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- W3025342824 abstract "Abstract In this paper, we estimate the cross-correlation power spectra between the Planck 2018 cosmic microwave background (CMB) temperature anisotropy map and the unresolved γ -ray background (UGRB) from the 9-years Fermi-Large Area Telescope (LAT) data. In this analysis, we use up to nine energy bins over a wide energy range of [0.631, 1000] GeV from the Fermi-LAT UGRB data. Firstly, we find that the Fermi data with the energy ranges [1.202, 2.290] GeV and [17.38, 36.31] GeV show the positive evidence for the Integrated Sachs-Wolfe (ISW) effect at 1 . 8 σ confidence level, and the significance would be increased to 2 . 7 σ when using these two energy bins together. Secondly, we apply the single power-law model to normalize the amplitude and use all the nine Fermi energy bins to measure the significance of the ISW effect, we obtained A amp = 0 . 95 ± 0 . 53 (68% C.L.). For the robustness test, we implement a null hypothesis by randomizing the Fermi mock maps of nine energy bins and obtain the non-detection of ISW effect, which confirms that the ISW signal comes from the Fermi-LAT diffuse γ -ray data and is consistent with the standard Λ CDM model prediction essentially. We use a cross-correlation coefficient to show the relation between different energy bins. Furthermore, we vary the cut ranges | b | of galactic plane on the mask of Fermi map and carefully check the consequent influence on the ISW signal detection." @default.
- W3025342824 created "2020-05-21" @default.
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- W3025342824 date "2020-09-01" @default.
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- W3025342824 title "Searching for Integrated Sachs–Wolfe Effect from Fermi-LAT diffuse <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline id=d1e979 altimg=si8.svg><mml:mi>γ</mml:mi></mml:math>-ray map" @default.
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- W3025342824 doi "https://doi.org/10.1016/j.dark.2020.100585" @default.
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