fullrun_all_xmm0656580301

Processing completion:

Field: xmm0656580301

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 6084 | 5749 | 4987 1.00 4.35 0/0 Yes orig clean ccd2:7326 ccd3:8973 ccd4:7954 ccd5:7783 ccd7:7051 filter=Medium
date-obs=2012-03-15T11:28:10
object=Mkn3
roll_angle=277.541290283
mos2 5910 | 5704 | 5638 1.00 4.35 0/0 Yes orig clean ccd2:6496 ccd3:6906 ccd4:5840 ccd5:6280 ccd6:8658 ccd7:6990 filter=Medium
date-obs=2012-03-15T18:15:45
object=Mkn3
roll_angle=277.541290283

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

2 source(s) in memory
Iteration: 2
Images:
|mos1 |mos2 |
PackageState
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
 No Skyview images present

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 Tue Jul 24 13:43:02 2012
This data set was last accessed on Tue Jul 24 13:43:02 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0656580301
Position of field target = 6 15 36.30 71 2 15.0
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