36 results on '"P Hibon"'
Search Results
2. A Lyman-α protocluster at redshift 6.9
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Hu, Weida, Wang, Junxian, Infante, Leopoldo, Rhoads, James E., Zheng, Zhen-Ya, Yang, Huan, Malhotra, Sangeeta, Barrientos, L. Felipe, Jiang, Chunyan, González-López, Jorge, Prieto, Gonzalo, Perez, Lucia A., Hibon, Pascale, Galaz, Gaspar, Coughlin, Alicia, Harish, Santosh, Kong, Xu, Kang, Wenyong, Khostovan, Ali Ahmad, Pharo, John, Valdes, Francisco, Wold, Isak, Walker, Alistair R., and Zheng, XianZhong
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- 2021
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3. Stellar feedback in a clumpy galaxy at z ∼ 3.4
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E Iani, A Zanella, J Vernet, J Richard, M Gronke, C M Harrison, F Arrigoni-Battaia, G Rodighiero, A Burkert, M Behrendt, Chian-Chou Chen, E Emsellem, J Fensch, P Hibon, M Hilker, E Le Floc’h, V Mainieri, A M Swinbank, F Valentino, E Vanzella, and M A Zwaan
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- 2021
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4. Impact of ICU transfers on the mortality rate of patients with COVID-19: insights from comprehensive national database in France
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Sanchez, Marc-Antoine, Vuagnat, Albert, Grimaud, Olivier, Leray, Emmanuelle, Philippe, Jean-Marc, Lescure, François-Xavier, Boutonnet, Mathieu, Coignard, Hélène, Hibon, Agnès Ricard, Sanchez, Stephane, and Pottecher, Julien
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- 2021
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5. The analysis of the geographical distribution of emergency departments’ frequent users: a tool to prioritize public health policies?
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Hellmann, Romain, Feral-Pierssens, Anne-Laure, Michault, Alain, Casalino, Enrique, Ricard-Hibon, Agnès, Adnet, Frederic, Brun-Ney, Dominique, Bouzid, Donia, Menu, Axelle, and Wargon, Mathias
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- 2021
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6. Onset of Cosmic Reionization: Evidence of an Ionized Bubble Merely 680 Myr After the Big Bang
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V. Tilvi, S. Malhotra, J. E. Rhoads, A. Coughlin, Z. Zheng, S. L. Finkelstein, S. Veilleux, B. Mobasher, J. Wang, R. Probst, R. Swaters, P. Hibon, B. Joshi, J. Zabl, T. Jiang, J Pharo, and H Yang
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Astronomy - Abstract
While most of the intergalactic medium (IGM) today is permeated by ionized hydrogen, it was largely filled with neutral hydrogen for the first 700 million years after the big bang. The process that ionized the IGM (cosmic reionization) is expected to be spatially inhomogeneous, with fainter galaxies likely playing a significant role. However, we still have only a few direct constraints on the reionization process. Here we report spectroscopic confirmation of two galaxies and very likely a third galaxy in a group (hereafter EGS77) at redshift z = 7.7, merely 680 Myr after the big bang. The physical separation among the three members is <0.7 Mpc. We estimate the radius of ionized bubble of the brightest galaxy to be about 1.02 Mpc, and show that the individual ionized bubbles formed by all three galaxies likely overlap significantly, forming a large yet localized ionized region, indicative of inhomogeneity in the reionization process. It is striking that two of three galaxies in EGS77 are quite faint in the continuum, thanks to our selection using their Lyα line emission in the narrowband filter. Indeed, one is the faintest spectroscopically confirmed galaxy yet discovered at such high redshifts. Our observations provide direct constraints on the process of cosmic reionization, and allow us to investigate the properties of sources responsible for reionizing the universe.
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- 2020
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7. Withholding and withdrawing life-support in adults in emergency care: joint position paper from the French Intensive Care Society and French Society of Emergency Medicine
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Reignier, Jean, Feral-Pierssens, Anne-Laure, Boulain, Thierry, Carpentier, Françoise, Le Borgne, Pierrick, Del Nista, Denis, Potel, Gilles, Dray, Sandrine, Hugenschmitt, Delphine, Laurent, Alexandra, Ricard-Hibon, Agnès, Vanderlinden, Thierry, Chouihed, Tahar, and For the French Society of Emergency Medicine (Société Française de Médecine d’Urgence, SFMU) and French Intensive Care Society (Société de Réanimation de Langue Française, SRLF)
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- 2019
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8. Publisher Correction: A Lyman-α protocluster at redshift 6.9
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Hu, Weida, Wang, Junxian, Infante, Leopoldo, Rhoads, James E., Zheng, Zhen-Ya, Yang, Huan, Malhotra, Sangeeta, Barrientos, L. Felipe, Jiang, Chunyan, González-López, Jorge, Prieto, Gonzalo, Perez, Lucia A., Hibon, Pascale, Galaz, Gaspar, Coughlin, Alicia, Harish, Santosh, Kong, Xu, Kang, Wenyong, Khostovan, Ali Ahmad, Pharo, John, Valdes, Francisco, Wold, Isak, Walker, Alistair R., and Zheng, XianZhong
