24 results on '"M, CHAIGNEAU"'
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2. The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager (Corrigendum)
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P. Rochus, F. Auchère, D. Berghmans, L. Harra, W. Schmutz, U. Schühle, P. Addison, T. Appourchaux, R. Aznar Cuadrado, D. Baker, J. Barbay, D. Bates, A. BenMoussa, M. Bergmann, C. Beurthe, B. Borgo, K. Bonte, M. Bouzit, L. Bradley, V. Büchel, E. Buchlin, J. Büchner, F. Cabé, L. Cadiergues, M. Chaigneau, B. Chares, C. Choque Cortez, P. Coker, M. Condamin, S. Coumar, W. Curdt, J. Cutler, D. Davies, G. Davison, J.-M. Defise, G. Del Zanna, F. Delmotte, V. Delouille, L. Dolla, C. Dumesnil, F. Dürig, R. Enge, S. François, J.-J. Fourmond, J.-M. Gillis, B. Giordanengo, S. Gissot, L. M. Green, N. Guerreiro, A. Guilbaud, M. Gyo, M. Haberreiter, A. Hafiz, M. Hailey, J.-P. Halain, J. Hansotte, C. Hecquet, K. Heerlein, M.-L. Hellin, S. Hemsley, A. Hermans, V. Hervier, J.-F. Hochedez, Y. Houbrechts, K. Ihsan, L. Jacques, A. Jérôme, J. Jones, M. Kahle, T. Kennedy, M. Klaproth, M. Kolleck, S. Koller, E. Kotsialos, E. Kraaikamp, P. Langer, A. Lawrenson, J.-C. Le Clech’, C. Lenaerts, S. Liebecq, D. Linder, D. M. Long, B. Mampaey, D. Markiewicz-Innes, B. Marquet, E. Marsch, S. Matthews, E. Mazy, A. Mazzoli, S. Meining, E. Meltchakov, R. Mercier, S. Meyer, M. Monecke, F. Monfort, G. Morinaud, F. Moron, L. Mountney, R. Müller, B. Nicula, S. Parenti, H. Peter, D. Pfiffner, A. Philippon, I. Phillips, J.-Y. Plesseria, E. Pylyser, F. Rabecki, M.-F. Ravet-Krill, J. Rebellato, E. Renotte, L. Rodriguez, S. Roose, J. Rosin, L. Rossi, P. Roth, F. Rouesnel, M. Roulliay, A. Rousseau, K. Ruane, J. Scanlan, P. Schlatter, D. B. Seaton, K. Silliman, S. Smit, P. J. Smith, S. K. Solanki, M. Spescha, A. Spencer, K. Stegen, Y. Stockman, N. Szwec, C. Tamiatto, J. Tandy, L. Teriaca, C. Theobald, I. Tychon, L. van Driel-Gesztelyi, C. Verbeeck, J.-C. Vial, S. Werner, M. J. West, D. Westwood, T. Wiegelmann, G. Willis, B. Winter, A. Zerr, X. Zhang, and A. N. Zhukov
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Space and Planetary Science ,Astronomy and Astrophysics - Published
- 2022
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3. The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager
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J. Hansotte, R. Müller, M. Hailey, P. Schlatter, A. Lawrenson, M. Monecke, Hardi Peter, Julien Rosin, Koen Stegen, Jean-Claude Vial, S. Parenti, Ali BenMoussa, Etienne Renotte, N. Szwec, Marie-Laure Hellin, R. Enge, M. Haberreiter, A. Philippon, P. Coker, B. Giordanengo, L. Dolla, K. Heerlein, Werner Schmutz, Matthew J. West, K. Ruane, J.-F. Hochedez, M. Chaigneau, M. Kahle, Emmanuel Mazy, J. Scanlan, J. Tandy, J. Barbay, B. Chares, T. Appourchaux, Laurence Rossi, C. Dumesnil, E. Pylyser, R. Aznar Cuadrado, Louise K. Harra, S. Meyer, F. Cabé, Benoit Marquet, Evgueni Meltchakov, Andrei Zhukov, D. Westwood, Bogdan Nicula, G. Willis, M.-F. Ravet-Krill, B. Borgo, S. Hemsley, Isabelle Tychon, N. Guerreiro, D. Linder, R. Mercier, Sylvie Liébecq, Thomas Wiegelmann, Philip J. Smith, M. Gyo, L. Mountney, G. Davison, Frédéric Rabecki, Jean-Marie Gillis, P. Langer, P. Roth, Sami K. Solanki, Luciano Rodriguez, Jean-Philippe Halain, L. Cadiergues, P. Addison, V. Büchel, D. Markiewicz-Innes, X. Zhang, Daniel Pfiffner, M. Roulliay, Antoine Rousseau, Stéphane Roose, Udo Schühle, M. Spescha, Jean-Yves Plesseria, Lionel Jacques, J. C. Le Clec’h, Yvan Stockman, G. Del Zanna, T. Kennedy, C. Beurthe, B. Mampaey, Franck Delmotte, C. Theobald, C. Choque Cortez, S. Meining, S. François, David Long, M. Bergmann, F. Rouesnel, S. Koller, C. Tamiatto, M. Bouzit, David Berghmans, D. Bates, L. Bradley, E. Kotsialos, A. Hafiz, D. Davies, J. B. L. Jones, S. Smit, Véronique Delouille, Gilles Morinaud, Aline Hermans, S. Coumar, J. Rebellato, Yvette Houbrechts, Stephan Werner, Werner Curdt, J. Cutler, K. Bonte, Daniel B. Seaton, Jean-Marc Defise, F. Moron, M. Klaproth, Eric Buchlin, J.-J. Fourmond, I. Phillips, Jörg Büchner, Pierre Rochus, M. Kolleck, Christophe Hecquet, Sarah A. Matthews, L. van Driel-Gesztelyi, Lucie M. Green, Cis Verbeeck, S. Gissot, F. Dürig, M. Condamin, Cedric Lenaerts, F. Auchère, K. Ihsan, K. Silliman, A. Guilbaud, Luca Teriaca, E. Kraaikamp, F. Monfort, A. Jérôme, Andreas Zerr, E. Marsch, Berend Winter, D. N. Baker, Alexandra Mazzoli, A. Spencer, V. Hervier, Institut d'astrophysique spatiale (IAS), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay, Centre Spatial de Liège (CSL), Université de Liège, Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Royal Observatory of Belgium [Brussels] (ROB), Mullard Space Science Laboratory (MSSL), University College of London [London] (UCL), Physikalisch-Meteorologisches Observatorium Davos/World Radiation Center (PMOD/WRC), Max-Planck-Institut für Sonnensystemforschung (MPS), Max-Planck-Gesellschaft, Max Planck Institute for Solar System Research (MPS), Laboratoire Charles Fabry / Optique XUV, Laboratoire Charles Fabry (LCF), Institut d'Optique Graduate School (IOGS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Institut d'Optique Graduate School (IOGS)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Faculty of mathematics Centre for Mathematical Sciences [Cambridge] (CMS), and University of Cambridge [UK] (CAM)
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010504 meteorology & atmospheric sciences ,Field of view ,Context (language use) ,Astrophysics ,01 natural sciences ,7. Clean energy ,law.invention ,Orbiter ,law ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Aerospace engineering ,010303 astronomy & astrophysics ,Chromosphere ,ComputingMilieux_MISCELLANEOUS ,0105 earth and related environmental sciences ,Physics ,business.industry ,[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] ,Ecliptic ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy and Astrophysics ,Corona ,13. Climate action ,Space and Planetary Science ,Extreme ultraviolet ,Physics::Space Physics ,Astrophysics::Earth and Planetary Astrophysics ,business ,[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] ,Heliosphere - Abstract
