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The Size and Pervasiveness of Ly$\alpha$-UV Spatial Offsets in Star-Forming Galaxies at $z\sim6$

Authors :
Lemaux, B. C.
Fuller, S.
Bradač, M.
Pentericci, L.
Hoag, A.
Strait, V.
Treu, T.
Alvarez, C.
Bolan, P.
Gandhi, P. J.
Jones, T.
Mason, C.
Pelliccia, D.
Ribeiro, B.
Ryan, R. E.
Schmidt, K. B.
Vanzella, E.
Khusanova, Y.
Fèvre, O. Le
Guaita, L.
Hathi, N. P.
Koekemoer, A.
Pforr, J.
Lemaux, B. C.
Fuller, S.
Bradač, M.
Pentericci, L.
Hoag, A.
Strait, V.
Treu, T.
Alvarez, C.
Bolan, P.
Gandhi, P. J.
Jones, T.
Mason, C.
Pelliccia, D.
Ribeiro, B.
Ryan, R. E.
Schmidt, K. B.
Vanzella, E.
Khusanova, Y.
Fèvre, O. Le
Guaita, L.
Hathi, N. P.
Koekemoer, A.
Pforr, J.
Publication Year :
2020

Abstract

We study the projected spatial offset between the ultraviolet continuum and Ly$\alpha$ emission for 65 lensed and unlensed galaxies in the Epoch of Reionization ($5\leq z\leq7$), the first such study at these redshifts, in order to understand the potential for these offsets to confuse estimates of the Ly$\alpha$ properties of galaxies observed in slit spectroscopy. While we find that ~40% of galaxies in our sample show significant projected spatial offsets ($|\Delta_{Ly\alpha-UV}|$), we find a modest average offset of 0.61$\pm$0.08 kpc. A small fraction of our sample, ~10%, exhibits offsets of 2-4 kpc, sizes that are larger than the effective radii of typical galaxies at these redshifts. An internal comparison and a comparison to studies at lower redshift yielded no significant evidence of evolution of $|\Delta_{Ly\alpha-UV}|$ with redshift. In our own sample, UV-bright galaxies showed offsets a factor of three greater than their fainter counterparts, 0.89$\pm$0.18 vs. 0.27$\pm$0.05 kpc, respectively. We argue that offsets are likely not the result of merging processes, but are rather due to internal anisotropic processes resulting from stellar feedback facilitates Ly$\alpha$ fluorescence and/or backscattering from nearby or outflowing gas. The reduction in the Ly$\alpha$ flux due to offset effects for various observational setups was quantified through mock observations of simple simulations. It was found that the loss of Ly$\alpha$ photons for galaxies with average offsets is not, if corrected for, a limiting factor for all but the narrowest slit widths (<0.4''). However, for the largest offsets, if such offsets are mostly perpendicular to the slit major axis, slit losses were found to be extremely severe in cases where slit widths of $\leq$1'' were employed, such as those planned for James Webb Space Telescope/NIRSpec observations. (abridged)<br />Comment: 21 pages, 7 figures, 2 tables. Updated with the accepted MNRAS version that includes minor changes to the text and two tables

Details

Database :
OAIster
Publication Type :
Electronic Resource
Accession number :
edsoai.on1176403482
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1093.mnras.stab924