Processing completion:

Field: xmm0109463601

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 5138 | 5138 | 5137 1.00 4.35 0.0033/0.0033/0.0033 Yes orig clean ccd2:1312 ccd3:1632 ccd4:1260 ccd5:1455 ccd6:1570 ccd7:1335 filter=Thin1
object=CP Tuc
mos2 5399 | 5399 | 5399 1.00 4.35 0.0032/0.0032/0.0032 Yes orig clean ccd1:82 ccd2:1353 ccd3:1559 ccd4:1254 ccd5:1360 ccd6:1705 ccd7:1358 filter=Thin1
object=CP Tuc
pn 4600 | 4600 | 4594 1.00 4.35 0.017/0.017/0.017 Yes orig clean ccd4:1512 filter=Thin1
object=CP Tuc

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

12 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 Nov 28 02:37:10 2011
This data set was last accessed on Mon Nov 28 02:37:10 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0109463601
Position of field target = 23 15 19.00 -59 10 28.0
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