5,923 results on '"Parker, Michael"'
Search Results
2. A Large Language Model Approach to Educational Survey Feedback Analysis
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Parker, Michael J., Anderson, Caitlin, Stone, Claire, and Oh, YeaRim
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- 2024
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3. Chapter 13 Ethical Hotspots in Infectious Disease Surveillance for Global Health Security Social justice and Pandemic Preparedness
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Parker, Michael
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Pandamic ,ethics ,infectious disease ,surveillance ,global health ,social justice ,preparedness ,bic Book Industry Communication::J Society & social sciences::JF Society & culture: general::JFM Ethical issues & debates - Abstract
At the time of writing, the world remains in the grip of the COVID-19 pandemic. Approximately 14.9 million people have died and every country in the world has been affected affectedaffectedaffectedaffected directly or indirectly (WHO 2022a). This, This,together with recent experiences of Ebola and Zika, has led to calls for the development and implementation of international strategies for pandemic preparedness, response, and prevention.
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- 2023
4. Transcendental Methods and Transcendental Arguments: A Criticism of Rahner’s Transcendental Theology
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Parker, Michael G.
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- 2017
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5. Twenty, Twenty-One
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Allison, Dorothy, Bergman, Megan Mayhew, Brown, Nic, Gingher, Marianne, Gurganus, Allan, House, Silas, Joy, David, Kenan, Randall, Knight, Michael, McCorkle, Jill, Parker, Michael, Perkins-Valdez, Dolen, Quatro, Jamie, Singleton, George, Smith, Katy Simpson, and Truong, Monique
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- 2016
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6. Prayer and Power: George Herbert and Renaissance Courtship (review)
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Parker, Michael P.
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- 2016
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7. Mud Doctoring: On Days of Heaven
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Parker, Michael
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- 2018
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8. A Large Language Model Approach to Educational Survey Feedback Analysis
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Parker, Michael J., Anderson, Caitlin, Stone, Claire, and Oh, YeaRim
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Computer Science - Computation and Language - Abstract
This paper assesses the potential for the large language models (LLMs) GPT-4 and GPT-3.5 to aid in deriving insight from education feedback surveys. Exploration of LLM use cases in education has focused on teaching and learning, with less exploration of capabilities in education feedback analysis. Survey analysis in education involves goals such as finding gaps in curricula or evaluating teachers, often requiring time-consuming manual processing of textual responses. LLMs have the potential to provide a flexible means of achieving these goals without specialized machine learning models or fine-tuning. We demonstrate a versatile approach to such goals by treating them as sequences of natural language processing (NLP) tasks including classification (multi-label, multi-class, and binary), extraction, thematic analysis, and sentiment analysis, each performed by LLM. We apply these workflows to a real-world dataset of 2500 end-of-course survey comments from biomedical science courses, and evaluate a zero-shot approach (i.e., requiring no examples or labeled training data) across all tasks, reflecting education settings, where labeled data is often scarce. By applying effective prompting practices, we achieve human-level performance on multiple tasks with GPT-4, enabling workflows necessary to achieve typical goals. We also show the potential of inspecting LLMs' chain-of-thought (CoT) reasoning for providing insight that may foster confidence in practice. Moreover, this study features development of a versatile set of classification categories, suitable for various course types (online, hybrid, or in-person) and amenable to customization. Our results suggest that LLMs can be used to derive a range of insights from survey text.
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- 2023
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9. Being as Symbol: On the Origins and Development of Karl Rahner’s Metaphysics by Stephen M. Fields, S.J. (review)
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Parker, Michael G.
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- 2017
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10. Are Children Always Vulnerable Research Participants?
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Cheah, Phaik Yeong and Parker, Michael
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- 2015
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11. Correction: Abeta targets of the biosimilar antibodies of Bapineuzumab, Crenezumab, Solanezumab in comparison to an antibody against N-truncted Abeta in sporadic Alzheimer disease cases and mouse models
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Bouter, Yvonne, Noguerola, Jose Socrates Lopez, Tucholla, Petra, Crespi, Gabriela A. N., Parker, Michael W., Wiltfang, Jens, Miles, Luke A., and Bayer, Thomas A.
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- 2024
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12. Afterword
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Bull, Susan, Parker, Michael, Selgelid, Michael J., Series Editor, Bull, Susan, editor, Parker, Michael, editor, Ali, Joseph, editor, Jonas, Monique, editor, Muthuswamy, Vasantha, editor, Saenz, Carla, editor, Smith, Maxwell J., editor, Voo, Teck Chuan, editor, Wright, Katharine, editor, and de Vries, Jantina, editor
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- 2024
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13. Introduction: Research Ethics and Health Policy in Epidemics and Pandemics
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Parker, Michael, Bull, Susan, Wright, Katharine, Selgelid, Michael J., Series Editor, Bull, Susan, editor, Parker, Michael, editor, Ali, Joseph, editor, Jonas, Monique, editor, Muthuswamy, Vasantha, editor, Saenz, Carla, editor, Smith, Maxwell J., editor, Voo, Teck Chuan, editor, Wright, Katharine, editor, and de Vries, Jantina, editor
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- 2024
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14. Stellar wind variability in Cygnus X-1 from high-resolution excess variance spectroscopy with Chandra
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Härer, Lucia K., Parker, Michael L., Mellah, Ileyk El, Grinberg, Victoria, Ballhausen, Ralf, Igo, Zsofi, Joyce, Amy, and Wilms, Jörn
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Solar and Stellar Astrophysics - Abstract
Stellar winds of massive stars are known to be driven by line absorption of UV photons, a mechanism which is prone to instabilities, causing the wind to be clumpy. The clumpy structure hampers wind mass-loss estimates, limiting our understanding of massive star evolution. The wind structure also impacts accretion in high-mass X-ray binary (HMXB) systems. We analyse the wavelength-dependent variability of X-ray absorption in the wind to study its structure. Such an approach is possible in HMXBs, where the compact object serves as an X-ray backlight. We probe different parts of the wind by analysing data taken at superior and inferior conjunction. We apply excess variance spectroscopy to study the wavelength-dependent soft X-ray variability of the HMXB Cygnus X-1 in the low/hard spectral state. Excess variance spectroscopy quantifies the variability of an object above the statistical noise as a function of wavelength, which allows us to study the variability of individual spectral lines. As one of the first studies, we apply this technique to high-resolution gratings spectra provided by Chandra, accounting for various systematic effects. The frequency dependence is investigated by changing the time binning. The strong orbital phase dependence we observe in the excess variance is consistent with column density variations predicted by a simple model for a clumpy wind. We identify spikes of increased variability with spectral features found by previous spectroscopic analyses of the same data set, most notably from silicon in over-dense clumps in the wind. In the silicon line region, the variability power is redistributed towards lower frequencies, hinting at increased line variability in large clumps. In prospect of the microcalorimetry missions that are scheduled to launch within the next decade, excess variance spectra present a promising approach to constrain the wind structure., Comment: Accepted by A&A
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- 2023
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15. UV/Optical disk reverberation lags despite a faint X-ray corona in the AGN Mrk 335