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- 2021
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9. Diabetes education of patients and their entourage: out-of-hospital national study (EDUCATED 2)
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Lapostolle, Frédéric, Hamdi, Nadia, Barghout, Majed, Soulat, Louis, Faucher, Anna, Lambert, Yves, Peschanski, Nicolas, Ricard-Hibon, Agnès, Chassery, Carine, Roti, Maryline, Bounes, Vincent, Debaty, Guillaume, Mokni, Tarak, Egmann, Gérald, Fort, Pierre-Arnaud, Boudenia, Karim, Alayrac, Laurent, Safraou, Mohamed, Galinski, Michel, and Adnet, Frédéric
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- 2017
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10. Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B
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K. Ward-Duong, J. Patience, K. Follette, R. J. De Rosa, J. Rameau, M. Marley, D. Saumon, E. L. Nielsen, A. Rajan, A. Z. Greenbaum, J. Lee, J. J. Wang, I. Czekala, G. Duchêne, B. Macintosh, S. Mark Ammons, V. P. Bailey, T. Barman, J. Bulger, C. Chen, J. Chilcote, T. Cotten, R. Doyon, T. M. Esposito, M. P. Fitzgerald, B. L. Gerard, S. J. Goodsell, J. R. Graham, P. Hibon, J. Hom, L.-W. Hung, P. Ingraham, P. Kalas, Q. Konopacky, J. E. Larkin, J. Maire, F. Marchis, C. Marois, S. Metchev, M. A. Millar-Blanchaer, R. Oppenheimer, D. Palmer, M. Perrin, L. Poyneer, L. Pueyo, F. T. Rantakyrö, B. Ren, J.-B. Ruffio, D. Savransky, A. C. Schneider, A. Sivaramakrishnan, I. Song, R. Soummer, M. Tallis, S. Thomas, J. Kent Wallace, S. Wiktorowicz, and S. Wolff
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- 2020
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11. Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager
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B. Macintosh, J. R. Graham, T. Barman, R. J. De Rosa, Q. Konopacky, M. S. Marley, C. Marois, E. L. Nielsen, L. Pueyo, A. Rajan, J. Rameau, D. Saumon, J. J. Wang, J. Patience, M. Ammons, P. Arriaga, E. Artigau, S. Beckwith, J. Brewster, S. Bruzzone, J. Bulger, B. Burningham, A. S. Burrows, C. Chen, E. Chiang, J. K. Chilcote, R. I. Dawson, R. Dong, R. Doyon, Z. H. Draper, G. Duchêne, T. M. Esposito, D. Fabrycky, M. P. Fitzgerald, K. B. Follette, J. J. Fortney, B. Gerard, S. Goodsell, A. Z. Greenbaum, P. Hibon, S. Hinkley, T. H. Cotten, L.-W. Hung, P. Ingraham, M. Johnson-Groh, P. Kalas, D. Lafreniere, J. E. Larkin, J. Lee, M. Line, D. Long, J. Maire, F. Marchis, B. C. Matthews, C. E. Max, S. Metchev, M. A. Millar-Blanchaer, T. Mittal, C. V. Morley, K. M. Morzinski, R. Murray-Clay, R. Oppenheimer, D. W. Palmer, R. Patel, M. D. Perrin, L. A. Poyneer, R. R. Rafikov, F. T. Rantakyrö, E. L. Rice, P. Rojo, A. R. Rudy, J.-B. Ruffio, M. T. Ruiz, N. Sadakuni, L. Saddlemyer, M. Salama, D. Savransky, A. C. Schneider, A. Sivaramakrishnan, I. Song, R. Soummer, S. Thomas, G. Vasisht, J. K. Wallace, K. Ward-Duong, S. J. Wiktorowicz, S. G. Wolff, and B. Zuckerman
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- 2015
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12. The VANDELS survey: Global properties of CIII]λ1908 Å emitting star-forming galaxies at z ∼ 3
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Ross J. McLure, P. Hibon, Daniel Schaerer, G. Zamorani, M. Castellano, D. J. McLeod, Ricardo Amorín, A. C. Carnall, Laura Pentericci, M. Llerena, Margherita Talia, A. Saxena, Angela Bongiorno, Adriano Fontana, F. Mannucci, A. Calabrò, Enrique Perez-Montero, Fergus Cullen, F. Marchi, Nimish P. Hathi, European Commission, and Ministerio de Ciencia e Innovación (España)
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Physics ,Galaxies: abundances ,Galaxies: high-redshift ,abundances [Galaxies] ,Galaxies: evolution ,Astronomy and Astrophysics ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Star (graph theory) ,Galaxies: formation ,evolution [Galaxies] ,formation [Galaxies] ,Galaxy ,galaxies [Ultraviolet] ,high-redshift [Galaxies] ,Space and Planetary Science ,Ultraviolet: galaxies ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
Context. Strong nebular emission is ubiquitous in galaxies that contribute to cosmic reionization at redshift z ≳ 6. High-ionization UV metal lines, such as CIII]λ1908 Å, show high equivalent widths (EW) in these early galaxies, suggesting harder radiation fields at low metallicity than low-z galaxies of similar stellar mass. Understanding the physical properties driving the observed UV nebular line emission at high-z requires large and very deep spectroscopic surveys, which are now only accessible out to z ∼ 4. Aims. We study the mean properties of a large representative sample of 217 galaxies showing CIII] emission at 2, his work is based on data products from observations made with ESO Telescopes at La Silla Paranal Observatory under ESO program ID 194.A-2003 (PIs: Laura Pentericci and Ross McLure). MLl acknowledges support from the National Agency for Research and Development (ANID)/Scholarship Program/Doctorado Nacional/2019-21191036. RA acknowledges support from ANID FONDECYT Regular Grant 1202007. This work has made extensive use of Python packages astropy (Astropy Collaboration 2018), numpy (Harris et al. 2020), and Matplotlib (Hunter 2007)., With funding from the Spanish government through the Severo Ochoa Centre of Excellence accreditation SEV-2017-0709.