Context.The Extreme Ultraviolet Imager (EUI) is part of the remote sensing instrument package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and observe the Sun from vantage points close to the Sun and out of the ecliptic. Solar Orbiter will advance the “connection science” between solar activity and the heliosphere.Aims.With EUI we aim to improve our understanding of the structure and dynamics of the solar atmosphere, globally as well as at high resolution, and from high solar latitude perspectives.Methods.The EUI consists of three telescopes, the Full Sun Imager and two High Resolution Imagers, which are optimised to image in Lyman-αand EUV (17.4 nm, 30.4 nm) to provide a coverage from chromosphere up to corona. The EUI is designed to cope with the strong constraints imposed by the Solar Orbiter mission characteristics. Limited telemetry availability is compensated by state-of-the-art image compression, onboard image processing, and event selection. The imposed power limitations and potentially harsh radiation environment necessitate the use of novel CMOS sensors. As the unobstructed field of view of the telescopes needs to protrude through the spacecraft’s heat shield, the apertures have been kept as small as possible, without compromising optical performance. This led to a systematic effort to optimise the throughput of every optical element and the reduction of noise levels in the sensor.Results.In this paper we review the design of the two elements of the EUI instrument: the Optical Bench System and the Common Electronic Box. Particular attention is also given to the onboard software, the intended operations, the ground software, and the foreseen data products.Conclusions.The EUI will bring unique science opportunities thanks to its specific design, its viewpoint, and to the planned synergies with the other Solar Orbiter instruments. In particular, we highlight science opportunities brought by the out-of-ecliptic vantage point of the solar poles, the high-resolution imaging of the high chromosphere and corona, and the connection to the outer corona as observed by coronagraphs.
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- 2020
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4. Inflight performance of the PILOT balloon-borne experiment
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C. Engel, F. Pajot, J. Martignac, F. Bousqet, Y. Lepennec, S. Maestre, Nicolas Bray, Matthew Joseph Griffin, Peter A. R. Ade, A. Hughes, Silvia Masi, J. Narbonne, G. Foënard, René J. Laureijs, Frederi Mirc, Christopher Tibbs, J. M. Nicot, P. deBernardis, Y. André, G. Roudil, L. Rodriguez, Pierre Tapie, L. Bautista, B. Maffei, P. Etcheto, Etienne Perot, Peter Charles Hargrave, J. A. Tauber, J. P. Dubois, S. Grabarnik, B. Mot, M. Bouzit, L. Montier, O. Boulade, C. Marty, E. Doumayrou, Giampaolo Pisano, Isabelle Ristorcelli, H. Roussel, Nicolas Ponthieu, B. Leriche, A. Mangilli, X. Dupac, C. Tucker, Ph. Gelot, Y. Longval, Giorgio Savini, A. Lacourt, J. Aumont, V. Buttice, R. Misawa, M. Charra, Johan Montel, J. Pimentao, Muriel Saccoccio, W. Marty, B. Crane, M. Chaigneau, J.-P. Bernard, G. Parot, S. Stever, Maria Salatino, O. Simonella, Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA), Institut d'Astrophysique de Paris (IAP), and Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
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Point spread function ,High energy particle ,Far infrared ,Residual ,01 natural sciences ,Glitches ,Background ,Inflight performances ,Interstellar dust ,PILOT ,Pointing ,Polarization ,Responses ,Straylight ,0103 physical sciences ,Calibration ,010303 astronomy & astrophysics ,Cosmic dust ,Remote sensing ,010308 nuclear & particles physics ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy and Astrophysics ,Polarization (waves) ,Wavelength ,[SDU]Sciences of the Universe [physics] ,Space and Planetary Science ,Environmental science - Abstract
International audience; The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of thermal dust at a wavelength of 240 µm (1.2 THz). A first PILOT flight of the experiment took place from Timmins, Ontario, Canada, in September 2015 and a second flight took place from Alice Springs, Australia in April 2017. In this paper, we present the inflight performance of the instrument. Here we concentrate on the instrument performance as measured during the second flight, but refer to the performance observed during the first flight, if it was significantly different. We present a short description of the instrument and the flights. We measure the time constants of the detectors using the decay of the observed signal during flight following high energy particle impacts (glitches) and switching off the instrument's internal calibration source. We use these time constants to deconvolve the timelines and analyze the optical quality of the instrument as measured on planets. We then analyze the structure and polarization of the instrumental background. We measure the detector response flat field and its time variations using the signal from the residual atmosphere and from the internal calibration source. Finally, we analyze the spectral and temporal properties of the detector noise. The inflight performance is found to be satisfactory and globally in line with expectations from ground calibrations. We conclude by assessing the expected inflight sensitivity of the instrument in light of the measured inflight performance.
