fullrun_all_xmm0122900701

Processing completion:

Field: xmm0122900701

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
pn 1001 | 1001 | 1000 1.00 4.35 0/0 Yes orig clean ccd1:387 ccd2:272 ccd3:211 ccd4:349 ccd5:279 ccd6:228 ccd7:393 ccd8:412 ccd9:254 ccd10:557 ccd11:310 ccd12:231 filter=Thin1
date-obs=2000-04-15T06:57:14
object=Canopus z-1.5
timedel=0.07
roll_angle=301.342926025

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

4 source(s) in memory
Iteration: 2
Images:
|pn |
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
 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 Feb 13 21:45:23 2012
This data set was last accessed on Mon Feb 13 21:45:23 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0122900701
Position of field target = 6 15 31.50 -51 55 36.5
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