Spectroscopic identification of a redshift 1.55 supernova host galaxy from the Subaru Deep Field Supernova Survey

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Table 1

Spectroscopic summary.

Line	Wavelength	Flux
	(nm)	(10^-19 erg s^-1 cm^-2)

Hα	1671.91 ± 0.05	37.8 ± 4.3
[N ii] 6583	1677.46 ± 0.12	8.3 ± 2.2
[S ii] 6716	1711.18 ± 0.13	12.9 ± 2.9
[S ii] 6731	1714.64 ± 0.09	8.5 ± 1.7

[O iii] 5007^a	...	< 23.2 ± 10.4
[O iii] 4959^a	...	< 9.1 ± 10.4

Notes.

^(a)

This is the 3σ upper limit on the flux, measured from the variance in the spectrum at the location of the lines.

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