Zobrazeno 1 - 10
of 17 246
pro vyhledávání: '"Smith Peter"'
Autor:
Little Paul, Francis Nick A, Stuart Beth, O’Reilly Gilly, Thompson Natalie, Becque Taeko, Hay Alastair D, Wang Kay, Sharland Michael, Harnden Anthony, Yao Guiqing, Raftery James, Zhu Shihua, Little Joseph, Hookham Charlotte, Rowley Kate, Euden Joanne, Harman Kim, Coenen Samuel, Read Robert C, Woods Catherine, Butler Christopher C, Faust Saul N, Leydon Geraldine, Wan Mandy, Hood Kerenza, Whitehurst Jane, Richards-Hall Samantha, Smith Peter, Thomas Michael, Moore Michael, Verheij Theo
Publikováno v:
Health Technology Assessment, Vol 27, Iss 09 (2023)
Background Antimicrobial resistance is a global health threat. Antibiotics are commonly prescribed for children with uncomplicated lower respiratory tract infections, but there is little randomised evidence to support the effectiveness of antibiotics
Externí odkaz:
https://doaj.org/article/6017c8482d9a4db985a6f9f910917261
Autor:
Deibert, Emily K., Langeveld, Adam B., Young, Mitchell E., Flagg, Laura, Turner, Jake D., Smith, Peter C. B., de Mooij, Ernst J. W., Jayawardhana, Ray, Chiboucas, Kristin, Gamen, Roberto, Hayes, Christian R., Heo, Jeong-Eun, Jeong, Miji, Kalari, Venu, Martioli, Eder, Placco, Vinicius M., Xu, Siyi, Diaz, Ruben, Gomez-Jimenez, Manuel, Quiroz, Carlos, Ruiz-Carmona, Roque, Simpson, Chris, McConnachie, Alan W., Pazder, John, Burley, Gregory, Ireland, Michael, Waller, Fletcher, Berg, Trystyn A. M., Robertson, J. Gordon, Jones, David O., Labrie, Kathleen, Ridgway, Susan, Thomas-Osip, Joanna
With high equilibrium temperatures and tidally locked rotation, ultra-hot Jupiters (UHJs) are unique laboratories within which to probe extreme atmospheric physics and chemistry. In this paper, we present high-resolution dayside spectroscopy of the U
Externí odkaz:
http://arxiv.org/abs/2407.11281
We present a new method to combine multimass equilibrium dynamical models and pulsar timing data to constrain the mass distribution and remnant populations of Milky Way globular clusters (GCs). We first apply this method to 47 Tuc, a cluster for whic
Externí odkaz:
http://arxiv.org/abs/2407.06274
Autor:
Kanumalla, Krishna, Line, Michael R., Mansfield, Megan Weiner, Welbanks, Luis, Smith, Peter C. B., Bean, Jacob L., Pino, Lorenzo, Brogi, Matteo, Panwar, Vatsal
High resolution spectroscopy of exoplanet atmospheres provides insights into their composition and dynamics from the resolved line shape and depth of thousands of spectral lines. WASP-127 b is an extremely inflated sub-Saturn (R$_\mathrm{p}$= 1.311 R
Externí odkaz:
http://arxiv.org/abs/2406.14072
Autor:
Wardenier, Joost P., Parmentier, Vivien, Line, Michael R., Mansfield, Megan Weiner, Tan, Xianyu, Tsai, Shang-Min, Bean, Jacob L., Birkby, Jayne L., Brogi, Matteo, Désert, Jean-Michel, Gandhi, Siddharth, Lee, Elspeth K. H., Levens, Colette I., Pino, Lorenzo, Smith, Peter C. B.
Ultra-hot Jupiters are among the best targets for atmospheric characterization at high spectral resolution. Resolving their transmission spectra as a function of orbital phase offers a unique window into the 3D nature of these objects. In this work,
Externí odkaz:
http://arxiv.org/abs/2406.09641
Autor:
Noguer, Federico R., Corley, Suber, Pearson, Kyle A., Zellem, Robert T., Simon, Molly N., Burt, Jennifer A., Huckabee, Isabela, August, Prune C., Mansfield, Megan Weiner, Dalba, Paul A., Smith, Peter C. B., Banks, Timothy, Bell, Ira, Daniel, Dominique, Dawson, Lindsay, De Mula, Jesús, Deldem, Marc, Deligeorgopoulos, Dimitrios, Di Sisto, Romina P., Dymock, Roger, Evans, Phil, Follero, Giulio, Fowler, Martin J. F., Fernández-Lajús, Eduardo, Hamrick, Alex, Iannascoli, Nicoletta, Kovacs, Andre O., Kulh, Denis Henrique, Lopresti, Claudio, Marino, Antonio, Martin, Bryan E., Matassa, Paolo Arcangelo, Napoleão, Tasso Augusto, Nastasi, Alessandro, Norris, Anthony, Odasso, Alessandro, Paschalis, Nikolaos I., Pintr, Pavel, Postiglione, Jake, Randolph, Justus, Regembal, François, Rousselot, Lionel, da Silva, Sergio José Gonçalves, Smith, Andrew, Tomacelli, Andrea
We present an updated ephemeris and physical parameters for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce the
Externí odkaz:
http://arxiv.org/abs/2405.19615
Autor:
Mansfield, Megan Weiner, Line, Michael R., Wardenier, Joost P., Brogi, Matteo, Bean, Jacob L., Beltz, Hayley, Smith, Peter, Zalesky, Joseph A., Batalha, Natasha, Kempton, Eliza M. -R., Montet, Benjamin T., Owen, James E., Plavchan, Peter, Rauscher, Emily
Measurements of the carbon-to-oxygen (C/O) ratios of exoplanet atmospheres can reveal details about their formation and evolution. Recently, high-resolution cross-correlation analysis has emerged as a method of precisely constraining the C/O ratios o
Externí odkaz:
http://arxiv.org/abs/2405.09769
Motivated by the ideal peak-to-average-power ratio and radar sensing capability of traditional frequency-coded radar waveforms, this paper considers the frequency shift keying (FSK) based waveform for joint communications and radar (JCR). An analysis
Externí odkaz:
http://arxiv.org/abs/2405.00945
Autor:
Smith, Peter, Line, Michael, Bean, Jacob, Brogi, Matteo, August, Prune, Welbanks, Luis, Desert, Jean-Michel, Lunine, Jonathan, Sanchez, Jorge, Mansfield, Megan, Pino, Lorenzo, Rauscher, Emily, Kempton, Eliza, Zalesky, Joseph, Fowler, Martin
Ground-based, high-resolution and space-based, low-resolution spectroscopy are the two main avenues through which transiting exoplanet atmospheres are studied. Both methods provide unique strengths and shortcomings, and combining the two can be a pow
Externí odkaz:
http://arxiv.org/abs/2312.13069