MUSE Analysis of Gas around Galaxies (MAGG) - V. Linking ionized gas traced by C iv and Si iv absorbers to Ly a emitting galaxies at z ˜ 3.0-4.5 (2023)
Attributed to:
The Virgo consortium for cosmological supercomputer simulations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stad2087
Publication URI: http://dx.doi.org/10.1093/mnras/stad2087
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3