86 citations · 244 across the 6 of their papers we have counts for
7 papers
A large, deep 3 deg survey of H, [OIII], and [OII] emitters from LAGER: constraining luminosity functions
Ali Ahmad Khostovan, Sangeeta Malhotra, James E. Rhoads +14
We present our measurements of the H, [OIII], and [OII] luminosity functions as part of the Lyman Alpha Galaxies at Epoch of Reionization (LAGER) survey using our samples of 157…
Lyman Alpha Galaxies in the Epoch of Reionization (LAGER): Spectroscopic Confirmation of Two Redshift ~ 7.0 Galaxies
Huan Yang, Leopoldo Infante, James E. Rhoads +7
We spectroscopically confirmed two narrow-band selected redshift 7.0 Ly galaxies and studied their restframe UV spectra. The Ly and other UV nebular lines are very useful to…
Design for the First Narrowband Filter for the Dark Energy Camera: Optimizing the LAGER Survey for z ~ 7 Galaxies
Zhen-Ya Zheng, James E. Rhoads, Junxian Wang +22
We present the design for the first narrowband filter NB964 for the Dark Energy Camera (DECam), which is operated on the 4m Blanco Telescope at the Cerro Tololo Inter-American Obse…
The Ly Luminosity Function and Cosmic Reionization at 7.0: a Tale of Two LAGER Fields
Weida Hu, Junxian Wang, Zhen-Ya Zheng +20
We present the largest-ever sample of 79 Ly emitters (LAEs) at 7.0 selected in the COSMOS and CDFS fields of the LAGER project (the Lyman Alpha Galaxies in the Epoch of…
An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift distribution
Drew Brisbin, Oskari Miettinen, Manuel Aravena +28
We carried out targeted ALMA observations of 129 fields in the COSMOS region at 1.25 mm, detecting 152 galaxies at S/N5 with an average continuum RMS of 150 Jy. These fiel…
An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
Oskari Miettinen, Ivan Delvecchio, Vernesa Smolčić +25
We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of mm, and followed up at $λ_{\rm o…