The IRX-β\beta relation: Insights from simulations

We study the relationship between the UV continuum slope and infrared excess (IRX$\equiv L_{\rm IR}/L_{\rm FUV}$) predicted by performing dust radiative transfer on a suite of hydrodynamical simulations of galaxies. Our suite includes both isolated disk galaxies and mergers intended to be representative of galaxies at both $z \sim 0$ and $z \sim 2-3$. Our low-redshift isolated disks and mergers often populate a region around the the locally calibrated \citet[][M99]{M99} relation but move well above the relation during merger-induced starbursts. Our high-redshift simulated galaxies are blue and IR-luminous, which makes them lie above the M99 relation. The value of UV continuum slope strongly depends on the dust type used in the radiative transfer calculations: Milky Way-type dust leads to significantly more negative (bluer) slopes compared with Small Magellanic Cloud-type dust. The effect on $\beta$ due to variations in the dust composition with galaxy properties or redshift can dominate over other sources of $\beta$ variations and is the dominant model uncertainty. The dispersion in $\beta$ is anticorrelated with specific star formation rate and tends to be higher for the $z \sim 2-3$ simulations. In the actively star-forming $z \sim 2-3$ simulated galaxies, dust attenuation dominates the dispersion in $\beta$, whereas in the $z \sim 0$ simulations, the contributions of SFH variations and dust are similar. For low-SSFR systems at both redshifts, SFH variations dominate the dispersion. Finally, the simulated $z \sim 2-3$ isolated disks and mergers both occupy a region in the \irxbeta\ plane consistent with observed $z \sim 2-3$ dusty star-forming galaxies (DSFGs). Thus, contrary to some claims in the literature, the blue colors of high-z DSFGs do not imply that they are short-lived starbursts.Comment: 20 pages+a 4-page appendix, Accepted for publication at Ap

A Simple Non-equilibrium Feedback Model for Galaxy-Scale Star Formation: Delayed Feedback and SFR Scatter

We explore a class of simple non-equilibrium star formation models within the framework of a feedback-regulated model of the ISM, applicable to kiloparsec-scale resolved star formation relations (e.g. Kennicutt-Schmidt). Combining a Toomre-Q-dependent local star formation efficiency per free-fall time with a model for delayed feedback, we are able to match the normalization and scatter of resolved star formation scaling relations. In particular, this simple model suggests that large ($\sim$dex) variations in star formation rates (SFRs) on kiloparsec scales may be due to the fact that supernova feedback is not instantaneous following star formation. The scatter in SFRs at constant gas surface density in a galaxy then depends on the properties of feedback and when we observe its star-forming regions at various points throughout their collapse/star formation "cycles". This has the following important observational consequences: (1) the scatter and normalization of the Kennicutt-Schmidt relation are relatively insensitive to the local (small-scale) star formation efficiency, (2) but gas depletion times and velocity dispersions are; (3) the scatter in and normalization of the Kennicutt-Schmidt relation is a sensitive probe of the feedback timescale and strength; (4) even in a model where $\tilde Q_{\rm gas}$ deterministically dictates star formation locally, time evolution, variation in local conditions (e.g., gas fractions and dynamical times), and variations between galaxies can destroy much of the observable correlation between SFR and $\tilde Q_{\rm gas}$ in resolved galaxy surveys. Additionally, this model exhibits large scatter in SFRs at low gas surface densities, in agreement with observations of flat outer HI disk velocity dispersion profiles.Comment: 15 pages, 6 figures, accepted by MNRAS (04/25/2019

An improved thin-film microelectrode array and signal conditioning board for measuring cardiac surface potentials.

The work outlined in this thesis expanded on previous work to improve a thin-film microfabricated electrode array intended for cardiac electrophysiology studies. A thin layer of silver was added in between titanium and platinum electrical trace layers to reduce electrode resistance. A 200 nm layer of silver decreased electrode resistance by an order of magnitude. In addition, a new high quality signal conditioning board was developed using precision operational amplifiers from Texas Instruments. Both new sensor and board design were verified together through in vivo studies using rabbit, goat, and dog hearts

Advertising and Dublin’s Consumer Culture in James Joyce’s Ulysses

This thesis reconsiders James Joyce’s representation of advertising and Dublin’s consumer culture in Ulysses. Against earlier, generalising accounts, it applies a carefully historicising methodology to demonstrate the cultural specificity of Joyce’s engagement. It does so in three ways. To begin with, it establishes that Irish consumerism did not simply follow British advances, but developed in a distinct and inflected fashion. Chapters 2 and 3 show that while Joyce incorporates all of the material characteristics of Dublin’s relatively advanced consumer culture, he downplays its advertising industry, making it appear less developed in 1904 than was historically the case. Secondly, it analyses the distortions introduced by Joyce’s own historical remove from the consumer culture he depicts. Chapter 4 identifies for the first time the sources of Joyce’s “Advertising” notes from his so-called “Notes on Business and Commerce,” and establishes that his representation of Bloom’s advertising consciousness reflects advances in advertising theory that only got seriously underway in the decade between 1904, when the novel is set, and 1914, when Joyce began to write it. Finally, having analysed the material and compositional background to Joyce’s portrayal of early-twentieth-century consumerism, this thesis analyses Joyce’s engagement with two of its dominant ideologies. Chapter 5 concentrates on the ‘Lestrygonians’ and ‘Ithaca’ episodes to argue that Joyce lays bare the overdetermined nature of colonial consumption, depicting the naturalisation of British commodities on the Irish market, and contesting the spurious claim to disinterestedness presented by imperial consumerist discourses. Chapter 6 develops intertextual readings of the ‘Nausicaa’ chapter to show that Joyce’s narrative is even more fully comprised of the language of female-oriented advertising than has been recognised. It argues that the chapter responds to a particular ideological complex, in which consumerist imperatives struggled with more conservative patriarchal interests. Overall, this thesis brings together historical, genetic and intertextual critical approaches to uncover the stylistic and chronological manipulations involved in Joyce’s fictionalisation of early-twentieth-century Irish consumerism. It argues that Ulysses stands as both a reflection of this crucial period of socio-economic change, and a politicised response to its dominant ideological coercions

What shapes the far-infrared spectral energy distributions of galaxies?

To explore the connection between the global physical properties of galaxies and their far-infrared (FIR) spectral energy distributions (SEDs), we study the variation in the FIR SEDs of a set of hydrodynamically simulated galaxies that are generated by performing dust radiative transfer in post-processing. Our sample includes both isolated and merging systems at various stages of the merging process and covers infrared (IR) luminosities and dust masses that are representative of both low- and high-redshift galaxies. We study the FIR SEDs using principle component analysis (PCA) and find that 97\% of the variance in the sample can be explained by two principle components (PCs). The first PC characterizes the wavelength of the peak of the FIR SED, and the second encodes the breadth of the SED. We find that the coefficients of both PCs can be predicted well using a double power law in terms of the IR luminosity and dust mass, which suggests that these two physical properties are the primary determinants of galaxies' FIR SED shapes. Incorporating galaxy sizes does not significantly improve our ability to predict the FIR SEDs. Our results suggest that the observed redshift evolution in the effective dust temperature at fixed IR luminosity is not driven by geometry: the SEDs of $z \sim 2-3$ ultraluminous IR galaxies (ULIRGs) are cooler than those of local ULIRGs not because the high-redshift galaxies are more extended but rather because they have higher dust masses at fixed IR luminosity. Finally, based on our simulations, we introduce a two-parameter set of SED templates that depend on both IR luminosity and dust mass.Comment: Submitted to ApJ, comments welcom