摘要：Mapping the large-scale structure through cosmic time has numerous applications in studies of cosmology and galaxy evolution. Atz ≳ 2, the structure can be traced by the neutral intergalactic medium (IGM) by way of observing the Lyαforest towards densely sampled lines of sight of bright background sources, such as quasars and star-forming galaxies. We investigate the scientific potential of MOSAIC, a planned multi-object spectrograph on the European Extremely Large Telescope (ELT), for the 3D mapping of the IGM atz ≳ 3. We simulated a survey of 3 ≲ z ≲ 4 galaxies down to a limiting magnitude ofmr ∼ 25.5 mag in an area of 1 degree2in the sky. Galaxies and their spectra (including the line-of-sight Lyαabsorption) were taken from the lightcone extracted from the Horizon-AGN cosmological hydrodynamical simulation. The quality of the reconstruction of the original density field was studied for different spectral resolutions (R = 1000 andR = 2000, corresponding to the transverse typical scales of 2.5 and 4 Mpc) and signal-to-noise ratios (S/N) of the spectra. We demonstrate that the minimum S/N (per resolution element) of the faintest galaxies that a survey like this has to reach isS/N = 4. We show that a survey with this sensitivity enables a robust extraction of cosmic filaments and the detection of the theoretically predicted galaxy stellar mass and star-formation rate gradients towards filaments. By simulating the realistic performance of MOSAIC, we obtainS/N(Tobs, R, mr) scaling relations. We estimate that ≲35 (65) nights of observation time are required to carry out the survey with the instrument’s high multiplex mode and with a spectral resolution ofR = 1000 (2000). A survey with a MOSAIC-concept instrument on the ELT is found to enable the mapping of the IGM atz > 3 on Mpc scales, and as such will be complementary to and competitive with other planned IGM tomography surveys.
关键词：enlarge-scale structure of Universecosmology: observationsgalaxies: evolutionintergalactic mediuminstrumentation: spectrographs
