Spatially Extended Low Ionization Emission Regions (LIERs) at $z\sim0.9$
R. E. Hviding, G. B. Brammer, I. G. Momcheva, B. F. Lundgren, D., Marchesini, N. Pirzkal, R. E. Ryan, A. Vang, D. A. Wake, M. Bourque, C., Martlin, K. V. Nedkova

TL;DR
This study presents spatially resolved emission diagnostics of eight galaxies at z~0.9, revealing extended LINER-like emission regions likely originating from star formation rather than active galactic nuclei, using modified BPT diagnostics.
Contribution
First evidence of non-AGN LINER-like emission at high redshift using spatially resolved diagnostics and a modified BPT diagram.
Findings
Extended LINER-like emission detected in all candidates.
X-ray data suggests star formation, not AGN, as the emission source.
First high-redshift evidence for non-AGN LINER-like emission.
Abstract
We present spatially resolved emission diagnostics for eight galaxies that demonstrate extended low ionization emission-line regions (LIERs) over kpc scales. Eight candidates are selected based on their spatial extent and emission line fluxes from slitless spectroscopic observations with the HST/WFC3 G141 and G800L grisms in the well-studied GOODS survey fields. Five of the candidates (62.5%) are matched to X-ray counterparts in the \textit{Chandra X-Ray Observatory} Deep Fields. We modify the traditional Baldwin-Philips-Terlevich (BPT) emission line diagnostic diagram to use [SII]/(H+[NII]) instead of [NII]/H to overcome the blending of [NII] and H+[NII] in the low resolution slitless grism spectra. We construct emission line ratio maps and place the individual pixels in the modified BPT. The extended LINER-like emission present in all of our…
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