First Sample of H$\hat{I}\pm$+[O III] $\hat{I}»$5007 Line Emitters at $z>6$ Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line Luminosity Functions

Abstract

We present a sample of four emission-line galaxies at $z=6.11-6.35$ that were serendipitously discovered using the commissioning data for the JWST/NIRCam wide-field slitless spectroscopy (WFSS) mode. One of them (at $z=6.11$) has been reported previously while the others are new discoveries. These sources are selected by the secure detections of both [O III] $\hat{I}»$5007 and H$\hat{I}\pm$ lines with other fainter lines tentatively detected in some cases (e.g., [O II] $\hat{I}»$3727, [O III] $\hat{I}»$4959). In the [O III]/H${\hat{I}}^2$ - [N II]/H$\hat{I}\pm$ Baldwin-Phillips-Terlevich diagram, these galaxies occupy the same parameter space as that of $z\sim 2$ star-forming galaxies, indicating that they have been enriched rapidly to sub-solar metallicities ($\sim$0.4 $Z_{\odot }$), similar to galaxies with comparable stellar masses at much lower redshifts. The detection of strong H$\hat{I}\pm$ lines suggests a higher ionizing photon production efficiency within galaxies in the early Universe. We find brightening of the [O III] $\hat{I}»$5007 line luminosity function (LF) from $z=3$ to 6, and weak or no redshift evolution of the H$\hat{I}\pm$ line LF from $z=2$ to 6. Both LFs are under-predicted at $z\sim 6$ by a factor of $\sim$10 in certain cosmological simulations. This further indicates a global Ly$\hat{I}\pm$ photon escape fraction of 7-10% at $z\sim 6$, slightly lower than previous estimates through the comparison of the UV-derived star-formation rate density and Ly$\hat{I}\pm$ luminosity density. Our sample recovers $66_{-44}^{+128}$% of $z=6.0-6.6$ galaxies in the survey volume with stellar masses greater than $5\times 10^8$ $M_{\odot }$, suggesting the ubiquity of strong H$\hat{I}\pm$ and [O III] line emitters in the Epoch of Reionization, which will be further uncovered in the era of JWST.

26 pages, 11 figures, accepted for publication in ApJ on May 11, 2023