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H2O:CO, at concentrations of (3:2) and (10:1), was condensed on CsI substrate at 15 K and irradiated with 46-MeV 58Ni11 + ion beam. Radiolysis induced by fast heavy ions was analyzed by infrared spectroscopy (FTIR). The formation of nine molecular species: CO2, H2O2, HCOOH, HCO, H2CO, 13CO2, CH3OH, O3, and C3O2 was observed. For both concentrations, carbon dioxide (CO2), formaldehyde (H2CO), formic acid (HCOOH), and hydrogen peroxide (H2O2) are the most abundant products species, and tricarbon dioxide (C3O2) is much less abundant. Precursor destruction cross-sections and formation cross-sections of products are determined. The CO destruction cross-section for the (3:2) concentration is almost five times higher than that of water, while those for the (10:1) concentration are practically the same. Atomic sputtering yields are estimated for the two ice films, the total mass sputtered is approximately 2.5 × 106 u per impact. These results contribute to figure out the chemical pathways of compounds synthesized from the two most abundant organic species (H2O and CO) observed in the ices of grain mantles of the circumstellar envelopes and interstellar medium. In additional, the finding results reveal that molecular astronomical percentages are comparable to those obtained after 15 eV molec−1 of deposited dose in current experiments compared with the relative concentration of molecules in solid phase observed in MYSO, LYSO, BG Stars, and Comets.

Radio bursts are sensitive tracers of non-thermal electron populations in the solar corona. They are produced by electron beams and shock waves propagating through the corona and the heliosphere, and by trapped electron populations in coronal mass ejections (CMEs) and in quiescent active regions. Combining space-borne and ground-based radio spectrographs allows one to track disturbances between the low corona, near or at the sites of particle acceleration, and the spacecraft. Radio observations are, therefore, a significant tool in probing the solar origin of heliospheric disturbances, which is a central research topic as witnessed by the Parker Solar Probe and Solar Orbiter missions. The full scientific return of these projects needs vigorous ground-based support, which at radio wavelengths covers altitudes up to about a solar radius above the photosphere. Besides research in solar and heliospheric physics, monitoring solar radio bursts also supports space weather services. On occasion, radio bursts can themselves be a space weather hazard. The Nançay radio astronomy station in central France has a long tradition of monitoring radio emission at decimetre-to-meter wavelengths. This article describes the radio spectrograph ORFEES (Observations Radiospectrographiques pour FEDOME et l’Etude des Eruptions Solaires). It observes the whole-Sun flux density between 144 and 1004 MHz, pertaining to regions between the low corona and about half a solar radius above the photosphere. ORFEES results from a partnership between Observatoire de Paris and the French Air Force, which operates the experimental space weather service FEDOME. The primary use of the instrument at the Paris Observatory is astrophysical observation. Low-resolution data with rapid availability are presently produced for the French Air Force. Similar information can be made available to a broader range of space weather service providers. This article gives an overview of the instrument design and access to the data and shows a few illustrative observations.

The Transient High-Energy Sky and Early Universe Surveyor (THESEUS) is a mission concept developed in the last years by a large European consortium, with interest in prospective participation by research groups in USA and other non-European countries. As detailed in Amati et al. 2017 (arXiv:1710.04638) and Stratta et al. 2017 (arXiv:1712.08153), THESEUS aims at exploiting high-redshift Gamma-Ray Bursts for getting unique clues on the early Universe and, being an unprecedentedly powerful machine for the detection, accurate location and redshift determination of all types of GRBs (long, short, high-z, under-luminous, ultra-long) and many other classes of transient sources and phenomena, at providing a substantial contribution to multi-messenger astrophysics and time-domain astronomy. Under these respects, THESEUS will show a beautiful synergy with the large observing facilities of the future, like E-ELT, TMT, SKA, CTA, ATHENA, in the electromagnetic domain, as well as with next-generation gravitational-waves and neutrino detectors, thus enhancing importantly their scientific return. Moreover, it will also operate as a flexible IR and X-ray observatory, thus providing an even larger involvement of the scientific community, as is currently the case for the Swift mission. In order to further explore the magnificent prospective science of the mission, the THESEUS consortium organized a Workshop in Naples on October 5-6 2017. The programme included about 50 reviews and talks from worldwide recognized experts of the fields. The topics ranged from the description of the mission concept, instrumentation and technologies to the main, additional and observatory science, further showing the strong impact that THESEUS observations would have on several fields of astrophysics, cosmology and fundamental physics., Comment: To be published in the Proceedings of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017.html), Journal of the Italian Astronomical Society (Mem.SAIt), Editors L. Amati, E. Bozzo, M. Della Valle, D. Gotz, P. O'Brien. Details on the THESEUS mission concept can be found in the white paper Amati et al. 2017 (arXiv:171004638) and Stratta et al. 2017 (arXiv:1712.08153)

The Sino-French space mission SVOM (Space-based multi-band astronomical Variable Objects Monitor) is mainly designed to detect and localize Gamma-Ray Burst events (GRBs). The satellite, to be launched late 2021, embarks a set of gamma-ray, X-ray and optical imagers. Thanks to its pointing strategy, quick slew capability and fast data connection to earth, ground based observations with large telescopes will allow us to measure redshifts for an unprecedented sample of GRBs. We discuss here the overall science goals of the SVOM mission in the framework of the multi-wavelength and multi-messenger panorama of the next decade. Finally we show how some developments of the SVOM mission will be helpful for the THESEUS project., Comment: To be published in the Proceedings of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017.html), Journal of the Italian Astronomical Society (Mem.SAIt), Editors L. Amati, E. Bozzo, M. Della Valle, D. Gotz, P. O'Brien. Details on the THESEUS mission concept can be found in the white paper Amati et al. 2017 (arXiv:171004638) and Stratta et al. 2017 (arXiv:1712.08153)

