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 | 31115 | 31112 | 27848 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:41806 ccd2:24016 ccd3:28846 ccd4:24759 ccd5:23197 ccd7:22941 |
filter=Medium date-obs=2008-04-20T11:49:38 object=PSR J1853+1303 roll_angle=74.474647522 |
|
mos2 | 31120 | 31120 | 27792 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:39108 ccd2:21588 ccd3:22553 ccd4:18813 ccd5:20575 ccd6:26374 ccd7:21361 |
filter=Medium date-obs=2008-04-20T11:49:38 object=PSR J1853+1303 roll_angle=74.474647522 |
16 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
|
|
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 Jul 30 08:49:10 2012
This data set was last accessed on Mon Jul 30 08:49:10 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0503190301
Position of field target = 18 53 57.32 13 3 44.1
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