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- 2022
13. No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at ≲ z ≲ 3.5
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A Saxena, L Pentericci, R S Ellis, L Guaita, A Calabrò, D Schaerer, E Vanzella, R Amorín, M Bolzonella, M Castellano, F Fontanot, N P Hathi, P Hibon, M Llerena, F Mannucci, A Saldana-Lopez, M Talia, and G Zamorani
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010504 meteorology & atmospheric sciences ,13. Climate action ,Space and Planetary Science ,0103 physical sciences ,Astronomy and Astrophysics ,010303 astronomy & astrophysics ,01 natural sciences ,0105 earth and related environmental sciences - Abstract
We present Lyman continuum (LyC) radiation escape fraction $f_{\rm{esc}}$ measurements for 183 spectroscopically confirmed star-forming galaxies in the redshift range $3.11 < z < 3.53$ in the \textit{Chandra} Deep Field South. We use ground-based imaging to measure $f_{\rm{esc}}$, and use ground- and space-based photometry to derive galaxy physical properties using spectral energy distribution (SED) fitting. We additionally derive [O III]+H$\beta$ equivalent widths (that fall in the observed K band) by including nebular emission in the SED fitting. After removing foreground contaminants, we report the discovery of 11 new candidate LyC leakers, with absolute LyC escape fractions, $f_{\rm{esc}}$ in the range $0.14-0.85$. From non-detections, we place $1\sigma$ upper limits of $f_{\rm{esc}}300$A. For candidate LyC leakers, we find a weak negative correlation between $f_{\rm{esc}}$ and galaxy stellar masses, no correlation between $f_{\rm{esc}}$ specific star-formation rates (sSFRs) and a positive correlation between $f_{\rm{esc}}$ and EW$_0$([O III]+H$\beta$). The weak/no correlations between stellar mass and sSFRs may be explained by misaligned viewing angles and/or non-coincident timescales of starburst activity and periods of high $f_{\rm{esc}}$. Alternatively, escaping radiation may predominantly occur in highly localised star-forming regions, or $f_{\rm{esc}}$ measurements may be impacted by stochasticity of the intervening neutral medium, obscuring any global trends with galaxy properties. These hypotheses have important consequences for models of reionisation.
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- 2022
14. Effect of the AutoPulse™ automated band chest compression device on hemodynamics in out-of-hospital cardiac arrest resuscitation
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Duchateau, François-Xavier, Gueye, Papa, Curac, Sonja, Tubach, Florence, Broche, Claire, Plaisance, Patrick, Payen, Didier, Mantz, Jean, and Ricard-Hibon, Agnès
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- 2010
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15. Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B
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Kimberly Ward-Duong, Bruce Macintosh, Jeffrey Chilcote, S. Mark Ammons, René Doyon, Quinn Konopacky, Inseok Song, Schuyler Wolff, Travis Barman, James R. Graham, Tara Cotten, S. Thomas, Dave Palmer, Vanessa P. Bailey, Mark S. Marley, Gaspard Duchêne, J. Lee, Lisa Poyneer, Michael P. Fitzgerald, Thomas M. Esposito, Jason J. Wang, Ian Czekala, Christine Chen, Stan Metchev, Abhijith Rajan, B. L. Gerard, Jean-Baptiste Ruffio, Anand Sivaramakrishnan, Eric L. Nielsen, Didier Saumon, Rebecca Oppenheimer, Franck Marchis, Katherine B. Follette, Laurent Pueyo, Christian Marois, Sloane J. Wiktorowicz, Julien Rameau, Paul Kalas, S. Goodsell, James E. Larkin, Max Millar-Blanchaer, Li Wei Hung, Joanna Bulger, R. J. De Rosa, Justin Hom, Fredrik T. Rantakyro, Adam C. Schneider, Jérôme Maire, P. Hibon, Dmitry Savransky, Alexandra Z. Greenbaum, J. Patience, Patrick Ingraham, Marshall D. Perrin, Bin Ren, Melisa Tallis, J. Kent Wallace, and Rémi Soummer
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010504 meteorology & atmospheric sciences ,1648, 185, 363, 2021, 1175 ,Population ,Brown dwarf ,FOS: Physical sciences ,Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,Orbital inclination ,Orbit determination ,Debris disks ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Gemini Planet Imager ,Substellar companion stars ,Substellar object ,education ,010303 astronomy & astrophysics ,Solar and Stellar Astrophysics (astro-ph.SR) ,Astrophysics::Galaxy Astrophysics ,0105 earth and related environmental sciences ,Physics ,Earth and Planetary Astrophysics (astro-ph.EP) ,education.field_of_study ,Debris disk ,Brown dwarfs ,Astronomy and Astrophysics ,Radius ,Effective temperature ,Exoplanet atmospheric composition ,Astrophysics - Solar and Stellar Astrophysics ,13. Climate action ,Space and Planetary Science ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics - Earth and Planetary Astrophysics - Abstract
We present new near-infrared Gemini Planet Imager (GPI) spectroscopy of HD 206893 B, a substellar companion orbiting within the debris disk of its F5V star. The $J$, $H$, $K1$, and $K2$ spectra from GPI demonstrate the extraordinarily red colors of the object, confirming it as the reddest substellar object observed to date. The significant flux increase throughout the infrared presents a challenging atmosphere to model with existing grids. Best-fit values vary from 1200 K to 1800 K for effective temperature and from 3.0 to 5.0 for log($g$), depending on which individual wavelength band is fit and which model suite is applied. The extreme redness of the companion can be partially reconciled by invoking a high-altitude layer of sub-micron dust particles, similar to dereddening approaches applied to the peculiar red field L-dwarf population. However, reconciling the HD 206893 B spectra with even those of the reddest low-gravity L-dwarf spectra still requires the contribution of additional atmospheric dust, potentially due to the debris disk environment in which the companion resides. Orbit fitting from four years of astrometric monitoring is consistent with a $\sim$30-year period, orbital inclination of 147$^{\circ}$, and semimajor axis of 10 au, well within the estimated disk inner radius of $\sim$50 au. As one of very few substellar companions imaged interior to a circumstellar disk, the properties of this system offer important dynamical constraints on companion-disk interaction and provide a benchmark for substellar and planetary atmospheric study., Accepted for publication in AJ (October 15, 2020). 35 pages, 20 figures, with tables and appendices presented in their entirety
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- 2020
16. A Ly α nebula at z ∼ 3.3
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R. Thomas, P. Hibon, F. Tang, and Kapteyn Astronomical Institute
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Physics ,Nebula ,Methods: observational ,010308 nuclear & particles physics ,Space and Planetary Science ,0103 physical sciences ,Galaxies: high-redshift ,Galaxies: evolution ,Astronomy and Astrophysics ,Astrophysics ,010303 astronomy & astrophysics ,01 natural sciences ,Methods observational - Abstract
Context. Searching for high-redshift galaxies is a field of intense activity in modern observational cosmology that will continue to grow with future ground-based and sky observatories. Over the last few years, a lot has been learned about the high-z Universe. Aims. Despite extensive Lyα blobs (LAB) surveys from low to high redshifts, giant LABs over 100 kpc have been found mostly at z ∼ 2–4. This redshift range is coincident with the transition epoch of galactic gas-circulation processes from inflows to outflows at z ∼ 2.5–3. This suggests that the formation of giant LABs may be related to a combination of gas inflows and outflows. Their extreme youth makes them interesting objects in the study of galaxy formation as they provide insight into some of the youngest known highly star forming galaxies, with only modest time investments using ground-based telescopes. Methods. Systematic narrow-band Lyα nebula surveys are ongoing, but they are limited in their covered redshift range and their comoving volume. This poses a significant problem when searching for such rare sources. To address this problem, we developed a systematic searching tool, ATACAMA (A Tool for seArChing for lArge LyMan Alpha nebulae) designed to find large Lyα nebulae at any redshift within deep multi-wavelength broad-band imaging. Results. We identified a Lyα nebula candidate at zphot ∼ 3.3 covering an isophotal area of 29.4arcsec2. Its morphology shows a bright core and a faint core which coincides with the morphology of previously known Lyα blobs. A first estimation of the Lyα equivalent width and line flux agree with the values from the study led by several groups.