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- 2019
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5. Pilot optical alignment
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Nicolas Ponthieu, F. Pajot, J. M. Nicot, M. Chaigneau, G. Parot, Giorgio Savini, Y. André, M. Bouzit, Nicolas Bray, Johan Montel, C. Tucker, J.-P. Dubois, J. Martignac, J. Aumont, Maria Salatino, O. Simonella, V. Buttice, Bruno Maffei, R. J. Laureijs, R. Misawa, J.-Ph. Bernard, Frederi Mirc, B. Mot, J. Narbonne, Silvia Masi, O. Boulade, C. Engel, Etienne Perot, E. Doumayrou, A. Caillat, J. A. Tauber, C. Coudournac, A. Hughes, I. Ristorcelli, Y. Lepennec, S. Maestre, Pierre Tapie, Y. Longval, P. de Bernardis, F. Bousquet, G. Foenard, S. Grabarnik, Giampaolo Pisano, G. Roudil, P. Etcheto, P. Gélot, B. Leriche, Muriel Saccoccio, J. P. Crussaire, J. Pimentao, C. Marty, Matthew Joseph Griffin, Peter A. R. Ade, L. Baustista, M. Charra, F. Douchin, J.-P. Torre, L. Rodriguez, L. Montier, Peter Charles Hargrave, B. Crane, W. Marty, and G. Versepuech
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Physics ,Optical alignment ,business.industry ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Polarization (waves) ,Galaxy ,Interstellar medium ,Wavelength ,Long wavelength ,Optics ,business ,Astrophysics::Galaxy Astrophysics ,Dust emission ,Ontario canada - Abstract
PILOT (Polarized Instrument for Long wavelength Observations of the Tenuous interstellar medium) is a balloonborne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy. The PILOT instrument allows observations at wavelengths 240 μm (1.2THz) with an angular resolution about two arc-minutes. The observations performed during the first flight in September 2015 at Timmins, Ontario Canada, have demonstrated the optical performances of the instrument.
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- 2017
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6. The MicrOmega Investigation Onboard Hayabusa2
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J.-P. Bibring, V. Hamm, Y. Langevin, C. Pilorget, A. Arondel, M. Bouzit, M. Chaigneau, B. Crane, A. Darié, C. Evesque, J. Hansotte, V. Gardien, L. Gonnod, J.-C. Leclech, L. Meslier, T. Redon, C. Tamiatto, S. Tosti, and N. Thoores
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- 2017
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7. The PILOT optical alignment for its first flight
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G. Roudil, B. Mot, Y. Longval, W. Marty, J. Aumont, R. Misawa, A. Caillat, Y. Lepennec, E. Doumayrou, G. Foënard, J. A. Tauber, A. Hughes, G. Parot, L. Montier, J. Pimentao, M. Chaigneau, F. Pajot, J.-Ph. Bernard, B. Crane, Johan Montel, B. Leriche, M. Bouzit, Nicolas Bray, V. Buttice, Nicolas Ponthieu, Pierre Tapie, Isabelle Ristorcelli, J. M. Nicot, Muriel Saccoccio, Giorgio Savini, F. Douchin, P. deBernardis, C. Coudournac, Frederi Mirc, J. Martignac, Etienne Perot, Bruno Maffei, J.-P. Torre, C. Engel, A. Mangilli, L. Rodriguez, Peter Charles Hargrave, S. Maestre, Y. André, Silvia Masi, L. Bautista, P. Etcheto, C. Marty, S. Stever, S. Grabarnik, Maria Salatino, O. Simonella, Giampaolo Pisano, J.-P. Dubois, Carole Tucker, P. Gélot, René J. Laureijs, F. Bousquet, Matthew Joseph Griffin, Peter A. R. Ade, J. Narbonne, Christopher Tibbs, and O. Boulade
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Cryostat ,Optical alignment ,Physics::Optics ,Aerospace Engineering ,Astrophysics ,01 natural sciences ,law.invention ,010309 optics ,Primary mirror ,Optics ,law ,Polarization ,0103 physical sciences ,Optical instrumentation ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,Gregorian telescope ,business.industry ,Submillimeter telescope ,Polarization (waves) ,Galaxy ,Interstellar medium ,Wavelength ,Space and Planetary Science ,business - Abstract
PILOT is a balloon-borne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy at wavelengths 240 and 550 µm with an angular resolution of about two arc-min. PILOT optics is composed of an off-axis Gregorian telescope and a refractive re-imager system. All these optical elements, except the primary mirror, are in a cryostat cooled to 3K. We used optical and 3D measurements combined with thermo-elastic modeling to perform the optical alignment. This paper describes the system analysis, the alignment procedure, and finally the performances obtained during the first flight in September 2015
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- 2017
8. The optical performance of the PILOT instrument from ground end‐to‐end tests
