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[29] Ishiwata, K., Macias, O., Ando, S., and Arimoto, M., “Probing heavy dark matter decays with multi-messenger astrophysical data”, [Journal of Cosmology and Astroparticle Physics], vol. 2020, no. 1, 2020. doi: https://doi.org/10.1088/1475-7516/2020/01/003.
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[27] Macias, O., Horiuchi, S., Kaplinghat, M., Gordon, C., Crocker, R. M., and Nataf, D. M., “Strong evidence that the galactic bulge is shining in gamma rays”, [Journal of Cosmology and Astroparticle Physics], vol. 2019, no. 9, 2019. doi: https://doi.org/10.1088/1475-7516/2019/09/042.
[26] Song, D., Macias, O., and Horiuchi, S., “Inverse Compton emission from millisecond pulsars in the Galactic bulge”, [Physical Review D], vol. 99, no. 12, 2019. doi: https://doi.org/10.1103/PhysRevD.99.123020.
[24] Hashimoto, D., “Measurement of redshift-dependent cross-correlation of HSC clusters and Fermi γ-rays”, [Monthly Notices of the Royal Astronomical Society], vol. 484, no. 4, pp. 5256–5266, 2019. doi: https://doi.org/10.1093/mnras/stz321.
[23] Shirasaki, M., Macias, O., Horiuchi, S., Yoshida, N., Lee, C.-H., and Nishizawa, A. J., “Correlation of extragalactic γ rays with cosmic matter density distributions from weak gravitational lensing”, [Physical Review D], vol. 97, no. 12, 2018. doi: https://doi.org/10.1103/PhysRevD.97.123015.
[22] Macias, O., “Galactic bulge preferred over dark matter for the Galactic centre gamma-ray excess”, [Nature Astronomy], vol. 2, pp. 387–392, 2018. doi: https://doi.org/10.1038/s41550-018-0414-3.
[21] Ploeg, H., Gordon, C., Crocker, R., and Macias, O., “Consistency between the luminosity function of resolved millisecond pulsars and the galactic center excess”, [Journal of Cosmology and Astroparticle Physics], vol. 2017, no. 8, 2017. doi: https://doi.org/10.1088/1475-7516/2017/08/015.
[20] Shirasaki, M., Macias, O., Horiuchi, S., Shirai, S., and Yoshida, N., “Cosmological constraints on dark matter annihilation and decay: Cross-correlation analysis of the extragalactic γ -ray background and cosmic shear”, [Physical Review D], vol. 94, no. 6, 2016. doi: https://doi.org/10.1103/PhysRevD.94.063522.
[19] Lacroix, T., Macias, O., Gordon, C., Panci, P., BÅ`hm, C., and Silk, J., “Spatial morphology of the secondary emission in the Galactic Center gamma-ray excess”, [Physical Review D], vol. 93, no. 10, 2016. doi: https://doi.org/10.1103/PhysRevD.93.103004.
[18] Horiuchi, S., Macias, O., Restrepo, D., Rivera, A., Zapata, O., and Silverwood, H., “The Fermi-LAT gamma-ray excess at the Galactic Center in the singlet-doublet fermion dark matter model”, [Journal of Cosmology and Astroparticle Physics], vol. 2016, no. 3, 2016. doi: https://doi.org/10.1088/1475-7516/2016/03/048.
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[2] Aartsen, M. G., “Search for Time-independent Neutrino Emission from Astrophysical Sources with 3 yr of IceCube Data”, [The Astrophysical Journal], vol. 779, no. 2, 2013. doi: https://doi.org/10.1088/0004-637X/779/2/132.
[1] Gordon, C. and Macías, O., “Dark matter and pulsar model constraints from Galactic Center Fermi-LAT gamma-ray observations”, [Physical Review D], vol. 88, no. 8, 2013. doi: https://doi.org/10.1103/PhysRevD.88.083521.