd5:35660 ccd6:37961 ccd7:31522 |
filter=Medium date-obs=2001-08-12T04:00:29 object=Proxima Centauri roll_angle=284.209411621 |
|
mos2 | 66442 | 66442 | 64975 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:137920 ccd2:31994 ccd3:36107 ccd4:28485 ccd5:31276 ccd6:41455 ccd7:34454 |
filter=Medium date-obs=2001-08-12T04:00:28 object=Proxima Centauri roll_angle=284.209411621 |
|
pn | 65645 | 65645 | 65644 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:450664 |
filter=Medium date-obs=2001-08-12T04:16:02 object=Proxima Centauri timedel=0.00 roll_angle=284.209411621 |
19 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |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 = 6.11
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 Sun Aug 19 09:55:04 2012
This data set was last accessed on Sun Aug 19 09:55:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0049350101
Position of field target = 14 29 42.08 -62 40 44.9
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