Galaxies through cosmic time illuminated by gamma-ray bursts and quasars
Kasper E. Heintz

TL;DR
This thesis uses gamma-ray bursts and quasars as luminous probes to study the distribution of cold gas, dust, and metals in the early universe, revealing insights into galaxy formation and cosmic chemical evolution.
Contribution
It demonstrates the importance of large, unbiased samples of GRB afterglows and quasars for understanding galaxy environments and cosmic chemical processes over time.
Findings
Large samples of GRB afterglows enable statistical analysis of host environments.
Quasar observations are crucial for studying intervening galaxy absorption systems.
Highlighting the need for unbiased quasar samples to study cosmic chemical evolution.
Abstract
In the early Universe, most of the cold neutral gas that will later form into individual stars and galaxies is practically invisible to us. These neutral gas reservoirs can, however, be illuminated by bright cosmic lightsources such as gamma-ray bursts (GRBs) and quasars. The aim of this thesis is to use these luminous objects as tools to study the environments of intervening or host galaxy absorption systems through cosmic time. Part I is dedicated to examining the gas, dust and metals in the immediate region surrounding GRBs. Part II presents a search for and the study of cold and molecular gas in high-z GRB host galaxy absorption systems. Part III focuses on using quasars to examine gas-rich intervening galaxies in the line of sight, with specific focus on absorption systems rich in dust and metals. This thesis demonstrates the importance of observing large samples of GRB afterglows…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · Astronomical Observations and Instrumentation
