4 research outputs found

    THE GALLERY AS A SITE OF CONVERGENCE: THE ROLE OF CREATIVE ENVIRONMENTS AT POSTSECONDARY INSTITUTIONS

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    Not enough research explores the role of creative environments at postsecondary institutions. In response, this qualitative research study focuses upon university galleries believing them to be exemplary artistic spaces within college campuses. Using a theoretical framework of place-consciousness, the researcher examined the functions of the Mary and Carter Thacher Gallery at the University of San Francisco (USF), paying close attention to the ways it engaged the academic community in terms of scholarship and instruction. Informed by grounded theory and phenomenology, this study interviewed five professors who integrated a gallery visit into their curriculum during the 2021-2022 academic year. Collecting these first-hand perspectives and experiences, the study arrived at a collective understanding of the gallery’s role at USF concerning its pedagogical, aesthetic, spatial and social dimensions

    HAWC and Fermi-LAT detection of extended emission from the unidentified source 2HWC J2006+341

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    The discovery of the TeV point source 2HWC J2006+341 was reported in the second HAWC gamma-ray catalog. We present a follow-up study of this source here. The TeV emission is best described by an extended source with a soft spectrum. At GeV energies, an extended source is significantly detected in Fermi-LAT data. The matching locations, sizes, and spectra suggest that both gamma-ray detections correspond to the same source. Different scenarios for the origin of the emission are considered and we rule out an association to the pulsar PSR J2004+3429 due to extreme energetics required, if located at a distance of 10.8 kpc.Universidad de Costa Rica/[112-B9-171]/UCR/Costa RicaUniversidad de Costa Rica/[112-B6-509]/UCR/Costa RicaUniversidad de Costa Rica/[829-B5-198]/UCR/Costa RicaUCR::Vicerrectoría de Docencia::Ciencias Básicas::Facultad de Ciencias::Escuela de Físic

    The High-Altitude water cherenkov (HAWC) observatory in México: The primary detector

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    The High-Altitude Water Cherenkov (HAWC) observatory is a second-generation continuously operated, wide field-of-view, TeV gamma-ray observatory. The HAWC observatory and its analysis techniques build on experience of the Milagro experiment in using ground-based water Cherenkov detectors for gamma-ray astronomy. HAWC is located on the Sierra Negra volcano in México at an elevation of 4100 meters above sea level. The completed HAWC observatory principal detector (HAWC) consists of 300 closely spaced water Cherenkov detectors, each equipped with four photomultiplier tubes to provide timing and charge information to reconstruct the extensive air shower energy and arrival direction. The HAWC observatory has been optimized to observe transient and steady emission from sources of gamma rays within an energy range from several hundred GeV to several hundred TeV. However, most of the air showers detected are initiated by cosmic rays, allowing studies of cosmic rays also to be performed. This paper describes the characteristics of the HAWC main array and its hardware.UCR::Vicerrectoría de Docencia::Ciencias Básicas::Facultad de Ciencias::Escuela de Físic
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