Processing completion:

Field: acisf13341

Detector Exposure (Original/Cleaned) Image binning Plate scale ("/pixel) Bgd. level (orig/cleaned, counts/sq. arcmin/s) GTI file Bgd. light curves Roll angle CCD counts Extra info
ccd6 1539 | 1539 1.00 0.49 0.0035/0.0035 Yes orig clean
ccd7 1539 | 1539 1.00 0.49 0.0065/0.0065 Yes orig clean
acis 1539 | 1539 4.00 1.97 0/0 Yes orig clean 17.5 ccd6:410 ccd7:754 ccd8:330 datamode=VFAINT
CCD Temp=-119
object=SDSS J1319+4456
ACIS data processing version=8.4.3
Original CALDB version=4.4.8
timedel=3.14 (full readout)
CIAO_version=CIAO 4.3

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

10 source(s) in memory
Iteration: 2
|ccd6 |ccd7 |acis |
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
CIAO version = 4.3.0
XAssist version = 1.000
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Mon May 6 00:30:06 2013
This data set was last accessed on Mon May 6 00:30:06 2013
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf13341
Position of field target = 13 19 27.60 44 56 56.5
Current telescope = chandra
Current detector = acis
Processing mode = proc
Processing status = OK
Detection method = wavelet
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Will skip analysis of CCD 8

Log files: processing messages |error messages |all messages (very detailed) |source logs