11 research outputs found

    Multi-messenger observations of a binary neutron star merger

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    On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

    Public policy for academic entrepreneurship initiatives: a review and critical discussion

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    The UBC ecosystem: putting together a comprehensive framework for university-business cooperation

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    The potential for a functional ‘triple helix’ to contribute to economic development is being increasingly accepted and embraced, particularly the bilateral relationship between higher education institutions (HEIs) and business. However, university-business cooperation (UBC) is still a fragmented and indistinct field of research, and the understanding of UBC remains inadequate since most research is undertaken around specific elements, rather than as an encompassing, overarching and interconnected system. This paper aims fills this gap in the literature by putting the pieces together to create an integrated and comprehensive conceptual UBC framework for HEIs, the UBC Ecosystem. The framework illustrates the components present in the UBC environment for HEIs, such as inputs, activities, outcomes, outputs, impacts, supporting mechanisms, circumstances and context, specifying a wide range of sub-elements for each of them. In doing so, this paper makes a strong theoretical contribution with the creation of a conceptual framework, highlighting the more important elements and their interrelations as well as suggesting future research. Additionally, the paper makes a practical contribution, establishing a common UBC schema for HEI managers and policymakers to make strategic and operative decisions, and used as a base for evidence-based management and policy
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