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- 2020
17. Comparison of respiratory rate and peripheral oxygen saturation to assess severity in trauma patients
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Raux, Mathieu, Thicoïpé, Michel, Wiel, Eric, Rancurel, Elisabeth, Savary, Dominique, David, Jean-Stéphane, Berthier, Frédéric, Ricard-Hibon, Agnès, Birgel, Frédéric, and Riou, Bruno
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- 2006
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18. Systemic pressure-flow reactivity to norepinephrine in rabbits: impact of endotoxin and fluid loading
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Ricard-Hibon, A., Losser, M. -R., Kong, R., Belouci, S, Teisseire, B., and Pay, D.
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- 1998
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19. Central nervous system lesions in hypomclanosis of Ito: an MRI and pathological study
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Malherbe, V., Pariente, D., Tardieu, M., Lacroix, C., Venencie, P. Y., Hibon, D., Vedrenne, J., and Landrieu, P.
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- 1993
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20. Out-of-hospital interventions by the French Emergency Medical Service are associated with a high survival in patients aged 80 year or over
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Duchateau, François-Xavier, Burnod, Alexis, Dahmani, Souhayl, Delpierre, Sandrine, Ricard-Hibon, Agnès, and Mantz, Jean
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- 2008
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21. ATACAMA, A Tool seArChing for lArge lyMan Alpha Nebula.
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Hibon, P. and Thomas, R.
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- 2019
22. First Scattered-light Images of the Gas-rich Debris Disk around 49 Ceti
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C. H. Chen, A. Boccaletti, Abhijith Rajan, C. del Burgo, Dimitri Mawet, J. C. Augereau, Anne-Marie Lagrange, Christophe Pinte, Julien Milli, Steve Ertel, Elena Gofas-Salas, S. Wolff, J. B. Hagan, Aki Roberge, Dean C. Hines, Mamadou N'Diaye, Rémi Soummer, M. D. Perrin, Z. Wahhaj, David A. Golimowski, Olivier Absil, W. R. F. Dent, Elodie Choquet, Julien Girard, P. Hibon, Glenn Schneider, Mark Booth, David Mouillet, Mark C. Wyatt, Luca Matrà, Laurent Pueyo, Grant M. Kennedy, John H. Debes, C. A. Gomez Gonzalez, Jet Propulsion Laboratory (JPL), California Institute of Technology (CALTECH)-NASA, European Southern Observatory [Santiago] (ESO), European Southern Observatory (ESO), Space Telescope Science Institute (STSci), Exoplanets and Stellar Astrophysics Lab, NASA Goddard Space Flight Center (GSFC), 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), Astrophysikalisches Institut und Universitätssternwarte, Pontificia Universidad Católica de Chile (UC), Space Sciences, Technologies and Astrophysics Research Institute (STAR), Université de Liège, 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), Instituto Nacional de Astrofísica, Óptica y Electrónica (INAOE), Atacama Large Millimeter/submillimeter Array (ALMA), Steward Observatory, University of Arizona, DOTA, ONERA, Université Paris Saclay [Palaiseau], ONERA-Université Paris-Saclay, Institute of Astronomy [Cambridge], University of Cambridge [UK] (CAM), Caltech Department of Astronomy [Pasadena], California Institute of Technology (CALTECH), Université Côte d'Azur (UCA), Arizona State University [Tempe] (ASU), Johns Hopkins University (JHU), NASA-California Institute of Technology (CALTECH), GSFC Exoplanets and Stellar Astrophysics Laboratory, 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]), 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), DOTA, ONERA, Université Paris Saclay (COmUE) [Palaiseau], ONERA-Université Paris Saclay (COmUE), COMUE Université Côte d'Azur (2015-2019) (COMUE UCA), Université Paris Saclay (COmUE)-ONERA, Kennedy, Grant [0000-0001-6831-7547], Matr<U+FFFD>, Luca [0000-0003-4705-3188], Wyatt, Mark [0000-0001-9064-5598], and Apollo - University of Cambridge Repository
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010504 meteorology & atmospheric sciences ,FOS: Physical sciences ,CIRCUMSTELLAR MATTER ,Astrophysics ,01 natural sciences ,0103 physical sciences ,TECHNIQUES: IMAGE PROCESSING ,Angular resolution ,Absorption (electromagnetic radiation) ,010303 astronomy & astrophysics ,0105 earth and related environmental sciences ,Earth and Planetary Astrophysics (astro-ph.EP) ,Physics ,[PHYS]Physics [physics] ,Debris disk ,Infrared excess ,Very Large Telescope ,Scattering ,Astronomy and Astrophysics ,stars: individual (49 Ceti) ,Debris ,[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph] ,13. Climate action ,Space and Planetary Science ,[SPI.OPTI]Engineering Sciences [physics]/Optics / Photonic ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,STAR : INDIVUDAL (49 CETI) ,Main sequence ,Astrophysics - Earth and Planetary Astrophysics - Abstract
