Evidence for hybrid gamma-ray emission from the supernova remnant G150.3+4.5

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Table 2

Results of energy-dependent extension measurements of SNR G150.3+4.5 with 2D Gaussian template.

Energy range	Best-fit position (RA, Dec)	Extension r₆₈	TS	TS_ext
2–10 GeV	(66.°43±0.°06, 55.°16±0.°05)	$1 \overset{°}{.} 31_{- 0 \overset{°}{.} 07}^{+ 0 \overset{°}{.} 06}$ $1\mathop .\limits^^\circ 31_{ - 0\mathop .\limits^^\circ 07}^{ + 0\mathop .\limits^^\circ 06}$	168	137
10–100 GeV	(66.°78 ± 0.°05, 55.°49 ± 0.°05)	$1 \overset{°}{.} 38_{- 0 \overset{°}{.} 05}^{+ 0 \overset{°}{.} 06}$ $1\mathop .\limits^^\circ 38_{ - 0\mathop .\limits^^\circ 05}^{ + 0\mathop .\limits^^\circ 06}$	381	310
100 GeV–1 TeV	(66.°82±0.°04, 55.°61 ± 0.°05)	$1 \overset{°}{.} 17_{- 0 \overset{°}{.} 05}^{+ 0 \overset{°}{.} 07}$ $1\mathop .\limits^^\circ 17_{ - 0\mathop .\limits^^\circ 05}^{ + 0\mathop .\limits^^\circ 07}$	94	42

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