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Kara, Erin, Barth, Aaron J., Cackett, Edward M., Gelbord, Jonathan, Montano, John, Li, Yan-Rong, Santana, Lisabeth, Horne, Keith, Alston, William N., Buisson, Douglas, Chelouche, Doron, Du, Pu, Fabian, Andrew C., Fian, Carina, Gallo, Luigi, Goad, Michael R., Grupe, Dirk, Buitrago, Diego H. Gonzalez, Santisteban, Juan V. Hernandez, Kaspi, Shai, Hu, Chen, Komossa, S., Kriss, Gerard A., Lewin, Collin, Lewis, Tiffany, Loewenstein, Michael, Lohfink, Anne, Masterson, Megan, McHardy, Ian M., Mehdipour, Missagh, Miller, Jake, Panagiotou, Christos, Parker, Michael L., Pinto, Ciro, Remillard, Ron, Reynolds, Christopher, Rogantini, Daniele, Wang, Jian-Min, Wang, Jingyi, and Wilkins, Dan
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Astrophysics of Galaxies - Abstract
We present the first results from a 100-day Swift, NICER and ground-based X-ray/UV/optical reverberation mapping campaign of the Narrow-Line Seyfert 1 Mrk 335, when it was in an unprecedented low X-ray flux state. Despite dramatic suppression of the X-ray variability, we still observe UV/optical lags as expected from disk reverberation. Moreover, the UV/optical lags are consistent with archival observations when the X-ray luminosity was >10 times higher. Interestingly, both low- and high-flux states reveal UV/optical lags that are 6-11 times longer than expected from a thin disk. These long lags are often interpreted as due to contamination from the broad line region, however the u band excess lag (containing the Balmer jump from the diffuse continuum) is less prevalent than in other AGN. The Swift campaign showed a low X-ray-to-optical correlation (similar to previous campaigns), but NICER and ground-based monitoring continued for another two weeks, during which the optical rose to the highest level of the campaign, followed ~10 days later by a sharp rise in X-rays. While the low X-ray countrate and relatively large systematic uncertainties in the NICER background make this measurement challenging, if the optical does lead X-rays in this flare, this indicates a departure from the zeroth-order reprocessing picture. If the optical flare is due to an increase in mass accretion rate, this occurs on much shorter than the viscous timescale. Alternatively, the optical could be responding to an intrinsic rise in X-rays that is initially hidden from our line-of-sight., Comment: Accepted for publication in the Astrophysical Journal. 15 pages, 8 figures, 3 tables
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- 2023
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16. The Power of Withholding: Politics, Gender, and Narrative Technique in William Trevor's Felicia's Journey
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Parker, Michael
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- 2013
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17. Re-Entry and Recanalisation Techniques in the Endovascular Management of Peripheral Arterial Disease
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Makris, Gregory, Parker, Michael, Ali, Tariq, Geroulakos, George, editor, Avgerinos, Efthymios, editor, Becquemin, Jean Pierre, editor, Makris, Gregory C., editor, and Froio, Alberto, editor
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- 2024
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18. Stop 'n' Go
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Parker, Michael
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- 2017
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19. Clinical exome sequencing efficacy and phenotypic expansions involving anomalous pulmonary venous return
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Huth, Emily A., Zhao, Xiaonan, Owen, Nichole, Luna, Pamela N., Vogel, Ida, Dorf, Inger L. H., Joss, Shelagh, Clayton-Smith, Jill, Parker, Michael J., Louw, Jacoba J., Gewillig, Marc, Breckpot, Jeroen, Kraus, Alison, Sasaki, Erina, Kini, Usha, Burgess, Trent, Tan, Tiong Y., Armstrong, Ruth, Neas, Katherine, Ferrero, Giovanni B., Brusco, Alfredo, Kerstjens-Frederikse, Wihelmina S., Rankin, Julia, Helvaty, Lindsey R., Landis, Benjamin J., Geddes, Gabrielle C., McBride, Kim L., Ware, Stephanie M., Shaw, Chad A., Lalani, Seema R., Rosenfeld, Jill A., and Scott, Daryl A.
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- 2023
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20. The outburst of the changing-look AGN IRAS23226-3843 in 2019
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Kollatschny, Wolfram, Grupe, Dirk, Parker, Michael L., Ochmann, Martin W., Schartel, Norbert, Romero-Colmenero, Encarni, Winkler, Hartmut, Komossa, Stefanie, Famula, Philipp, Probst, Malte A., and Santos-Lleo, Maria
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Astrophysics of Galaxies - Abstract
IRAS23226-3843 has previously been classified as a changing-look AGN based on X-ray and optical spectral variations. In 2019, Swift observations revealed a strong rebrightening in X-ray and UV fluxes in comparison to observations in 2017. We took follow-up Swift, XMM-Newton, and NuSTAR observations together with optical spectra (SALT and SAAO 1.9m telescope) from 2019 until 2021. IRAS23226-3843 showed a strong X-ray and optical outburst in 2019. It varied in the X-ray and optical continuum by a factor of 5 and 1.6, respectively, within two months. This corresponds to a factor of 3 in the optical after correction for the host galaxy contribution. The Balmer and FeII emission-line intensities showed comparable variability amplitudes. The Halpha profiles changed from a blue-peaked profile in the years 1997 and 1999 to a broad double-peaked profile in 2017 and 2019. However, there were no major profile variations in the extremely broad double-peaked profiles despite the strong intensity variations in 2019. One year after the outburst, the optical spectral type changed and became a Seyfert type 2 in 2020. Blue outflow components are present in the Balmer lines and in the Fe band in the X-rays. A deep broadband XMM-Newton/NuSTAR spectrum was taken during the maximum state in 2019. This spectrum is qualitatively very similar to a spectrum taken in 2017, but by a factor of 10 higher. The soft X-ray band appears featureless. The soft excess is well modeled with a Comptonization model. A broadband fit with a power-law continuum, Comptonized soft excess, and Galactic absorption gives a good fit to the combined EPIC-pn and NuSTAR spectrum. In addition, we see a complex and broadened Fe K emission-line profile in the X-rays. The changing-look character in IRAS23226-3843 is most probably caused by changes in the accretion rate -- based on the short-term variations on timescales of weeks to months., Comment: 21 pages, 14 figures, Astronomy & Astrophysics in press
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- 2022
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21. Physics Beyond the Standard Model with Future X-ray Observatories: Projected Constraints on Very-Light Axion-Like Particles with $Athena$ and $AXIS$
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Sisk-Reynés, Júlia, Reynolds, Christopher S., Parker, Michael L., Matthews, James H., and Marsh, M. C. David
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Astrophysics - High Energy Astrophysical Phenomena ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Astrophysics - Astrophysics of Galaxies ,Astrophysics - Instrumentation and Methods for Astrophysics ,High Energy Physics - Phenomenology - Abstract
Axion-Like Particles (ALPs) are well-motivated extensions of the Standard Model of Particle Physics and a generic prediction of some string theories. X-ray observations of bright Active Galactic Nuclei (AGN) hosted by rich clusters of galaxies are excellent probes of very-light ALPs, with masses $\mathrm{log}(m_\mathrm{a}/\mathrm{eV}) < -12.0$. We evaluate the potential of future X-ray observatories, particularly $Athena$ and the proposed $AXIS$, to constrain ALPs via observations of cluster-hosted AGN, taking NGC 1275 in the Perseus cluster as our exemplar. Assuming perfect knowledge of instrument calibration, we show that a modest exposure (200-ks) of NGC 1275 by $Athena$ permits us to exclude all photon-ALP couplings $g_\mathrm{a\gamma} > 6.3 \times 10^{-14} \ {\mathrm{GeV}}^{-1}$ at the 95% level, as previously shown by $Conlon \ et \ al. \ (2018)$, representing a factor of 10 improvement over current limits. We then proceed to assess the impact of realistic calibration uncertainties on the $Athena$ projection by applying a standard $Cash$ likelihood procedure, showing the projected constraints on $g_\mathrm{a\gamma}$ weaken by a factor of 10 (back to the current most sensitive constraints). However, we show how the use of a deep neural network can disentangle the energy-dependent features induced by instrumental miscalibration and those induced by photon-ALP mixing, allowing us to recover most of the sensitivity to the ALP physics. In our explicit demonstration, the machine learning applied allows us to exclude $g_\mathrm{a\gamma} > 2.0 \times 10^{-13} \ {\mathrm{GeV}}^{-1}$, complementing the projected constraints of next-generation ALP dark matter birefringent cavity searches for very-light ALPs. Finally, we show that a 200-ks $AXIS$/on-axis observation of NGC 1275 will tighten the current best constraints on very-light ALPs by a factor of 3., Comment: 22 pages, 10 figures, 3 tables. Accepted for publication at the Astrophysical Journal. Comments welcome
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- 2022
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22. Combination of bazedoxifene with chemotherapy and SMAC-mimetics for the treatment of colorectal cancer
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Dmello, Rhynelle S., Palmieri, Michelle, Thilakasiri, Pathum S., Doughty, Larissa, Nero, Tracy L., Poh, Ashleigh R., To, Sarah Q., Lee, Erinna F., Douglas Fairlie, W., Mielke, Lisa, Parker, Michael W., Poon, Ivan K. H., Batlle, Eduard, Ernst, Matthias, and Chand, Ashwini L.
