118 results on '"Willis, Jon"'
Search Results
2. A systematic review of psychotropic drug prescribing for prisoners
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Griffiths, Elise V, Willis, Jon, and Spark, M. Joy
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- 2012
3. 'So we tell them': Articulating strong black masculinities in an urban indigenous community
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Mukandi, Bryan, Singh, David, Brady, Karla, Willis, Jon, Sinha, Tanya, Askew, Deborah, and Bond, Chelsea
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- 2019
4. A spectroscopic survey for gravitational lenses
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Willis, Jon Paul
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523.01 - Published
- 2000
5. The XXL Survey L. AGN contamination in galaxy clusters: detection and cosmological impact
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Bhargava, Sunayana, Garrel, Christian, Koulouridis, Elias, Pierre, Marguerite, Valtchanov, Ivan, Cerardi, Nicolas, Maughan, Ben J., Aguena, Michel, Benoist, Christophe, Baguley, Cale, Ramos-Ceja, Miriam E., Adami, Christophe, Chiappetti, Lucio, Vignali, Cristian, Willis, Jon P., Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
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[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] - Abstract
International audience; X-ray observations of galaxy clusters are impacted by the presence of active galactic nuclei (AGN) in a manner that is challenging to quantify, leading to biases in the detection and measurement of cluster properties for both astrophysics and cosmological applications. Using automated X-ray pipeline techniques, we introduce a new automated class for AGN-contaminated (AC) clusters in the XXL source detection software. The majority of these systems are otherwise missed by current X-ray cluster detection methods. The AC selection is also effective at distinguishing AGN and cool core presence using supplementary optical and infrared information. We present 33 AC objects, consisting of 25 clusters in the redshift range, $0.14 \leq z \leq 1.03$, and 8 other sources with significantly peaked central emission based on X-ray observations. Six of these are new confirmed clusters. We compute the missed fraction of the XXL survey, defined as the fraction of genuine clusters that are undetected due to their centrally peaked X-ray profiles. We report seven undetected AC clusters above $z > 0.6$, in the range where X-ray cluster detection efficiency drops significantly. The missed fraction is estimated to be at the level of $5\%$ for the 50 square degree XXL area. The impact on cosmological estimates from missed clusters is negligible for XXL, but produces a $\sim 3\sigma$ tension with the fiducial cosmology when considering larger survey areas. This work demonstrates the first systematic attempt to quantify the percentage of missed clusters in X-ray surveys as a result of central AGN contamination. Looking towards surveys such as eROSITA and Athena, larger areas and increased sensitivity will significantly enhance cluster detection, therefore robust methods for characterising AGN contamination will be crucial for precise cluster cosmology, particularly in the redshift $z > 1$ regime.
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- 2023
6. Compounded progesterone: Why is it acceptable to Australian women?
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Spark, M. Joy, Willis, Jon, and Byrne, Graeme
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- 2012
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7. Systematic review of progesterone use by midlife and menopausal women
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Spark, M. Joy and Willis, Jon
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- 2012
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8. What Do Gay Men Know About Human Papillomavirus? Australian Gay Men's Knowledge and Experience of Anal Cancer Screening and Human Papillomavirus
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PITTS, MARIAN K., FOX, CHRISTOPHER, WILLIS, JON, and ANDERSON, JONATHON
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- 2007
9. What really improves employee health and wellbeing: findings from regional Australian workplaces.
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Dr.. Dickson-Swift, Virginia, Dr.. Fox, Christopher, Mrs.. Marshall, Karen, Dr.. Welch, Nicky, Dr.. Willis, Jon, Dr.. Makrides, Lydia, and Ms.. Seymour, Andrea
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- 2014
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10. Mapping Indigenous Risk Workshop - Report to ANCAHRD
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Willis, Jon
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- 2001
11. Compounded progesterone and the Behavioral Model of Health Services Use
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Spark, Joy M., Willis, Jon, and Iacono, Teresa
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- 2014
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12. Application of cognitive interviewing to improve self-administered questionnaires used in small scale social pharmacy research
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Spark, Joy M. and Willis, Jon
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- 2014
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13. ZEN and the search for high-redshift galaxies
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Willis, Jon, Courbin, Frédéric, Kneib, Jean-Paul, and Minniti, Dante
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- 2006
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14. Do clinical pathways enhance access to evidence-based acute myocardial infarction treatment in rural emergency departments?
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Kinsman, Leigh D., Rotter, Thomas, Willis, Jon, Snow, Pamela C., Buykx, Penny, and Humphreys, John S.
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- 2012
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15. No more heroes
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Willis, Jon
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- 2010
16. Science, Technical and Strategic benefits of Canadian partnership with Subaru
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Balogh, Michael, Sawicki, Marcin, Damjanov, Ivana, Courteau, Stephane, Yee, Howard, Abraham, Bob, Bovy, Jo, Drout, Maria, Sivanandam, Suresh, Moon, Dae-Sik, Muzzin, Adam, Parker, Laura, Hudson, Mike, Percival, Will, Cami, Jan, O'Dea, Chris, Heyl, Jeremy, van Waerbeke, Ludo, Ellison, Sara, Willis, Jon, Venn, Kim, Bradley, Colin, Webb, Tracy, McConnachie, Alan, Marois, Christian, Kavelaars, JJ, Ferrarese, Laura, Cote, Pat, Gwyn, Stephen, Simard, Luc, Doyon, Rene, and Lafreniere, David
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astrophysics - Abstract
Recent developments have opened up an opportunity to join the Subaru telescope under favourable terms. With the demonstrated success of SCExAO and HSC, and first light of the PFS nearly upon us, the immediate prospects for Subaru to make breakthrough discoveries that align well with Canadian interests are excellent. In this white paper we describe the scientific and technical (instrumentation) opportunities that a partnership with Subaru would enable. IWe highlight the important synergies with TMT, MSE and Euclid, and how a relatively small investment in Subaru can significantly enhance our ability to take advantage of those facilities. In particular, access to PFS in the decade before MSE sees first light will be critical for ensuring Canadians have the technical and scientific expertise to fully exploit, and lead, science with that next generation spectroscopic facility. The partnership also has strategic value, as it represents an important step toward building an alliance of observatories on Maunakea, which itself has the potential for dramatically increasing scientific impact and reducing costs., White paper identifier W006
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- 2019
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17. The Maunakea Spectroscopic Explorer
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Hall, Pat, Balogh, Michael, Barmby, Pauline, Blakeslee, John, Bovy, Jo, Bradley, Colin, Bridges, Terry, Cami, Jan, Chapman, Scott, Chateauneuf, Francois, Cowan, Nick, Cote, Patrick, Damjanov, Ivana, Drout, Maria, Eadie, Gwendoyn, Ellison, Aara, Ferrarese, Laura, Fraser, Wesley, Gaensler, Bryan, Gallagher, Sarah, Haggard, Daryl, Henault-Brunet, Vincent, Herwig, Falk, Hill, Alexis, Hlavacek-Larrondo, Julie, Hudson, Mike, Johnson, Matt, Khatu, Viraja, Laporte, Chervin, McConnachie, Alan, McNamara, Brian, Mohammad, Faizan, Muzzin, Adam, Neilson, Hilding, Nemec, James, O'dea, Christopher, Parker, Laura, Patton, David, Percival, Will, Rogerson, Jesse, Ruan, John J., Sakara, Charli, Sawicki, Marcin, Simons, Doug, Sivakoff, Greg, Szeto, Kei, Tesfamariam, Solomon, Thanjavur, Karun, Thibeault, Simon, Thomas, Guillaume, Van Waerbeke, Ludovic, Venn, Kim, Webb, Tracy, Willis, Jon, and Woo, Joanna
