Gamma-ray detection of newly discovered Ancora supernova remnant: G288.8–6.3

Open Access

Table 3

Naima fit parameters.

Model	W_e/p	s	E_cut	B₀
	(erg)	–	(GeV)	(µG)
	>1 GeV
2 , leptonic
2 , hadronic			–	–

3 , leptonic
3 , hadronic			–	–

Notes. We used an exponentially cutoff power-law model for the underlying electron and proton distributions to fit the data points of model 2 and model 3.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.