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- 2024
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23. From Winter Seeds to Wintering Out : The Evolution of Heaney's Third Collection
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Parker, Michael
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- 2007
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24. I'm Talking about Shaft
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Parker, Michael
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- 2006
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25. Ethics and Tropical Diseases: Some Global Considerations
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Jamrozik, Euzebiusz, primary, Parker, Michael, additional, and Bull, Susan, additional
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- 2024
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26. CONTRIBUTORS
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Abahuje, Egide, primary, Abrahim, Orit, additional, Adetifa, Ifedayo M.O., additional, Ajjampur, Sitara S.R., additional, Alexander, Suceena, additional, PhD, Chiara Altare,, additional, Alves, Fabiana, additional, Andrianaivoarimanana, Voahangy, additional, Angelakis, Emmanouil, additional, Aronson, Jeffrey K., additional, Atukorala, Inoshi G., additional, Baily, Guy, additional, Baker, Stephen, additional, Barrett, Alan D.T., additional, Basnyat, Buddha, additional, Bastawrous, Andrew, additional, Bates, Imelda, additional, Bausch, Daniel G., additional, Baxter, Cheryl, additional, Beare, Nicholas A.V., additional, Beeching, Nick J., additional, Bekker, Linda-Gail, additional, Berlin, Anita, additional, FRS, Zulfiqar A. Bhutta, additional, Bloom, David E., additional, Blumberg, Lucille, additional, Boelaert, Marleen, additional, Brett-Major, David, additional, Brooker, Simon J., additional, Brouwer, Matthijs C., additional, Brunetti, Enrico, additional, Bull, Susan, additional, Bundy, Donald A.P., additional, Burri, Christian, additional, Bustinduy, Amaya L., additional, Caillet, Céline, additional, Chai, Jong Yil, additional, Chang, Thashi, additional, Chappuis, François, additional, Chibi, Buyisile, additional, Chiodini, Peter L., additional, Chowdhury, Rajiv, additional, Chowdhury, Sudipta Dhar, additional, Clemens, John D., additional, Cooke, Graham S., additional, Cotton, Mark F., additional, Currie, Bart J., additional, Cusack, Tomas-Paul, additional, Dance, David A.B., additional, Davis, Emily H., additional, Day, Nicholas P.J., additional, Deen, Jacqueline, additional, Dondorp, Arjen M., additional, Dünser, Martin W., additional, Eitzen, Edward, additional, Chebib, Hassan El, additional, Enria, Delia, additional, Faust, Christina, additional, Fekadu, Abebaw, additional, Fink, Günther, additional, Fischer, Peter U., additional, Fletcher, Tom, additional, Franco-Paredes, Carlos, additional, French, Neil, additional, Frumkin, Howard, additional, Garcia, Hector H., additional, Gerada, Alessandro, additional, Glass, Roger I., additional, Gordon, Stephen B., additional, Gottstein, Bruno, additional, Goyal, Alpesh, additional, Grey, Jonathan, additional, Gupta, Yashdeep, additional, Haines, Andy, additional, Hampson, Katie, additional, Hanlon, Charlotte, additional, Harrison, Mark, additional, Haswell, Melissa R., additional, Hawkesworth, Sophie, additional, Hay, Roderick J., additional, Heckmann, Jeannine M., additional, Heimesaat, Markus M., additional, Henao-Martínez, Andrés F., additional, Hien, Tran Tinh, additional, Hoerauf, Achim, additional, Irfan, Omar, additional, PhD, Euzebiusz Jamrozik, additional, Jobe, Modou, additional, John, George T., additional, Jones, Nick K., additional, Jones, Malcolm K., additional, Junghanss, Thomas, additional, Kaewkes, Sasithorn, additional, Karim, Quarraisha Abdool, additional, Keiser, Jennifer, additional, Kelly, Paul, additional, Khan, Amira M., additional, King, Charles H., additional, Kishore, Sandeep P., additional, Lang, Trudie, additional, Le, Thuy, additional, Liesenfeld, Oliver, additional, Lockwood, Diana N.J., additional, Mabey, David C.W., additional, Madkour, M. Monir, additional, Manesh, Abi, additional, Masekela, Refiloe, additional, Mäser, Pascal, additional, Mayaud, Philippe, additional, Mbanya, Dora, additional, McCarthy, James S., additional, McCartney, Daniel J., additional, McGready, Rose, additional, McKee, Martin, additional, Mc, Namara, Paul S., additional, Meara, John G., additional, Meintjes, Graeme, additional, Merson, Laura, additional, Mola, Glen, additional, Morassutti, Alessandra L., additional, Morris-Jones, Rachael, additional, Mortimer, Kevin J., additional, Muliyil, Divya Elizabeth, additional, Mumcuoglu, Kosta Y., additional, Munoz, Flor M., additional, Murphy, Adrianna, additional, Mutabingwa, Theonest, additional, Nawa, Yukifumi, additional, Newton, Paul N., additional, Nightingale, Sam, additional, Nokes, D. James, additional, Nosten, François H., additional, O’Hea, Jennifer, additional, Olliaro, Piero, additional, Ong, Jason J., additional, Oommen, Anu Mary, additional, Parashar, Umesh D., additional, Paris, Daniel H., additional, Parker, Michael, additional, Pluschke, Gerd, additional, Preidis, Geoffrey A., additional, Prentice, Andrew M., additional, Quail, Geoffrey, additional, Quinn, Thomas C., additional, Rabie, Helena, additional, Rajashekharaiah, Harsha, additional, Rajerison, Minoarisoa, additional, Ranganathan, Kannan, additional, Raoult, Didier, additional, Rassi,, Anis, additional, Ravi, Vasanthapuram, additional, Reddy, K. Srinath, additional, Rees, Claire, additional, Reynolds, Steven J., additional, Richter, Joachim, additional, Rijken, Marcus J., additional, Riviello, Robert, additional, Robinson, Janet, additional, Salazar, Juan C., additional, Schultz, Marcus J., additional, Schwarz, Dan, additional, Sendagire, Ibrahim, additional, Sharma, Savitri, additional, Shawon, Shajedur Rahman, additional, Singh, Bhagteshwar, additional, Sithithaworn, Paiboon, additional, Siwila, Joyce, additional, Solomon, Tom, additional, Spiegel, Paul, additional, Sridhar, Devi, additional, Sripa, Banchob, additional, Srour, M. Leila, additional, Stojković, Marija, additional, Strader, Christopher, additional, Suárez, Jose A., additional, Sundar, Shyam, additional, Tamarozzi, Francesca, additional, Tandon, Nikhil, additional, Tate, Jacqueline E., additional, Thachil, Jecko, additional, Thomson, Madeleine C., additional, Thwaites, Guy, additional, Thwaites, C. Louise, additional, van Daalen, Kim R., additional, Beek, Diederik van de, additional, van Doorn, H. Rogier, additional, Vega-Lopez, Francisco, additional, von Seidlein, MD, PhD, Lorenz, additional, Wakeham, Katie, additional, Walker, Stephen L., additional, Wallace, Ryan M., additional, Ward, Honorine, additional, Warrell, David A., additional, Weber, Tim Frederik, additional, Weil, Gary J., additional, White, Nicholas J., additional, White, MB Ch, B, Graham B., additional, Wong, Vanessa, additional, Wood, Robin, additional, Wood, Georgina, additional, Wyllie, Sarah, additional, Yacoub, Sophie, additional, Yen, Lam Minh, additional, Young, Paul R., additional, and Zafren, Ken, additional
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- 2024
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27. Comparing Reflection and Absorption Models for the Soft X-ray Variability in the NLS1 AGN UGC 11763
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Jiang, Jiachen, Gallo, Luigi C., Grupe, Dirk, and Parker, Michael L.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present a spectral analysis of two XMM-Newton observations of the narrow-line Seyfert 1 galaxy UGC 11763. UGC 11763 shows very different soft X-ray spectral shapes in the two observations separated by 12 years. Three spectral models are considered to explain the multi-epoch X-ray variability of UGC 11763, one based on the relativistic disc reflection model, one based on multiple partially-covering absorbers combined with the warm corona model, and a hybrid model. In the first model, the X-ray variability of UGC 11763 is caused by the emission from a compact coronal region with a variable size. The resulting disc reflection component changes accordingly. A warm absorption model with a modest column density is required in this model too. In the partially-covering absorption scenario, the X-ray variability of UGC 11763 is caused by the variable covering factors of two absorbers located within a region of $r<\approx100r_{\rm g}$. Moreover, the temperature and strength of the warm corona have to change significantly too to explain the variable underlying soft X-ray emission. Lastly, we investigate the possibility of variable intrinsic power-law emission from the hot corona combined with variable absorption in UGC 11763 without changing the geometry of the corona in the third model. This hybrid model provides a slightly better fit than the partially-covering absorption model with improvements in fitting the iron emission band. Current CCD-resolution data cannot distinguish these spectral models for UGC 11763. Future high-resolution X-ray missions, e.g. Athena and XRISM, will test them by resolving different spectral components., Comment: 13 pages, 10 figures, accepted by MNRAS
