Sharma, Monu;
(2024)
Star Formation in galaxies at
redshifts of 0.6−1.2.
Doctoral thesis (Ph.D), UCL (University College London).
Preview |
Text
Monu_Sharma_Thesis_Monu_Sharma.pdf - Accepted Version Download (38MB) | Preview |
Abstract
The Cosmic Noon marks an epoch in the history of the Universe, when it was bustling with star formation activity and the cosmic star formation rate (SFR) reached its peak. Despite being a well-studied redshift regime, questions regarding the evolution of the star-forming galaxies before, during and after the cosmic noon are awaiting satisfactory answers. This thesis is concerned with the after part, i.e. how the star formation changes in the cosmic afternoon. I study star formation in galaxies within the redshift range 0.6−1.2, using observations from the XMM-Newton Optical Monitor (OM) and the Herschel Space Observatory.
| Type: | Thesis (Doctoral) |
|---|---|
| Qualification: | Ph.D |
| Title: | Star Formation in galaxies at redshifts of 0.6−1.2 |
| Open access status: | An open access version is available from UCL Discovery |
| Language: | English |
| Additional information: | Copyright © The Author 2023. Original content in this thesis is licensed under the terms of the Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0) Licence (https://creativecommons.org/licenses/by-nc/4.0/). Any third-party copyright material present remains the property of its respective owner(s) and is licensed under its existing terms. Access may initially be restricted at the author’s request. |
| UCL classification: | UCL UCL > Provost and Vice Provost Offices > UCL BEAMS UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics |
| URI: | https://discovery.ucl.ac.uk/id/eprint/10189284 |
Archive Staff Only
 |
View Item |