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Y. Longval, O. Boulade, Maria Salatino, O. Simonella, René J. Laureijs, Nicolas Ponthieu, B. Leriche, Y. André, L. Bautista, J. Narbonne, J. A. Tauber, J. P. Dubois, Muriel Saccoccio, Carole Tucker, G. Roudil, Matthew Joseph Griffin, Peter A. R. Ade, Giorgio Savini, Isabelle Ristorcelli, J. Pimentao, L. Rodriguez, A. Caillat, B. Mot, M. Bouzit, A. Hughes, Peter Charles Hargrave, C. Engel, F. Bousqet, J. Montel, B. Maffei, E. Doumayrou, Silvia Masi, J.-P. Bernard, D. Alina, S. Maestre, G. Foënard, P. de Bernardis, L. Montier, M. Chaigneau, J. Aumont, R. Misawa, M. Charra, F. Douchin, W. Marty, Etienne Perot, C. Marty, V. Buttice, S. Grabarnik, Giampaolo Pisano, F. Pajot, B. Crane, Laboratoire d'Astrophysique de Marseille (LAM), and Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
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Point spread function ,Image quality ,Far infrared ,01 natural sciences ,010309 optics ,Optics ,Polarization ,0103 physical sciences ,PILOT ,Straylight ,010303 astronomy & astrophysics ,QB ,Remote sensing ,Cosmic dust ,Physics ,[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] ,Linear polarization ,business.industry ,Detector ,Interstellar dust ,Astronomy and Astrophysics ,Space and Planetary Science ,Polarization (waves) ,Wavelength ,Cardinal point ,business - Abstract
International audience; The Polarized Instrument for Long‐wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon‐borne astronomy experiment designed to study the linear polarization of thermal dust emission in two photometric bands centred at wavelengths 240 mu m (1.2 THz) and 550 mu m (545 GHz), with an angular resolution of a few arcminutes. Several end‐to‐end tests of the instrument were performed on the ground between 2012 and 2014, in order to prepare for the first scientific flight of the experiment that took place in September 2015 from Timmins, Ontario, Canada. This paper presents the results of those tests, focussing on an evaluation of the instrument's optical performance. We quantify image quality across the extent of the focal plane, and describe the tests that we conducted to determine the focal plane geometry, the optimal focus position, and sources of internal straylight. We present estimates of the detector response, obtained using an internal calibration source, and estimates of the background intensity and background polarization.
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- 2017
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9. Inflight performance of the PILOT balloon-borne experiment
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P. Etcheto, G. Foenard, I. Ristorcelli, W. Marty, F. Bousquet, Maria Salatino, O. Simonella, S. Grabarnik, Nicolas Ponthieu, Frederi Mirc, L. Rodriguez, J. A. Tauber, B. Mot, Pierre Tapie, Nicolas Bray, Giampaolo Pisano, Etienne Perot, R. Misawa, L. Montier, Giorgio Savini, Y. Lepennec, S. Maestre, Peter Charles Hargrave, B. Crane, J. Aumont, Bruno Maffei, C. Tucker, J.-P. Dubois, G. Parot, E. Doumayrou, L. Bautista, J.-Ph. Bernard, Johan Montel, V. Buttice, A. Caillat, M. Bouzit, Y. Longval, P. de Bernardis, R. J. Laureijs, C. Engel, Silvia Masi, J. Martignac, A. Hughes, G. Roudil, B. Leriche, Muriel Saccoccio, P. Gélot, M. Chaigneau, J. M. Nicot, J. Narbonne, Y. André, J.-P. Torre, J. P. Crussaire, J. Pimentao, C. Marty, F. Pajot, O. Boulade, M. Charra, F. Douchin, Matthew Joseph Griffin, and Peter A. R. Ade
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Physics ,010504 meteorology & atmospheric sciences ,Applied Mathematics ,Far infrared ,Dust ,Computer Science Applications1707 Computer Vision and Pattern Recognition ,Condensed Matter Physics ,01 natural sciences ,Ceiling balloon ,Polarization ,0103 physical sciences ,Balloon ,ISM ,PILOT ,Electronic, Optical and Magnetic Materials ,Electrical and Electronic Engineering ,Electronic ,Optical and Magnetic Materials ,010303 astronomy & astrophysics ,Flight data ,0105 earth and related environmental sciences ,Remote sensing - Abstract
PILOT is a stratospheric experiment designed to measure the polarization of dust FIR emission, towards the diffuse interstellar medium. The first PILOT flight was carried out from Timmins in Ontario-Canada on September 20th 2015. The flight has been part of a launch campaign operated by the CNES, which has allowed to launch 4 experiments, including PILOT. The purpose of this paper is to describe the performance of the instrument in flight and to perform a first comparison with those achieved during ground tests. The analysis of the flight data is on-going, in particular the identification of instrumental systematic effects, the minimization of their impact and the quantification of their remaining effect on the polarization data. At the end of this paper, we shortly illustrate the quality of the scientific observations obtained during this first flight, at the current stage of systematic effect removal.
