Testing the molecular cloud paradigm for ultra-high-energy gamma ray emission from the direction of SNR G106.3+2.7

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Volume 691 (November 2024)

A&A, 691 (2024) A89

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Table 1.

Best-fit results from the source search.

RA [°]	Dec [°]	Radius [°]
337.20 $_{(- 0.12)}^{(+ 0.12)}_{(- 0.33)}^{(+ 0.26)}$ $^{(+0.12)}_{(-0.12)} ^{(+0.26)}_{(-0.33)}$	60.92 $_{(- 0.05)}^{(+ 0.05)}_{(- 0.11)}^{(+ 0.13)}$ $^{(+0.05)}_{(-0.05)} ^{(+0.13)}_{(-0.11)}$	0.34 $_{(- 0.04)}^{(+ 0.04)}_{(- 0.13)}^{(+ 0.12)}$ $^{(+0.04)}_{(-0.04)} ^{(+0.12)}_{(-0.13)}$

N₀ [×10⁻¹⁵ cm⁻² TeV⁻¹ s⁻¹]	α	β

1.86 $_{(- 0.27)}^{(+ 0.32)}_{(- 1.10)}^{(+ 1.33)}$ $^{(+0.32)}_{(-0.27)} ^{(+1.33)}_{(-1.10)}$	2.76 $_{(- 0.16)}^{(+ 0.16)}_{(- 0.60)}^{(+ 0.84)}$ $^{(+0.16)}_{(-0.16)} ^{(+0.84)}_{(-0.60)}$	0.32 $_{(- 0.13)}^{(+ 0.13)}_{(- 0.49)}^{(+ 1.05)}$ $^{(+0.13)}_{(-0.13)} ^{(+1.05)}_{(-0.49)}$

Notes. The first uncertainties listed are statistical and the second uncertainties are systematic. The spectral values are quoted assuming the spectral parameters as defined in Equation (2).

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