Processing completion:

Field: xmm0083150201

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 15091 | 15083 | 15019 1.00 4.35 0/0 Yes orig clean ccd1:33393 ccd2:4850 ccd3:6057 ccd4:4516 ccd5:5022 ccd6:5630 ccd7:4299 filter=Thin1
mos2 15101 | 15083 | 15019 1.00 4.35 0/0 Yes orig clean ccd1:34352 ccd2:4631 ccd3:5374 ccd4:4318 ccd5:4563 ccd6:5964 ccd7:5082 filter=Thin1
pn 12722 | 12080 | 10549 1.00 4.35 0/0 Yes orig clean ccd1:17268 ccd2:13596 ccd3:9155 ccd4:56491 ccd5:15434 ccd6:9187 ccd7:26568 ccd8:15366 ccd9:9060 ccd10:14360 ccd11:12150 ccd12:8743 filter=Thin1

Source List (gives positions and fluxes and links for detailed analyses)

47 source(s) in memory
Iteration: 2
|mos1 |mos2 |pn |
init Complete
acquire Complete
reduce Complete
detect Complete
timeclean Complete
simplespatial Complete
assess Complete
extract Complete
reassess Complete
spectral Complete
temporal Complete
spatial Complete
correl Skip
sim Skip
qlook Skip
xray image
skyview image

Xray image, smoothed with a 2 pixel gaussian

Skyview image(s) of FOV (with X-ray sources marked)

Color code (marks may only appear on detector-specific images for multi-detector missions, see links above): green = point source, red = problematic/questionable source, blue = extended source, magenta = asymmetric source (may be extended), cyan = estimated detector boundary, purple = "Region of Interest" (if set)

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 = 6.13
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 May 5 00:38:03 2013
This data set was last accessed on Sun May 5 00:38:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0083150201
Position of field target = 23 36 30.84 21 8 46.0
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