129 research outputs found

    Fogler Library Workshop: How to Do a Literature Review

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    This recorded online workshop, How to Do a Literature Review, discusses tools and strategies to help graduate students make literature searches more efficient, including strategic searching, organizational methods, and synthesizing information. Presented by Lindsay Decker, Fogler Library Science Reference Librarian, University of Maine, Orono.https://digitalcommons.library.umaine.edu/umaine_video/1008/thumbnail.jp

    Fogler Library Workshop: Staying on Top of Literature [in Your Field]

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    Fogler Library Workshop: Staying on Top of Literature, presented by Lindsay Decker, includes tools and strategies for staying current in your field of research, including the use of search alerts, citation alerts, and working with subject specialist librarians.https://digitalcommons.library.umaine.edu/umaine_video/1010/thumbnail.jp

    A Blending of Purpose: The Juxtaposition of Functional and Aesthetic Qualities in Pots of Use.

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    This thesis supports the Master of Fine Arts exhibition entitled A Blending of Purpose at East Tennessee State University, Carroll Reece Museum, Johnson City, Tennessee, November 4 – 22, 2004. It discusses the artist’s desire to create exceptionally crafted functional work which focuses on both compelling aesthetics and strong utilitarian considerations. Topics include the artistic validity of functional works, aesthetic and functional qualities, tactile sensation as a consideration, machine-made works versus hand-made works, a characteristic described as the Life Quality, and the piece’s completion in use. The artist examines her influences including work ceramists Dan Finnegan, Nick Joerling and Ken Sedberry, as well as form and design elements found in the art and architecture of India. Practical application in form and process of these ideas and influences is discussed

    Fogler Library: STEAM in Horror Fiction

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    This video slideshow explores aspects of science, technology, engineering, and mathematics in works of horror and fiction. It was part of a display in Fogler Library October 17, 2022 through November 18, 2022. For more information on science resources and instruction at Fogler Library, the science reference librarians are here to help. No audio.https://digitalcommons.library.umaine.edu/umaine_video/1014/thumbnail.jp

    Validity and Wearability of Consumer-based Fitness Trackers in Free-living Children

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    International Journal of Exercise Science 12(5): 471-482, 2019. Over the past decade wearable fitness trackers (WFTs) have grown in popularity with more recent versions able to capture the pulse rate noninvasively on the wrist of the wearer. Most of evidence on the validity of WFTs have explored adults in clinical settings. Thus, the purpose of this study is to 1) evaluate the validity of a wrist-placed WFT in determining heart rate, and 2) examine the wear compliance of a wrist-placed WFT, in children in free-living settings. In study 1, 19 children (5-12yrs) wore a Fitbit Charge HR© and a Polar chest strap heart rate (HR) monitor for 2 hours while performing sedentary-to-vigorous activities at a holiday camp in December 2016. In study 2, 20 children with mild developmental disabilities (8-13yrs) were asked to wear a Fitbit Alta HR© during summer 2017. In study 1, mean absolute percent difference between the WFT HR and criterion was 6.9%. Overall, \u3e75% of WFT HRs were within 5-10% of the criterion. Bland Altman plots indicated a moderate-to-high level of agreement between the WFT and criterion (mean difference 4.1%; Limits of Agreement 26.8, -18.5%). In study 2, participants had the device in their possession for 43 days (SD±14, range 14 – 56 days) and wore it on 67% of those days (range: 20 – 96%) for at least 10 hours/day. Preliminary evidence suggests that WFTs can provide comparable HR estimates to a criterion field-based measure and children can wear WFTs for extended monitoring periods in free-living settings

    Ontologies on the semantic web

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    As an informational technology, the World Wide Web has enjoyed spectacular success. In just ten years it has transformed the way information is produced, stored, and shared in arenas as diverse as shopping, family photo albums, and high-level academic research. The “Semantic Web” was touted by its developers as equally revolutionary but has not yet achieved anything like the Web’s exponential uptake. This 17 000 word survey article explores why this might be so, from a perspective that bridges both philosophy and IT

    A Cool and Inflated Progenitor Candidate for the Type Ib Supernova 2019yvr at 2.6 Years Before Explosion

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    We present Hubble Space Telescope imaging of a pre-explosion counterpart to SN 2019yvr obtained 2.6 years before its explosion as a type Ib supernova (SN Ib). Aligning to a post-explosion Gemini-S/GSAOI image, we demonstrate that there is a single source consistent with being the SN 2019yvr progenitor system, the second SN Ib progenitor candidate after iPTF13bvn. We also analyzed pre-explosion Spitzer/IRAC imaging, but we do not detect any counterparts at the SN location. SN 2019yvr was highly reddened, and comparing its spectra and photometry to those of other, less extinguished SNe Ib we derive E(BV)=0.51+0.270.16E(B-V)=0.51\substack{+0.27\\-0.16} mag for SN 2019yvr. Correcting photometry of the pre-explosion source for dust reddening, we determine that this source is consistent with a log(L/L)=5.3±0.2\log(L/L_{\odot}) = 5.3 \pm 0.2 and Teff=6800+400200T_{\mathrm{eff}} = 6800\substack{+400\\-200} K star. This relatively cool photospheric temperature implies a radius of 320+3050R\substack{+30\\-50} R_{\odot}, much larger than expectations for SN Ib progenitor stars with trace amounts of hydrogen but in agreement with previously identified SN IIb progenitor systems. The photometry of the system is also consistent with binary star models that undergo common envelope evolution, leading to a primary star hydrogen envelope mass that is mostly depleted but seemingly in conflict with the SN Ib classification of SN 2019yvr. SN 2019yvr had signatures of strong circumstellar interaction in late-time (>>150 day) spectra and imaging, and so we consider eruptive mass loss and common envelope evolution scenarios that explain the SN Ib spectroscopic class, pre-explosion counterpart, and dense circumstellar material. We also hypothesize that the apparent inflation could be caused by a quasi-photosphere formed in an extended, low-density envelope or circumstellar matter around the primary star.Comment: 22 pages, 9 figures, submitted to MNRA
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