MUSE Analysis of Gas around Galaxies (MAGG) -- V: Linking ionized gas traced by CIV and SiIV absorbers to Ly$a$ emitting galaxies at $z\approx 3.0-4.5$ (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/10.48550/arxiv.2302.00021
Publication URI: https://arxiv.org/abs/2302.00021
Type: Other