Peter Cottrell | Searcharxiv

arXiv2021

Design not Lost in Translation: A Case Study of an Intimate-Space Socially Assistive Robot for Emotion Regulation

We present a Research-through-Design case study of the design and development of an intimate-space tangible device perhaps best understood as a socially assistive robot, aimed at scaffolding children's efforts at emotional regulation. This case study covers the initial research device development, as well as knowledge transfer to a product development company towards translating the research into a workable commercial product that could also serve as a robust research product for field trials. Key contributions to the literature include: 1. sharing of lessons learned from the knowledge transfer process that can be useful to others interested in developing robust products, whether commercial or research, that preserve design values, while allowing for large scale deployment and research; 2. articulation of a design space in HCI/HRI--Human Robot Interaction--of intimate space socially assistive robots, with the current artifact as a central exemplar, contextualized alongside other related HRI artifacts.

cs.HC↗

arXiv2020

The GALAH survey: tracing the Galactic disk with Open Clusters

Open clusters are unique tracers of the history of our own Galaxy's disk. According to our membership analysis based on \textit{Gaia} astrometry, out of the 226 potential clusters falling in the footprint of GALAH or APOGEE, we find that 205 have secure members that were observed by at least one of the survey. Furthermore, members of 134 clusters have high-quality spectroscopic data that we use to determine their chemical composition. We leverage this information to study the chemical distribution throughout the Galactic disk of 21 elements, from C to Eu. The radial metallicity gradient obtained from our analysis is $-$0.076$\pm$0.009 dex kpc$^{-1}$, which is in agreement with previous works based on smaller samples. Furthermore, the gradient in the [Fe/H] - guiding radius (r$_{\rm guid}$) plane is $-$0.073$\pm$0.008 dex kpc$^{-1}$. We show consistently that open clusters trace the distribution of chemical elements throughout the Galactic disk differently than field stars. In particular, at given radius, open clusters show an age-metallicity relation that has less scatter than field stars. As such scatter is often interpreted as an effect of radial migration, we suggest that these differences are due to the physical selection effect imposed by our Galaxy: clusters that would have migrated significantly also had higher chances to get destroyed. Finally, our results reveal trends in the [X/Fe]$-$r$_{\rm guid}$$-$age space, which are important to understand production rates of different elements as a function of space and time.

astro-ph.GA↗