A major challenge in understanding complex rheumatologic and inflammatory diseases has been to understand the relative contributions and influences of multiple cytokines and cell types to disease pathogenesis. Progress has been limited by our inadequate knowledge of the underlying mechanisms responsible for regulating inflammatory responses, both in circumstances of human disease, but also at a fundamental level of how transcription factors (TFs), chromatin, and diverse stimuli regulate inducible transcription in immune cells. We have utilized in-vitro models of mouse macrophage activation combined with hi-throughput sequencing in order to provide a high-resolution view of the inflammatory response. The long- term goal is to identify modes of regulation governing inducible gene expression with the expectation that the knowledge gained will provide insight into how the immune response can be manipulated in the setting of human disease. Here, we provide evidence for both broad trends governing inducible transcription as well as examples of highly specific forms of regulation occurring at individual genes. We further provide support for utilizing mouse models in relation to questions regarding human physiology, as well as address the role of Interluekin-10 in the inhibition of inducible chromatin at sites upstream of inhibited genes.
Galaxy Clusters (GCls) are the largest known virialized objects in the Universe. About one-third of GCls exhibit an extended radio halo associated with a population of nonthermal electrons emitting synchrotron radiation in a microgauss level magnetic field. The cooling time for the nonthermal electrons is about two orders of magnitude below the diffusion time needed to explain the radio halo, indicating that the electrons are created locally. The electrons may either be accelerated directly in the turbulent cluster medium or created as secondary products from nonthermal protons colliding with the intracluster medium. Observed gamma-ray emission can therefore resolve the contribution from these two mechanisms. Despite the empirical and theoretical motivation for the existence of gamma-ray emission from GCls, so far it remains undetected. In this talk VERITAS observations are used to analyze a 6x8 degree field of the Coma galaxy cluster and evaluate the existence of possible extended gamma-ray emission. To achieve this, a method is developed which utilizes cosmic rays as a calibration source to determine a background measurement across the full field of view. The resulting excess demonstrates a small significance of 2.7 sigma in the central 1.5 degree radius of the cluster. This observed central excess, while alone is not significant, has an angular extent in agreement with simulations and corresponds to a similar significance level seen by Fermi-LAT in the same region, and hence it is worth further investigation by VERITAS and future instruments such as CTA.
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