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- 2022
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28. Northern Odyssey: John Montague's "The Cry" (1964) in Its Political Contexts
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Parker, Michael
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- 2003
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29. The long-stable hard state of XTE J1752-223 and the disk truncation dilemma
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Connors, Riley M. T., Garcia, Javier A., Tomsick, John, Mastroserio, Guglielmo, Grinberg, Victoria, Steiner, James F., Jiang, Jiachen, Fabian, Andrew C., Parker, Michael L., Harrison, Fiona, Hare, Jeremy, Mallick, Labani, and Lazar, Hadar
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
The degree to which the thin accretion disks of black hole X-ray binaries are truncated during hard spectral states remains a contentious open question in black hole astrophysics. During its singular observed outburst in $2009\mbox{--}2010$, the black hole X-ray binary XTE J1752-223 spent $\sim1$~month in a long-stable hard spectral state at a luminosity of $\sim0.02\mbox{--}0.1~L_{\rm Edd}$. It was observed with 56 RXTE pointings during this period, with simultaneous Swift-XRT daily coverage during the first 10 days of the RXTE observations. Whilst reflection modeling has been extensively explored in the analysis of these data, there is a disagreement surrounding the geometry of the accretion disk and corona implied by the reflection features. We re-examine the combined, high signal-to-noise, simultaneous Swift and RXTE observations, and perform extensive reflection modeling with the latest relxill suite of reflection models, including newer high disk density models. We show that reflection modeling requires that the disk be within $\sim5~R_{\rm ISCO}$ during the hard spectral state, whilst weaker constraints from the thermal disk emission imply higher truncation ($R_{\rm in}=6\mbox{--}80~R_{\rm ISCO}$). We also explore more complex coronal continuum models, allowing for two Comptonization components instead of one, and show that the reflection features still require only a mildly truncated disk. Finally we present a full comparison of our results to previous constraints found from analyses of the same dataset., Comment: 18 pages, 9 figures, accepted by ApJ
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- 2022
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30. A Disc Reflection Model for Ultra-Soft Narrow-Line Seyfert 1 Galaxies
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Jiang, Jiachen, Gallo, Luigi C., Fabian, Andrew C., Parker, Michael L., and Reynolds, Christopher S.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present a detailed analysis of the XMM-Newton observations of five narrow-line Seyfert 1 galaxies (NLS1s). They all show very soft continuum emission in the X-ray band with a photon index of $\Gamma\gtrsim 2.5$. Therefore, they are referred to as `ultra-soft' NLS1s in this paper. By modeling their optical/UV-X-ray spectral energy distribution (SED) with a reflection-based model, we find indications that the disc surface in these ultra-soft NLS1s is in a higher ionisation state than other typical Seyfert 1 AGN. Our best-fit SED models suggest that these five ultra-soft NLS1s have an Eddington ratio of $\lambda_{\rm Edd}=1-20$ assuming available black hole mass measurements. In addition, our models infer that a significant fraction of the disc energy in these ultra-soft NLS1s is radiated away in the form of non-thermal emission instead of the thermal emission from the disc. Due to their extreme properties, X-ray observations of these sources in the iron band are particularly challenging. Future observations, e.g. from Athena, will enable us to have a clearer view of the spectral shape in the iron band and thus distinguish the reflection model from other interpretations of their broadband spectra., Comment: 16 pages, 11 figures; published in MNRAS, Volume 498, Issue 3, November 2020. The Reflionx model used in this work is available for download at https://www.michaelparker.space/reflionx-models
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- 2022
31. A NuSTAR and Swift View of the Hard State of MAXI J1813-095
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Jiang, Jiachen, Buisson, Douglas J. K., Dauser, Thomas, Fabian, Andrew C., Fürst, Felix, Gallo, Luigi C., Harrison, Fiona A., Parker, Michael L., Steiner, James F., Tomsick, John A., Ubach, Santiago, and Walton, Dominic J.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present an analysis of the NuSTAR and Swift spectra of the black hole candidate MAXI J1813-095 in a failed-transition outburst in 2018. The NuSTAR observations show evidence of reflected emission from the inner region of the accretion disc. By modelling the reflection component in the spectra, we find a disc inner radius of $R_{\rm in}<7$ $r_{\rm g}$. This result suggests that either a slightly truncated disc or a non-truncated disc forms at a few percent of the Eddington limit in MAXI J1813-095. Our best-fit reflection models indicate that the geometry of the innermost accretion remains consistent during the period of NuSTAR observations. The spectral variability of MAXI J1813-095 from multi-epoch observations is dominated by the variable photon index of the Comptonisation emission., Comment: 9 pages, 12 figures, accepted for publication in MNRAS
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- 2022
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32. Exome sequencing efficacy and phenotypic expansions involving esophageal atresia/tracheoesophageal fistula plus.
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Sy, Mary, Chauhan, Jaynee, Prescott, Katrina, Imam, Aliza, Kraus, Alison, Beleza, Ana, Salkeld, Lee, Hosdurga, Saraswati, Parker, Michael, Vasudevan, Pradeep, Islam, Lily, Goel, Himanshu, Bain, Nicole, Park, Soo-Mi, Mohammed, Shehla, Dieterich, Klaus, Coutton, Charles, Satre, Véronique, Vieville, Gaëlle, Donaldson, Alan, Beneteau, Claire, Ghoumid, Jamal, Van Den Bogaert, Kris, Boogaerts, Anneleen, Boudry, Elise, Vanlerberghe, Clémence, Petit, Florence, Bernardini, Laura, Torres, Barbara, Mattina, Teresa, Carli, Diana, Mandrile, Giorgia, Pinelli, Michele, Brunetti-Pierri, Nicola, Neas, Katherine, Beddow, Rachel, Tørring, Pernille, Faletra, Flavio, Spedicati, Beatrice, Gasparini, Paolo, Mussa, Alessandro, Ferrero, Giovanni, Lampe, Anne, Lam, Wayne, Bi, Weimin, Bacino, Carlos, Kuwahara, Akela, Zhao, Xiaonan, Luna, Pamela, Shaw, Chad, Rosenfeld, Jill, Scott, Daryl, and Bush, Jeffrey
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Fanconi anemia ,NRXN1 ,TCF4 ,esophageal atresia ,exome sequencing ,tracheoesophageal fistula ,Humans ,Tracheoesophageal Fistula ,Esophageal Atresia ,Exome ,Exome Sequencing - Abstract
Esophageal atresia/tracheoesophageal fistula (EA/TEF) is a life-threatening birth defect that often occurs with other major birth defects (EA/TEF+). Despite advances in genetic testing, a molecular diagnosis can only be made in a minority of EA/TEF+ cases. Here, we analyzed clinical exome sequencing data and data from the DECIPHER database to determine the efficacy of exome sequencing in cases of EA/TEF+ and to identify phenotypic expansions involving EA/TEF. Among 67 individuals with EA/TEF+ referred for clinical exome sequencing, a definitive or probable diagnosis was made in 11 cases for an efficacy rate of 16% (11/67). This efficacy rate is significantly lower than that reported for other major birth defects, suggesting that polygenic, multifactorial, epigenetic, and/or environmental factors may play a particularly important role in EA/TEF pathogenesis. Our cohort included individuals with pathogenic or likely pathogenic variants that affect TCF4 and its downstream target NRXN1, and FANCA, FANCB, and FANCC, which are associated with Fanconi anemia. These cases, previously published case reports, and comparisons to other EA/TEF genes made using a machine learning algorithm, provide evidence in support of a potential pathogenic role for these genes in the development of EA/TEF.
