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 | 110059 | 110059 | 104363 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:120305 ccd2:64452 ccd3:78680 ccd4:65648 ccd5:66414 ccd7:60620 |
filter=Medium date-obs=2011-04-14T10:33:22 object=PSR J2022+3842 roll_angle=90.4519729614 |
|
mos2 | 109657 | 109649 | 108177 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:55408 ccd3:55531 ccd4:46239 ccd5:52300 ccd6:65898 ccd7:53635 |
filter=Medium date-obs=2011-04-14T10:35:45 object=PSR J2022+3842 roll_angle=90.4519729614 |
51 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 May 28 13:11:03 2012
This data set was last accessed on Mon May 28 13:11:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0652770101
Position of field target = 20 22 22.00 38 42 15.0
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