We present the first scattered-light images of the debris disk around 49 ceti, a ~40 Myr A1 main sequence star at 59 pc, famous for hosting two massive dust belts as well as large quantities of atomic and molecular gas. The outer disk is revealed in reprocessed archival Hubble Space Telescope NICMOS F110W images, as well as new coronagraphic H band images from the Very Large Telescope SPHERE instrument. The disk extends from 1.1" (65 AU) to 4.6" (250 AU), and is seen at an inclination of 73degr, which refines previous measurements at lower angular resolution. We also report no companion detection larger than 3 M_Jup at projected separations beyond 20 AU from the star (0.34"). Comparison between the F110W and H-band images is consistent with a grey color of 49 ceti's dust, indicating grains larger than >2microns. Our photometric measurements indicate a scattering efficiency / infrared excess ratio of 0.2-0.4, relatively low compared to other characterized debris disks. We find that 49 ceti presents morphological and scattering properties very similar to the gas-rich HD 131835 system. From our constraint on the disk inclination we find that the atomic gas previously detected in absorption must extend to the inner disk, and that the latter must be depleted of CO gas. Building on previous studies, we propose a schematic view of the system describing the dust and gas structure around 49 ceti and hypothetic scenarios for the gas nature and origin., Accepted for publication in ApJL. 7 pages, 4 figures
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- 2017
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23. Performance of the Gemini Planet Imager's adaptive optics system.
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Poyneer, Lisa A., Palmer, David W., Macintosh, Bruce, Savransky, Dmitry, Sadakuni, Naru, Thomas, Sandrine, Véran, Jean-Pierre, Follette, Katherine B., Greenbaum, Alexandra Z., Ammons, S. Mark, Bailey, Vanessa P., Bauman, Brian, Cardwell, Andrew, Dillon, Daren, Gavel, Donald, Hartung, Markus, Hibon, Pascale, Perrin, Marshall D., Rantakyrö, Fredrik T., and Sivaramakrishnan, Anand
- Published
- 2016
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24. Sialendoscopy: A new diagnostic and therapeutic tool.
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Meyer, A., Delas, B., Hibon, R., Faure, F., Dehesdin, D., and Choussy, O.
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SALIVARY gland diseases ,CALCULI ,SURGICAL complications ,RETROSPECTIVE studies ,STENOSIS ,ENDOSCOPIC surgery ,THERAPEUTICS - Abstract
Summary: Background: Sialendoscopy is a recently developed minimally invasive diagnostic and therapeutic procedure for the management of obstructive diseases of the salivary glands. This report describes our early experience with this new tool and compares our results with the literature data. Material and methods: This was a retrospective analysis of the 33 first cases treated at a teaching hospital from October 2009 to June 2011. Results: The success rate for diagnostic sialendoscopy was 94%. Sialolithiasis was found in 19 cases and salivary duct stenosis in 11; no canal anomaly was found in two cases. The success rate for stone removal was 79%, while treatment of strictures failed in four cases. Longer surgical experience led to shorter operating times and improved indications as well as better therapeutic outcomes. There were no complications. Conclusion: Sialendoscopy is a safe technique that can easily be learned by surgeons familiar with endoscopic surgery. However, practical experience is needed to reduce operating times, lower failure rates and determine its precise indications. [Copyright &y& Elsevier]
- Published
- 2013
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25. Management of voice prosthesis leakage with Blom-Singer large esophage and tracheal flange voice prostheses.
- Author
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Choussy, O., Hibon, R., Mardion, N. Bon, and Dehesdin, D.
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ARTIFICIAL larynges ,ESOPHAGUS ,TRACHEA ,MEDICAL rehabilitation ,LARYNGECTOMY ,DISEASE complications - Abstract
Summary: Introduction: Voice rehabilitation after total laryngectomy is a major socio-economic challenge. Voice rehabilitation can be achieved by voice prostheses, which provide rapid patient satisfaction. Enlarged tracheo-oesophageal puncture is a frequent complication and can be difficult to manage. Material and method: A prospective study was conducted from November 2010 to October 2011 on 28 Blom-Singer large oesophageal and tracheal flange voice prostheses placed in 18 patients with enlarged tracheo-oesophageal puncture causing leakage around the voice prosthesis. Result: Leakage around the voice prosthesis resolved in all patients with a mean prosthesis lifespan of 95 days. The patients considered voice quality to be similar to that obtained with the initial voice prosthesis. Conclusion: The Blom-Singer large oesophageal and tracheal flange voice prosthesis is a useful solution for the management of periprosthetic leakage ensuring similar voice quality and an identical lifespan to that of other voice prostheses. [Copyright &y& Elsevier]
- Published
- 2013
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- View/download PDF
26. Out-of-Hospital Tracheal Intubation With Single-Use Versus Reusable Metal Laryngoscope Blades: A Multicenter Randomized Controlled Trial.
