New insights and methods for the clustering of emission line galaxies.
| dc.contributor.advisor | Padilla, Nelson | |
| dc.contributor.author | Jiménez Henríquez, Esteban | |
| dc.contributor.other | Pontificia Universidad Católica de Chile. Instituto de Astrofísica | |
| dc.date.accessioned | 2019-08-22T14:05:55Z | |
| dc.date.available | 2019-08-22T14:05:55Z | |
| dc.date.issued | 2019 | |
| dc.description | Tesis (Magíster en Astrofísica)--Pontificia Universidad Católica de Chile, 2019 | |
| dc.description.abstract | We study the dependence of emission line galaxies (ELG) clustering in halo properties besides mass, an effect known as assembly bias (AB). This AB signature is scale-dependent in some ELG samples and may contribute with potential systematic effects on cosmology constraints. We test different implementations of the halo occupation distribution (HOD) model to construct mock galaxy catalogues that mimic ELG selected samples produced by a semi-analytical model (SAM). These catalogues are useful to understand the future observational samples. We select galaxies from two different SAMs, applied to the Millennium-WMAP7 and the MultiDark Plank 2 simulation. We use fixed number density galaxy samples selected according to stellar mass, star formation rate (SFR), and emission line luminosity from Hα, [OIII]λ5007, and [OII]λλ3727 − 3729 emission, obtained from a photoionization code. We develop three different schemes to populate haloes with galaxies with increasing complexity, considering the scatter of the satellites HOD as an additional parameter in the modellings. The quality of the HOD modelling is determined by comparing the two-point correlation function (2PCF) of the HOD mocks and the SAM samples. The HOD modelling that uses the HOD of centrals and satellites separately, and assume a negative binomial distribution for the satellite HOD, produce the best clustering predictions. The scatter in the satellites HOD is a key consideration for HOD mock catalogues that mimic ELG selected samples in future galaxy surveys. The origin of the scale-dependent AB seems to be related to an environment selection effect rather than a physical reason. We found that galaxies in underdense regions and low gas metallicity, make the main contribution to the scale-dependent signature. We obtain that the peak of the Baryon Acoustic Oscillation (BAO) for some ELG samples is in lower scales than expected, and the β parameter is non-constant in large scales. Hence, this selection effect can introduce systematic in the inferred cosmology from ELGs. | |
| dc.format.extent | iii, 62 páginas | |
| dc.identifier.doi | 10.7764/tesisUC/AST/23683 | |
| dc.identifier.uri | https://doi.org/10.7764/tesisUC/AST/23683 | |
| dc.identifier.uri | https://repositorio.uc.cl/handle/11534/23683 | |
| dc.language.iso | en | |
| dc.nota.acceso | Contenido completo | |
| dc.rights | acceso abierto | |
| dc.subject.ddc | 520 | |
| dc.subject.dewey | Astronomía | es_ES |
| dc.subject.other | Galaxias - Cúmulos | es_ES |
| dc.subject.other | Galaxias - Velocidad radial | es_ES |
| dc.title | New insights and methods for the clustering of emission line galaxies. | es_ES |
| dc.type | tesis de maestría | |
| sipa.codpersvinculados | 1003598 |