Detection of very-high-energy γ-ray emission from the colliding wind binary η Car with H.E.S.S.

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Table 1

Properties of the data sets used in this work to calculate the spectral points and the light-curve shown in Figs. 3 and 4, respectively.

Data Set	Observation time	Phase	Live time
(DS)	Modified Julian date (MJD)		(h)
I	56439−56444	0.78	0.9
	56666−56667	0.89	0.8
	56741−56751	0.93	9.4
	56775−56778	0.95	0.9
	56797−56799	0.96	1.8

II	56803−56807	0.96	3.3
	57066−57074	1.09	8.6
	57077−57079	1.10	4.0

All	56439−57079	0.78−1.10	29.7

Notes. The time interval of the H.E.S.S. observations, the total live time corresponding to the individual data sets, along with the covered orbital phase are summarised.

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