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Browsing by Subject "QB857.5.E96"
Now showing items 1-11 of 11
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(Halifax, N.S. : Saint Mary's University, 2020)It has long been appreciated that galaxy formation involves physics that can be subject to chaos. Numerical simulations introduce an additional source of noise in the form of approximations and floating point arithmetic ...
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(Halifax, N.S. : Saint Mary's University, 2013)The dust properties of star forming galaxies at z ~ 2 are examined using a sample of BX objects selected from the Keck Deep Fields (KDF) using colour-colour selection criteria. Spectral energy distribution (SED) fitting ...
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(Halifax, N.S. : Saint Mary's University, 2019)Studying the evolution of galaxies is important in understanding many other astrophysical phenomenon. However, this process required numerical work due to long timescales over which evolution occurs. To study the effects ...
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(Halifax, N.S. : Saint Mary's University, 2020)The study of galaxy morphology can provide important information about how galaxies evolve. In this thesis, we study size and concentration of light profiles for ∼15000 star-forming galaxies (SFGs, M∗
(Halifax, N.S. : Saint Mary's University, 2010)We use photometric galaxy samples and spectral synthesis models to investigate the ability of three dramatically divergent star formation histories (SFHs) to describe the build-up of stellar mass in galaxy populations ...
(Halifax, N.S. : Saint Mary's University, 2016)The numerical algorithm used to implement stellar feedback in a galactic simulation will strongly influence the resulting disk. Using two disks from the MUGS2 simulation suite (Keller et al., 2015), we study the morphologies ...
(Halifax, N.S. : Saint Mary's University, 2018)We build a K-selected catalog of z ∼ 1.6 gzKs galaxies in the Deep and Wide fields of the Canada-France-Hawaii Legacy Survey, with a final effective area of 27.6 deg2. This catalog allows us to recover ...
(Halifax, N.S. : Saint Mary's University, 2019)Satellite galaxies around massive central galaxies can provide important information about galactic environmental effect. In this thesis, we selected thousands of massive (log(Mcen/M☉) > 11.15) ...
(Halifax, N.S. : Saint Mary's University, 2015)Emissions from high redshift (i.e. z ~ 2.5), star forming galaxies provide a unique window into the state the universe at earlier epochs, and how these galaxies evolve over time. Accurate studies of these galaxies, however, ...
(Halifax, N.S. : Saint Mary's University, 2011)In this work we use the latest results from the four Deep Fields of the Canada France Hawaii Telescope Legacy Survey (CFHTLS) combined with the WIRCam Deep Survey (WIRDs) covering 2 .51 deg [superscript 2] to study the ...
(Halifax, N.S. : Saint Mary's University, 2009)In this work, we set out to test the feasibility and limitations of using the 1.6[mu]m bump as a photometric redshift indicator and selection technique using publicly available Spitzer/IRAC images in the GOODS fields. We ...
Now showing items 1-11 of 11