Health-related quality of life in patients undergoing peritoneal dialysis : effects of a nurse-led case management programme

Author name used in this publication: Frances K. Y. Wong2009-2010 > Academic research: refereed > Publication in refereed journalVersion of RecordPublishe

A restraint reduction program in a local old age home

Author name used in this publication: Claudia K Y LaiAuthor name used in this publication: Sarah K F KongAuthor name used in this publication: Susan K Y Chow2002-2003 > Academic research: refereed > Publication in policy or professional journalVersion of RecordPublishe

Coping and caring : support for family caregivers of stroke survivors

Author name used in this publication: Susan K. Y. ChowAuthor name used in this publication: Frances K. Y. Wong2006-2007 > Academic research: refereed > Publication in refereed journalVersion of RecordPublishe

The effect of a restraint reduction program on physical restraint rates in rehabilitation settings in Hong Kong

Author name used in this publication: Claudia K. Y. LaiAuthor name used in this publication: Susan K. Y. ChowAuthor name used in this publication: Lorna K. P. Suen2011-2012 > Academic research: refereed > Publication in refereed journalVersion of RecordPublishe

Community nursing services for postdischarge chronically ill patients

Author name used in this publication: Susan K. Y. ChowAuthor name used in this publication: Frances K. Y. WongAuthor name used in this publication: Loretta Y. F. Chung2007-2008 > Academic research: refereed > Publication in refereed journalVersion of RecordPublishe

Patients' experiences of peritoneal dialysis at home: a phenomenological approach

The aim of this study was to highlight the meaning of home dialysis as experienced by patients with chronic renal failure. The research design was influenced by Ricoeur´s phenomenology. Nineteen patients from a Brazilian public hospital were interviewed, from May to September 2009. Interviews were guided by the question: "Tell me about your experiences lived undergoing PD". Findings unveiled the patients' perception of the drastic changes in their existence, consequent to disease and treatment; and the perception of themselves in that process. The feeling of anguish, physical pain and deprivations were part of living that condition. They foresee an uncertain future, depending on the expertise of health care providers and the demands on support of significant others. Findings suggest that individual aspects of patients' experiences must be considered if health care providers are to facilitate positive health outcomes.El objetivo de este estudio fue comprender la experiencia de la diálisis peritoneal domiciliaria, a partir de la narración de los pacientes. El abordaje del estudio se inspiró en la fenomenología hermenéutica de Paul Ricoeur. Fueron entrevistados 19 pacientes en la unidad de hemodiálisis de un hospital público brasileño, de marzo a septiembre de 2009. Las entrevistas fueron orientadas por la pregunta: describa su experiencia en la diálisis peritoneal. Los resultados revelaron la percepción de los participantes sobre el significado de la enfermedad en sus vidas y las drásticas transformaciones personales sufridas en ese proceso. Sentimientos de angustia y dolor física fueron acompañados por importantes limitaciones personales y sociales, impuestas por el tratamiento. Ellos esperan un futuro desconocido, reconociendo su dependencia de la ayuda de los familiares y de los profesionales de la salud. Los resultados revelan las dificultades y la falta de perspectivas experimentadas por los pacientes en diálisis, demostrando el papel crucial que le cabe a los profesionales que los acompañan. Ayudarlos a desarrollar el autocuidado y maximizar su calidad de vida es una prioridad en la asistencia a esos pacientes.O objetivo deste estudo foi compreender a experiência da diálise peritoneal domiciliar, a partir da narrativa dos pacientes. A abordagem do estudo inspirou-se na fenomenologia hermenêutica de Paul Ricoeur. Foram entrevistados 19 pacientes na unidade de hemodiálise de um hospital público brasileiro, de março a setembro de 2009. As entrevistas foram orientadas pela questão: descreva sua experiência na diálise peritoneal. Os resultados desvelaram a percepção dos participantes sobre o significado da doença em suas vidas e as drásticas transformações pessoais sofridas nesse processo. Sentimentos de angústia e dor física foram acompanhados por importantes limitações pessoais e sociais, impostas pelo tratamento. Eles esperam por um futuro incerto, reconhecendo sua dependência da ajuda dos familiares e dos profissionais da saúde. Os resultados desvelam as dificuldades e a falta de perspectivas vividas pelos pacientes em diálise, demonstrando o papel crucial que cabe aos profissionais que os acompanham. Ajudá-los a desenvolver o autocuidado e maximizar sua qualidade de vida é prioridade na assistência a esses pacientes

Supplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)

This Supplement provides supporting material for Abbott et al. (2016a). We briefly summarize past electromagnetic (EM) follow-up efforts as well as the organization and policy of the current EM follow-up program. We compare the four probability sky maps produced for the gravitational-wave transient GW150914, and provide additional details of the EM follow-up observations that were performed in the different bands

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

Localization and Broadband Follow-up of the Gravitational-wave Transient GW150914

A gravitational-wave (GW) transient was identified in data recorded by the Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) detectors on 2015 September 14. The event, initially designated G184098 and later given the name GW150914, is described in detail elsewhere. By prior arrangement, preliminary estimates of the time, significance, and sky location of the event were shared with 63 teams of observers covering radio, optical, near-infrared, X-ray, and gamma-ray wavelengths with ground- and space-based facilities. In this Letter we describe the low-latency analysis of the GW data and present the sky localization of the first observed compact binary merger. We summarize the follow-up observations reported by 25 teams via private Gamma-ray Coordinates Network circulars, giving an overview of the participating facilities, the GW sky localization coverage, the timeline, and depth of the observations. As this event turned out to be a binary black hole merger, there is little expectation of a detectable electromagnetic (EM) signature. Nevertheless, this first broadband campaign to search for a counterpart of an Advanced LIGO source represents a milestone and highlights the broad capabilities of the transient astronomy community and the observing strategies that have been developed to pursue neutron star binary merger events. Detailed investigations of the EM data and results of the EM follow-up campaign are being disseminated in papers by the individual teams. </p