ORCID Profile
0000-0003-3428-1106
Current Organisation
University of Florida
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Publisher: Emerald
Date: 04-11-2019
DOI: 10.1108/EEMCS-05-2019-0107
Abstract: The learning outcomes are as follows: understanding online, traditional and omnichannel retail and the challenges and benefits of each method evaluating the effect of consumer buying behaviour on a company’s growth strategy assessing the effect of changing industry dynamics and technology on consumer behaviour and understanding the role of consistent customer experience across different retail mediums. This case looks at Yuppiechef, a successful e-commerce business, and their move from “clicks to bricks” with the introduction of retail stores. Founder and CEO of Yuppiechef, Andrew Smith, shares the current business status and considers how to maintain the brand’s culture with the growth of retail and being an omnichannel pioneer. The primary target audience for this teaching case is postgraduate business students, especially students of digital marketing, strategy and e-commerce. This teaching case is intended to be used as case study in postgraduate business programmes such as Master of Business Administration (MBA), a specialist masters’ programme such as MM (Entrepreneurship), post-graduate diploma in management (PGDip), as well as selected executive education programmes. Teaching Notes are available for educators only. CSS 8: Marketing.
Publisher: American Astronomical Society
Date: 03-08-2020
Publisher: Oxford University Press (OUP)
Date: 17-05-2019
Abstract: We present deep, multiwavelength radio observations of SpARCS104922.6 + 564032.5, a z = 1.71 galaxy cluster with a starbursting core. Observations were made with the Karl G. Jansky Very Large Array (JVLA) in three bands: 1–2 GHz, 4–8 GHz, and 8–12 GHz. We detect a radio source coincident with the brightest cluster galaxy (BCG) that has a spectral index of α = 0.44 ± 0.29 and is indicative of emission from an active galactic nucleus. The radio luminosity is consistent with the average luminosity of the lower redshift BCG s le, but the flux densities are 6σ below the predicted values of the star-forming spectral energy distribution based on far infrared data. Our new fit fails to simultaneously describe the far infrared and radio fluxes. This, coupled with the fact that no other bright source is detected in the vicinity of the BCG implies that the star formation region, traced by the infrared emission, is extended or clumpy and not located directly within the BCG. Thus, we suggest that the star-forming core might not be driven by a single major wet merger, but rather by several smaller galaxies stripped of their gas or by a displaced cooling flow, although more data are needed to confirm any of those scenarios.
No related grants have been discovered for Ariane Trudeau.