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Showing 1 to 5 of 5 for “"Dusty Star Forming Galaxies"”.

  1. Unveiling gravitationally lensed, high-redshift dusty star forming galaxies with JWST

    Submission published under a 24 month embargo labeled 'U of I Access', the embargo will last until 2026-08-01

    uiuc Repository record for Unveiling gravitationally lensed, high-redshift dusty star forming galaxies with JWST (opens in a new tab)

  2. Multi-Wavelength Extragalactic Surveys: Star Formation of IR-Submm Selected Galaxies

    … a range of redshifts in order to evaluate the star formation history over cosmic time. Explicitly focusing on the infrared to submillimetre regime, I carried out a comprehensive multi-wavelength approach at the North and South Ecliptic Poles (NEP/SEP). I explore four different methods to select …

    the-open-u Repository record for Multi-Wavelength Extragalactic Surveys: Star Formation of IR-Submm Selected Galaxies (opens in a new tab)

  3. The evolution of galaxies and AGN

    … current questions regarding the evolution of galaxies and AGN. We first argue that the bright submillimetre number counts may be dominated by obscured AGN rather than ultraluminous starbursts. Through statistical analyses of the ECDFS and WHDF, we show that N_H > 10^22 cm^−2 AGN are typically …

    durham Repository record for The evolution of galaxies and AGN (opens in a new tab)

  4. Cosmology with Velocity Dispersion based Counts of Groups and the Effect of AGN Feedback on Host Galaxy Morphology

    … velocity dispersion of the cluster galaxies. I show that the velocity dispersion of groups/clusters can be theoretically predicted as robustly as mass but, unlike mass, it can also be directly observed, thus circumventing the main systematic bias in traditional cluster counts …

    liverpool-jm Repository record for Cosmology with Velocity Dispersion based Counts of Groups and the Effect of AGN Feedback on Host Galaxy Morphology (opens in a new tab)

  5. Studying the Building Blocks of the Universe: the faint, low-mass galaxies

    Faint, low-mass galaxies are the next frontier in extending our understanding of how our universe evolved into its present-day state that we observe. As the ever-advancing technological prowess brings about the next generation of cutting-edge observational facilities, the limit down to which we can …

    umn Repository record for Studying the Building Blocks of the Universe: the faint, low-mass galaxies (opens in a new tab)