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Question ID = 0030

Assigned Member (担当者)

2006-11-16 Y. Urata
2006-12-25 Y. Terada

Name and Institute (質問者/機関)

Oleg Kargaltsev (Penn State University, USA)

Question (質問)

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

Answer from(回答の文責)

Y.Terada (Software team / Suzaku Help)

Answer (答え)

  • 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.

Status (詳細なステータス)

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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