Processing completion:

Field: xmm0550451201

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 17639 | 14683 | 4443 1.00 4.35 0/0 Yes orig clean ccd1:156670 ccd2:92505 ccd3:99030 ccd4:95789 ccd5:111203 ccd7:95508 filter=Thin1
object=IGR J16185-5928
mos2 17467 | 15461 | 5599 1.00 4.35 0/0 Yes orig clean ccd1:161452 ccd2:82554 ccd3:77839 ccd4:70095 ccd5:73056 ccd6:97727 ccd7:82905 filter=Thin1
object=IGR J16185-5928
pn 17992 | 17832 | 12032 1.00 4.35 0/0 Yes orig clean ccd4:187409 filter=Thin1
object=IGR J16185-5928

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

8 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 = xmm0550451201
Position of field target = 16 18 36.48 -59 27 18.0
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