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astrophysics - Abstract
The Maunakea Spectroscopic Explorer (MSE) is a project to design and construct a wide-field spectroscopic telescope at a site with excellent natural seeing, and in so doing to continue the tradition of Canadian leadership in wide-field astronomy established with the Canada-France-Hawaii Telescope. MSE is an end-to-end science platform for the design, execution and scientific exploitation of transformative, high-precision spectroscopic surveys at low-, medium-, and high-resolution from 0.37 to 1.8 microns. It will unveil the composition and dynamics of the faint Universe and impact nearly every field of astrophysics across spatial scales from individual stars to the largest scale structures in the Universe. Major pillars in the MSE science program include: (i) high spectral resolution Gaia follow-up to understand the chemistry and dynamics of the distant Milky Way in unprecedented detail; (ii) a revolutionary study of galaxy formation and evolution over billions of years back to `cosmic noon' when the Universe was at its peak of star formation; (iii) a large-volume, redshift survey to constrain inflationary physics and determine the mass of the neutrino; (iv) high fidelity measurements of the density profiles of the dark matter halos of Milky Way satellites; and (v) the largest sample yet of quasars with black hole masses measured from reverberation mapping, used to calibrate relationships enabling black hole mass estimates for millions of quasars. The MSE design features an 11.25m aperture telescope dedicated to multi-object spectroscopy over a 1.5 square degree field of view. A total of 3249 fibers will feed spectrographs operating at low (R ~= 3000) and moderate (R ~= 6000) spectral resolution, and an additional 1083 fibers will simultaneously feed high resolution spectrographs (R ~= 20,000-40,000). It is expected that 80% of useful observing time will be dedicated to large, multi-year Legacy Surveys proposed by MSE partners and chosen in a competitive, peer-reviewed process. The remaining 20% of observing time will be allocated to the partners, based on their relative share in MSE, for smaller Strategic Surveys. All MSE data will be available to all partners, with a proprietary period of several years before becoming publicly available. A set of Design Reference Surveys will be created and iterated during the design and construction phases so that the MSE science community is ready to propose surveys that take full advantage of all of the capabilities of MSE. Numerous international studies have concluded that the capabilities provided by MSE would be a critical hub in the emerging international network of front-line astronomical facilities over the coming decades, naturally complementing and extending the scientific power of TMT, SKA, Euclid, LSST, and many other facilities. High rankings in ongoing national reviews and success in peer-reviewed funding competitions will pave the way for detailed design of MSE in 2021-2025, construction in 2026-2031, and operation in the 2030s and well beyond. The cost to build the MSE conceptual design is US$420M, including risk margins, and the cost to operate the facility is estimated at US$25M/year, all in 2018 dollars. A model with several roughly equal major partners instead of one dominant partner is anticipated. The current MSE partnership consists of Canada, France, U. Hawaii, Australia, China, and India, plus observers from Texas A&M University, the US National Optical Astronomy Observatories, and a consortium of UK universities and research institutes. The MSE Science Team consists of approximately 400 scientists worldwide, including about 36 from Canada and an equal number from France, exceeded only by the number of members from the US. Recommendations: It is not realistic to expect that Canada can be a part of every single scientifically exciting astronomical facility that exists, will be built, or is proposed. Projects and facilities undertaken at a national level in Canada therefore need to be strategic investments that increase scientific and industrial capacity, build upon strengths, leverage past investments, and provide collaborative and leadership opportunities within the worldwide community. The MSE project fulfills those criteria and fills a major missing link in the future international network of multi-wavelength astronomical facilities. In that context, and given the benefits of an MSE facility to the Canadian community, we recommend: 1) that the community prioritizes continued Canadian involvement in the MSE project through its preliminary design phase, its final design phase, and its construction and operation on a suitable site, subject to successful design reviews and successful funding by an international partnership. 2) that the community supports a Canadian share in an MSE facility of at least 20%, ensuring that Canada has a significant voice in the project as one of the top 3 or 4 partners., White paper identifier W030
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- 2019
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18. The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition
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The MSE Science Team, Babusiaux, Carine, Bergemann, Maria, Burgasser, Adam, Ellison, Sara, Haggard, Daryl, Huber, Daniel, Kaplinghat, Manoj, Li, Ting, Marshall, Jennifer, Martell, Sarah, McConnachie, Alan, Percival, Will, Robotham, Aaron, Shen, Yue, Thirupathi, Sivarani, Tran, Kim-Vy, Yeche, Christophe, Yong, David, Adibekyan, Vardan, Aguirre, Victor Silva, Angelou, George, Asplund, Martin, Balogh, Michael, Banerjee, Projjwal, Bannister, Michele, Barría, Daniela, Battaglia, Giuseppina, Bayo, Amelia, Bechtol, Keith, Beck, Paul G., Beers, Timothy C., Bellinger, Earl P., Berg, Trystyn, Bestenlehner, Joachim M., Bilicki, Maciej, Bitsch, Bertram, Bland-Hawthorn, Joss, Bolton, Adam S., Boselli, Alessandro, Bovy, Jo, Bragaglia, Angela, Buzasi, Derek, Caffau, Elisabetta, Cami, Jan, Carleton, Timothy, Casagrande, Luca, Cassisi, Santi, Catelan, Márcio, Chang, Chihway, Cortese, Luca, Damjanov, Ivana, Davies, Luke J. M., de Grijs, Richard, de Rosa, Gisella, Deason, Alis, di Matteo, Paola, Drlica-Wagner, Alex, Erkal, Denis, Escorza, Ana, Ferrarese, Laura, Fleming, Scott W., Font-Ribera, Andreu, Freeman, Ken, Gänsicke, Boris T., Gabdeev, Maksim, Gallagher, Sarah, Gandolfi, Davide, García, Rafael A., Gaulme, Patrick, Geha, Marla, Gennaro, Mario, Gieles, Mark, Gilbert, Karoline, Gordon, Yjan, Goswami, Aruna, Greco, Johnny P., Grillmair, Carl, Guiglion, Guillaume, Hénault-Brunet, Vincent, Hall, Patrick, Handler, Gerald, Hansen, Terese, Hathi, Nimish, Hatzidimitriou, Despina, Haywood, Misha, Santisteban, Juan V. Hernández, Hillenbrand, Lynne, Hopkins, Andrew M., Howlett, Cullan, Hudson, Michael J., Ibata, Rodrigo, Ilić, Dragana, Jablonka, Pascale, Ji, Alexander, Jiang, Linhua, Juneau, Stephanie, Karakas, Amanda, Karinkuzhi, Drisya, Kim, Stacy Y., Kong, Xu, Konstantopoulos, Iraklis, Krogager, Jens-Kristian, Lagos, Claudia, Lallement, Rosine, Laporte, Chervin, Lebreton, Yveline, Lee, Khee-Gan, Lewis, Geraint F., Lianou, Sophia, Liu, Xin, Lodieu, Nicolas, Loveday, Jon, Mészáros, Szabolcs, Makler, Martin, Mao, Yao-Yuan, Marchesini, Danilo, Martin, Nicolas, Mateo, Mario, Melis, Carl, Merle, Thibault, Miglio, Andrea, Mohammad, Faizan Gohar, Molaverdikhani, Karan, Monier, Richard, Morel, Thierry, Mosser, Benoit, Nataf, David, Necib, Lina, Neilson, Hilding R., Newman, Jeffrey A., Nierenberg, A. M., Nord, Brian, Noterdaeme, Pasquier, O'Dea, Chris, Oshagh, Mahmoudreza, Pace, Andrew B., Palanque-Delabrouille, Nathalie, Pandey, Gajendra, Parker, Laura C., Pawlowski, Marcel S., Peter, Annika H. G., Petitjean, Patrick, Petric, Andreea, Placco, Vinicius, Popović, Luka Č., Price-Whelan, Adrian M., Prsa, Andrej, Ravindranath, Swara, Rich, R. Michael, Ruan, John, Rybizki, Jan, Sakari, Charli, Sanderson, Robyn E., Schiavon, Ricardo, Schimd, Carlo, Serenelli, Aldo, Siebert, Arnaud, Siudek, Malgorzata, Smiljanic, Rodolfo, Smith, Daniel, Sobeck, Jennifer, Starkenburg, Else, Stello, Dennis, Szabó, Gyula M., Szabo, Robert, Taylor, Matthew A., Thanjavur, Karun, Thomas, Guillaume, Tollerud, Erik, Toonen, Silvia, Tremblay, Pier-Emmanuel, Tresse, Laurence, Tsantaki, Maria, Valentini, Marica, Van Eck, Sophie, Variu, Andrei, Venn, Kim, Villaver, Eva, Walker, Matthew G., Wang, Yiping, Wang, Yuting, Wilson, Michael J., Wright, Nicolas, Xu, Siyi, Yildiz, Mutlu, Zhang, Huawei, Zwintz, Konstanze, Anguiano, Borja, Bedell, Megan, Chaplin, William, Collet, Remo, Cuillandre, Jean-Charles, Duc, Pierre-Alain, Flagey, Nicolas, Hermes, JJ, Hill, Alexis, Kamath, Devika, Laychak, Mary Beth, Małek, Katarzyna, Marley, Mark, Sheinis, Andy, Simons, Doug, Sousa, Sérgio