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Jabre, Patricia, Galinski, Michel, Ricard-Hibon, Agnes, Devaud, Marie Laure, Ruscev, Mirko, Kulstad, Erik, Vicaut, Eric, Adnet, Fréderic, Margenet, Alain, Marty, Jean, and Combes, Xavier
- Abstract
Study objective: Emergency tracheal intubation is reported to be more difficult with single-use plastic than with reusable metal laryngoscope blades in both inhospital and out-of-hospital settings. Single-use metal blades have been developed but have not been compared with conventional metal blades. This controlled trial compares the efficacy and safety of single-use metal blades with reusable metal blades in out-of-hospital emergency tracheal intubation. Methods: This randomized controlled trial was carried out in France with out-of-hospital emergency medical units (Services de Médecine d''Urgence et de Réanimation). This was a multicenter prospective noninferiority randomized controlled trial in adult out-of-hospital patients requiring emergency tracheal intubation. Patients were randomly assigned to either single-use or reusable metal laryngoscope blades and intubated by a senior physician or a nurse anesthetist. The primary outcome was first-pass intubation success. Secondary outcomes were incidence of difficult intubation, need for alternate airway devices, and early intubation-related complications (esophageal intubation, mainstem intubation, vomiting, pulmonary aspiration, dental trauma, bronchospasm or laryngospasm, ventricular tachycardia, arterial desaturation, hypotension, or cardiac arrest). Results: The study included 817 patients, including 409 intubated with single-use blades and 408 with a reusable blade. First-pass intubation success was similar in both groups: 292 (71.4%) for single-use blades, 290 (71.1%) for reusable blades. The 95% confidence interval (CI) for the difference in treatments (0.3%; 95% CI –5.9% to 6.5%) did not include the prespecified inferiority margin of –7%. There was no difference in rate of difficult intubation (difference 3%; 95% CI –7% to 2%), need for alternate airway (difference 4%; 95% CI –8% to 1%), or early complication rate (difference 3%; 95% CI –3% to 8%). Conclusion: First-pass out-of-hospital tracheal intubation success with single-use metal laryngoscopy blades was noninferior to first-pass success with reusable metal laryngoscope blades. [Copyright &y& Elsevier]
- Published
- 2011
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27. Acute coronary angiographic findings in survivors of out-of-hospital cardiac arrest.
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Anyfantakis, Zacharias Alexandros, Baron, Gabriel, Aubry, Pierre, Himbert, Dominique, Feldman, Laurent J., Juliard, Jean-Michel, Ricard-Hibon, Agnès, Burnod, Alexis, Cokkinos, Dennis V., and Steg, Philippe Gabriel
- Abstract
Background: Diagnosis of acute coronary artery disease in survivors of out-of-hospital cardiac arrest (OHCA) is difficult. The role of emergency coronary angiography and percutaneous coronary intervention (PCI) in this setting is debated. The objective of this study was to assess the prevalence of coronary lesions on emergency angiography in survivors of OHCA. Methods: Seventy-two consecutive OHCA survivors underwent systematic emergency coronary angiography. Patients with critical stenoses or occlusion underwent ad hoc PCI. Results: Most (63.9%) OHCA survivors had angiographic coronary artery disease (≥1 lesion >50%), but only a minority (37.5%) had clinical or angiographic evidence of an acute coronary syndrome due to either an acute occlusion (16.7%) or an irregular lesion suggestive of ruptured plaque or thrombus (25.0%). A final diagnosis of myocardial infarction was assigned in 27 patients (37.5%). Percutaneous coronary intervention was attempted and successful in 33.3% of the total cohort (n = 24). Hospital survival was 48.6%. By multivariable analysis, use of PCI was not an independent correlate of survival. ST-segment elevation on admission was an independent correlate of acute myocardial infarction (odds ratio 64.2, 95% CI 7.6-544.2, P = .0001), with high positive (82.6%) and negative (83.7%) predictive values. Conclusions: A minority of OHCA patients has angiographic evidence of an acute coronary syndrome and one-third undergo PCI, but PCI is not an independent correlate of survival. The presence of ST elevation on admission was a strong independent correlate of acute myocardial infarction and may be used to triage OHCA patients to emergency angiography with a view to PCI. [Copyright &y& Elsevier]
- Published
- 2009
- Full Text
- View/download PDF
28. Correlation of arterial Pco2 and Petco2 in prehospital controlled ventilation.
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Belpomme V, Ricard-Hibon A, Devoir C, Dileseigres S, Devaud M, Chollet C, and Marty J
- Abstract
INTRODUCTION: This study was carried out to estimate the relationship between arterial PCO2 (PaCO2) and end-tidal carbon dioxide (PETCO2) during prehospital controlled ventilation and also to evaluate variation of the gradient between PCO2 and PETCO2 during prehospital transport. METHODS: Measurements of PETCO2 from capnography values and PaCO2 from arterial blood gases were registered at the beginning (T(0)) and at the end (T(end)) of out-of-hospital management. For all patients requiring invasive ventilation, the gradient between PCO2 and PETCO2 was calculated for T(0) and T(end), the PaCO2-PETCO2 variation between T(end) and T(0) was also calculated. RESULTS: One hundred patients were included in this study (mean age, 58.4 +/- 16.4 years; 57 were male). There was no variation of the mean gradient (DeltaPaCO2-PETCO2 ) during transport (8.64 +/- 13.5 mm Hg at T(0) and 7.26 +/- 12.94 mm Hg at T(end)). Thirty-six percent of patients (n = 36) had a gradient above +10 mm Hg, and for 6% of patients (n = 4) the gradient was lower than -10 mm Hg. The PaCO2-PETCO2 gradient was not significantly different according to the pathology, but was significantly higher in hypercapnic patients compared with hypocapnic or normocapnic patients. In patients with severe head injury, the capnia was normalized in 80% of patients at the end of the transport according to the last blood gas result. In this subgroup the DeltaPaCO2-PETCO2 (T(end) - T(0)) gradient was stable between T(0) and T(end) except in 20% of the patients for whom the DeltaPaCO2-PETCO2 was lower than -10 mm Hg. Fifty-four percent of critical care physicians had modified the respiratory setting after the first arterial blood gas results. CONCLUSIONS: The PaCO2 cannot be estimated by the PETCO2 in the prehospital setting. There is wide variation in the gradient between PCO2 and PETCO2 depending on patient condition, and over time, the relationship does not remain constant and thus cannot be useful in prehospital ventilation management. Copyright © 2005 by Elsevier Inc. [ABSTRACT FROM AUTHOR]
- Published
- 2005
- Full Text
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29. Correlation of arterial Pco 2 and Petco 2 in prehospital controlled ventilation.
