Mapping galaxy evolution at multiple wavelengths and cosmic epochs

Some of the most fundamental measurements we can make of the Universe are where and when stars formed in galaxies. In recent years, astronomers have converged on a picture in which the star formation rate density of the Universe peaks at approximately redshift (z) 2, when the Universe is around a quarter of its present age. There, star-forming galaxies harbour large reservoirs of molecular gas, assemble stellar mass rapidly, and typically display disordered morphologies. In this thesis, I study the evolution of galaxies on large and small scales, with a particular focus on the epoch around the peak of cosmic star formation. My overarching aim is to understand the physical processes that drive and quench star formation in galaxies over cosmic time. In the first half of this thesis, I focus on global measurements of star formation, using the High-z Emission line survey (HiZELS), a deep, near-infrared narrow-band survey, which identifies star-forming galaxies at z=0.8-2.2. I characterise the dark matter halo environments of these galaxies via a clustering analysis, along with a Halo Occupation Distribution model fitting procedure, then study the relationships between host dark matter halo environment and galaxy properties. I show that the clustering strength and the host dark matter halo masses of the HiZELS galaxies increase linearly with H-alpha luminosity (and, by implication, star formation rate) at all three redshifts. The typical galaxies in our samples are star-forming centrals, residing in dark matter haloes of mass ~10^12M_sol. I find a remarkably tight redshift-independent relation between the H-alpha luminosity scaled by the characteristic luminosity, L_H-alpha/L_H-alpha*(z), and the host dark matter halo mass of central galaxies. Simple analytic modelling suggests that this is consistent with a model in which the dark matter halo environment is a strong driver of galaxy star formation rate and therefore of the evolution of the star formation rate density in the Universe. I investigate this further by distinguishing the stellar mass and star formation rate dependencies of the clustering of HiZELS galaxies. I compare my observational results to the predictions of a pioneering cosmological hydrodynamical simulation, the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments project, known as EAGLE. In the subsequent chapters of this thesis, I focus more heavily on simulations of galaxy formation, which are important tools for constraining and understanding the physics at play in galaxies. I use EAGLE to investigate the quenching of star formation in simulated galaxies via a novel application of Principal Component Analysis. I show that the key relations between halo mass, stellar mass and star formation rate are in good agreement with observed low-redshift galaxies. Having studied the global properties of star-forming galaxies, I then turn to smaller scales, investigating what we can learn from spatially-resolved imaging. I present a detailed study of the spatially-resolved dust continuum emission of realistic simulated high-redshift galaxies. These galaxies, drawn from the FIRE-2 simulations, reach Milky Way masses by z~2. Post-processing them using radiative transfer techniques, I obtain predictions for the full rest-frame far-ultraviolet to far-infrared Spectral Energy Distributions of these simulated galaxies, as well as maps of their emission across the wavelength spectrum. As has been observed in distant galaxies, the rest-frame far-infrared emission of the simulated galaxies is compact, spanning half-light radii of ~0.5-4kpc. The derived morphologies of simulated galaxies are notably different in different wavebands; a galaxy can appear clumpy and extended in the far-ultraviolet yet compact at far-infrared wavelengths. Finally, I perform a multi-wavelength study of a single observed galaxy, SHiZELS-14 (z=2.24), drawn from the HiZELS survey and subsequently imaged at 0.15'' resolution at multiple wavelengths. The data comprise kpc-resolution imaging in three different widely used tracers of star formation: the H-alpha emission line (from SINFONI/VLT), rest-frame far-ultraviolet continuum (from HST F606W imaging), and the rest-frame far-infrared (from ALMA), as well as the rest-frame optical (from HST F140W imaging). SHiZELS-14 displays a compact, dusty centre, as well as extended emission in both H-alpha and the rest-frame FIR. The ultraviolet emission is spatially offset from the extended dust emission, and appears to trace holes in the dust distribution. I find that the dust attenuation varies across the spatial extent of the galaxy, reaching up to ~5 magnitudes of extinction at H-alpha wavelengths in the most dusty regions. Global star formation rates inferred using standard calibrations to the different tracers vary from ~10-1000M_sol, and are particularly discrepant in the galaxy's dusty centre. This galaxy highlights the biased view of galaxy evolution provided by short-wavelength data in the absence of long-wavelength data, and is in line with my simulations

Influence of school community and fitness on prevalence of overweight in Australian school children

