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Question ID = 0152

Assigned Member (担当者)

2012-01-19, M.Nakajima

Name and Institute (質問者/機関)

Yang Huan
University of Science and Technology of China
(Graduated student, first year)

Question (質問)

The question is about the calibration uncertainty of XIS at energy <1 kev.
We extracted spectra of Mrk 352 using the latest calibration,
and fit the XIS and PIN spectra simultaneously. The spectra <1 kev
seem to have large uncertainty. And XIS0 spectra at energy <1 kev are
not consistent with XIS3. We find that a "pcfabs" component is needed
in the best fit model, but this is very sensitive to the soft band
spectra. We hope to make sure that if the need of this component is
due to the <1 kev uncertainty. From the "Suzaku Memo", the effective
area of XRT response at energy <1 kev are not well calibrated. How can
we deal with these uncertainty? Are there some compromised way, for
example, drop the XIS0 and XIS3 spectra below 1kev, only use XIS1?

Answer from(回答の文責)

Takayuki Tamura

Answer (答え)

Your question was answered by an expert on the XIS from the XIS help team as given below.

from here --------------------------
The inconsistency in the soft-band response between XIS0 and XIS3 clearly suggests that the problem stems from the uncertainty in the calibration of the OBF contamination. You can find a discussion on this issue in Sect.5.4.3 in the following documents.

http://www.astro.isas.jaxa.jp/~tsujimot/td_xis.pdf.

All the sensors suffer the same problem in a different degree and the calibration uncertainty is different among the sensors. Users need to make a judgement which senrors to use in what energy band based on their scientific goals.

For conpromise, you can adjust the contamination model by yourself. The model includes the H, C, N, and O column densities as a function of time for each sensor. You can refer to the closest calibration observations of PKS2155-304 and RXJ1856.5-3754 to guess the values of these free parameters. For a detailed procedure, contact the XIS help at xishelp AT astro.isas.jaxa.jp.
end here --------------------------

You can also check the following pages and papers on the calibration in general.

Status (詳細なステータス)

2012-01-19 Accept
2012-01-26 Answered
2012-02-06 Done

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