G., Szeto, Kei, Ting, Yuan-Sen, Vegetti, Simona, Wells, Lisa, Babas, Ferdinand, Bauman, Steve, Bosselli, Alessandro, Côté, Pat, Colless, Matthew, Comparat, Johan, Courtois, Helene, Crampton, David, Croom, Scott, Davies, Luke, Denny, Kelly, Devost, Daniel, Driver, Simon, Fernandez-Lorenzo, Mirian, Guhathakurta, Raja, Han, Zhanwen, Higgs, Clare, Hill, Vanessa, Ho, Kevin, Hopkins, Andrew, Hudson, Mike, Isani, Sidik, Jarvis, Matt, Johnson, Andrew, Jullo, Eric, Kaiser, Nick, Kneib, Jean-Paul, Koda, Jun, Koshy, George, Mignot, Shan, Murowinski, Rick, Newman, Jeff, Nusser, Adi, Pancoast, Anna, Peng, Eric, Peroux, Celine, Pichon, Christophe, Poggianti, Bianca, Richard, Johan, Salmon, Derrick, Seibert, Arnaud, Shastri, Prajval, Smith, Dan, Sutaria, Firoza, Tao, Charling, Taylor, Edwar, Tully, Brent, van Waerbeke, Ludovic, Vermeulen, Tom, Walker, Matthew, Willis, Jon, Willot, Chris, Withington, Kanoa, International Max Planck Research School for Astronomy and Cosmic Physics (University of Heidelberg), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Center for Astrophysics and Space Sciences [La Jolla] (CASS), University of California [San Diego] (UC San Diego), University of California-University of California, Cognition, Langues, Langage, Ergonomie (CLLE-ERSS), École pratique des hautes études (EPHE)-Université Toulouse - Jean Jaurès (UT2J)-Université Bordeaux Montaigne-Centre National de la Recherche Scientifique (CNRS), Technicolor R & I [Cesson Sévigné], Technicolor, University of Edinburgh, University of Texas-Pan American (UTPA), University of Texas-Pan, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Max-Planck-Institut für Astrophysik (MPA), Max-Planck-Gesellschaft, Australian National University (ANU), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Max-Planck-Institut für Astronomie (MPIA), Lund Observatory, Lund University [Lund], Anglo-Australian Observatory (AAO), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Zentrum für Astronomie der Universität Heidelberg (ZAH), Universität Heidelberg [Heidelberg], Department of Physics and Astronomy [London, ON], University of Western Ontario (UWO), National Research Council of Canada (NRC), STScI, Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy, University of Cambridge [UK] (CAM), Joseph Louis LAGRANGE (LAGRANGE), Université Nice Sophia Antipolis (... - 2019) (UNS), Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Observatoire de la Côte d'Azur, Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Galaxies, Etoiles, Physique, Instrumentation (GEPI), PSL Research University (PSL)-PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Caltech Department of Astronomy [Pasadena], California Institute of Technology (CALTECH), Département d'Astrophysique (ex SAP) (DAP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), European Southern Observatory (ESO), Institut de Physique de Rennes (IPR), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-Centre National de la Recherche Scientifique (CNRS), Lawrence Berkeley National Laboratory [Berkeley] (LBNL), State Key Laboratory of Fine Chemicals, Franche-Comté Électronique Mécanique, Thermique et Optique - Sciences et Technologies (UMR 6174) (FEMTO-ST), Université de Franche-Comté (UFC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Technologie de Belfort-Montbeliard (UTBM), School of Physics and Astronomy, University of Birmingham [Birmingham], Laboratoire Univers et Particules de Montpellier (LUPM), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Department of Physics and Astronomy [Pittsburgh], University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE)-Pennsylvania Commonwealth System of Higher Education (PCSHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Sciences, Philosophie, Histoire (SPHERE UMR 7219), Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [UCLA Los Angeles], University of California [Los Angeles] (UCLA), Institute of Space Sciences [Barcelona] (ICE-CSIC), Spanish National Research Council [Madrid] (CSIC), Stellar Astrophysics Centre [Aarhus] (SAC), Aarhus University [Aarhus], High Speed Networks Laboratory, Dept. of Telecommunications and Media Informatics, Budapest University of Technology and Economics [Budapest] (BME), Laboratoire Interdisciplinaire Carnot de Bourgogne (LICB), Université de Bourgogne (UB)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique et de Géophysique [Liège], Université de Liège, College of Life Sciences, Peking Univertsity, Department of Mathematics [UCLA], Department of Psychology, St John's University, Canada-France-Hawaii Telescope Corporation (CFHT), National Research Council of Canada (NRC)-Centre National de la Recherche Scientifique (CNRS)-University of Hawai'i [Honolulu] (UH), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Departamento de FisicaTeorica e IFT-UAM/CSIC, Universidad Autonoma de Madrid (UAM), Institut de Physique Nucléaire de Lyon (IPNL), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Herzberg Institute of Astrophysics, Department of electronic engineering, Chang Gung University, Observatoire astronomique de Strasbourg (ObAS), Université de Strasbourg (UNISTRA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), The Open Group Research Institute (TOGRI), Université Joseph Fourier - Grenoble 1 (UJF), École normale supérieure - Paris (ENS Paris), Laboratoire Astrophysique de Toulouse-Tarbes (LATT), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Observatoire astronomique de Strasbourg (OAS), Institut national des sciences de l'Univers (INSU - CNRS)-Université Louis Pasteur - Strasbourg I-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), MSE Science Team, Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), École pratique des hautes études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Toulouse - Jean Jaurès (UT2J)-Université Bordeaux Montaigne-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institute of Astronomy [Cambridge], Université Côte d'Azur (UCA)-Université Nice Sophia Antipolis (... - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC), Sciences, Philosophie, Histoire (SPHERE (UMR_7219)), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Bourgogne (UB), University of California (UC)-University of California (UC), École Pratique des Hautes Études (EPHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Toulouse - Jean Jaurès (UT2J), Université de Toulouse (UT)-Université de Toulouse (UT)-Université Bordeaux Montaigne (UBM)-Centre National de la Recherche Scientifique (CNRS), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Universität Heidelberg [Heidelberg] = Heidelberg University, Université Nice Sophia Antipolis (1965 - 2019) (UNS), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur, COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS), Université de Rennes (UR)-Centre National de la Recherche Scientifique (CNRS), Université de Technologie de Belfort-Montbeliard (UTBM)-Ecole Nationale Supérieure de Mécanique et des Microtechniques (ENSMM)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC), Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Interdisciplinaire Carnot de Bourgogne (ICB), Peking University [Beijing], Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Universidad Autónoma de Madrid (UAM), École normale supérieure - Paris (ENS-PSL), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), and Lebreton, Yveline
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[PHYS]Physics [physics] ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::Instrumentation and Methods for Astrophysics ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies ,[PHYS] Physics [physics] ,[SDU] Sciences of the Universe [physics] ,[SDU]Sciences of the Universe [physics] ,Astrophysics of Galaxies (astro-ph.GA) ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Astrophysics::Galaxy Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unveil the composition and dynamics of the faint Universe and impact nearly every field of astrophysics across all spatial scales, from individual stars to the largest scale structures in the Universe. Major pillars in the science program for MSE include (i) the ultimate Gaia follow-up facility for understanding the chemistry and dynamics of the distant Milky Way, including the outer disk and faint stellar halo at high spectral resolution (ii) galaxy formation and evolution at cosmic noon, via the type of revolutionary surveys that have occurred in the nearby Universe, but now conducted at the peak of the star formation history of the Universe (iii) derivation of the mass of the neutrino and insights into inflationary physics through a cosmological redshift survey that probes a large volume of the Universe with a high galaxy density. MSE is positioned to become a critical hub in the emerging international network of front-line astronomical facilities, with scientific capabilities that naturally complement and extend the scientific power of Gaia, the Large Synoptic Survey Telescope, the Square Kilometer Array, Euclid, WFIRST, the 30m telescopes and many more., 9 chapters, 301 pages, 100 figures. This version of the DSC is a comprehensive update of the original version, released in 2016, which can be downloaded at arXiv:1606.00043. A detailed summary of the design of MSE is available in the MSE Book 2018, available at arXiv:1810.08695
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- 2019
19. Rural Australian community pharmacists' views on complementary and alternative medicine: a pilot study