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- 2016
10. PILOT: a balloon-borne experiment to measure the polarized FIR emission of dust grains in the interstellar medium
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J. Pimentao, G. Parot, L. Montier, J. Aumont, Bruno Maffei, M. Bouzit, L. Bautista, R. Misawa, B. Crane, B. Leriche, S. Grabarnik, A. Caillat, Nicolas Ponthieu, M. Charra, F. Bousquet, Peter Charles Hargrave, Giampaolo Pisano, Y. Lepennec, J. Narbonne, S. Maestre, Y. André, Maria Salatino, O. Simonella, F. Mirc, F. Douchin, A. Hughes, J.-P. Bernard, Matthew Joseph Griffin, P. Etcheto, Peter A. R. Ade, J. A. Tauber, Giorgio Savini, Carole Tucker, P. Gélot, G. Foënard, G. Roudil, J. P. Crussaire, W. Marty, C. Engel, Muriel Saccoccio, M. Chaigneau, F. Pajot, J. M. Nicot, Y. Longval, Isabelle Ristorcelli, L. Rodriguez, O. Boulade, P. de Bernardis, J.-P. Torre, Silvia Masi, Johan Montel, J. Martignac, E. Pérot, Nicolas Bray, B. Mot, V. Buttice, C. Marty, E. Doumayrou, René J. Laureijs, J.-P. Dubois, and P. Tapie
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Cosmic microwave background ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,01 natural sciences ,Cosmology ,Space exploration ,law.invention ,010309 optics ,law ,instrumentation ,interstellar medium ,polarization ,Astronomy and Astrophysics ,Space and Planetary Science ,0103 physical sciences ,010303 astronomy & astrophysics ,Astrophysics::Galaxy Astrophysics ,Physics ,Pilot experiment ,Bolometer ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy ,Polarization (waves) ,Galaxy ,Interstellar medium - Abstract
Future cosmology space missions will concentrate on measuring the polarization of the Cosmic Microwave Background, which potentially carries invaluable information about the earliest phases of the evolution of our universe. Such ambitious projects will ultimately be limited by the sensitivity of the instrument and by the accuracy at which polarized foreground emission from our own Galaxy can be subtracted out. We present the PILOT balloon project, which aims at characterizing one of these foreground sources, the polarized continuum emission by dust in the diffuse interstellar medium. The PILOT experiment also constitutes a test-bed for using multiplexed bolometer arrays for polarization measurements. This paper presents the instrument and its expected performances. Performance measured during ground calibrations of the instrument and in flight will be described in a forthcoming paper.
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- 2016
11. The history of women and hemophilia: a narrative review of evolving beliefs and testing practices.
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Chaigneau M, Bowman M, Wilton P, Card R, Poon MC, Lillicrap D, Sholzberg M, and James P
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The history of hemophilia is well documented, yet reports focus heavily on the male perspective and severe forms of the disease. Although hemophilia was initially believed to only affect men with women seen as silent carriers, it is now universally acknowledged that women and girls can also be affected. In this narrative review, we tracked the progression of beliefs about women and hemophilia as documented in the literature from pre-1800s to the present time. We present a timeline of evolving beliefs and testing practices and identified 9 distinct time periods when key shifts occurred related to various scientific discoveries. Our review highlights how women affected by hemophilia experienced complete dismissal of their health issues despite evidence of bleeding symptoms as early as the 1900s. We identified 1990 as a major timepoint for shifting beliefs when large scale acknowledgment that hemophilia also affects women is documented and systematic testing for bleeding risk is first suggested. Women evolve from being seen as unaffected genetic transmitters only, to being recognized as a population affected by hemophilia in unique ways requiring timely testing and effective treatment. Yet, despite this clear progress, recent publications continue to document many persistent issues such as delayed diagnosis, untreated symptoms, and barriers to care. Ongoing research and advocacy efforts are required to improve knowledge translation until real-world outcomes are seen in screening, diagnosis, treatment, and prevention of bleeding., Competing Interests: Declaration of competing interests P.J. has received research funding from Bayer and consultancy with Star/Vega, Band/Guardian, Roche, and Biomarin. D.L. has received research funding from Biomarin, CSL-Behring, and Sanofi and acted in an advisory role for Biomarin, CSL-Behring, Novo Nordisk, Pfizer, and Takeda. M.S. has received research funding from Octapharma and Pfizer (to institution), and honoraria for speaking engagements from Pfizer, Octapharma, Takeda, Sobi, and Medison. All other authors have no competing interests to declare., (Copyright © 2024 The Authors. Published by Elsevier Inc. All rights reserved.)
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- 2024
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12. Haemophilia testing of young girls in Canada: Describing the current recommendations for factor level and genetic testing and the experiences of Canadian parents.
