2006-11-16 Y. Urata 
2006-12-25 Y. Terada 
Oleg Kargaltsev (Penn State University, USA)
I am looking at the header of the ae501109010hxd_0_pinno_cl.evt file
which came with the data distribution. 
 
 I am wondering, why in this observation the elapsed time
(TSTOP-TSTART) is about 150 ks while on source time is only about 47
ks. What is the reason for such a big difference? What was happening
during ~70\% of the observing time while the detector was not
observing the source? 
 
 
dmlist ae501109010hxd_0_pinno_cl.evt header | grep TIME 
0027 ONTIME                   46913.0341929495           Real8        On-source time 
 --  HISTORY              TIME START STOP TELAPSE (s) : 205809057.0 205958954.0    149897.0 
 --  HISTORY              START DATE TIME in UTC (MJD): 2006-07-10 01:10:56 (53926.04925926) 
 --  HISTORY              STOP  DATE TIME in UTC (MJD): 2006-07-11 18:49:13 (53927.78417824) 
0061 LIVETIME                 46913.0341929495           Real8        On-source time 
 
Y.Terada (Software team / Suzaku Help)
- 
There's no problem on the pipe-line processing. The value of 
ONTIME is the same value of "TSTART - TSTOP", and the value 
TELAPSE is the same as the summation of 50 time-intervals in 
GTI extension. It is OK.
 
 - 
The reason the efficiency of TELAPSE par ONTIME is low (31%)
is the condition of your observation, we checked. The spacecraft 
has about 90-minutes orbital-period, and sometimes the satellite 
observes the earth (i.e., not the source). In addition, the quality
of the observation becomes bad during the spacecraft passes the SAA, 
or during the time interval that COR is less than 8 GV for the HXD.
 
You can check how the exposure is reduced by accepting cleaning 
criteria, one by one, from unscreened events list, by using the 
following commands on xselct; 
> read event . 
   ae501109010hxd_1_wel_uf.evt ae501109010hxd_2_wel_uf.evt 
> read hk . 
   ae501109010.ehk.gz 
   yes 
> select hk 
    ELV>5 
> extract event 
> save event 
The results are as follows. Thus, about 60 ksec observation of the 
earth and 15 ksec bad-COR intervals are included in your 150 ksec
observation.  
 
Step-0. Unscreened event  
	148956.     seconds 
Step-1. Exclude Earth observation (ELV>5 && DYE_ELV>20) 
	84360.     seconds 
Step-2. Exclude bad COR interval  (++ && COR>8) 
	59701.     seconds 
Step-3. Exclude SAA passage       (++ && SAA_HXD.eq.0 && T_SAA_HXD>436) 
        43932.     seconds 
 
 
Please note that the earth event is very useful if you want to 
check systematic errors of the NXB model of the HXD.
   
2006-11-16 Accept (Y.Urata) 
2006-11-16 Circulated to the Processing team (Assign, Y.Terada) 
2006-11-17 Got Log file in processing 
2006-12-25 Resolved. Got answer from Processing team (Y.Terada) 
2006-12-25 Done (Y.Terada)
 
 
 
 
 
 
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