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Willis Jon A, Dickson-Swift Virginia A, Bushett Nicole J, and Wood Pene
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Other systems of medicine ,RZ201-999 - Abstract
Abstract Background Complementary and alternative medicines (CAMs) are being used increasingly across the world. In Australia, community pharmacists are a major supplier of these products but knowledge of the products and interactions with other medicines is poor. Information regarding the use of CAMs by metropolitan pharmacists has been documented by the National Prescribing Service (NPS) in Australia but the views of rural/regional community pharmacists have not been explored. The aim of this pilot study was to explore the knowledge, attitudes and information seeking of a cohort of rural community pharmacists towards CAMs and to compare the findings to the larger NPS study. Methods A cross sectional self-administered postal questionnaire was mailed to all community pharmacists in one rural/regional area of Australia. Using a range of scales, data was collected regarding attitudes, knowledge, information seeking behaviour and demographics. Results Eighty eligible questionnaires were returned. Most pharmacists reported knowing that they should regularly ask consumers if they are using CAMs but many lacked the confidence to do so. Pharmacists surveyed for this study were more knowledgeable in regards to side effects and interactions of CAMs than those in the NPS survey. Over three quarters of pharmacists surveyed reported sourcing CAM information at least several times a month. The most frequently sought information was drug interactions, dose, contraindications and adverse effects. A variety of resources were used to source information, the most popular source was the internet but the most useful resource was CAM text books. Conclusions Pharmacists have varied opinions on the use of CAMs and many lack awareness of or access to good quality CAMs information. Therefore, there is a need to provide pharmacists with opportunities for further education. The data is valuable in assisting interested stakeholders with the development of initiatives to address the gaps in attitudes, knowledge and to improve effectiveness of information seeking behaviour.
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- 2011
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20. What is a clinical pathway? Development of a definition to inform the debate
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Snow Pamela, James Erica, Rotter Thomas, Kinsman Leigh, and Willis Jon
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Medicine - Abstract
Abstract Background Clinical pathways are tools used to guide evidence-based healthcare that have been implemented internationally since the 1980s. However, there is widespread lack of agreement on the impact of clinical pathways on hospital resources and patient outcomes. This can be partially attributed to the confusion for both researchers and healthcare workers regarding what constitutes a clinical pathway. This paper describes efforts made by a team of Cochrane Review authors to develop criteria to assist in the objective identification of clinical pathway studies from the literature. Methods We undertook a four-stage process aiming to develop criteria to define a clinical pathway: (1) identify publications exploring the definition of a clinical pathway; (2) derive draft criteria; (3) pilot test the criteria; and (4) modify criteria to maximise agreement between review authors. Results Previous literature and liaison with the European Pathways Association resulted in five criteria being used to define a clinical pathway: (1) the intervention was a structured multidisciplinary plan of care; (2) the intervention was used to translate guidelines or evidence into local structures; (3) the intervention detailed the steps in a course of treatment or care in a plan, pathway, algorithm, guideline, protocol or other 'inventory of actions'; (4) the intervention had timeframes or criteria-based progression; and (5) the intervention aimed to standardise care for a specific clinical problem, procedure or episode of healthcare in a specific population. After pilot testing it was decided that if an intervention met the first criteria (a structured multidisciplinary plan of care) plus three out of the other four criteria then it was included as a clinical pathway for the purposes of this review. In all, 27 studies were included in the final review. The authors of the included studies referred to these interventions as 'clinical pathways', 'protocols', 'care model', 'care map', 'multidisciplinary care', evidence-based care' and 'guideline'. Conclusions The criteria used for the identification of relevant studies for this Cochrane Review can be used as a foundation for the development of a standardised, internationally accepted definition of a clinical pathway.
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- 2010
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21. A cluster randomised trial to assess the impact of clinical pathways on AMI management in rural Australian emergency departments
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Snow Pamela C, Humphreys John S, Buykx Penny, Kinsman Leigh D, and Willis Jon
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Public aspects of medicine ,RA1-1270 - Abstract
Abstract Background People living in rural Australia are more likely to die in hospital following an acute myocardial infarction than those living in major cities. While several factors, including time taken to access hospital care, contribute to this risk, it is also partially attributable to the lower uptake of evidence-based guidelines for the administration of thrombolytic drugs in rural emergency departments where up to one-third of eligible patients do not receive this life-saving intervention. Clinical pathways have the potential to link evidence to practice by integrating guidelines into local systems, but their impact has been hampered by variable implementation strategies and sub-optimal research designs. The purpose of this study is to determine the impact of a five-step clinical pathways implementation process on the timely and efficient administration of thrombolytic drugs for acute myocardial infarctions managed in rural Australian emergency departments. Methods/Design The design is a two-arm, cluster-randomised trial with rural hospital emergency departments that treat and do not routinely transfer acute myocardial infarction patients. Six rural hospitals in the state of Victoria will participate, with three in the intervention group and three in the control group. Intervention hospitals will participate in a five-step clinical pathway implementation process: engagement of clinicians, pathway development according to local resources and systems, reminders, education, and audit and feedback. Hospitals in the control group will each receive a hard copy of Australian national guidelines for chest pain and acute myocardial infarction management. Each group will include 90 cases to give a power of 80% at 5% significance level for the two primary outcome measures: proportion of those eligible for thrombolysis receiving the drug and time to delivery of thrombolytic drug. Discussion Improved compliance with thrombolytic guidelines via clinical pathways will increase acute myocardial infarction survival rates in rural hospitals and thereby help to reduce rural-urban mortality inequalities. Such knowledge translation has the potential to be adapted for a range of clinical problems in a wide array of settings. Trial registration Australia New Zealand Clinical Trials Registry code ACTRN12608000209392.
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- 2009
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22. All These Worlds Are Yours : The Scientific Search for Alien Life
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Willis, Jon and Willis, Jon
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- Life on other planets, Exobiology
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Long before space travel was possible, the idea of life beyond Earth transfixed humans. In this fascinating book, astronomer Jon Willis explores the science of astrobiology and the possibility of locating other life in our own galaxy. Â Describing the most recent discoveries by space exploration missions, including the Kepler space telescope, the Mars Curiosity rover, and the New Horizons probe, Willis asks readers to imagine—and choose among—five scenarios for finding life. He encourages us to wonder whether life might exist within Mars's subsoil ice. He reveals the vital possibilities on the water-ice moons Europa and Enceladus. He views Saturn's moon Titan through the lens of our own planet's ancient past. And, he even looks beyond our solar system, investigating the top candidates for a “second Earth” in a myriad of exoplanets and imagining the case of a radio signal arriving from deep space. Covering the most up-to-date research, this accessibly written book provides readers with the basic knowledge necessary to decide where they would look for alien life.