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- 2022
33. Assessing the Knowledge and Comfort Level of US Family Medicine Residents Regarding Consenting and Confidentiality in Adolescent Health Care
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Eniola, Kehinde, Brown, Carina, Pray, Margaret, Foster, Krys E., Richter, Scott, Parker, Michael, and Carvajal, Diana N.
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- 2024
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34. XMM-Newton Observations of the Narrow-Line Seyfert 1 Galaxy IRAS 13224$-$3809 : X-ray Spectral Analysis II
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Jiang, Jiachen, Dauser, Thomas, Fabian, Andrew C., Alston, William N., Gallo, Luigi C., Parker, Michael L., and Reynolds, Christopher S.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
Previously, we modelled the X-ray spectra of the narrow-line Seyfert 1 galaxy IRAS 13224$-$3809 using a disc reflection model with a fixed electron density of $10^{15}$ cm$^{-3}$. An additional blackbody component was required to fit the soft X-ray excess below 2 keV. In this work, we analyse simultaneously five flux-resolved XMM-Newton spectra of this source comprising data collected over 2 Ms. A disc reflection model with an electron density of $n_{\rm e}\approx10^{20}$ cm$^{-3}$ and an iron abundance of $Z_{\rm Fe}=3.2\pm0.5Z_{\odot}$ is used to fit the broad-band spectra of this source. No additional component is required to fit the soft excess. Our best-fit model provides consistent measurements of black hole spin and disc inclination angle as in previous models where a low disc density was assumed. In the end, we calculate the average illumination distance between the corona and the reflection region in the disc of IRAS 13224$-$3809 based on best-fit density and ionisation parameters, which changes from 0.43$\sqrt{f_{\rm AD}/f_{\rm INF}}$ $r_{\rm g}$ in the lowest flux state to 1.71$\sqrt{f_{\rm AD}/f_{\rm INF}}$ $r_{\rm g}$ in the highest flux state assuming a black hole mass of $2\times10^{6}M_{\odot}$. $f_{\rm AD}/f_{\rm INF}$ is the ratio between the flux of the coronal emission that reaches the accretion disc and infinity. This ratio depends on the geometry of the coronal region in IRAS 13224$-$3809. So we only discuss its value based on the simple `lamp-post' model, although detailed modelling of the disc emissivity profile of IRAS 13224$-$3809 is required in future to reveal the exact geometry of the corona., Comment: 17 pages, 15 figures including appendices; accepted for publication in MNRAS
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- 2022
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35. Ejection-accretion connection in NLS1 AGN 1H 1934-063
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Xu, Yerong, Pinto, Ciro, Kara, Erin, Masterson, Megan, García, Javier A., Fabian, Andrew C., Parker, Michael L., Barret, Didier, Alston, William N., and Cusumano, Giancarlo
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
Accretion and ejection of matter in active galactic nuclei (AGN) are tightly connected phenomena and represent fundamental mechanisms regulating the growth of the central supermassive black hole and the evolution of the host galaxy. However, the exact physical processes involved are not yet fully understood. We present a high-resolution spectral analysis of a simultaneous \xmm\ and \nustar\ observation of the narrow line Seyfert 1 (NLS1) AGN 1H 1934-063, during which the X-ray flux dropped by a factor of $\sim6$ and subsequently recovered within 140 kiloseconds. By means of the time-resolved and flux-resolved X-ray spectroscopy, we discover a potentially variable warm absorber and a relatively stable ultra-fast outflow (UFO, $v_\mathrm{UFO}\sim-0.075\,c$) with a mild ionization state ($\log(\xi/\mathrm{erg\,cm\,s^{-1})}\sim1.6$). The detected emission lines (especially a strong and broad feature around 1\,keV) are of unknown origin and cannot be explained with emission from plasmas in photo- or collisional-ionization equilibrium. Such emission lines could be well described by a strongly blueshifted ($z\sim-0.3$) secondary reflection off the base of the equatorial outflows, which may reveal the link between the reprocessing of the inner accretion flow photons and the ejection. However, this scenario although being very promising is only tentative and will be tested with future observations., Comment: 15 pages, 17 figures, 1 table, accepted for publication in MNRAS
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- 2022
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36. The disk wind in GRS 1915+105 as seen by Insight-HXMT
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Liu, Honghui, Fu, Yuhan, Bambi, Cosimo, Jiang, Jiachen, Parker, Michael L., Ji, Long, Kong, Lingda, Zhang, Liang, Zhang, Shu, and Zhang, Yuexin
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We analyze three observations of GRS 1915+105 in 2017 by Insight-HXMT when the source was in a spectrally soft state. We find strong absorption lines from highly ionized iron, which are due to absorption by disk wind outflowing at a velocity of $\sim$ 1000 km s$^{-1}$ along our line of sight. Two of the three observations show large amplitude oscillation in their light curves and the variation pattern corresponds to state $\kappa$ of GRS 1915+105. From time-averaged and flux-resolved analysis, we find that the variation of the ionization state of the disk wind follows the X-ray continuum on timescales from hundreds seconds to months. The radial location of the disk wind is consistent with thermal driving. The mass-loss rate due to the outflowing wind is comparable to the mass accretion rate in the inner disk, which demonstrates the important role of the disk wind in the disk accretion system., Comment: 8 pages, 5 figures. v2: refereed version
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- 2022
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37. The challenges and potential solutions of achieving meaningful consent amongst research participants in northern Thailand: a qualitative study
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Greer, Rachel C, Kanthawang, Nipaphan, Roest, Jennifer, Perrone, Carlo, Wangrangsimakul, Tri, Parker, Michael, Kelley, Maureen, and Cheah, Phaik Yeong
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- 2023
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38. Structures of the interleukin 11 signalling complex reveal gp130 dynamics and the inhibitory mechanism of a cytokine variant
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Metcalfe, Riley D., Hanssen, Eric, Fung, Ka Yee, Aizel, Kaheina, Kosasih, Clara C., Zlatic, Courtney O., Doughty, Larissa, Morton, Craig J., Leis, Andrew P., Parker, Michael W., Gooley, Paul R., Putoczki, Tracy L., and Griffin, Michael D. W.
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- 2023
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39. COVID-19 vaccination in pregnancy: the impact of multimorbidity and smoking status on vaccine hesitancy, a cohort study of 25,111 women in Wales, UK
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Mhereeg, Mohamed, Jones, Hope, Kennedy, Jonathan, Seaborne, Mike, Parker, Michael, Kennedy, Natasha, Akbari, Ashley, Zuccolo, Luisa, Azcoaga-Lorenzo, Amaya, Davies, Alisha, Nirantharakumar, Krishnarajah, and Brophy, Sinead
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- 2023
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40. Beyond translations, perspectives for researchers to consider to enhance comprehension during consent processes for health research in sub-saharan Africa: a scoping review
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Busisiwe, Nkosi, Seeley, Janet, Strode, Ann, and Parker, Michael
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- 2023
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41. Relativistic X-ray Reflection Models for Accreting Neutron Stars
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Garcia, Javier A., Dauser, Thomas, Ludlam, Renee, Parker, Michael, Fabian, Andrew, Harrison, Fiona A., and Wilms, Joern
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We present new reflection models specifically tailored to model the X-ray radiation reprocessed in accretion disks around neutron stars, in which the primary continuum is characterized by a single temperature blackbody spectrum, emitted either at the surface of the star, or at the boundary layer. These models differ significantly from those with a standard power-law continuum, typically observed in most accreting black holes. We show comparisons with earlier reflection models, and test their performance in the NuSTAR observation of the neutron star 4U 1705-44. Simulations of upcoming missions such as XRISM-Resolve and Athena X-IFU are shown to highly the diagnostic potential of these models for high-resolution X-ray reflection spectroscopy. These new reflection models xillverNS, and their relativistic counterpart relxillNS, are made publicly available to the community as an additional flavor in the relxill suite of reflection models., Comment: 16 pages, 9 figures. Accepted for publication in ApJ
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- 2021
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42. Reaction hijacking of tyrosine tRNA synthetase as a new whole-of-life-cycle antimalarial strategy.
