Processing completion:

Field: xmm0094780101

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 715 | 710 | 709 1.00 4.35 0/0 Yes orig clean ccd1:212 ccd2:136 ccd3:135 ccd4:124 ccd5:109 ccd6:139 ccd7:132 filter=Thick
mos2 712 | 712 | 712 1.00 4.35 0/0 Yes orig clean ccd1:249 ccd2:124 ccd3:141 ccd4:108 ccd5:102 ccd6:131 ccd7:130 filter=Thick
pn 1058 | 1058 | 993 1.00 4.35 0/0 Yes orig clean ccd1:716 ccd2:922 ccd3:490 ccd4:767 ccd5:643 ccd6:497 ccd7:714 ccd8:824 ccd9:493 ccd10:813 ccd11:626 ccd12:498 filter=Thick

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

20 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 = 6.11
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 Aug 13 09:55:03 2012
This data set was last accessed on Mon Aug 13 09:55:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0094780101
Position of field target = 3 47 18.00 24 22 31.0
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