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- 2016
23. Beyond the pipeline: a critique of the discourse surrounding the development of an Indigenous primary healthcare workforce in Australia.
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Bond, Chelsea, Brough, Mark, Willis, Jon, Stajic, Janet, Mukandi, Bryan, Canuto, Condy, Springer, Shannon, Askew, Deborah, Angus, Lynnell, and Lewis, Tara
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CULTURE ,ETHNOPSYCHOLOGY ,HEALTH services accessibility ,HEALTH status indicators ,LABOR supply ,PRIMARY health care ,RACISM ,ORGANIZATIONAL structure ,ACCESS to information - Abstract
A central strategy in addressing health disparities experienced by Indigenous people has been based on a concern with workforce improvement. In this paper, the Indigenous Australian healthcare workforce literature since 1977 is reviewed and its scope of concern, as being often limited to questions of 'supply', is critiqued. The pipeline metaphor, whether used explicitly or implied, regularly focuses attention on closing the gap on Indigenous representation within the health workforce. The exception though is the discourse concerning Indigenous Health Workers (IHWs), where questions concerning the legitimacy of the role continue to abound within a workforce hierarchy where community knowledge, though shown to be crucial to culturally safe health service provision, is trumped by the other health professions whose knowledges and legitimacy are not in question. This contrast exemplifies the need to examine the working of power not just 'supply'. The pipeline metaphor is disrupted with concerns about a range of other 'gaps' – gaps in the recognition of Indigenous knowledges, in organisational structures, in governance and in self-awareness by the health professions of their whiteness. As the health system continues to measure workforce development in terms of pipeline capacity, our study questions what happens beyond the pipeline. [ABSTRACT FROM AUTHOR]
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- 2019
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24. The multiwavelength survey by yale-chile (musyc): wide k-band imaging, photometric catalogs, clustering, and physical properties of galaxies at z similar to 2
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Blanc, Guillermo A., Lira, Paulina, Barrientos, L. Felipe, Aguirre, Paula, Francke, Harold, Taylor, Edward N., Quadri, Ryan, Marchesini, Danilo, Infante, Leopoldo, Gawiser, Eric, Hall, Patrick B., Willis, Jon P., Herrera, David, and Maza, Jose
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- 2008
25. The science of thermal imaging: Jon Willis, Flir training manager, ITC North EMEA, looks at the science of thermal imaging
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Willis, Jon
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Materials -- Thermal properties ,Cameras -- Usage -- Maintenance and repair ,Engineering and manufacturing industries - Abstract
Thermal imaging cameras are simultaneously becoming cheaper and more powerful. Alongside advances in hardware, the parallel development of software is making the technology exceptionally easy to use and significantly extending [...]
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- 2011
26. Health Benefits of Going On-Country.
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David, Gwendolyn, Yantarrnga, Jennifer, von Hippel, William, Shannon, Cindy, and Willis, Jon
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EMPLOYER-sponsored health insurance ,INDIGENOUS peoples ,EMOTIONS ,SUSTAINABLE development ,ENVIRONMENTAL policy - Published
- 2018
27. Improving the sexual health of Indigenous Australians: An evaluation of the Tri-State HIV/STD project
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Willis, Jon M, Wilson, Gai, Anderson, Ian, Rosenthal, Doreen, Smith, Anthony, Fairley, Christopher, and McDonald, Karalyn
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- 2002
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28. No more heroes: Jon Willis argues that healthcare services need collegiate, not charismatic, leadership
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Willis, Jon
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Leadership -- Methods ,Nurses -- Practice -- Social aspects ,Health ,Health care industry - Abstract
WHO WOULD you rather be led by: an engaging nurse or a heroic one? Is it better to be led by a charismatic visionary who is faster than a speeding [...]
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- 2010
29. Enhancing workplace health and wellbeing: A case study.
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Dickson-Swift, Virginia, Willis, Jon, Fox, Christopher, and Marshall, Karen
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- *
PREVENTIVE medicine , *CHRONIC diseases , *MENTAL illness , *INDUSTRIAL hygiene - Abstract
Preventative health initiatives have gained prominence in Australia as chronic diseases and mental illness are on the rise. Commonwealth and State governments in Australia are investing heavily in programs to protect and promote health, acknowledging the role of the workplace as an important setting for health promotion. This study was commissioned by the Victorian State Department of Health and carried out by researchers from La Trobe University Bendigo, Australia. A range of data was collected using a mixed method approach combining interviews and surveys. A range of barriers and facilitators for health promotion in the workplace were identified and recommendations for policy makers and employers are made that provide examples of ways to prioritize worker health and to incorporate workplace health promotion into the core business of organizations. [ABSTRACT FROM AUTHOR]
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- 2012
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30. What really improves employee health and wellbeingFindings from regional Australian workplaces.
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Dickson-Swift, Virginia, Fox, Christopher, Marshall, Karen, Welch, Nicky, and Willis, Jon
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Purpose – Factors for successful workplace health promotion (WHP) are well described in the literature, but often sourced from evaluations of wellness programmes. Less well understood are the features of an organisation that contribute to employee health which are not part of a health promotion programme. The purpose of this paper is to inform policy on best practice principles and provide real life examples of health promotion in regional Victorian workplaces. Design/methodology/approach – Individual case studies were conducted on three organisations, each with a health and wellbeing programme in place. In total, 42 employers and employees participated in a face to face interview. Interviews were transcribed verbatim and the qualitative data were thematically coded. Findings – Employers and senior management had a greater focus on occupational health and safety than employees, who felt that mental/emotional health and happiness were the areas most benefited by a health promoting workplace. An organisational culture which supported the psychosocial needs of the employees emerged as a significant factor in employee's overall wellbeing. Respectful personal relationships, flexible work, supportive management and good communication were some of the key factors identified as creating a health promoting working environment. Practical implications – Currently in Australia, the main focus of WHP programmes is physical health. Government workplace health policy and funding must expand to include psychosocial factors. Employers will require assistance to understand the benefits to their business of creating environments which support employee's mental and emotional health. Originality/value – This study took a qualitative approach to an area dominated by quantitative biomedical programme evaluations. It revealed new information about what employees really feel is impacting their health at work. [ABSTRACT FROM AUTHOR]
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- 2014
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31. So Far, So Good: Maintenance of Prevention Is Required to Stem HIV Incidence in Aboriginal and Torres Strait Islander Communities in Australia.
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Ward, James, Costello-Czok, Michael, Willis, Jon, Saunders, Mark, and Shannon, Cindy
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HIV prevention ,HEALTH promotion ,INTRAVENOUS drug abuse ,COMMUNITIES ,LABOR supply ,STRATEGIC planning ,MEDICAL care of indigenous peoples ,HEALTH of indigenous peoples ,DISEASE prevalence ,HEALTH & social status - Abstract
Indigenous people globally remain resilient yet vulnerable to the threats of HIV. Although Australian Aboriginal and Torres Strait Islander peoples experience the worst health status of any identifiable group in Australia, with a standardized morbidity rate three times that of non-Indigenous Australians, the Australian response to HIV has resulted in relatively low and stable rates of HIV infection among Australia's Indigenous peoples. This paper examines the reasons for the success of HIV prevention efforts. These include early recognition by Indigenous peoples of the potential effect that HIV could have on their communities; the supply of health hardware (needle and syringe programs and condoms); the development and implementation of culturally-appropriate health promotion messages such as the internationally-recognized Condoman campaign; the inclusion of dedicated Aboriginal and Torres Strait Islander Sexual Health Workers in communities; and an inclusive policy and partnership approach. Furthermore, the efforts of peak Aboriginal health organizations including NACCHO and its member services and Indigenous programs in peak mainstream organizations like AFAO and its member organizations, have all contributed to prevention success. Efforts need to be maintained however to ensure an escalated epidemic does not occur, particularly among heterosexual people, especially women, and people who inject drugs. New ideas are required as we enter a new era of HIV prevention within the context of the new paradigm of treatment as prevention, and getting to zero new infections. [ABSTRACT FROM AUTHOR]
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- 2014
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32. The multifaceted nature of access to compounded progesterone: A cross-sectional study from Australia.
