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 | 88553 | 88095 | 75306 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:392345 ccd2:93603 ccd3:113949 ccd4:102031 ccd5:98790 ccd7:89489 |
filter=Thin1 date-obs=2009-01-02T19:33:18 object=NGC5506 roll_angle=112.994720459 |
|
mos2 | 88558 | 88101 | 76013 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:387560 ccd2:81862 ccd3:87759 ccd4:71434 ccd5:79358 ccd6:102013 ccd7:82541 |
filter=Thin1 date-obs=2009-01-02T19:33:17 object=NGC5506 roll_angle=112.994720459 |
|
pn | 88407 | 88407 | 87255 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:1011730 |
filter=Thin1 date-obs=2009-01-02T19:38:29 object=NGC5506 timedel=0.00 roll_angle=112.994720459 |
22 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 Mon May 28 20:01:28 2012
This data set was last accessed on Mon May 28 20:01:28 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0554170101
Position of field target = 14 13 14.90 -3 12 27.0
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