The Infra-Red Telescope (IRT) on board the Transient High Energy Sky and Early Universe Surveyor (THESEUS) ESA M5 candidate mission will play a key role in identifying and characterizing moderate to high redshift Gamma-Ray Bursts afterglows. The IRT is the enabling instrument on board THESEUS for measuring autonomously the redshift of the several hundreds of GRBs detected per year by the Soft X-ray Imager (SXI) and the X- and Gamma-Ray Imaging Spectrometer (XGIS), and thus allowing the big ground based telescopes to be triggered on a redshift pre-selected sample, and finally fulfilling the cosmological goals of the mission. The IRT will be composed by a primary mirror of 0.7 m of diameter coupled to a single camera in a Cassegrain design. It will work in the 0.7-1.8 {\mu}m wavelength range, and will provide a 10x10 arc min imaging field of view with sub-arc second localization capabilities, and, at the same time, a 5x5 arc min field of view with moderate (R up to ~500) spectroscopic capabilities. Its sensitivity, mainly limited by the satellite jitter, is adapted to detect all the GRBs, localized by the SXI/XGIS, and to acquire spectra for the majority of them., Comment: To be published in the Proceedings of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017.html), Journal of the Italian Astronomical Society (Mem.SAIt), Editors L. Amati, E. Bozzo, M. Della Valle, D. Gotz, P. O'Brien. Details on the THESEUS mission concept can be found in the white paper Amati et al. 2017 (arXiv:171004638) and Stratta et al. 2017 (arXiv:1712.08153)

International audience; En este artículo se reflexiona sobre las aportaciones de la cartografía para el análisis geográfico de los filmes, buscando concomitancias y vínculos entre las películas, el espacio y el mapa. En la primera parte, mediante una aproximación teórica, se justifica y contextualiza el método heurístico desarrollado por los autores. En la segunda parte se abordan cuestiones y planteamientos metodológicos sobre el tratamiento cartográfico de las películas de ficción que se aplican analizando la representación de Hong Kong en la filmografía. Con este estudio se valora la cartográfica como un instrumento de representación y de análisis.; This paper considers the role of cartography within the analysis of cinematic geography and addresses the similarities and links that are forged between film, space, and mapping. The authors establish a theoretical approach that justifies and contextualizes their methodological and heuristic positions. The second part of the paper focuses on methodological questions and issues that arise as a result of mapping in feature films. Finally, maps drawing on cinematic representations of Hong Kong are presented. This cartographic application facilitates a pragmatic response to the questions and issues previously highlighted.; L’article propose une réflexion sur l’apport de la cartographie dans le cadre des analyses ciné-géographiques. Il aborde les proximités et les liens qui se tissent entre le film, l’espace, et la carte : une approche théorique qui permet de justifier et de contextualiser le positionnement méthodologique et heuristique des auteures. Le second temps de l’article est dédié aux interrogations méthodologiques qu’implique le traitement cartographique de films de fictions. Enfin, les cartes produites à partir du cas de Hong Kong au cinéma sont présentées : une application cartographique permettant de répondre de manière pratique aux problématiques mises en évidence.

International audience; En este artículo se reflexiona sobre las aportaciones de la cartografía para el análisis geográfico de los filmes, buscando concomitancias y vínculos entre las películas, el espacio y el mapa. En la primera parte, mediante una aproximación teórica, se justifica y contextualiza el método heurístico desarrollado por los autores. En la segunda parte se abordan cuestiones y planteamientos metodológicos sobre el tratamiento cartográfico de las películas de ficción que se aplican analizando la representación de Hong Kong en la filmografía. Con este estudio se valora la cartográfica como un instrumento de representación y de análisis.; This paper considers the role of cartography within the analysis of cinematic geography and addresses the similarities and links that are forged between film, space, and mapping. The authors establish a theoretical approach that justifies and contextualizes their methodological and heuristic positions. The second part of the paper focuses on methodological questions and issues that arise as a result of mapping in feature films. Finally, maps drawing on cinematic representations of Hong Kong are presented. This cartographic application facilitates a pragmatic response to the questions and issues previously highlighted.; L’article propose une réflexion sur l’apport de la cartographie dans le cadre des analyses ciné-géographiques. Il aborde les proximités et les liens qui se tissent entre le film, l’espace, et la carte : une approche théorique qui permet de justifier et de contextualiser le positionnement méthodologique et heuristique des auteures. Le second temps de l’article est dédié aux interrogations méthodologiques qu’implique le traitement cartographique de films de fictions. Enfin, les cartes produites à partir du cas de Hong Kong au cinéma sont présentées : une application cartographique permettant de répondre de manière pratique aux problématiques mises en évidence.

International audience; We describe regularized methods for image reconstruction and focus on the question of hyperparameter and instrument parameter estimation, i.e. unsupervised and myopic problems. We developed a Bayesian framework that is based on the \post density for all unknown quantities, given the observations. This density is explored by a Markov Chain Monte-Carlo sampling technique based on a Gibbs loop and including a Metropolis-Hastings step. The numerical evaluation relies on the SPIRE instrument of the Herschel observatory. Using simulated and real observations, we show that the hyperparameters and instrument parameters are correctly estimated, which opens up many perspectives for imaging in astrophysics.