Global ETD Search
Search theses and dissertations gathered from participating repositories worldwide. Every result links back to the library that holds it. No account is needed.
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Showing 1 to 12 of 12 for “"Photometric redshift"”.
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The integrated Sachs-Wolfe effect with Planck and the 2Mass Photometric Redshift Catalogue
… large-scale structure data are from the 2MASS Photometric Redshift Catalogue (2MPZ). The galaxy data were divided into redshift shells, and HEALPix was used to create pixelised maps of the CMB temperature anisotropies and the galaxy overdensity. The linear galaxy bias, relating the galaxy …
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Probabilistic photometric redshifts in the era of petascale astronomy
With the growth of large photometric surveys, accurately estimating photometric redshifts, preferably as a probability density function (PDF), and fully understanding the implicit systematic uncertainties in this process has become increasingly important. These surveys are expected to obtain images …
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The cosmic web in the Laduma field
… complete samples of galaxies with spectroscopic redshift measurements are available. In this thesis, I investigate filaments in the cosmic volume targeted by the Looking at the Distant Universe with the MeerKAT Array (LADUMA) survey at higher redshifts. LADUMA's ancillary data catalogue provides …
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The FORS Deep Field Spectroscopic Survey
… properties of galaxy populations at different redshifts provides important constraints on current models of galaxy formation and evolution. In order to investigate this evolutionary process systematically, we obtained high S/N spectra for 265 galaxies at redshifts up to 5.0 with the FORS …
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Searching for Distant Galaxy Clusters : Optical Observations, Cluster Search Algorithms and the Cluster Selection Function
… using a multi-color classification scheme in the redshift range 0.5 < z < 1.5. After contributing to the survey specifications, tests of the multi-color classification with the observational setup showed the feasibility of the project. The photometric redshift accuracy of delta(z) = 0.076 was …
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Dust-Obscured Galaxy Protocluster and Cluster Survey (DOGPACS): Identifying Large-Scale Structures 9−10 Billion Light-Years Away
… of nearly 300 galaxy cluster candidates at redshift 1.3 < z < 1.8 (9-10 billion light-years away) during the formation epoch of the galaxy clusters. This study leverages the fact that high-z galaxy clusters and protoclusters exhibit enhanced star-formation and AGN activity in their cores. …
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N(th)-Order Correlation Functions of Galaxies From the Sloan Digital Sky Survey
… in terms of bias parameters. Using photometric redshift catalogs from SDSS DR5 data, I have created two volume limited samples of galaxies, allowing me to measure o N(theta) as a function of type, redshift, and luminosity. I have found that the higher-order bias of early-type …
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Early Type Galaxies And Reliable Galaxy Cluster Selection
… mass distribution of clusters as a function of redshift enables fundamental tests of this structure formation process. My projects have initially been motivated by an intellectual inquiry into how we can effectively and accurately analyze data from large cluster surveys, such as the South Pole …
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The Search for the Highest Redshift Quasars using the Dark Energy Survey
… material. This allows studies of the IGM at high redshift along different sight lines, providing insight into the metallicity, temperature and homogeneity of the Universe. This thesis discusses a new method of finding high redshift quasars using new multi wavelength data from the Dark Energy …
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The role of obscured activity in galaxy formation
… which would transform into CMR galaxies at lower redshifts as the star-formation terminates. I detect 36 sources in observations of 0.1 deg^2 of the cluster centre and identify counterparts to ~50% of these submillimetre galaxies (SMGs) using radio, 24-um and IRAC data. Photometric redshifts …
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The XMM-Newton/SDSS galaxy cluster survey
… optical counterparts as well as to measure their redshifts that are mandatory to measure their physical properties. The overlap area be- tween the XMM-Newton fields and the SDSS-DR7 imaging, the latest SDSS data release at the starting of the survey, is 210 deg^2. The survey comprises 1180 X-ray …