Processing completion:

Field: xmm0111510101

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 25370 | 25370 | 22552 1.00 4.35 0/0 Yes orig clean ccd1:71442 ccd2:12983 ccd3:17028 ccd4:12890 ccd5:14044 ccd6:16305 ccd7:13004 filter=Medium
object=AT Microscopii
mos2 24323 | 24310 | 22142 1.00 4.35 0/0 Yes orig clean ccd2:13299 ccd3:14257 ccd4:11946 ccd5:12346 ccd6:15923 ccd7:13729 filter=Medium
object=AT Microscopii
pn 25072 | 25072 | 25071 1.00 4.35 0/0 Yes orig clean ccd4:238810 filter=Medium
object=AT Microscopii

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

21 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 Tue Mar 6 22:41:03 2012
This data set was last accessed on Tue Mar 6 22:41:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111510101
Position of field target = 20 41 51.16 -32 26 6.8
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