465 citations · 985 across the 23 of their papers we have counts for
6 papers · 1 filter
Efficient simulations of ionized ISM emission lines: A detailed comparison between the FIRE high-redshift suite and observations
Shengqi Yang, Adam Lidz, Aaron Smith +2
The Atacama Large Millimeter/Submillimeter Array (ALMA) in the sub-millimeter and the James Webb Space Telescope (JWST) in the infrared have achieved robust spectroscopic detection…
Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
Yucheng Zhang, Anthony R. Pullen, Rachel S. Somerville +5
Line-intensity mapping (LIM) is a promising technique to constrain the global distribution of galaxy properties. To combine LIM experiments probing different tracers with tradition…
An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift
Shengqi Yang, Gergö Popping, Rachel S. Somerville +3
Sub-millimeter emission lines produced by the interstellar medium (ISM) are strong tracers of star formation and are some of the main targets of line intensity mapping (LIM) survey…
The prospects for observing [OIII] 52 micron emission from galaxies during the Epoch of Reionization
Shengqi Yang, Adam Lidz, Gergö Popping
The [OIII] 88 m fine structure emission line has been detected into the Epoch of Reionization (EoR) from star-forming galaxies at redshifts with ALMA. These m…
Multitracer cosmological line intensity mapping mock lightcone simulation
Shengqi Yang, Rachel S. Somerville, Anthony R. Pullen +3
Sub-millimeter emission lines are important tracers of the cold gas and ionized environments of galaxies and are the targets for future line intensity mapping surveys. Physics-base…
An analytic model for OIII fine structure emission from high redshift galaxies
Shengqi Yang, Adam Lidz
Recent ALMA measurements have revealed bright OIII 88 micron line emission from galaxies during the Epoch of Reionization (EoR) at redshifts as large as . We introduce an…