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Question ID = 0140

Assigned Member (担当者)

2011-03-17 T. Tamura
2011-03-21 Y.Terada

Name and Institute (質問者/機関)

Mr. Yang Huan (Univ. of Science and Technology of China)

Question (質問)

After the standard reprocess pipeline, the exposure time of XIS clean events is about 106 ks, while that of HXD(PIN&GSO) clean events is only about 6ks. The clean events of PIN have only about 3000 counts in a 100ks observation! Why most of the HXD events have been filtered while the XIS events seem to be ok? I check the filtering GTI files, and the cause may be HXD telemetry saturation. If this is true, then what causes the telemetry saturation?

Answer from(回答の文責)

Y.Terada (HXD team) and N.Yamasaki, M.Ishida (Operation team)

Answer (答え)

  • Technical Answers
    The small number of the exposure of the HXD of OBSID = 704016010 is caused by the telemetry saturation of the data acquisition system on-board the spacecraft. During this observation, the electrical noises of PIN diodes are tentatively high around the lower energy channels and thus most of the telemetry is occupied by such noise events.
  • Political notes
    As described in the Technical description of Suzaku (see the reference below), an exposure of an observation as a point of view of the data rights for PIs is calculated only by the XIS, and the PI of the observation of OBSID = 704016010 agreed on the above situation, thus this observation was completed. No additional observations were performed.
  • (ref) Technical description, Section 4.4
    Note that this will be judged based on the good time intervals of the cleaned XIS event files after the standard screening. Dead times (including those due to the use of the burst option) are not taken into account. Also, the standard screening for the HXD is more strict, so the effective exposure for the HXD is of ten smaller than that of the XIS by 20% or more. Additional observations will be scheduled automatically for those non-time-critical targets the observations of which are considered incomplete by the project scientist at ISAS. In the case of time-critical observations which are incomplete or unusable, it will be the PI's responsibility to determine the best course of action.

Status (詳細なステータス)

2011-03-17 Accepted
2011-03-17 Resolved, HXD team
2011-03-22 Circulated to the Suzaku operation for policy
2011-03-22 Resolved, Suzaku team
2011-03-25 Answer to GO
2011-03-26 Closed

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