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Spark, M. Joy, Willis, Jon, Byrne, Graeme, and Iacono, Teresa
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- *
PROGESTERONE , *CROSS-sectional method , *QUESTIONNAIRES , *PRINCIPAL components analysis , *HORMONE therapy - Abstract
Abstract: Objective: To explore the influences on accessibility of compounded progesterone therapy for Australian women. Study design: A cross-sectional survey of a stratified sample of Australian women who use progesterone only products using the ‘Perspectives on Progesterone’ questionnaire. Main outcome measures: Principle components analysis (PCA) to determine components of access to progesterone treatment and multi-way analysis of variance to compare groups. Results: Women using compounded progesterone were likely to have made at least one lifestyle adaptation (73%), and to have tried and stopped using at least one complementary and alternative medicine therapy (63%) or conventional hormone therapy (41%). PCA revealed six components of access to progesterone treatment: affordable, values natural treatments and is concerned about other treatments, conventionally available, perceived knowledge, values information gathered from a variety of sources, and rural & disadvantaged. The multifaceted nature of progesterone use illustrates that there are multiple aspects to use of non-conventional medicines. Women looking for non-conventional treatment are neither stupid nor uninformed, their understandings, based on experience and research, need to be addressed by health professionals while assessing their condition prior to discussing the risks and benefits of non-conventional medicines. Conclusion: Access to compounded progesterone is multifaceted, and many of the women who use it have tried other treatments first. Despite the clinical ambivalence towards progesterone as an alternative for women who may have tried and rejected other treatments, including conventional hormone therapy, the women described in this paper are using it. [Copyright &y& Elsevier]
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- 2014
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33. The Effects of Clinical Pathways on Professional Practice, Patient Outcomes, Length of Stay, and Hospital Costs: Cochrane Systematic Review and Meta-Analysis.
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Rotter, Thomas, Kinsman, Leigh, James, Erica, Machotta, Andreas, Willis, Jon, Snow, Pamela, and Kugler, Joachim
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HOSPITAL costs ,META-analysis ,HEALTH outcome assessment ,EVALUATION of medical care ,MEDICAL personnel - Abstract
This paper is a summary version of the previously published Cochrane review. It may increase the reach of the topic to health researchers and practitioners and encourage further discussion. The systematic review aims to summarize the evidence and assess the effect of clinical pathways on professional practice, patient outcomes, length of hospital stay, and hospital costs. The authors searched the Database of Abstracts of Reviews of Effectiveness, the Effective Practice and Organisation of Care Register, the Cochrane Central Register of Controlled Trials and bibliographic databases including MEDLINE, EMBASE, CINAHL, NHS EED, and Global Health. Twenty-seven studies considering a total of 11,398 participants were included for analysis. The main results were a reduction in in-hospital complications (odds ratio 0.58: 95% CI [0.36, 0.94] and improved documentation (odds ratio 11.95: 95% CI [4.72, 30.30]) associated with clinical pathways. Considerable variation in study design and settings prevented statistical pooling of results for length of stay (LOS) and hospital costs. The authors concluded that clinical pathways are associated with reduced in-hospital complications and improved documentation. [ABSTRACT FROM AUTHOR]
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- 2012
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34. Have We Drawn the Wrong Conclusions About the Value of Care Pathways? Is a Cochrane Review Appropriate? Response to the Commentary Article Published by Kris Vanhaecht et al.
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Rotter, Thomas, Kinsman, Leigh, James, Erica, Machotta, Andreas, Willis, Jon, Snow, Pamela, and Kugler, Joachim
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HOSPITAL care ,HEALTH care reform ,EVALUATION of medical care ,HOSPITAL care quality - Abstract
The commentary provided by Vanhaecht et al. from the European Pathways Association (EPA) questions whether conclusions derived from the review of effects of clinical pathways in hospitals are appropriate. They provide some methodological discussion that indicates a poor appreciation of the detailed content of the review as published in the Cochrane Library and a lack of understanding of the methodological requirements for complex interventions of the Cochrane Effective Practice and Organisation of Care (EPOC) group. In addition, Vanhaecht et al. misrepresent some important points from the review relating to the intervention reviewed. The critical commentary offered by Vanhaecht et al. is a misrepresentation of the process and content of the review and suggests they have not taken the time and effort to thoroughly read and understand this comprehensive review. [ABSTRACT FROM AUTHOR]
- Published
- 2012
- Full Text
- View/download PDF
35. PANIC AT THE DISCO-URSE: EPISODES FROM AN ANALYTIC AUTOETHNOGRAPHY ABOUT LIVING WITH HIV.
- Author
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Willis, Jon
- Subjects
- *
ANTIVIRAL agents , *SERODIAGNOSIS , *DIAGNOSIS of HIV infections , *AIDS , *ATTITUDE (Psychology) , *HUMAN body , *DISCOURSE analysis , *GROUP identity , *PATIENT compliance , *PATHOLOGICAL psychology , *SELF-perception , *HUMAN sexuality , *PSYCHOLOGY of the sick , *SOCIAL stigma , *PSYCHOLOGY of AIDS patients , *ETHNOLOGY research , *VIRAL load , *PSYCHOLOGY ,HIV infections & psychology - Abstract
Critical theorists from Walter Benjamin to Arthur Kroker and Debra Lupton have commented on how end-of-century or end-of-millennium social anxieties manifest in crises of social or subjective integrity including widespread social panic responses to perceived threats to such integrity. During the last 2 decades we have seen such a response to a range of public health issues, including obesity, drug use in sport, binge drinking, rural mental health, and the sexual health of social minorities. In this series of autoethnographic reflections, based in the framework of analytic autoethnography established by Leon Anderson (2006), 1 examine the impact of these panic discourses on the experience of living with a chronic disease. Particularly I examine the medicalization of HIV-infected bodies, the surveillance and governance of HIV-positive bodies, and the systematic distortions to self-care that result from the internalization of tropes of toxic or panic bodies. I also explore the possibilities for an emancipatory resistance to these tropes, and the place of hope and public health citizenship in the subjectivities of the chronically ill. [ABSTRACT FROM AUTHOR]
- Published
- 2011
- Full Text
- View/download PDF
36. Luminosity functions of XMM–LSS C1 galaxy clusters.
- Author
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Alshino, Abdulmonem, Khosroshahi, Habib, Ponman, Trevor, Willis, Jon, Pierre, Marguerite, Pacaud, Florian, and Smith, Graham P.
- Subjects
REDSHIFT ,GALAXY clusters ,ASTRONOMY ,ASTROPHYSICS ,METAPHYSICAL cosmology - Abstract
Canada–France–Hawaii Telescope Legacy Survey optical photometry has been used to study the galaxy luminosity functions (LFs) of 14 X-ray selected clusters from the XMM Large Scale Survey (XMM–LSS) survey. These are mostly groups and poor clusters, with masses ( M
500 ) in the range 0.6 to and redshifts . Hence, these are some of the highest redshift X-ray selected groups to have been studied. Lower and upper colour cuts were used to determine cluster members. We derive individual LFs for all clusters as well as redshift-stacked and temperature-stacked LFs in three filters, and , down to . All LFs were fitted by Schechter functions which constrained the faint-end slope, α, but did not always fit well to the bright end. Derived values of α ranged from −1.03 to as steep as −2.1. We find no evidence for upturns at faint magnitudes. Evolution in α was apparent in all bands: it becomes shallower with increasing redshift; for example, in the band it flattened from −1.75 at low redshift to −1.22 in the redshift range . Eight of our systems lie at , and we combine these to generate a galaxy LF in three colours for X-ray selected groups and poor clusters at redshift 0.3. We find that at is steeper (−1.67) in the green band than it is (−1.30) in the red band. This colour trend disappears at low redshift, which we attribute to reddening of faint blue galaxies from to 0. We also calculated the total optical luminosity and found it to correlate strongly with X-ray luminosity , and also with ICM temperature , consistent with expectations for self-similar clusters with constant mass-to-light ratio. We did not find any convincing correlation of Schechter parameters with mean cluster temperature. [ABSTRACT FROM AUTHOR]- Published
- 2010
- Full Text
- View/download PDF
37. A cluster randomised trial to assess the impact of clinical pathways on AMI management in rural Australian emergency departments.