- Author
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Chaigneau M, Grabell J, Wijnker E, Bowman M, and James P
- Subjects
- Humans, Canada, Female, Surveys and Questionnaires, Child, Adolescent, Adult, Genetic Testing methods, Hemophilia A genetics, Hemophilia A diagnosis, Parents psychology
- Abstract
Introduction: It is widely acknowledged that haemophilia affects women and girls, yet current testing recommendations for factor level and genetic testing vary and do not universally incorporate updated research. Canadian parents have expressed frustration at inconsistent recommendations and reported instances where delayed testing led to missed diagnosis and preventable bleeding., Aim: Study aim was to explore and describe the practice of haemophilia-related testing of young girls in Canada., Methods: A mixed methods study was carried out with two populations: (1) Nurses working in haemophilia care completed a survey regarding the current testing recommendations of their Haemophilia Treatment Centre (HTC), (2) Parents of obligate or potential haemophilia carriers completed a structured interview with questions about their family experience of haemophilia and testing decisions for daughters., Results: Twenty-six survey responses were received and showed wide variation in the usual recommendations of Canadian HTCs. Different factor level testing recommendations may be given to obligate and potential carriers despite no difference in bleeding risk. Only a minority of HTCs currently recommend an early baseline factor level (< 10 years) to obligate carriers (27%) or potential carriers (15%). For genetic testing of potential carriers, 70% of HTC would approve a family request for genetic testing of a minor with specific conditions. The majority of parents interviewed felt dissatisfied with their testing experience (58%) and highlighted many issues related to delayed testing recommendations., Conclusion: Updated, nationally affirmed testing recommendations are needed that align with research on bleeding in women and girls affected by haemophilia., (© 2024 The Author(s). Haemophilia published by John Wiley & Sons Ltd.)
- Published
- 2024
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13. Molybdenum Disulfide Nanoribbons with Enhanced Edge Nonlinear Response and Photoresponsivity.
- Author
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Ghimire G, Ulaganathan RK, Tempez A, Ilchenko O, Unocic RR, Heske J, Miakota DI, Xiang C, Chaigneau M, Booth T, Bøggild P, Thygesen KS, Geohegan DB, and Canulescu S
- Abstract
MoS
2 nanoribbons have attracted increased interest due to their properties, which can be tailored by tuning their dimensions. Herein, the growth of MoS2 nanoribbons and triangular crystals formed by the reaction between films of MoOx (22 nanoribbons arising from distinct contributions from the single-layer edges and multilayer core. Nanoscale imaging reveals a blue-shifted exciton emission of the monolayer edge compared to the isolated MoS 2 monolayers due to built-in local strain and disorder. We further report on an ultrasensitive photodetector made of a single MoS2 nanoribbon with a responsivity of 8.72 × 102 A W-1 at 532 nm, among the highest reported up-to-date for single-nanoribbon photodetectors. These findings can inspire the design of MoS2 semiconductors with tunable geometries for efficient optoelectronic devices., (© 2023 The Authors. Advanced Materials published by Wiley-VCH GmbH.)- Published
- 2023
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14. Characterization of the First Animal Toxin Acting as an Antagonist on AT1 Receptor.
- Author
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Van Baelen AC, Iturrioz X, Chaigneau M, Kessler P, Llorens-Cortes C, Servent D, Gilles N, and Robin P
- Subjects
- Humans, Angiotensin II metabolism, Angiotensin Receptor Antagonists, beta-Arrestin 2 metabolism, Peptides metabolism, Receptor, Angiotensin, Type 2 metabolism, Receptors, Angiotensin metabolism, Renin-Angiotensin System physiology, Animals, Hypertension, Receptor, Angiotensin, Type 1 metabolism
- Abstract
The renin-angiotensin system (RAS) is one of the main regulatory systems of cardiovascular homeostasis. It is mainly composed of angiotensin-converting enzyme (ACE) and angiotensin II receptors AT1 and AT2. ACE and AT1 are targets of choice for the treatment of hypertension, whereas the AT2 receptor is still not exploited due to the lack of knowledge of its physiological properties. Peptide toxins from venoms display multiple biological functions associated with varied chemical and structural properties. If Brazilian viper toxins have been described to inhibit ACE, no animal toxin is known to act on AT1/AT2 receptors. We screened a library of toxins on angiotensin II receptors with a radioligand competition binding assay. Functional characterization of the selected toxin was conducted by measuring second messenger production, G-protein activation and β-arrestin 2 recruitment using bioluminescence resonance energy transfer (BRET) based biosensors. We identified one original toxin, A-CTX-cMila, which is a 7-residues cyclic peptide from Conus miliaris with no homology sequence with known angiotensin peptides nor identified toxins, displaying a 100-fold selectivity for AT1 over AT2. This toxin shows a competitive antagonism mode of action on AT1, blocking Gαq, Gαi3, GαoA, β-arrestin 2 pathways and ERK
1/2 activation. These results describe the first animal toxin active on angiotensin II receptors.- Published
- 2023
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15. A decreased and less sustained response to surrogates of haemostatic stress correlates with bleeding in type 1 von Willebrand disease.
- Author
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Kloosterman R, Zago-Schmitt M, Grabell J, Thibeault L, Chaigneau M, Hinds M, Hopman W, Bowman M, Harpell L, Johri AM, Good D, and James P
- Subjects
- Humans, Hemorrhage complications, Hemostasis, von Willebrand Factor, Hemostatics therapeutic use, von Willebrand Disease, Type 1 complications, von Willebrand Diseases complications
- Published
- 2023
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- View/download PDF
16. Spatially-Localized Functionalization on Nanostructured Surfaces for Enhanced Plasmonic Sensing Efficacy.
- Author
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Bryche JF, Vega M, Tempez A, Brulé T, Carlier T, Moreau J, Chaigneau M, Charette PG, and Canva M
- Abstract
This work demonstrates the enhancement in plasmonic sensing efficacy resulting from spatially-localized functionalization on nanostructured surfaces, whereby probe molecules are concentrated in areas of high field concentration. Comparison between SERS measurements on nanostructured surfaces (arrays of nanodisks 110 and 220 nm in diameter) with homogeneous and spatially-localized functionalization with thiophenol demonstrates that the Raman signal originates mainly from areas with high field concentration. TERS measurements with 10 nm spatial resolution confirm the field distribution profiles predicted by the numerical modeling. Though this enhancement in plasmonic sensing efficacy is demonstrated with SERS, results apply equally well to any type of optical/plasmonic sensing on functionalized surfaces with nanostructuring.
