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 | 6647 | 6647 | 6646 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1151 ccd2:1810 ccd3:2260 ccd4:1696 ccd5:1906 ccd6:2004 ccd7:1705 |
filter=Medium date-obs=2001-03-09T21:08:43 object=NOVA Sgr 1998 roll_angle=88.5137405396 |
|
mos2 | 6646 | 6646 | 6645 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1141 ccd2:1739 ccd3:2103 ccd4:1623 ccd5:1748 ccd6:2346 ccd7:1872 |
filter=Medium date-obs=2001-03-09T21:08:48 object=NOVA Sgr 1998 roll_angle=88.5137405396 |
|
pn | 4951 | 4949 | 4949 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:2595 ccd2:2450 ccd3:2139 ccd4:3261 ccd5:2404 ccd6:2364 ccd7:2707 ccd8:2749 ccd9:2209 ccd10:2261 ccd11:2234 ccd12:2088 |
filter=Medium date-obs=2001-03-09T21:32:23 object=NOVA Sgr 1998 timedel=0.05 roll_angle=88.5137405396 |
12 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 Jun 3 09:13:15 2012
This data set was last accessed on Sun Jun 3 09:13:15 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0085581201
Position of field target = 18 21 40.47 -27 31 38.0
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