18 research outputs found

    Detecting Friendship Within Dynamic Online Interaction Networks

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    In many complex social systems, the timing and frequency of interactions between individuals are observable but friendship ties are hidden. Recovering these hidden ties, particularly for casual users who are relatively less active, would enable a wide variety of friendship-aware applications in domains where labeled data are often unavailable, including online advertising and national security. Here, we investigate the accuracy of multiple statistical features, based either purely on temporal interaction patterns or on the cooperative nature of the interactions, for automatically extracting latent social ties. Using self-reported friendship and non-friendship labels derived from an anonymous online survey, we learn highly accurate predictors for recovering hidden friendships within a massive online data set encompassing 18 billion interactions among 17 million individuals of the popular online game Halo: Reach. We find that the accuracy of many features improves as more data accumulates, and cooperative features are generally reliable. However, periodicities in interaction time series are sufficient to correctly classify 95% of ties, even for casual users. These results clarify the nature of friendship in online social environments and suggest new opportunities and new privacy concerns for friendship-aware applications that do not require the disclosure of private friendship information.Comment: To Appear at the 7th International AAAI Conference on Weblogs and Social Media (ICWSM '13), 11 pages, 1 table, 6 figure

    Agency, ‘good motherhood’ and ‘a load of mush’: Constructions of baby-led weaning in the press

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    In this age of ‘intensive motherhood’, new mothers are flooded with information on the best ways in which to raise their children. One of the key issues is infant feeding, in particular, the timing and method of weaning their children onto solid food. This paper examines a new approach called ‘baby-led weaning’ (BLW) in which the child feeds themselves instead of being spoon-fed, that came into popular parenting culture in recent years, considering the ways in which it is represented in National and International newspapers. The media search database Proquest International Newsstand, was searched for ‘baby-led weaning’, producing an eventual sample of 78 articles from a number of countries. The articles were subjected to a critical discursive psychological analysis. The key themes that emerged from the newspapers focused around two main areas; the infant as agentive in their eating behaviours; and, constructions of maternal identities and resisting ‘good motherhood’

    SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Massive Helium-Shell Detonation in a Star-Forming Galaxy

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    The detonation of a thin (≲\lesssim0.03 M⊙0.03\,\mathrm{M_\odot}) helium shell (He-shell) atop a ∼\sim1 M⊙1\,\mathrm{M_\odot} white dwarf (WD) is a promising mechanism to explain normal Type Ia supernovae (SNe Ia), while thicker He-shells and less massive WDs may explain some recently observed peculiar SNe Ia. We present observations of SN 2020jgb, a peculiar SN Ia discovered by the Zwicky Transient Facility (ZTF). Near maximum light, SN 2020jgb is slightly subluminous (ZTF gg-band absolute magnitude MgM_g between −18.2-18.2 and −18.7-18.7 mag depending on the amount of host galaxy extinction) and shows an unusually red color (gZTF−rZTFg_\mathrm{ZTF}-r_\mathrm{ZTF} between 0.4 and 0.2 mag) due to strong line-blanketing blueward of ∼\sim5000 A˚\r{A}. These properties resemble those of SN 2018byg, a peculiar SN Ia consistent with a thick He-shell double detonation (DDet) SN. Using detailed radiative transfer models, we show that the optical spectroscopic and photometric evolution of SN 2020jgb are broadly consistent with a ∼\sim0.95 M⊙0.95\,\mathrm{M_\odot} (C/O core + He-shell; up to ∼\sim1.00 M⊙1.00\,\mathrm{M_\odot} depending on the total host extinction) progenitor ignited by a thick (∼\sim0.13 M⊙0.13\,\mathrm{M_\odot}) He-shell. We detect a prominent absorption feature at ∼\sim1 μm\mu\mathrm{m} in the near-infrared (NIR) spectrum of SN 2020jgb, which could originate from unburnt helium in the outermost ejecta. While the sample size is limited, similar 1 μm\mu\mathrm{m} features have been detected in all the thick He-shell DDet candidates with NIR spectra obtained to date. SN 2020jgb is also the first subluminous, thick He-shell DDet SN discovered in a star-forming galaxy, indisputably showing that He-shell DDet objects occur in both star-forming and passive galaxies, consistent with the normal SN Ia population.Comment: 23 pages, 10 figures. Updated to accepted version (ApJ

    Using Novel Amine Dehydrogenase Enzymes in the in the Asymmetric Synthesis of Amines

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    This presentation was given at the Armstrong Student Scholarship Symposium
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