paper

HII Region Metallicity Constraints Near the Site of the Strongly Lensed Supernova "SN Refsdal" at Redshift 1.49

arXiv:1503.08822 · doi:10.1088/2041-8205/804/1/L14

Abstract

We present the local HII region metallicity near the site of the recently discovered multiply lensed supernova (SN; "SN Refsdal") at redshift 1.49. "SN Refsdal" is located at the outer spiral arm (7 kpc) of the lensed host galaxy, which we have previously reported to exhibit a steep negative galactocentric metallicity gradient. Based on our updated near-infrared integral field spectroscopic data, the gas-phase metallicity averaged in an intrinsic radius of 550 pc surrounding an HII region 200 pc away from the SN site is 12 + log(O/H) 8.67. The metallicity averaged over nine HII regions at similar galactocentric distances (5-7 kpc) as "SN Refsdal" is constrained to be 12 + log(O/H) 8.11. Given the fortuitous discovery of "SN Refsdal" in an advantageously lensed face-on spiral, this is the first observational constraint on the local metallicity environment of an SN site at redshift .

5 pages, 3 figures, 1 table; accepted for publication in ApJ Letters

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