A Tentative Detection of an Emission Line at 1.6 {\mu}m for the z~12 Candidate UDFj-39546284
Gabriel B. Brammer, Pieter G. van Dokkum, Garth D. Illingworth,, Rychard J. Bouwens, Ivo Labbe, Marijn Franx, Ivelina Momcheva, Pascal A., Oesch

TL;DR
This study reports a tentative detection of an emission line in a high-redshift galaxy candidate, exploring whether it indicates a z~12 galaxy or a lower-redshift interloper, with implications for early universe observations.
Contribution
The paper introduces a novel spectroscopic analysis technique for slitless HST data and presents the first tentative emission line detection in a z~12 galaxy candidate.
Findings
Detected a 2.7σ emission line at 1.599 μm in the candidate galaxy.
The line could be Ly-α at z=12.12 or [O III] at z=2.19, with current evidence favoring the latter.
Identified nearby [O III] emitters and a z=1.605 [O III] blob supporting a lower-redshift interpretation.
Abstract
We present deep WFC3 grism observations of the candidate z~12 galaxy UDFj-39546284 in the HST Ultra Deep Field (UDF), by combining spectroscopic data from the 3D-HST and CANDELS surveys. The total exposure time is 40.5 ks and the spectrum covers 1.10 < {\lambda} < 1.65{\mu}m. We search for faint emission lines by cross-correlating the 2D G141 spectrum with the observed H160 morphology, a technique that is unique to slitless spectroscopy at HST resolution. We find a 2.7{\sigma} detection of an emission line at 1.599 {\mu}m---just redward of the JH140 filter---with flux 3.5 +/- 1.3x10-18 erg/s/cm2. Assuming the line is real, it contributes 110 +/- 40% of the observed H160 flux and has an observed equivalent width > 7300 {\AA}. If the line is confirmed, it could be Ly-{\alpha} at z = 12.12. However, a more plausible interpretation, given current results, could be a lower redshift feature…
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