Optimal deployment of components of cloud-hosted application for guaranteeing multitenancy isolation

One of the challenges of deploying multitenant cloud-hosted services that are designed to use (or be integrated with) several components is how to implement the required degree of isolation between the components when there is a change in the workload. Achieving the highest degree of isolation implies deploying a component exclusively for one tenant; which leads to high resource consumption and running cost per component. A low degree of isolation allows sharing of resources which could possibly reduce cost, but with known limitations of performance and security interference. This paper presents a model-based algorithm together with four variants of a metaheuristic that can be used with it, to provide near-optimal solutions for deploying components of a cloud-hosted application in a way that guarantees multitenancy isolation. When the workload changes, the model based algorithm solves an open multiclass QN model to determine the average number of requests that can access the components and then uses a metaheuristic to provide near-optimal solutions for deploying the components. Performance evaluation showed that the obtained solutions had low variability and percent deviation when compared to the reference/optimal solution. We also provide recommendations and best practice guidelines for deploying components in a way that guarantees the required degree of isolation

Multi-messenger observations of a binary neutron star merger

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

Of Red Threads and Green Dragons: Austrian Sociotechnical Imaginaries about STI cooperation with China

In this chapter, we address intersections of Science and Technology Studies (STS) and International Relations Theories (IR) by looking at how Austrian science, technology & innovation (STI) policy makers and related stakeholders envision and enact a close relationship between China and Austria in the field of green technologies. Analytically, we draw on the concept of ‘sociotechnical imaginaries’ as proposed by Jasanoff and Kim, which attempts to grasp how visions of social order and technological development become entangled in the processes of science and technology policy and politics. China is currently arising as one of the key global players in STI. It is intensely courted by numerous countries seeking collaboration and market access. China’s most recent Five-Year-Plan has introduced a focus on environmental sustainability to complement economic growth. Based on interviews, participant observation and document analysis, we show how Austrian STI actors connect their national positioning activities to this recent focus on sustainability. We trace how they attempt to find common ground for relating to the rising and ever so dynamic People’s Republic by drawing on a nationally accepted narrative about Austrian technopolitical history and culture that casts the country as pioneer of environmental awareness and green technologies. We understand and analyze this process as part of a broader Austrian sociotechnical imaginary in the making that constitutes a situated response to an increasingly globalized STI system, while building on and reaffirming central elements of Austria’s local technopolitical culture and history