tar-forming and starburst galaxies (SFGs and SBGs) are powerful emitters of non-thermal γ-rays and neutrinos, due to their intense phases of star-formation activity, which should confine high-energy Cosmic-Rays (CRs) inside their environments. In this paper, using the publicly-available \texttt{fermitools}, we analyse 15.3 years of γ-ray between 1−1000GeV data for 70 sources, 56 of which were not previously detected. We find at 4σ level an indication of γ-ray emission for other two SBGs, namely M 83 and NGC 1365. By contrast, we find that, even with the new description of background, the significance for the γ-ray emission of M 33 (initially reported as discovered) still stands at ∼4σ (as already reported by previous works). Along with previous findings, the flux of each detected source is consistent with a ∼E−2.3/2.4 spectrum, compatible with the injected CR flux inferred for CRs in the Milky-Way. We notice that the correlation between the calorimetric fraction Fcal of high-energy protons in SFGs and SBGs (the fraction of high-energy protons actually producing high-energy γ-rays and neutrinos) and the SFR is in accordance with the expected scaling relation for CR escape dominated by advection. We remark that undiscovered sources strongly constrain Fcal at 95\% CL, providing fundamental information when we interpret the results as common properties of SFGs and SBGs. Finally, we find that these sources might contribute (12±3)% to the EGB, while the corresponding diffuse neutrino flux strongly depends on the spectral index distribution along the source class.
Constraining the hadronic properties of star-forming galaxies above 1 GeV with 15-years Fermi-LAT data
Chianese, M.;
2024-01-01
Abstract
tar-forming and starburst galaxies (SFGs and SBGs) are powerful emitters of non-thermal γ-rays and neutrinos, due to their intense phases of star-formation activity, which should confine high-energy Cosmic-Rays (CRs) inside their environments. In this paper, using the publicly-available \texttt{fermitools}, we analyse 15.3 years of γ-ray between 1−1000GeV data for 70 sources, 56 of which were not previously detected. We find at 4σ level an indication of γ-ray emission for other two SBGs, namely M 83 and NGC 1365. By contrast, we find that, even with the new description of background, the significance for the γ-ray emission of M 33 (initially reported as discovered) still stands at ∼4σ (as already reported by previous works). Along with previous findings, the flux of each detected source is consistent with a ∼E−2.3/2.4 spectrum, compatible with the injected CR flux inferred for CRs in the Milky-Way. We notice that the correlation between the calorimetric fraction Fcal of high-energy protons in SFGs and SBGs (the fraction of high-energy protons actually producing high-energy γ-rays and neutrinos) and the SFR is in accordance with the expected scaling relation for CR escape dominated by advection. We remark that undiscovered sources strongly constrain Fcal at 95\% CL, providing fundamental information when we interpret the results as common properties of SFGs and SBGs. Finally, we find that these sources might contribute (12±3)% to the EGB, while the corresponding diffuse neutrino flux strongly depends on the spectral index distribution along the source class.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
