New spectroscopic confirmations of Lyman-$\hat{I}\pm$ emitters at z $\sim$ 7 from the LAGER survey

Abstract

We report spectroscopic confirmations of 15 Lyman-alpha galaxies at $z\sim 7$, implying a spectroscopic confirmation rate of $\sim$80% on candidates selected from LAGER (Lyman-Alpha Galaxies in the Epoch of Reionization), which is the largest (24 deg${}^2$) survey aimed at finding Lyman-alpha emitters (LAEs) at $z\sim 7$ using deep narrow-band imaging from DECam at CTIO. LAEs at high-redshifts are sensitive probes of cosmic reionization and narrow-band imaging is a robust and effective method for selecting a large number of LAEs. In this work, we present results from the spectroscopic follow-up of LAE candidates in two LAGER fields, COSMOS and WIDE-12, using observations from Keck/LRIS. We report the successful detection of Ly$\hat{I}\pm$ emission in 15 candidates (11 in COSMOS and 4 in WIDE-12 fields). Three of these in COSMOS have matching confirmations from a previous LAGER spectroscopic follow-up and are part of the overdense region, LAGER-$z7$OD1. Additionally, two candidates that were not detected in the LRIS observations have prior spectroscopic confirmations from Magellan. Including these, we obtain a spectroscopic confirmation success rate of $\sim$$80$% for LAGER LAE candidates. Apart from Ly$\hat{I}\pm$, we do not detect any other UV nebular lines in our LRIS spectra; however, we estimate a 2$\ddot{I}ƒ$ upper limit for the ratio of NV/Ly$\hat{I}\pm$, $f_{NV}/f_{Ly\hat{I}\pm }\lesssim 0.27$, which implies that ionizing emission from these sources is mostly dominated by star formation. Including confirmations from this work, a total of 33 LAE sources from LAGER are now spectroscopically confirmed. LAGER has more than doubled the sample of spectroscopically confirmed LAE sources at $z\sim 7$.

8 pages, 4 figures; Submitted to ApJ