Measurement of the extragalactic background light imprint on the spectra of the brightest blazars observed with H.E.S.S.

Free Access

Table 5

EBL wavelength range probed by the data sets used in this study.

Data set	z	E_min − E_max	λ_min − λ_max
		[TeV]	[μm]

Mrk 421 (1)	0.031	0.95−41	1.2−49
Mrk 421 (2)	0.031	0.95−37	1.2−44
Mrk 421 (3)	0.031	0.95−45	1.2−53
PKS 2005 - 489 (1)	0.071	0.16−37	0.22−44
PKS 2005 - 489 (2)	0.071	0.18−25	0.25−30
PKS 2155 - 304 (2008)	0.116	0.13 − 19	0.30−23
PKS 2155 - 304 (1)	0.116	0.13 − 5.7	0.19−6.8
PKS 2155 - 304 (2)	0.116	0.13 − 9.3	0.19−11
PKS 2155 - 304 (3)	0.116	0.13 − 14	0.19−17
PKS 2155 - 304 (4)	0.116	0.18 − 4.6	0.19−5.5
PKS 2155 - 304 (5)	0.116	0.13 − 5.7	0.27−6.8
PKS 2155 - 304 (6)	0.116	0.15 − 5.7	0.19−6.8
PKS 2155 - 304 (7)	0.116	0.20 − 7.6	0.22−9.0
1ES 0229+200	0.14	0.29 − 25	0.45−30
H 2356 - 309	0.165	0.11 − 34	0.18−40
1ES 1101-232	0.186	0.12 − 23	0.20−27
1ES 0347-121	0.188	0.13 − 11	0.22−13

Notes. The redshifts of the sources are given in Col. 2. The energy range of the spectra (in TeV) is given in Col. 3, and the EBL wavelengths probed with the subsets are given in Col. 4, where only the peak of the pair-creation cross-section is taken into account.

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.