- Published
- 2022
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17. Challenges and knowledge gaps facing hemophilia carriers today: Perspectives from patients and health care providers.
- Author
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Chaigneau M, Botros M, Grabell J, Hopman W, and James P
- Abstract
Background: Hemophilia carriers experience abnormal bleeding symptoms; however, a lack of awareness about this topic coupled with additional knowledge gaps and barriers leads to suboptimal care for this population., Objective: The primary objective was to describe the current knowledge gaps and challenges from the perspective of both hemophilia carriers and their health care providers., Methods: We carried out a mixed methods descriptive study with two population groups between September and December 2020. The hemophilia carrier perspective was obtained through both focus groups and questionnaires, whereas the health care providers perspective obtained via questionnaire sent to the Association of Hemophilia Care Directors of Canada and the Canadian Association of Nurses in Hemophilia Care. Focus groups were analyzed using descriptive thematic analysis and quantitative survey data was also analyzed., Results: Eleven hemophilia carriers participated along with 19 health care providers (11 physicians, eight nurses). Hemophilia carrier focus group discussions identified four areas representing major challenges or knowledge gaps: (1) negative psychosocial impacts; (2) difficulty determining symptom significance; (3) need for self-advocacy; (4) testing concerns. Survey results from both groups were aligned with the most important topics for ongoing education identified as information on abnormal bleeding symptoms, where to seek treatment, and considerations for heavy menstrual bleeding/menstruation. The majority of both study groups believe obligate or potential carriers should have factor levels checked regardless of age if symptoms of abnormal bleeding occur or before an invasive procedure. However, hemophilia carriers were significantly more in favor of genetic testing under the age of consent than health care providers in all scenarios evaluated., (© 2022 The Authors. Research and Practice in Thrombosis and Haemostasis published by Wiley Periodicals LLC on behalf of International Society on Thrombosis and Haemostasis (ISTH).)
- Published
- 2022
- Full Text
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18. Approach to the Patient with Bleeding.
- Author
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Chaigneau M and James PD
- Subjects
- Humans, von Willebrand Diseases, von Willebrand Factor, Hemorrhage diagnosis, Hemorrhage therapy
- Abstract
Approach to the patient with bleeding begins with a thorough bleeding, medical, and family history to determine the nature of bleeding and severity of bleeding symptoms. Use of a Bleeding Assessment Tool allows the clinician to obtain a comprehensive bleeding history and ultimately determine the individual bleeding score that reflects bleeding severity and is classifiable as either normal or abnormal. In the absence of significant findings within patient history or presenting symptoms clearly pointing to a specific bleeding pathology, an approach to laboratory investigation is presented that proceeds through first-line, second-line, and third-line testing., Competing Interests: Disclosure P. James has research funding from Bayer., (Copyright © 2021 Elsevier Inc. All rights reserved.)
- Published
- 2021
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19. Visualising structural modification of patterned graphene nanoribbons using tip-enhanced Raman spectroscopy.
- Author
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Su W, Esfandiar A, Lancry O, Shao J, Kumar N, and Chaigneau M
- Abstract
Graphene nanoribbons (GNRs) fabricated using electron beam lithography are investigated using tip-enhanced Raman spectroscopy (TERS) with a spatial resolution of 5 nm under ambient conditions. High-resolution TERS imaging reveals a structurally modified 5-10 nm strip of disordered graphene at the edge of the GNRs. Furthermore, hyperspectral TERS imaging discovers the presence of nanoscale organic contaminants on the GNRs. These results pave the way for nanoscale chemical and structural characterisation of graphene-based devices using TERS.
- Published
- 2021
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20. Nanometer-Scale Uniform Conductance Switching in Molecular Memristors.
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Goswami S, Deb D, Tempez A, Chaigneau M, Rath SP, Lal M, Ariando, Williams RS, Goswami S, and Venkatesan T
- Abstract
One common challenge highlighted in almost every review article on organic resistive memory is the lack of areal switching uniformity. This, in fact, is a puzzle because a molecular switching mechanism should ideally be isotropic and produce homogeneous current switching free from electroforming. Such a demonstration, however, remains elusive to date. The reports attempting to characterize a nanoscopic picture of switching in molecular films show random current spikes, just opposite to the expectation. Here, this longstanding conundrum is resolved by demonstrating 100% spatially homogeneous current switching (driven by molecular redox) in memristors based on Ru-complexes of azo-aromatic ligands. Through a concurrent nanoscopic spatial mapping using conductive atomic force microscopy and in operando tip-enhanced Raman spectroscopy (both with resolution <7 nm), it is shown that molecular switching in the films is uniform from hundreds of micrometers down to the nanoscale and that conductance value exactly correlates with spectroscopically determined molecular redox states. This provides a deterministic molecular route to obtain spatially homogeneous, forming-free switching that can conceivably overcome the chronic problems of robustness, consistency, reproducibility, and scalability in organic memristors., (© 2020 Wiley-VCH GmbH.)
- Published
- 2020
- Full Text
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21. Probing the nanoscale light emission properties of a CVD-grown MoS 2 monolayer by tip-enhanced photoluminescence.