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Xie, Stanley, Metcalfe, Riley, Dunn, Elyse, Morton, Craig, Huang, Shih-Chung, Puhalovich, Tanya, Du, Yawei, Wittlin, Sergio, Nie, Shuai, Luth, Madeline, Ma, Liting, Kim, Mi-Sook, Pasaje, Charisse, Kumpornsin, Krittikorn, Giannangelo, Carlo, Houghton, Fiona, Churchyard, Alisje, Famodimu, Mufuliat, Barry, Daniel, Gillett, David, Dey, Sumanta, Kosasih, Clara, Newman, William, Niles, Jacquin, Lee, Marcus, Baum, Jake, Ottilie, Sabine, Creek, Darren, Williamson, Nicholas, Parker, Michael, Brand, Stephen, Langston, Steven, Dick, Lawrence, Griffin, Michael, Gould, Alexandra, Tilley, Leann, and Winzeler, Elizabeth
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Adenosine ,Animals ,Antimalarials ,Crystallography ,X-Ray ,Humans ,Malaria ,Falciparum ,Mice ,Molecular Targeted Therapy ,Plasmodium falciparum ,Protein Biosynthesis ,Protein Conformation ,Protozoan Proteins ,Sulfonic Acids ,Tyrosine-tRNA Ligase - Abstract
Aminoacyl transfer RNA (tRNA) synthetases (aaRSs) are attractive drug targets, and we present class I and II aaRSs as previously unrecognized targets for adenosine 5-monophosphate-mimicking nucleoside sulfamates. The target enzyme catalyzes the formation of an inhibitory amino acid-sulfamate conjugate through a reaction-hijacking mechanism. We identified adenosine 5-sulfamate as a broad-specificity compound that hijacks a range of aaRSs and ML901 as a specific reagent a specific reagent that hijacks a single aaRS in the malaria parasite Plasmodium falciparum, namely tyrosine RS (PfYRS). ML901 exerts whole-life-cycle-killing activity with low nanomolar potency and single-dose efficacy in a mouse model of malaria. X-ray crystallographic studies of plasmodium and human YRSs reveal differential flexibility of a loop over the catalytic site that underpins differential susceptibility to reaction hijacking by ML901.
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- 2022
43. Wind-luminosity evolution in NLS1 AGN 1H 0707-495
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Xu, Yerong, Pinto, Ciro, Bianchi, Stefano, Kosec, Peter, Parker, Michael L., Walton, Dominic J., Fabian, Andrew C., Guainazzi, Matteo, Barret, Didier, and Cusumano, Giancarlo
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
Ultra-fast outflows (UFOs) have been detected in the high-quality X-ray spectra of a number of active galactic nuclei (AGN) with fairly high accretion rates and are thought to significantly contribute to the AGN feedback. After a decade of dedicated study, their launching mechanisms and structure are still not well understood, but variability techniques may provide useful constraints. In this work, therefore, we perform a flux-resolved X-ray spectroscopy on a highly accreting and variable NLS1 AGN, 1H 0707-495, using all archival XMM-Newton observations to study the structure of the UFO. We find that the wind spectral lines weaken at higher luminosities, most likely due to an increasing ionization parameter as previously found in a few similar sources. Instead, the velocity is anticorrelated with the luminosity, which is opposite to the trend observed in the NLS1 IRAS 13224-3809. Furthermore, the detection of the emission lines, which are not observed in IRAS 13224-3809, indicates a wind with a larger opening angle in 1H 0707-495, presumably due to a higher accretion rate. The emitting gas is found to remain broadly constant with the luminosity. We describe the variability of the wind with a scenario where the strong radiation extends the launch radius outwards and shields the outer emitting gas, similarly to super-Eddington compact objects, although other possible explanations are discussed. Our work provides several hints for a multi-phase outflow in 1H 0707-495., Comment: 20 pages, 9 figures, accepted for publication in MNRAS
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- 2021
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44. American Crusade: Catholic Youth in the World Mission Movement from World War I through Vatican II (review)
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Parker, Michael
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- 2011
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45. Developing a performance index to measure soft skills on construction projects : a Delphi study
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Parker, Michael Anthony
- Abstract
Recent research suggests that project teams need to become more socially aware, particularly in how project professionals interact with one another, and that soft skills need to be assessed in the same way that the traditional 'iron triangle' of cost, time and quality are. At present they are either not measured at all or at best very poorly, despite being recognised for how important they are to project success. Four relevant theories were reviewed to identify where this research could make a contribution to each of them. In professional practice, the development of a soft skills performance measurement index would allow professional bodies to formally acknowledge the importance of soft skills measurement in their technical guidance for becoming professionally qualified. The research has a social constructionist ontology and primarily adopted an interpretivist epistemology. The methodology used a multi-phase mixed methods approach using the consensus-building research technique, the Delphi Method, collecting both qualitative and quantitative data in iterations. This approach enabled five soft skills (termed the 'performance pentagon') and a composite performance index (CPI) for construction projects to be derived. Mitigating actions were taken to keep participants engaged in each iteration, following the impact of the Covid-19 pandemic. The synthesis and modification of existing theories led to the phenomenon of measured goal interest (MGI), an original contribution to the academic literature on the subject, the term "measured goal interest" never having been used previously. The fact that both a major client and major consultancy in the UK construction sector have since permanently adopted the 'performance pentagon' soft skills within their own performance measurement models shows how successful this study has already been in making a contribution to professional practice.
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- 2022
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46. On the impact of an intermediate duration X-ray burst on the accretion environment in IGR J17062-6143
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Bult, Peter, Altamirano, Diego, Arzoumanian, Zaven, Ballantyne, David R., Chenevez, Jerome, Fabian, Andrew C., Gendreau, Keith C., Homan, Jeroen, Jaisawal, Gaurava K., Malacaria, Christian, Miller, Jon M., Parker, Michael L., and Strohmayer, Tod E.