AbstractThe study objectives were (1) to determine the variation in prevalence of overweight between school communities, (2) to evaluate the relationship between cardiorespiratory fitness and the probability of being overweight among different school communities, and (3) to test whether this relationship varies between school communities. Using a repeated cross-sectional design, data from 31,424 (15,298 girls, 16,126 boys) Australian school children who had objective assessments of body composition and physical performance were used. Ninety-one schools located across 5 states and territories were included. Independent samples were taken across 12 school years (2000–2011). Analysis used generalised linear mixed models in R with a two-level hierarchical structure—children, nested within school communities. Predictor variables considered were: level 1—gender, age, cardiorespiratory fitness and year of measurement; level 2—school community. A total of 24.6% of the children were overweight and 69% were of low fitness. Variation in the prevalence of overweight between school communities was significant, ranging from 19% to 34%. The probability of being overweight was negatively associated with increasing cardiorespiratory fitness. The relationship was steepest at low fitness and varied markedly between school communities. Children of low fitness had probabilities of being overweight ranging between 26% and 75% depending on school community, whereas those of high fitness had probabilities of <2%. Our findings suggest that most might be gained from a public health perspective by focusing intervention on the least fit children in the worst-performing communities

Study protocol - Indigenous Australian social networks and the impact on smoking policy and programs in Australia: Protocol for a mixed-method prospective study

Background: Tobacco use is the most preventable cause of morbidity and mortality in Australia. Comprehensive tobacco control has reduced smoking rates in Australia from approximately 34 per cent in 1980 to 15 per cent in 2010. However, 46 per cent of Abo

Is Walk Score associated with hospital admissions from chronic diseases? Evidence from a cross-sectional study in a high socioeconomic status Australian city-state

Objectives: To explore patterns of non-communicable diseases (NCDs) in the Australian Capital Territory (ACT).To ascertain the effect of the neighbourhood built environmental features and especially walkability on health outcomes, specifically for hospital admissions from NCDs. Design: A cross-sectional analysis of public hospital episode data (2007–2013). Setting: Hospitalisations from the ACT, Australia at very small geographic areas. Participants: Secondary data on 75 290 unique hospital episodes representing 39 851 patients who were admitted to ACT hospitals from 2007 to 2013. No restrictions on age, sex or ethnicity. Main exposure measures: Geographic Information System derived or compatible measures of general practitioner access, neighbourhood socioeconomic status, alcohol access, exposure to traffic and Walk Score walkability. Main outcome measures: Hospitalisations of circulatory diseases, specific endocrine, nutritional and metabolic diseases, respiratory diseases and specific cancers. Results: Geographic clusters with significant high and low risks of NCDs were found that displayed an overall geographic pattern of high risk in the outlying suburbs of the territory. Significant relationships between neighbourhood walkability as measured by Walk Score and the likelihood of hospitalisation with a primary diagnosis of myocardial infarction (heart attack) were found. A possible relationship was also found with the likelihood of being hospitalised with 4 major lifestylerelated cancers. Conclusions: Our research augments the growing literature underscoring the relationships between the built environment and health outcomes. In addition, it supports the importance of walkable neighbourhoods, as measured by Walk Score, for improved health.Full Tex

Longitudinal patterns of physical activity in children aged 8 to 12 years: the LOOK study

BACKGROUND Data on longitudinal monitoring of daily physical activity (PA) patterns in youth over successive years is scarce but may provide valuable information for intervention strategies aiming to promote PA. METHODS Participants were 853 children (starting age ~8 years) recruited from 29 Australian elementary schools. Pedometers were worn for a 7-day period each year over 5 consecutive years to assess PA volume (steps per day) and accelerometers were worn concurrently in the final 2 years to assess PA volume (accelerometer counts (AC) per day), moderate and vigorous PA (MVPA), light PA (LPA) and sedentary time (SED). A general linear mixed model was used to examine daily and yearly patterns. RESULTS A consistent daily pattern of pedometer step counts, AC, MVPA and LPA emerged during each year, characterised by increases on school days from Monday to Friday followed by a decrease on the weekend. Friday was the most active and Sunday the least active day. The percentage of girls and boys meeting international recommendations of 11,000 and 13,000 steps/day respectively on a Monday, Friday and Sunday were 36%, 50%, 21% for boys and 35%, 45%, 18% for girls. The equivalent percentages meeting the recommended MVPA of >60 min/day on these days were 29%, 39%, 16% for boys and 15%, 21%, 10% for girls. Over the 5 years, boys were more active than girls (mean steps/day of 10,506 vs 8,750; p<0.001) and spent more time in MVPA (mean of 42.8 vs 31.1 min/day; p<0.001). Although there was little evidence of any upward or downward trend in steps/day from age 8 to 12 years, there was a trend toward lower MVPA, LPA and a corresponding increase in SED from age 11 to 12 years. CONCLUSION A weekly pattern of PA occurred in children as young as age 8 on a day by day basis; these patterns persisting through to age 12. In addition to supporting previous evidence of insufficient PA in children, our data, in identifying the level and incidence of insufficiency on each day of the week, may assist in the development of more specific strategies to increase PA in community based children

