Euclid: ERO -- NISP-only sources and the search for luminous $z=6-8$ galaxies

TL;DR

This study utilizes Euclid's NISP data to identify high-redshift galaxies at z=6-8, revealing a sample of UV-bright candidates and analyzing their properties to enhance understanding of early galaxy formation.

Contribution

It introduces a method for selecting z=6-8 galaxy candidates using Euclid NISP data and characterizes their spectral properties, expanding the known high-redshift galaxy sample.

Findings

Identified 29 Lyman-break galaxy candidates at z≈6-8.

Discovered 139 extremely red sources with diverse properties.

Analyzed contamination sources, including dwarfs and instrumental effects.

Abstract

This paper presents a search for high redshift galaxies from the Euclid Early Release Observations program "Magnifying Lens." The 1.5 deg$^2$ area covered by the twin Abell lensing cluster fields is comparable in size to the few other deep near-infrared surveys such as COSMOS, and so provides an opportunity to significantly increase known samples of rare UV-bright galaxies at $z\approx6-8$ ($M_{\rm UV}\lesssim-22$). Beyond their still uncertain role in reionisation, these UV-bright galaxies are ideal laboratories from which to study galaxy formation and constrain the bright-end of the UV luminosity function. Of the 501994 sources detected from a combined $Y_{\rm E}$, $J_{\rm E}$, and $H_{\rm E}$ NISP detection image, 168 do not have any appreciable VIS/$I_{\rm E}$ flux. These objects span a range in spectral colours, separated into two classes: 139 extremely red sources; and 29 Lyman-break galaxy candidates. Best-fit redshifts and spectral templates suggest the former is composed of both $z\gtrsim5$ dusty star-forming galaxies and $z\approx1-3$ quiescent systems. The latter is composed of more homogeneous Lyman break galaxies at $z\approx6-8$. In both cases, contamination by L- and T-type dwarfs cannot be ruled out with Euclid images alone. Additional contamination from instrumental persistence is investigated using a novel time series analysis. This work lays the foundation for future searches within the Euclid Deep Fields, where thousands more $z\gtrsim6$ Lyman break systems and extremely red sources will be identified.