- Author
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Okuno Y, Lancry O, Tempez A, Cairone C, Bosi M, Fabbri F, and Chaigneau M
- Abstract
Two-dimensional transition metal dichalcogenides are gaining increasing interest due to their promising optical properties. In particular, molybdenum disulfide (MoS
2 ) which displays a band-gap change from indirect at 1.29 eV for bulk materials to direct at 1.8 eV for the material monolayer. This particular effect can lead to a strong light interaction which can pave the way for a new approach to the next generation of visible light emitting devices. In this work we show the nanoscale variation of light emission properties by tip-enhanced photoluminescence microscopy and spectroscopy in the MoS2 monolayer, grown by chemical vapour deposition. The variations of the light emission properties are due to different effects depending on the shape of the MoS2 single layer, for instance, a different concentration of point defect in an irregularly shaped flake and the presence of a nanoscale terrace in a triangular monolayer. Simultaneously, atomic force microscopy reveals indeed the presence of a nanometric terrace, composed of an additional layer of MoS2 , and tip-enhanced PL intensity imaging shows a localized intensity decrease.- Published
- 2018
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22. In situ topographical chemical and electrical imaging of carboxyl graphene oxide at the nanoscale.
- Author
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Su W, Kumar N, Krayev A, and Chaigneau M
- Abstract
Visualising the distribution of structural defects and functional groups present on the surface of two-dimensional (2D) materials such as graphene oxide challenges the sensitivity and spatial resolution of the most advanced analytical techniques. Here we demonstrate mapping of functional groups on a carboxyl-modified graphene oxide (GO-COOH) surface with a spatial resolution of ≈10 nm using tip-enhanced Raman spectroscopy (TERS). Furthermore, we extend the capability of TERS by measuring local electronic properties in situ, in addition to the surface topography and chemical composition. Our results reveal that the Fermi level at the GO-COOH surface decreases as the I
D /IG ratio increases, correlating the local defect density with the Fermi level at nanometre length-scales. The in situ multi-parameter microscopy demonstrated in this work significantly improves the accuracy of nanoscale surface characterisation, eliminates measurement artefacts, and opens up the possibilities for characterising optoelectronic devices based on 2D materials under operational conditions.- Published
- 2018
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23. Cortical areas involved in behavioral expression of external pallidum dysfunctions: A PET imaging study in non-human primates.
- Author
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Galineau L, Kas A, Worbe Y, Chaigneau M, Herard AS, Guillermier M, Delzescaux T, Féger J, Hantraye P, and Tremblay L
- Subjects
- Animals, Bicuculline administration & dosage, Brain drug effects, Compulsive Behavior metabolism, Dyskinesias metabolism, Fluorodeoxyglucose F18, GABA-A Receptor Antagonists administration & dosage, Globus Pallidus drug effects, Hyperkinesis metabolism, Macaca fascicularis, Macaca mulatta, Positron-Emission Tomography, Behavior, Animal, Brain metabolism, Globus Pallidus metabolism
- Abstract
The external pallidum (GPe) is a component of the indirect pathway centrally placed in the basal ganglia. Studies already demonstrated that the pharmacological disinhibition of the sensorimotor, associative, and limbic GPe produced dyskinesia, hyperactivity, and compulsive behaviors, respectively. The aim of this study was to investigate the cortical regions altered by the disinhibition of each GPe functional territory. Thus, 5 macaques were injected with bicuculline in sensorimotor, associative, and limbic sites of the GPe producing dyskinesia, hyperactivity, and compulsive behaviors, and underwent in vivo positron tomography with
18 F-2-fluoro-2-deoxy-D-glucose to identify cortical dysfunctions related to GPe disinhibition. Blood cortisol levels were also quantified as a biomarker of anxiety for each condition. Our results showed that pallidal bicuculline injections in anesthetized animals reproducibly modified the activity of specific ipsilateral and contralateral cortical areas depending on the pallidal territory targeted. Bicuculline injections in the limbic GPe led to increased ipsilateral activations in limbic cortical regions (anterior insula, amygdala, and hippocampus). Injections in the associative vs. sensorimotor GPe increased the activity in the ipsilateral midcingulate vs. somatosensory and parietal cortices. Moreover, bicuculline injections increased blood cortisol levels only in animals injected in their limbic GPe. These are the first functional results supporting the model of opened cortico-striato-thalamo-cortical loops where modifications in a functional pallidal territory can impact cortical activities of the same functional territory but also cortical activities of other functional territories. This highlights the importance of the GPe as a crucial node in the top-down control of the cortico-striato-thalamo-cortical circuits from the frontal cortex to influence the perception, attention, and emotional processes at downstream (or non-frontal) cortical levels. Finally, we showed the implication of the ventral pallidum with the amygdala and the insular cortex in a circuit related to aversive processing that should be crucial for the production of anxious disorders., (Copyright © 2016 Elsevier Inc. All rights reserved.)- Published
- 2017
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24. Vibrational modes of aminothiophenol: a TERS and DFT study.
- Author
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Merlen A, Chaigneau M, and Coussan S
- Abstract
We report Tip Enhanced Raman Spectroscopy (TERS) mapping and Density Functional (DFT) calculations of aminothiophenol (ATP) grafted on a gold surface. The TERS mapping has demonstrated Raman modes of (ATP) and its dimerised derivative Dimercaptoazobenzene (DMAB). This feature confirms that the plasmon activated chemical reaction of ATP has occurred during TERS measurements. In some specific part of the samples some unidentified Raman modes are observed. We suggest that they could come from intermediate species formed during the conversion of ATP into DMAB. These modes are compared with calculated Raman spectra of some possible intermediate species. These results confirm the high potentiality of TERS measurements for nanochemistry.
- Published
- 2015
- Full Text
- View/download PDF
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