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 | 3515 | 3497 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:31212 ccd3:38971 ccd4:30066 ccd5:32354 ccd6:36265 ccd7:30596 |
filter=Medium date-obs=2002-10-04T12:48:02 object=Her X-1 roll_angle=251.419998169 |
|
mos2 | 3562 | 2450 | 1285 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:63562 ccd2:29364 ccd3:31858 ccd4:25931 ccd5:28679 ccd6:36284 ccd7:30059 |
filter=Medium date-obs=2002-10-04T12:47:57 object=Her X-1 roll_angle=251.419998169 |
1 source(s) in memory Iteration: 1 Images: |mos1 |mos2 |
|
|
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 = 6.13
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 Sep 9 02:16:02 2013
This data set was last accessed on Mon Sep 9 02:16:02 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111062301
Position of field target = 16 57 49.80 35 20 32.6
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = Warning, bgd. level not computed because source mask doesn't exist
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