Melinda Rackham (Art Forum)

Contemporary artists easily slip between emerging technologies, traditional hand crafted practices, the world of fashion and wearable arts, painting, sculpture, performance, live action role playing and networked environments. As forms of practice blur and intertwine, how do we approach the outcomes; how are they exhibited; and must we find new languages to engage with them? Dr Melinda Rackham is a pioneering networked artist, critic, curator, consultant and cultural producer. Melinda was the first Curator of Networked Media at ACMI, and established -empyre-, one of the world’s leading online media arts critical theory forums. Recently as Director of ANAT she lead Australia's foremost emerging art and technologies organisation to new levels of public engagement. Currently Adjunct Professor at RMIT University, her focus is curating and writing on electronic art and cultures manifested in networked, virtual, responsive, biological, wearable and distributed practices and environments. Her most recent project is curating a large outdoor screen exhibition of Australian Moving Image work in Beijing in late 2010

Couplings and Alignment

Discussion Grou

HST/WFC3 transmission spectroscopy of the cold rocky planet TRAPPIST-1h

TRAPPIST-1 is a nearby ultra-cool dwarf star transited by seven rocky planets. We observed three transits of its outermost planet, TRAPPIST-1h, using the G141 grism of the Wide Field Camera 3 instrument aboard the Hubble Space Telescope to place constraints on its potentially cold atmosphere. In order to deal with the effect of stellar contamination, we model TRAPPIST-1 active regions as portions of a cooler and a hotter photosphere, and generate multi-temperature models that we compare to the out-of-transit spectrum of the star. Using the inferred spot parameters, we produce corrected transmission spectra for planet h under five transit configurations and compare these data to planetary atmospheric transmission models using the forward model CHIMERA. Our analysis reveals that TRAPPIST-1h is unlikely to host an aerosol-free H/He-dominated atmosphere. While the current data precision limits the constraints we can put on the planetary atmosphere, we find that the likeliest scenario is that of a flat, featureless transmission spectrum in the WFC3/G141 bandpass due to a high mean molecular weight atmosphere (>1000x solar), no atmosphere, or an opaque aerosol layer, all in absence of stellar contamination. This work outlines the limitations of modeling active photospheric regions with theoretical stellar spectra, and those brought by our lack of knowledge of the photospheric structure of ultracool dwarf stars. Further characterization of the planetary atmosphere of TRAPPIST-1h would require higher precision measurements over wider wavelengths, which will be possible with the James Webb Space Telescope

Couplings and Alignment

Discussion Grou

Computational Stem Cell Biology: Open Questions and Guiding Principles

Computational biology is enabling an explosive growth in our understanding of stem cells and our ability to use them for disease modeling, regenerative medicine, and drug discovery. We discuss four topics that exemplify applications of computation to stem cell biology: cell typing, lineage tracing, trajectory inference, and regulatory networks. We use these examples to articulate principles that have guided computational biology broadly and call for renewed attention to these principles as computation becomes increasingly important in stem cell biology. We also discuss important challenges for this field with the hope that it will inspire more to join this exciting area

Global analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey

ABSTRACT We conducted a global analysis of the TRAPPIST Ultra-Cool Dwarf Transit Survey – a prototype of the SPECULOOS transit search conducted with the TRAPPIST-South robotic telescope in Chile from 2011 to 2017 – to estimate the occurrence rate of close-in planets such as TRAPPIST-1b orbiting ultra-cool dwarfs. For this purpose, the photometric data of 40 nearby ultra-cool dwarfs were reanalysed in a self-consistent and fully automated manner starting from the raw images. The pipeline developed specifically for this task generates differential light curves, removes non-planetary photometric features and stellar variability, and searches for transits. It identifies the transits of TRAPPIST-1b and TRAPPIST-1c without any human intervention. To test the pipeline and the potential output of similar surveys, we injected planetary transits into the light curves on a star-by-star basis and tested whether the pipeline is able to detect them. The achieved photometric precision enables us to identify Earth-sized planets orbiting ultra-cool dwarfs as validated by the injection tests. Our planet-injection simulation further suggests a lower limit of 10 per cent on the occurrence rate of planets similar to TRAPPIST-1b with a radius between 1 and 1.3 R⊕ and the orbital period between 1.4 and 1.8 d.</jats:p

The discovery of ash dieback in the UK: the making of a focusing event

Why did the identification of ‘Ash Dieback’ (Chalara Fraxinea) in 2012 in the UK catch the national media, public and political zeitgeist, and lead to policy changes, in a way that no other contemporary tree pest or pathogen outbreak has?The identification of Ash Dieback in the UK is conceptualised as a successful ‘focusing event’ and the ways in which it was socially constructed by the media, stakeholders and the government are analysed. National newspaper coverage contributed to the way that the disease was understood and was significant in driving the political response. Ash Dieback’s focal power derived from the perceived scale and nature of its impact; the initial attribution of blame on government; the ‘war-like’ response from the government; and Ash’s status as a threatened ‘native’ tree. The Ash Dieback focusing event has increased the salience of plant health issues amongst policymakers, the public and conservation organisations in the UK