- Author
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Kinsman, Leigh D., Buykx, Penny, Humphreys, John S., Snow, Pamela C., and Willis, Jon
- Subjects
MYOCARDIAL infarction ,EMERGENCY medical services ,RANDOMIZED controlled trials ,MEDICAL emergencies ,HEALTH outcome assessment - Abstract
Background: People living in rural Australia are more likely to die in hospital following an acute myocardial infarction than those living in major cities. While several factors, including time taken to access hospital care, contribute to this risk, it is also partially attributable to the lower uptake of evidence-based guidelines for the administration of thrombolytic drugs in rural emergency departments where up to one-third of eligible patients do not receive this life-saving intervention. Clinical pathways have the potential to link evidence to practice by integrating guidelines into local systems, but their impact has been hampered by variable implementation strategies and sub-optimal research designs. The purpose of this study is to determine the impact of a five-step clinical pathways implementation process on the timely and efficient administration of thrombolytic drugs for acute myocardial infarctions managed in rural Australian emergency departments. Methods/Design: The design is a two-arm, cluster-randomised trial with rural hospital emergency departments that treat and do not routinely transfer acute myocardial infarction patients. Six rural hospitals in the state of Victoria will participate, with three in the intervention group and three in the control group. Intervention hospitals will participate in a five-step clinical pathway implementation process: engagement of clinicians, pathway development according to local resources and systems, reminders, education, and audit and feedback. Hospitals in the control group will each receive a hard copy of Australian national guidelines for chest pain and acute myocardial infarction management. Each group will include 90 cases to give a power of 80% at 5% significance level for the two primary outcome measures: proportion of those eligible for thrombolysis receiving the drug and time to delivery of thrombolytic drug. Discussion: Improved compliance with thrombolytic guidelines via clinical pathways will increase acute myocardial infarction survival rates in rural hospitals and thereby help to reduce rural-urban mortality inequalities. Such knowledge translation has the potential to be adapted for a range of clinical problems in a wide array of settings. Trial registration: Australia New Zealand Clinical Trials Registry code ACTRN12608000209392. [ABSTRACT FROM AUTHOR]
- Published
- 2009
- Full Text
- View/download PDF
38. Combined analysis of weak lensing and X-ray blind surveys.
- Author
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Berg, Joel, Pacaud, Florian, Réfrégier, Alexandre, Massey, Richard, Pierre, Marguerite, Amara, Adam, Birkinshaw, Mark, Paulin-Henriksson, Stéphane, Smith, Graham P., and Willis, Jon
- Subjects
GALAXY clusters ,STAR observations ,INERTIA (Mechanics) ,ASTRONOMICAL observations ,GRAVITATION - Abstract
We present a joint weak lensing and X-ray analysis of 4 deg
2 from the CFHTLS and XMM-LSS surveys. Our weak lensing analysis is the first analysis of a real survey using shapelets, a new generation weak lensing analysis method. We create projected mass maps of the images, and extract six weak-lensing-detected clusters of galaxies. We show that their counts can be used to constrain the power-spectrum normalization for . We show that despite the large scatter generally observed in the mass–temperature relation derived from lensing masses, tight constraints on both its slope and normalization M* can be obtained with a moderate number of sources provided that the covered mass range is large enough. Adding clusters given by Bardeau et al. to our sample, we measure . Although they are dominated by shot noise and sample variance, our measurements are consistent with currently favoured values, and set the stage for future surveys. We thus investigate the dependence of those estimates on survey size, depth and integration time, for joint weak lensing and X-ray surveys. We show that deep surveys should be dedicated to the study of the physics of clusters and groups of galaxies. For a given exposure time, wide surveys provide a larger number of detected clusters and are therefore preferred for the measurement of cosmological parameters, such as σ8 and M* . We show that a wide survey of a few hundred square degrees is needed to improve upon current measurements of these parameters. More ambitious surveys covering 7000 deg2 will provide the 1 per cent accuracy in the estimation of the power-spectrum and the relation normalizations. [ABSTRACT FROM AUTHOR]- Published
- 2008
- Full Text
- View/download PDF
39. Three intervening galaxy absorbers towards GRB 060418: faint and dusty?
- Author
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Ellison, Sara L., Vreeswijk, Paul, Ledoux, Cédric, Willis, Jon P., Jaunsen, Andreas, Wijers, Ralph A. M. J., Smette, Alain, Fynbo, Johan P. U., Møller, Palle, Hjorth, Jens, and Kaufer, Andreas
- Subjects
GAMMA ray bursts ,REDSHIFT ,SPECTRUM analysis ,ATMOSPHERIC density ,MAGELLANIC clouds ,GALAXIES - Abstract
We present an analysis of three strong, intervening Mg II absorption systems towards the optical afterglow of gamma-ray burst (GRB) 060418. From high-resolution Ultraviolet and Visual Echelle Spectrograph (UVES) spectra we measure metal column densities and find that the highest redshift absorber exhibits a large amount of dust depletion compared with damped Lyman absorbers (DLAs) seen in quasi-stellar object (QSO) spectra. The intervening absorber is also unusual in exhibiting a clear 2175-Å bump, the first time this feature has been definitively detected in a GRB spectrum. The GRB afterglow spectrum is best fitted with a two-component extinction curve: a Small Magellanic Cloud (SMC) extinction law at (the redshift of the host) with and a Galactic extinction curve at with . We also present a moderately deep New Technology Telescope (NTT) R-band image of the GRB 060418 field and spectroscopy of four galaxies within 1 arcmin. None of these objects has a redshift that matches any of the intervening absorbers, and we conclude that the galaxies responsible for the two intervening Mg ii absorbers at have luminosities . [ABSTRACT FROM AUTHOR]
- Published
- 2006
- Full Text
- View/download PDF
40. Serendipity and the Sloan Digital Sky Survey: Discovery of the Largest Known Planetary Nebula on the Sky.
- Author
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Hewett, Paul C., Irwin, Michael J., Skillman, Evan D., Foltz, Craig B., Willis, Jon P., Warren, Stephen J., and Walton, Nicholas A.
- Published
- 2003
- Full Text
- View/download PDF
41. Gemini-South+FLAMINGOS Demonstration Science: Near-Infrared Spectroscopy of the z = 5.77 Quasar SDSS J083643.85+005453.3Based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Particle Physics and Astronomy Research Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), CNPq (Brazil), and CONICET (Argentina).
