Although the universe at redshifts greater than six represents only the first one billion years
(< 10%) of cosmic time, the dense nature of the early universe led to vigorous galaxy …

We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

Broadband photometry of galaxies measures an unresolved mix of complex stellar
populations, gas, and dust. Interpreting these data is a challenge for models: many studies …

We use the age–metallicity distribution of 96 Galactic globular clusters (GCs) to infer the
formation and assembly history of the Milky Way (MW), culminating in the reconstruction of …

We present results from the Cosmic Evolution Early Release Survey on the stellar
population parameters for 28 galaxies with redshifts 4< z< 9 using imaging data from the …

Globular clusters (GCs) formed when the Milky Way experienced a phase of rapid assembly.
We use the wealth of information contained in the Galactic GC population to quantify the …

The majority of massive disk galaxies in the local Universe show a stellar barred structure in
their central regions, including our Milky Way,. Bars are supposed to develop in dynamically …

Galaxy observations are influenced by many physical parameters: stellar masses, star
formation rates (SFRs), star formation histories (SFHs), metallicities, dust, black hole activity …

We explore star formation histories (SFHs) of galaxies based on the evolution of the star
formation rate stellar mass relation (SFR–M*). Using data from the FourStar Galaxy …

We present a novel implementation of supermassive black hole (SMBH) formation,
dynamics and accretion in the massively parallel tree+ SPH code, ChaNGa. This approach …