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Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report on a spectroscopic analysis of the X-ray emission from IGR J17062-6143 in the aftermath of its June 2020 intermediate duration Type I X-ray burst. Using the Neutron Star Interior Composition Explorer, we started observing the source three hours after the burst was detected with MAXI/GSC, and monitored the source for the subsequent twelve days. We observed the tail end of the X-ray burst cooling phase, and find that the X-ray flux is severely depressed relative to its historic value for a three day period directly following the burst. We interpret this intensity dip as the inner accretion disk gradually restoring itself after being perturbed by the burst irradiation. Superimposed on this trend we observed a $1.5$ d interval during which the X-ray flux is sharply lower than the wider trend. This drop in flux could be isolated to the non-thermal components in the energy spectrum, suggesting that it may be caused by an evolving corona. Additionally, we detected a 3.4 keV absorption line at $6.3\sigma$ significance in a single $472$ s observation while the burst emission was still bright. We tentatively identify the line as a gravitationally redshifted absorption line from burning ashes on the stellar surface, possibly associated with ${}^{40}{\rm Ca}$ or ${}^{44}{\rm Ti}$., Comment: 14 pages, 7 figures, 3 tables. Accepted for publication in ApJ
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- 2021
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47. Biallelic CRELD1 variants cause a multisystem syndrome, including neurodevelopmental phenotypes, cardiac dysrhythmias, and frequent infections
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Borras, Silvia, Clark, Caroline, Dean, John, Miedzybrodzka, Zosia, Ross, Alison, Tennant, Stephen, Dabir, Tabib, Donnelly, Deirdre, Humphreys, Mervyn, Magee, Alex, McConnell, Vivienne, McKee, Shane, McNerlan, Susan, Morrison, Patrick J., Rea, Gillian, Stewart, Fiona, Cole, Trevor, Cooper, Nicola, Cooper-Charles, Lisa, Cox, Helen, Islam, Lily, Jarvis, Joanna, Keelagher, Rebecca, Lim, Derek, McMullan, Dominic, Morton, Jenny, Naik, Swati, O’Driscoll, Mary, Ong, Kai-Ren, Osio, Deborah, Ragge, Nicola, Turton, Sarah, Vogt, Julie, Williams, Denise, Bodek, Simon, Donaldson, Alan, Hills, Alison, Low, Karen, Newbury-Ecob, Ruth, Norman, Andrew M., Roberts, Eileen, Scurr, Ingrid, Smithson, Sarah, Tooley, Madeleine, Abbs, Steve, Armstrong, Ruth, Dunn, Carolyn, Holden, Simon, Park, Soo-Mi, Paterson, Joan, Raymond, Lucy, Reid, Evan, Sandford, Richard, Simonic, Ingrid, Tischkowitz, Marc, Woods, Geoff, Bradley, Lisa, Comerford, Joanne, Green, Andrew, Lynch, Sally, McQuaid, Shirley, Mullaney, Brendan, Berg, Jonathan, Goudie, David, Mavrak, Eleni, McLean, Joanne, McWilliam, Catherine, Reavey, Eleanor, Azam, Tara, Cleary, Elaine, Jackson, Andrew, Lam, Wayne, Lampe, Anne, Moore, David, Porteous, Mary, Baple, Emma, Baptista, Júlia, Brewer, Carole, Castle, Bruce, Kivuva, Emma, Owens, Martina, Rankin, Julia, Shaw-Smith, Charles, Turner, Claire, Turnpenny, Peter, Tysoe, Carolyn, Bradley, Therese, Davidson, Rosemarie, Gardiner, Carol, Joss, Shelagh, Kinning, Esther, Longman, Cheryl, McGowan, Ruth, Murday, Victoria, Pilz, Daniela, Tobias, Edward, Whiteford, Margo, Williams, Nicola, Barnicoat, Angela, Clement, Emma, Faravelli, Francesca, Hurst, Jane, Jenkins, Lucy, Jones, Wendy, Ajith Kumar, V.K., Lees, Melissa, Loughlin, Sam, Male, Alison, Morrogh, Deborah, Rosser, Elisabeth, Scott, Richard, Wilson, Louise, Beleza, Ana, Deshpande, Charu, Flinter, Frances, Holder, Muriel, Irving, Melita, Izatt, Louise, Josifova, Dragana, Mohammed, Shehla, Molenda, Aneta, Robert, Leema, Roworth, Wendy, Ruddy, Deborah, Ryten, Mina, Yau, Shu, Bennett, Christopher, Blyth, Moira, Campbell, Jennifer, Coates, Andrea, Dobbie, Angus, Hewitt, Sarah, Hobson, Emma, Jackson, Eilidh, Jewell, Rosalyn, Kraus, Alison, Prescott, Katrina, Sheridan, Eamonn, Thomson, Jenny, Bradshaw, Kirsty, Dixit, Abhijit, Eason, Jacqueline, Haines, Rebecca, Harrison, Rachel, Mutch, Stacey, Sarkar, Ajoy, Searle, Claire, Shannon, Nora, Sharif, Abid, Suri, Mohnish, Vasudevan, Pradeep, Canham, Natalie, Ellis, Ian, Greenhalgh, Lynn, Howard, Emma, Stinton, Victoria, Swale, Andrew, Weber, Astrid, Banka, Siddharth, Breen, Catherine, Briggs, Tracy, Burkitt-Wright, Emma, Chandler, Kate, Clayton-Smith, Jill, Donnai, Dian, Douzgou, Sofia, Gaunt, Lorraine, Jones, Elizabeth, Kerr, Bronwyn, Langley, Claire, Metcalfe, Kay, Smith, Audrey, Wright, Ronnie, Bourn, David, Burn, John, Fisher, Richard, Hellens, Steve, Henderson, Alex, Montgomery, Tara, Splitt, Miranda, Straub, Volker, Wright, Michael, Zwolinski, Simon, Allen, Zoe, Bernhard, Birgitta, Brady, Angela, Brooks, Claire, Busby, Louise, Clowes, Virginia, Ghali, Neeti, Holder, Susan, Ibitoye, Rita, Wakeling, Emma, Blair, Edward, Carmichael, Jenny, Cilliers, Deirdre, Clasper, Susan, Gibbons, Richard, Kini, Usha, Lester, Tracy, Nemeth, Andrea, Poulton, Joanna, Price, Sue, Shears, Debbie, Stewart, Helen, Wilkie, Andrew, Albaba, Shadi, Baker, Duncan, Balasubramanian, Meena, Johnson, Diana, Parker, Michael, Quarrell, Oliver, Stewart, Alison, Willoughby, Josh, Crosby, Charlene, Elmslie, Frances, Homfray, Tessa, Jin, Huilin, Lahiri, Nayana, Mansour, Sahar, Marks, Karen, McEntagart, Meriel, Saggar, Anand, Tatton-Brown, Kate, Butler, Rachel, Clarke, Angus, Corrin, Sian, Fry, Andrew, Kamath, Arveen, McCann, Emma, Mugalaasi, Hood, Pottinger, Caroline, Procter, Annie, Sampson, Julian, Sansbury, Francis, Varghese, Vinod, Baralle, Diana, Callaway, Alison, Cassidy, Emma J., Daniels, Stacey, Douglas, Andrew, Foulds, Nicola, Hunt, David, Kharbanda, Mira, Lachlan, Katherine, Mercer, Catherine, Side, Lucy, Temple, I. Karen, Wellesley, Diana, Ambrose, J.C., Arumugam, P., Baple, E.L., Bleda, M., Boardman-Pretty, F., Boissiere, J.M., Boustred, C.R., Caulfield, M.J., Chan, G.C., Craig, C.E.H., Daugherty, L.C., de Burca, A., Devereau, A., Elgar, G., Foulger, R.E., Fowler, T., FurióTarí, P., Hackett, J.M., Halai, D., Hamblin, A., Henderson, S., Holman, J.E., Hubbard, T.J.P., Ibáñez, K., Jackson, R., Jones, L.J., Kasperaviciute, D., Kayikci, M., Lahnstein, L., Lawson, K., Leigh, S.E.A., Leong, I.U.S., Lopez, F.J., MaleadyCrowe, F., Mason, J., McDonagh, E.M., Moutsianas, L., Mueller, M., Murugaesu, N., Need, A.C., Odhams, C.A., Patch, C., Perez-Gil, D., Polychronopoulos, D., Pullinger, J., Rahim, T., Rendon, A., Riesgo-Ferreiro, P., Rogers, T., Ryten, M., Savage, K., Sawant, K., Scott, R.H., Siddiq, A., Sieghart, A., Smedley, D., Smith, K.R., Sosinsky, A., Spooner, W., Stevens, H.E., Stuckey, A., Sultana, R., Thomas, E.R.A., Thompson, S.R., Tucci, A., Walsh, E., Watters, S.A., Welland, M.J., Williams, E., Witkowska, K., Acosta, Maria