- Author
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Stern, Daniel, Hall, Patrick B., Barrientos, L. Felipe, Bunker, Andrew J., Elston, Richard, Ledlow, M. J., Raines, S. Nicholas, and Willis, Jon
- Published
- 2003
- Full Text
- View/download PDF
42. Condoms are for whitefellas: barriers to Pitjantjatjara men's use of safe sex technologies.
- Author
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Willis, Jon
- Subjects
- *
SAFE sex in AIDS prevention , *CONDOMS , *PITJANTJATJARA (Australian people) , *MASCULINITY - Abstract
This paper reports on ethnographic research on the culture-specific barriers that masculinity poses to preventing HIV transmission in the sexual lives of Pitjantjatjara men. The investigation had three objectives: investigating how the Pitjantjatjara people model the physical and social development of adult male bodies; describing the nature, range and cultural dynamics of sexual practice among Pitjantjatjara men; and delineating health and infection risks posed by sexual practice. The study used classical ethnographic approaches to investigate the deployment of men's bodies within systems of cultural production and reproduction, and post-Foucauldian analysis to examine culture-specific technologies of the self. Data were collected using participant observation, key informant interviews, and sexual life history interviews. Key findings are that the Pitjantjatjara deploy the capacities for reproduction and pleasure of men's bodies in culturally specific ways, and that men are trained in culturally approved uses of these capacities in ways that are resistant to change. The introduction of safe sex technologies in this context requires close attention to the specific content and methods by which men's self understandings are developed. [ABSTRACT FROM AUTHOR]
- Published
- 2003
- Full Text
- View/download PDF
43. Heteronormativity and the deflection of male same-sex attraction among the Pitjantjatjara people of Australia's Western Desert.
- Author
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Willis, Jon
- Subjects
- *
HOMOSEXUALITY , *BLOODBORNE infections , *PITJANTJATJARA (Australian people) - Abstract
This paper describes findings from fieldwork conducted among Pitjantjatjara tribespeople of Central Australia between 1989 and 1997. The study examined the impact of a distinctive gender system and practices of masculinity, particularly sexual and ritual practices, on the risk of contracting sexually transmissible infections and other blood-borne diseases. The research was designed as an ethnography of masculinity, conducted via participant observation, life history interviews, ritual analysis, and critical reflection on the work of early ethnographers. The paper presents selected field data, examined in the light of early twentieth century anthropological description of Pitjantjatjara sexuality. It identifies a systematic deflection of male same-sex attraction away from possible resolution through sexual practices between men. Key components of this deflection are the ritual construction of a culturally distinctive masculinity, the inextricable linkage between masculinity rites and the system for arranging marriages, and the cultural coding of the penis during ritual. The paper concludes that although men may feel erotic attraction for each other, the gender and kinship systems of the Pitjantjatjara conspire to limit completely the possibilities for the physical, sexual expression of this attraction. The findings reported here add to our understanding of the cultural basis of heteronormativity. [ABSTRACT FROM AUTHOR]
- Published
- 2003
- Full Text
- View/download PDF
44. Voices from the Frontline: Insights on Aboriginal and Torres Strait Islander Housing Advocacy.
- Author
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Currie, Jody, Castiello, Cecilia, Brunker, Raymond, Khalaj, Nafiseh, Meakin, Cody, Kefford, Glenn, Lewis, Ivy, Leitch, Jonathan, Aleckson, Jarryd, and Willis, Jon
- Subjects
- *
INDIGENOUS Australians , *HOUSING stability , *AUSTRALIANS , *HOUSING policy , *CULTURAL competence , *INDIGENOUS children , *HOMELESSNESS - Abstract
Homelessness is a significant issue in Australia, particularly for Aboriginal and Torres Strait Islander people, who are disproportionally affected compared to non-Indigenous Australians. In this article, we present new findings into the barriers and enablers of housing stability for Aboriginal and Torres Strait Islander people in the Brisbane and Logan areas of Queensland. The aim of the study was to document workers perceptions of barriers and enablers faced by Aboriginal and Torres Strait Islander people in Queensland when seeking to access housing. We drew on extensive interview data with front-line staff from an Aboriginal Community-Controlled Health Organisation (ACCHO) and in doing so identified five key themes: Bureaucratic Barriers and Inaccessibility of Services; Experiences of Discrimination; Impact of Family Dynamics on Housing Stability; Geographic Location; Comprehensive Support Needs. We demonstrated that consistent with the scholarly literature the interplay of systemic, structural, and cultural factors continues to impact housing stability. These findings suggest more work is required if governments are to address housing stability for Aboriginal and Torres Strait Islander individuals and families.IMPLICATIONSPresenting original data from social workers at an Aboriginal Community-Controlled Health Organisation (ACCHO) contributes to available understandings.In addressing housing challenges, cultural connection and competency are of vital importance.Voices from social workers can provide guidance for policymakers aiming to address homelessness for Aboriginal and Torres Strait Islander people.Presenting original data from social workers at an Aboriginal Community-Controlled Health Organisation (ACCHO) contributes to available understandings.In addressing housing challenges, cultural connection and competency are of vital importance.Voices from social workers can provide guidance for policymakers aiming to address homelessness for Aboriginal and Torres Strait Islander people. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF
45. Dying in country: implications of culture in the delivery of palliative care in indigenous Australian communities.
- Author
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Willis, Jon
- Subjects
- *
PITJANTJATJARA (Australian people) , *MATRILINEAL kinship - Abstract
Presents a study on the aspects of dying for Pitjantjatjara Aboriginal people in Central Australia. Preference of dying in Pitjantjatjara's home country; Provision of palliative care through matrilineal kin structures; Correlation of Pitjantjatjara's way of dying in their cultural way of living.
- Published
- 1999
- Full Text
- View/download PDF
46. Fatal attraction: do high-technology treatments for end-stage renal disease benefit Aboriginal patients in central Australia?
- Author
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Willis, Jon
- Published
- 1995
- Full Text
- View/download PDF
47. What is a clinical pathway? Development of a definition to inform the debate.
- Author
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Kinsman, Leigh, Rotter, Thomas, James, Erica, Snow, Pamela, and Willis, Jon
- Subjects
MEDICAL care ,ALGORITHMS ,TECHNICAL specifications ,EXAMINATIONS ,MEDICAL literature - Abstract
Background: Clinical pathways are tools used to guide evidence-based healthcare that have been implemented internationally since the 1980s. However, there is widespread lack of agreement on the impact of clinical pathways on hospital resources and patient outcomes. This can be partially attributed to the confusion for both researchers and healthcare workers regarding what constitutes a clinical pathway. This paper describes efforts made by a team of Cochrane Review authors to develop criteria to assist in the objective identification of clinical pathway studies from the literature. Methods: We undertook a four-stage process aiming to develop criteria to define a clinical pathway: (1) identify publications exploring the definition of a clinical pathway; (2) derive draft criteria; (3) pilot test the criteria; and (4) modify criteria to maximise agreement between review authors. Results: Previous literature and liaison with the European Pathways Association resulted in five criteria being used to define a clinical pathway: (1) the intervention was a structured multidisciplinary plan of care; (2) the intervention was used to translate guidelines or evidence into local structures; (3) the intervention detailed the steps in a course of treatment or care in a plan, pathway, algorithm, guideline, protocol or other 'inventory of actions'; (4) the intervention had timeframes or criteria-based progression; and (5) the intervention aimed to standardise care for a specific clinical problem, procedure or episode of healthcare in a specific population. After pilot testing it was decided that if an intervention met the first criteria (a structured multidisciplinary plan of care) plus three out of the other four criteria then it was included as a clinical pathway for the purposes of this review. In all, 27 studies were included in the final review. The authors of the included studies referred to these interventions as 'clinical pathways', 'protocols', 'care model', 'care map', 'multidisciplinary care', evidence-based care' and 'guideline'. Conclusions: The criteria used for the identification of relevant studies for this Cochrane Review can be used as a foundation for the development of a standardised, internationally accepted definition of a clinical pathway. [ABSTRACT FROM AUTHOR]
- Published
- 2010
- Full Text
- View/download PDF
48. The answer to this month's trouble shooter is provided by Jon Willis at FLIR Systems.
- Author
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Willis, Jon
- Subjects
THERMOGRAPHY ,IMAGE processing ,IMAGING systems - Published
- 2018
49. 20,000 pings under the sea.
- Author
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Willis, Jon
- Published
- 2017
- Full Text
- View/download PDF
50. On Piste/Off Piste.
- Author
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Willis, Jon
- Published
- 2017
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