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Timing Analysis with INTEGRAL: Comparing Different Reconstruction AlgorithmsINTEGRAL is one of the few instruments capable of detecting X-rays above 20keV. It is therefore in principle well suited for studying X-ray variability in this regime. Because INTEGRAL uses coded mask instruments for imaging, the reconstruction of light curves of X-ray sources is highly non-trivial. We present results from the comparison of two commonly employed algorithms, which primarily measure flux from mask deconvolution (ii-lc-extract) and from calculating the pixel illuminated fraction (ii-light). Both methods agree well for timescales above about 10 s, the highest time resolution for which image reconstruction is possible. For higher time resolution, ii-light produces meaningful results, although the overall variance of the lightcurves is not preserved.
Document ID
20110007123
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Grinberg, V.
(Remeis Observatory Bamberg, Germany)
Kreykenboehm, I.
(Remeis Observatory Bamberg, Germany)
Fuerst, F.
(Remeis Observatory Bamberg, Germany)
Wilms, J.
(Remeis Observatory Bamberg, Germany)
Pottschmidt, K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Bel, M. Cadolle
(European Space Astronomy Center (ESAC) Madrid, Spain)
Rodriquez, J.
(Saclay Research Centre Gif-sur-Yvette, France)
Marcu, D. M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Suchy, S.
(California Univ., San Diego La Jolla, CA, United States)
Markowitz, A.
(California Univ., San Diego La Jolla, CA, United States)
Nowak, M. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Date Acquired
August 25, 2013
Publication Date
April 14, 2010
Subject Category
Astronomy
Meeting Information
Meeting: 7th INTEGRAL/BART Workshop
Location: Carlsbad
Country: Czech Republic
Start Date: April 14, 2010
End Date: April 18, 2010
Funding Number(s)
CONTRACT_GRANT: NNG06E090A
Distribution Limits
Public
Copyright
Public Use Permitted.
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