T., Adam, Margaret, Adams, David R., Agrawal, Pankaj B., Alejandro, Mercedes E., Alvey, Justin, Amendola, Laura, Andrews, Ashley, Ashley, Euan A., Azamian, Mahshid S., Bacino, Carlos A., Bademci, Guney, Baker, Eva, Balasubramanyam, Ashok, Baldridge, Dustin, Bale, Jim, Bamshad, Michael, Barbouth, Deborah, Bayrak-Toydemir, Pinar, Beck, Anita, Beggs, Alan H., Behrens, Edward, Bejerano, Gill, Bennet, Jimmy, Berg-Rood, Beverly, Bernstein, Jonathan A., Berry, Gerard T., Bican, Anna, Bivona, Stephanie, Blue, Elizabeth, Bohnsack, John, Bonnenmann, Carsten, Bonner, Devon, Botto, Lorenzo, Boyd, Brenna, Briere, Lauren C., Brokamp, Elly, Brown, Gabrielle, Burke, Elizabeth A., Burrage, Lindsay C., Butte, Manish J., Byers, Peter, Byrd, William E., Carey, John, Carrasquillo, Olveen, Peter Chang, Ta Chen, Chanprasert, Sirisak, Chao, Hsiao-Tuan, Clark, Gary D., Coakley, Terra R., Cobban, Laurel A., Cogan, Joy D., Coggins, Matthew, Cole, F. Sessions, Colley, Heather A., Cooper, Cynthia M., Craigen, William J., Crouse, Andrew B., Cunningham, Michael, D'Souza, Precilla, Dai, Hongzheng, Dasari, Surendra, Davids, Mariska, Dayal, Jyoti G., Deardorff, Matthew, Dell'Angelica, Esteban C., Dhar, Shweta U., Dipple, Katrina, Doherty, Daniel, Dorrani, Naghmeh, Douine, Emilie D., Draper, David D., Duncan, Laura, Earl, Dawn, Eckstein, David J., Emrick, Lisa T., Eng, Christine M., Esteves, Cecilia, Estwick, Tyra, Falk, Marni, Fernandez, Liliana, Ferreira, Carlos, Fieg, Elizabeth L., Findley, Laurie C., Fisher, Paul G., Fogel, Brent L., Forghani, Irman, Fresard, Laure, Gahl, William A., Glass, Ian, Godfrey, Rena A., Golden-Grant, Katie, Goldman, Alica M., Goldstein, David B., Grajewski, Alana, Groden, Catherine A., Gropman, Andrea L., Gutierrez, Irma, Hahn, Sihoun, Hamid, Rizwan, Hanchard, Neil A., Hassey, Kelly, Hayes, Nichole, High, Frances, Hing, Anne, Hisama, Fuki M., Holm, Ingrid A., Hom, Jason, Horike-Pyne, Martha, Huang, Alden, Huang, Yong, Isasi, Rosario, Jamal, Fariha, Jarvik, Gail P., Jarvik, Jeffrey, Jayadev, Suman, Johnston, Jean M., Karaviti, Lefkothea, Kelley, Emily G., Kennedy, Jennifer, Kiley, Dana, Kohane, Isaac S., Kohler, Jennefer N., Krakow, Deborah, Krasnewich, Donna M., Kravets, Elijah, Korrick, Susan, Koziura, Mary, Krier, Joel B., Lalani, Seema R., Lam, Byron, Lam, Christina, Lanpher, Brendan C., Lanza, Ian R., Lau, C. Christopher, LeBlanc, Kimberly, Lee, Brendan H., Lee, Hane, Levitt, Roy, Lewis, Richard A., Lincoln, Sharyn A., Liu, Pengfei, Liu, Xue Zhong, Longo, Nicola, Loo, Sandra K., Loscalzo, Joseph, Maas, Richard L., Macnamara, Ellen F., MacRae, Calum A., Maduro, Valerie V., Majcherska, Marta M., Mak, Bryan, Malicdan, May Christine V., Mamounas, Laura A., Manolio, Teri A., Mao, Rong, Maravilla, Kenneth, Markello, Thomas C., Marom, Ronit, Marth, Gabor, Martin, Beth A., Martin, Martin G., Martínez-Agosto, Julian A., Marwaha, Shruti, McCauley, Jacob, McCormack, Colleen E., McCray, Alexa T., McGee, Elisabeth, Mefford, Heather, Merritt, J. Lawrence, Might, Matthew, Mirzaa, Ghayda, Morava, Eva, Moretti, Paolo M., Morimoto, Marie, Mulvihill, John J., Murdock, David R., Nakano-Okuno, Mariko, Nath, Avi, Nelson, Stan F., Newman, John H., Nicholas, Sarah K., Nickerson, Deborah, Nieves-Rodriguez, Shirley, Novacic, Donna, Oglesbee, Devin, Orengo, James P., Pace, Laura, Pak, Stephen, Pallais, J. Carl, Papp, Jeanette C., Parker, Neil H., Phillips, John A., Posey, Jennifer E., Potocki, Lorraine, Pusey, Barbara N., Quinlan, Aaron, Raskind, Wendy, Raja, Archana N., Rao, Deepak A., Renteria, Genecee, Reuter, Chloe M., Rives, Lynette, Robertson, Amy K., Rodan, Lance H., Rosenfeld, Jill A., Rosenwasser, Natalie, Ruzhnikov, Maura, Sacco, Ralph, Sampson, Jacinda B., Samson, Susan L., Saporta, Mario, Scott, C. Ron, Schaechter, Judy, Schedl, Timothy, Scott, Daryl A., Sharma, Prashant, Shin, Jimann, Signer, Rebecca, Sillari, Catherine H., Silverman, Edwin K., Sinsheimer, Janet S., Sisco, Kathy, Smith, Edward C., Smith, Kevin S., Solem, Emily, Solnica-Krezel, Lilianna, Stoler, Joan M., Stong, Nicholas, Sullivan, Jennifer A., Sun, Angela, Sutton, Shirley, Sweetser, David A., Sybert, Virginia, Tabor, Holly K., Tamburro, Cecelia P., Tekin, Mustafa, Telischi, Fred, Thorson, Willa, Tifft, Cynthia J., Toro, Camilo, Tran, Alyssa A., Tucker, Brianna M., Urv, Tiina K., Vanderver, Adeline, Velinder, Matt, Viskochil, Dave, Vogel, Tiphanie P., Wahl, Colleen E., Wallace, Stephanie, Walley, Nicole M., Walsh, Chris A., Walker, Melissa, Wambach, Jennifer, Wan, Jijun, Wang, Lee-Kai, Wangler, Michael F., Ward, Patricia A., Wegner, Daniel, Wener, Mark, Wenger, Tara, Perry, Katherine Wesseling, Westerfield, Monte, Wheeler, Matthew T., Whitlock, Jordan, Wolfe, Lynne A., Woods, Jeremy D., Yamamoto, Shinya, Yang, John, Yu, Guoyun, Zastrow, Diane B., Zhao, Chunli, Zuchner, Stephan, Jeffries, Lauren, Mis, Emily K., McWalter, Kirsty, Donkervoort, Sandra, Brodsky, Nina N., Carpier, Jean-Marie, Ji, Weizhen, Ionita, Cristian, Roy, Bhaskar, Morrow, Jon S., Darbinyan, Armine, Iyer, Krishna, Aul, Ritu B., Chao, Katherine R., Cobbold, Laura, Cohen, Stacey, Custodio, Helena M., Drummond-Borg, Margaret, Finanger, Erika, Hainline, Bryan E., Helbig, Ingo, Hewson, Stacy, Hu, Ying, Jackson, Adam, Konstantino, Monica, Leach, Meganne E., McCormick, David, Nelson, Stanley, Nguyen, Joanne, Nugent, Kimberly, Ortega, Lucy, Goodkin, Howard P., Roeder, Elizabeth, Roy, Sani, Sapp, Katie, Saade, Dimah, Sisodiya, Sanjay M., Stals, Karen, Towner, Shelley, Wilson, William, Khokha, Mustafa K., Bönnemann, Carsten G., Lucas, Carrie L., and Lakhani, Saquib A.
- Published
- 2024
- Full Text
- View/download PDF
48. Vehicle modeling in Unreal Engine 4
- Author
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Sapienza, Francis, primary, Parker, Michael, additional, Bodie, Mark, additional, and Shoop, Sally, additional
- Published
- 2023
- Full Text
- View/download PDF
49. Commentary on "True Wishes"
- Author
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Parker, Michael
- Published
- 2009
50. The golden ticket
- Author
-
Parker, Michael
- Published
- 2023
- Full Text
- View/download PDF
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