- Author
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Belpomme, Vanessa, Ricard-Hibon, Agnès, Devoir, Cyrille, Dileseigres, Sylvie, Devaud, Marie-Laure, Chollet, Charlotte, and Marty, Jean
- Abstract
Abstract: Introduction: This study was carried out to estimate the relationship between arterial Pco
2 (Paco2 ) and end-tidal carbon dioxide (Petco2 ) during prehospital controlled ventilation and also to evaluate variation of the gradient between Pco2 and Petco2 during prehospital transport. Methods: Measurements of Petco2 from capnography values and Paco2 from arterial blood gases were registered at the beginning (T0 ) and at the end (Tend ) of out-of-hospital management. For all patients requiring invasive ventilation, the gradient between Pco2 and Petco2 was calculated for T0 and Tend , the Paco2 − Petco2 variation between Tend and T0 was also calculated. Results: One hundred patients were included in this study (mean age, 58.4 ± 16.4 years; 57 were male). There was no variation of the mean gradient (ΔPaco2 − Petco2 ) during transport (8.64 ± 13.5 mm Hg at T0 and 7.26 ± 12.94 mm Hg at Tend ). Thirty-six percent of patients (n = 36) had a gradient above +10 mm Hg, and for 6% of patients (n = 4) the gradient was lower than −10 mm Hg. The Paco2 − Petco2 gradient was not significantly different according to the pathology, but was significantly higher in hypercapnic patients compared with hypocapnic or normocapnic patients. In patients with severe head injury, the capnia was normalized in 80% of patients at the end of the transport according to the last blood gas result. In this subgroup the ΔPaco2 − Petco2 (Tend − T0 ) gradient was stable between T0 and Tend except in 20% of the patients for whom the ΔPaco2 − Petco2 was lower than −10 mm Hg. Fifty-four percent of critical care physicians had modified the respiratory setting after the first arterial blood gas results. Conclusions: The Paco2 cannot be estimated by the Petco2 in the prehospital setting. There is wide variation in the gradient between Pco2 and Petco2 depending on patient condition, and over time, the relationship does not remain constant and thus cannot be useful in prehospital ventilation management. [Copyright &y& Elsevier]- Published
- 2005
- Full Text
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30. Analgesia with nitrous oxide/oxygen and acetaminophen compared to morphine analgesia in patients with acute myocardial infarction: Results from the SCADOL II clinical trial.
- Author
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Charpentier, S., Galinski, M., Bounes, V., Ricard-Hibon, A., El Khoury, Carlos, Elbaz, Meyer, Ageron, F.X., Manzo-Silberman, Stéphane, Soulat, Louis, Lapostolle, Frédéric, Gérard, A., Bregeaud, D., Bongard, Vanina, and Bonnefoy-Cudraz, E.
- Abstract
Background The safety of morphine use has been questioned in the management of ST Elevation Myocardial Infarction (STEMI). Are there other analgesics that are at least as effective without adverse effects? Purpose Evaluate the non-inferiority of nitrous oxide/oxygen plus acetaminophen versus morphine in pre-hospital patients with STEMI. Method Multi-center, randomized, non-inferiority cluster study. Thirty-eight mobile intensive care unit centres were randomized. Inclusion criteria: patients with STEMI and pain intensity score ≥ 4 on the numerical rating scale (NRS). Outcome: proportion of patient with NRS ≤ 3, 30 minutes after starting analgesia without adding morphine in the nitrous oxide/oxygen group. Expected or unexpected events were measured at 30 minutes and 1 month. Estimated number of subjects: 684. Per protocol (PP) and intention to treat (ITT) statistical analyses were planned. A non-inferiority margin was specified as an absolute difference of − 10% in proportions. The cluster design of the trial was taken into account through generalised estimating equations. Results A total of 684 patients were included in ITT analysis and 644 in PP analysis. Pain relief was obtained in 73.6% patients in the morphine group versus 51.7% patients in the nitrous oxide/oxygen group in the PP analysis. The absolute risk difference was − 21.7% (95% CI − 29.6 to − 13.8) and was below the non-inferiority margin of − 10%. The incidence of expected and serious adverse events were 10.2% and 3.5% respectively in the morphine group versus 13.2% and 6.2% in the nitrous oxide/oxygen group. Conclusion Oxide/oxygen plus acetaminophen is inferior to morphine analgesia in patients with STEMI. Adverse effects were not different between the groups. [ABSTRACT FROM AUTHOR]
- Published
- 2019
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31. THE SPITZER-IRAC/MIPS EXTRAGALACTIC SURVEY (SIMES) IN THE SOUTH ECLIPTIC POLE FIELD.
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I. Baronchelli, C. Scarlata, G. Rodighiero, A. Franceschini, P. L. Capak, S. Mei, M. Vaccari, L. Marchetti, P. Hibon, C. Sedgwick, C. Pearson, S. Serjeant, K. Menéndez-Delmestre, M. Salvato, M. Malkan, H. I. Teplitz, M. Hayes, J. Colbert, C. Papovich, and M. Devlin
- Published
- 2016
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- View/download PDF
32. Does aging influence quality of care for acute myocardial infarction in the prehospital setting? Elderly patients with acute myocardial infarction.
- Author
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Duchateau FX, Ricard-Hibon A, Devaud ML, Burnod A, and Mantz J
- Published
- 2006
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33. Design For The First Narrowband Filter For The Dark Energy Camera: Optimizing The LAGER Survey For Z ~ 7 Galaxies.