Longitudinal patterns of physical activity in children aged 8 to 12 years: The LOOK study

BACKGROUND: Data on longitudinal monitoring of daily physical activity (PA) patterns in youth over successive years is scarce but may provide valuable information for intervention strategies aiming to promote PA. METHODS: Participants were 853 children (starting age ~8 years) recruited from 29 Australian elementary schools. Pedometers were worn for a 7-day period each year over 5 consecutive years to assess PA volume (steps per day) and accelerometers were worn concurrently in the final 2 years to assess PA volume (accelerometer counts (AC) per day), moderate and vigorous PA (MVPA), light PA (LPA) and sedentary time (SED). A general linear mixed model was used to examine daily and yearly patterns. RESULTS: A consistent daily pattern of pedometer step counts, AC, MVPA and LPA emerged during each year, characterised by increases on school days from Monday to Friday followed by a decrease on the weekend. Friday was the most active and Sunday the least active day. The percentage of girls and boys meeting international recommendations of 11,000 and 13,000 steps/day respectively on a Monday, Friday and Sunday were 36%, 50%, 21% for boys and 35%, 45%, 18% for girls. The equivalent percentages meeting the recommended MVPA of >60 min/day on these days were 29%, 39%, 16% for boys and 15%, 21%, 10% for girls. Over the 5 years, boys were more active than girls (mean steps/day of 10,506 vs 8,750; p<0.001) and spent more time in MVPA (mean of 42.8 vs 31.1 min/day; p<0.001). Although there was little evidence of any upward or downward trend in steps/day from age 8 to 12 years, there was a trend toward lower MVPA, LPA and a corresponding increase in SED from age 11 to 12 years. CONCLUSION: A weekly pattern of PA occurred in children as young as age 8 on a day by day basis; these patterns persisting through to age 12. In addition to supporting previous evidence of insufficient PA in children, our data, in identifying the level and incidence of insufficiency on each day of the week, may assist in the development of more specific strategies to increase PA in community based children

Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn

Recent discoveries of a significant population of bright galaxies at cosmic dawn $\left(z \gtrsim 10\right)$ have enabled critical tests of cosmological galaxy formation models. In particular, the bright end of the galaxy UV luminosity function (UVLF) appears higher than predicted by many models. Using approximately 25,000 galaxy snapshots at $8 \leq z \leq 12$ in a suite of FIRE-2 cosmological "zoom-in'' simulations from the Feedback in Realistic Environments (FIRE) project, we show that the observed abundance of UV-bright galaxies at cosmic dawn is reproduced in these simulations with a multi-channel implementation of standard stellar feedback processes, without any fine-tuning. Notably, we find no need to invoke previously suggested modifications such as a non-standard cosmology, a top-heavy stellar initial mass function, or a strongly enhanced star formation efficiency. We contrast the UVLFs predicted by bursty star formation in these original simulations to those derived from star formation histories (SFHs) smoothed over prescribed timescales (e.g., 100 Myr). The comparison demonstrates that the strongly time-variable SFHs predicted by the FIRE simulations play a key role in correctly reproducing the observed, bright-end UVLFs at cosmic dawn: the bursty SFHs induce order-or-magnitude changes in the abundance of UV-bright ($M_\mathrm{UV} \lesssim -20$) galaxies at $z \gtrsim 10$. The predicted bright-end UVLFs are consistent with both the spectroscopically confirmed population and the photometrically selected candidates. We also find good agreement between the predicted and observationally inferred integrated UV luminosity densities, which evolve more weakly with redshift in FIRE than suggested by some other models.Comment: 12 pages, 4 figures + 1 table, submitted to ApJ