Electromagnetic cascade masquerade: a way to mimic γ-axion-like particle mixing effects in blazar spectra

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Table 1

Observations of extreme TeV blazars used in this paper.

N	Source	z	Observational period	References

1	H 1426+428	0.129	1999–2000	1
2	H 1426+428	0.129	1998–2000	2
3	H 1426+428	0.129	2001	3
4	1ES 0229+200	0.140	2005–2006	4
5	1ES 0229+200	0.140	2010–2012	5
6	1ES 1218+304	0.182	2012–2013	6
7	1ES 1101-232	0.186	2004–2005	7
8	1ES 1101-232	0.186	2004–2005	8
9	1ES 0347-121	0.188	Aug.–Dec. 2006	9
10	1ES 0414+009	0.287	2005–2009	10

Reference. (1) Aharonian et al. (2003); (2) Djannati-Atai et al. (2002); (3) Horan et al. (2002); (4) Aharonian et al. (2007a); (5) Aliu et al. (2014); (6) Madhavan et al. (2013); (7) Aharonian et al. (2007b); (8) Aharonian et al. (2006); (9) Aharonian et al. (2007c); (10) Abramowski et al. (2012).

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