- Author
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Zheng ZY, Rhoads JE, Wang J, Malhotra S, Walker A, Mooney T, Jiang C, Hu W, Hibon P, Jiang L, Infante L, Barrientos LF, Galaz G, Valdes F, Wester W, Yang H, Coughlin A, Harish S, Kang W, Khostovan AA, Kong X, Perez LA, Pharo J, Wold I, and Zheng X
- Abstract
We present the design for the first narrowband filter NB964 for the Dark Energy Camera (DECam), which is operated on the 4m Blanco Telescope at the Cerro Tololo Inter-American Observatory. The NB964 filter profile is essentially defined by maximizing the power of searching for Lyman alpha emitting galaxies (LAEs) in the epoch of reionization, with the consideration of the night sky background in the near-infrared and the DECam quantum efficiency. The NB964 filter was manufactured by Materion in 2015. It has a central wavelength of 964.2 nm and a full width at half maximum (FWHM) of 9.2 nm. An NB964 survey named LAGER (Lyman Alpha Galaxies in the Epoch of Reionization) has been ongoing since December 2015. Here we report results of lab tests, on-site tests and observations with the NB964 filter. The excellent performances of this filter ensure that the LAGER project is able to detect LAEs at z ~ 7 with a high efficiency.
- Published
- 2019
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34. First light of the Gemini Planet imager.
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Macintosh B, Graham JR, Ingraham P, Konopacky Q, Marois C, Perrin M, Poyneer L, Bauman B, Barman T, Burrows AS, Cardwell A, Chilcote J, De Rosa RJ, Dillon D, Doyon R, Dunn J, Erikson D, Fitzgerald MP, Gavel D, Goodsell S, Hartung M, Hibon P, Kalas P, Larkin J, Maire J, Marchis F, Marley MS, McBride J, Millar-Blanchaer M, Morzinski K, Norton A, Oppenheimer BR, Palmer D, Patience J, Pueyo L, Rantakyro F, Sadakuni N, Saddlemyer L, Savransky D, Serio A, Soummer R, Sivaramakrishnan A, Song I, Thomas S, Wallace JK, Wiktorowicz S, and Wolff S
- Abstract
The Gemini Planet Imager is a dedicated facility for directly imaging and spectroscopically characterizing extrasolar planets. It combines a very high-order adaptive optics system, a diffraction-suppressing coronagraph, and an integral field spectrograph with low spectral resolution but high spatial resolution. Every aspect of the Gemini Planet Imager has been tuned for maximum sensitivity to faint planets near bright stars. During first-light observations, we achieved an estimated H band Strehl ratio of 0.89 and a 5-σ contrast of 10(6) at 0.75 arcseconds and 10(5) at 0.35 arcseconds. Observations of Beta Pictoris clearly detect the planet, Beta Pictoris b, in a single 60-s exposure with minimal postprocessing. Beta Pictoris b is observed at a separation of 434 ± 6 milliarcseconds (mas) and position angle 211.8 ± 0.5°. Fitting the Keplerian orbit of Beta Pic b using the new position together with previous astrometry gives a factor of 3 improvement in most parameters over previous solutions. The planet orbits at a semimajor axis of [Formula: see text] near the 3:2 resonance with the previously known 6-AU asteroidal belt and is aligned with the inner warped disk. The observations give a 4% probability of a transit of the planet in late 2017.
- Published
- 2014
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35. Epidemiological and serological study of hepatitis A virus outbreaks in France: a comparison between immunoadherence and radioimmunoassay.
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Coursaget P, Drucker J, Maupas P, Hibon P, Goudeau A, Bernard D, Sauvage D, and Lelord G
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- Adult, Child, Child, Preschool, France, Hepatitis A etiology, Hepatitis A immunology, Humans, Antibodies, Viral analysis, Disease Outbreaks epidemiology, Hepatitis A epidemiology, Hepatovirus immunology, Immune Adherence Reaction, Radioimmunoassay
- Abstract
An epidemiological study and the simultaneous evaluation of anti-HAV antibody using radio immunoassay (RIA) and immunoadherence hemagglutination assay (IAHA) was performed during three hepatitis A epidemics in the Tours area (France). Fifty-seven sera from 35 subjects with viral hepatitis type A and 16 sera from nine children who did not develop any clinical signs of hepatitis were studied. The more explosive epidemic occurred in an institution for mentally retarded children (attack rate 68%). The two major outbreaks observed were due to the introduction of the institutions of individuals infected with hepatitis A virus. Two out of three of the index cases had a seafood dinner three to four weeks before onset of jaundice. Sera taken one week after jaundice were always found to be anti-HAV positive by both RIA and IAHA, and sera taken more than three days before the appearance of jaundice were negative by both methods. Sera taken at the peak of the transaminase elevation were anti-HAV positive by RIA but only one out of two were positive by IAHA. The anti-HAV titre by RIA increased from the time of the appearance of jaundice and the highest titres, over 1/20000 were seen only after several months. Observations of subjects in close contact with patients who seroconverted without any manifestation of hepatitis, confirmed the existence of clinically mute infections.
- Published
- 1981
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36. Hepatitis A diagnosis in man: radioimmunoassay for hepatitis A antigen detection in faeces.
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Coursaget P, Maupas P, Hibon P, Lesage G, and Hubert M
- Subjects
- Alanine Transaminase blood, Child, Child, Preschool, Epitopes, Female, Humans, Male, Antigens, Viral analysis, Feces immunology, Hepatitis A diagnosis, Hepatovirus immunology, Radioimmunoassay methods
- Abstract
A new radioimmunoassay (RIA) procedure using a double-sandwich technique was developed for the detection of hepatitis A antigen (HAV) in crude faecal extracts for patients involved in three outbreaks of type A hepatitis. Stools were obtained from 24 residents suffering from acute hepatitis A and from six children who remained asymptomatic throughout the epidemic. In addition, the HAV detection was performed in sera from 13 patients with hepatitis. HAV was detected in stools as early as five days before and as late as five days after the onset of jaundice. In this procedure, positive activity was only found in stools from patients with type A hepatitis, but not in negative controls. HAV was not detected in acute-phase sera. The double-sandwich RIA test used appears to be a reliable test for the large-scale screening of HAV in stool samples from patients suffering from type A hepatitis.
- Published
- 1980
- Full Text
- View/download PDF
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