Conceptual study for a sub-pupil instrument having 4 high order adaptive optics paths for parallel multi-wavelength high contrast imaging, and medium resolution spectrometry

We present the concept of an instrument that will create 4 circular sub-pupils of 3 m in diameter. Each sub-pupil path will be corrected by a high order adaptive optics system (SR~80% in H) without spider and M2 obstruction. These four independent channels, obviously all pointed towards the same field, allows the possibility of covering totally different parts of the electromagnetic spectrum simultaneously without compromising Signal to Noise Ratio. Each channel can be dedicated to very specialized but complementary purposes: high contrast imaging, pseudo-wide field imaging, high precision multi-color photometry, medium-resolution spectroscopy, polarimetry and sparse-aperture masking

Early Miocene carbonate ramp development in a warm ocean, North West Shelf, Australia

Although carbonate ramps are widely described from the geological record,there is still a debate on the relative influence of water temperature, trophicconditions and type of carbonate factories on their development. Theca2400 km long Australian North West Shelf is among the largest Cenozoic car-bonate provinces worldwide, and records a transition from an early Mioceneramp to a middle Miocene rimmed platform. This change is observable onpublicly available seismic data, giving the opportunity to investigate envi-ronmental influences on platform evolution. This study combines macro-scopic and petrographic descriptions of early Miocene strata cropping out inthe Cape Range Anticline (North West Cape, southern end of the North WestShelf) and of time-equivalent well cuttings from the adjacent, offshoreExmouth Sub-basin. Particular emphasis is placed on the identification oflarger benthic foraminifera at a broad generic level, because differing taxahave a limited range of habitable conditions that serve as environmentalproxies. The results show that early Miocene strata are dominantly com-posed of larger benthic foraminifera with minor coralline algae in the proxi-mal platform, grading to micropackstones in the more distal platform. Aramp margin is inferred from the lithological data on the basis of the lack offramework builders and the presence of open oceanic indicators. Facies shal-low upward through individual outcrops, with a proximal to distal trendtowards the north-west. These trends along outcrops are consistent with theseismic interpretations. Identification of taxa with warm, oligotrophic wateraffinity suggests that the ramp was formed in an oligotrophic and warmocean, despite the absence of coral reefs. Changes of carbonate facies withdepth do not seem to be associated with changes in ramp morphology, andthe latter may have been controlled by physical oceanic parameters, such asoffshore currents and waves.Early Miocene carbonate ramp development in a warm ocean, North West Shelf, AustraliapublishedVersio

Linking the High-Resolution Architecture of Modern and Ancient Wave-Dominated Deltas : Processes, Products and Forcing Factors

Many thoughts and concepts used in this paper were initially developed as a result of work conducted with funding provided to the WAVE Consortium at the Australian School of Petroleum, University of Adelaide (RBA, BKV and JB). The consortium sponsors (Apache, BAPETCO, BHPBP, BG, BP, Chevron, ConocoPhillips, Nexen, OMV, Shell, Statoil, Todd Energy, and Woodside Energy) are thus thanked for making this work possible. We are indebted to journal reviewers Cornel Olariu and Howard Feldman, and to Associate Editor Janok Bhattacharya for numerous comments and suggestions that improved the clarity of the manuscript.Peer reviewedPostprin

Ergonomic assessment of an active orthosis for the rehabilitation of flexion and extension of Wrist

Muscular stiffness and limb rigidity are two main consequences of Parkinson’s disease. These motor symptoms may be present in distinct parts of the body, influencing functional tasks executed by hands. To aid people suffering from these motor symptoms, we developed an active wrist orthosis whose purpose is to enable increase the flexion and extension range of motion of the wrist joint. We identified five relevant ergonomic variables that should be considered when using the orthosis in the clinical practice: (i) device stability, (ii) forearm position; (iii) muscular strength; (iv) amplitude of motion; and (v) mass of the device. These variables were identified based on the observation of movements while users executed the flexion and extension of the wrist with and without the device. In this research, we present a description of the developed orthosis and an evaluation of the ergonomic variables (i), (ii) and (iii). An enhanced support structure has been used with the orthosis and shown to lead to a stability improvement. Electromyographic analysis showed that the use of the orthosis does not introduce undue muscular load on the user at distinct angular positions of the forearm

VLTI status update: a decade of operations and beyond

We present the latest update of the European Southern Observatory's Very Large Telescope interferometer (VLTI). The operations of VLTI have greatly improved in the past years: reduction of the execution time; better offering of telescopes configurations; improvements on AMBER limiting magnitudes; study of polarization effects and control for single mode fibres; fringe tracking real time data, etc. We present some of these improvements and also quantify the operational improvements using a performance metric. We take the opportunity of the first decade of operations to reflect on the VLTI community which is analyzed quantitatively and qualitatively. Finally, we present briefly the preparatory work for the arrival of the second generation instruments GRAVITY and MATISSE.Comment: 10 pages, 7 figures, Proceedings of the SPIE, 9146-1

Microscopy-BIDS: An Extension to the Brain Imaging Data Structure for Microscopy Data

The Brain Imaging Data Structure (BIDS) is a specification for organizing, sharing, and archiving neuroimaging data and metadata in a reusable way. First developed for magnetic resonance imaging (MRI) datasets, the community-led specification evolved rapidly to include other modalities such as magnetoencephalography, positron emission tomography, and quantitative MRI (qMRI). In this work, we present an extension to BIDS for microscopy imaging data, along with example datasets. Microscopy-BIDS supports common imaging methods, including 2D/3D, ex/in vivo, micro-CT, and optical and electron microscopy. Microscopy-BIDS also includes comprehensible metadata definitions for hardware, image acquisition, and sample properties. This extension will facilitate future harmonization efforts in the context of multi-modal, multi-scale imaging such as the characterization of tissue microstructure with qMRI

Multiple star systems in the Orion nebula

This is the author accepted manuscript. The final fersion is available from EDP Sciences via the DOI in this record.This work presents an interferometric study of the massive-binary fraction in the Orion Trapezium cluster with the recently comissioned GRAVITY instrument. We observed a total of 16 stars of mainly OB spectral type. We find three previously unknown companions for θ1 Ori B, θ2 Ori B, and θ2 Ori C. We determined a separation for the previously suspected companion of NU Ori. We confirm four companions for θ1 Ori A, θ1 Ori C, θ1 Ori D, and θ2 Ori A, all with substantially improved astrometry and photometric mass estimates. We refined the orbit of the eccentric high-mass binary θ1 Ori C and we are able to derive a new orbit for θ1 Ori D. We find a system mass of 21.7 M⊙ and a period of 53 days. Together with other previously detected companions seen in spectroscopy or direct imaging, eleven of the 16 high-mass stars are multiple systems. We obtain a total number of 22 companions with separations up to 600 AU. The companion fraction of the early B and O stars in our sample is about two, significantly higher than in earlier studies of mostly OB associations. The separation distribution hints toward a bimodality. Such a bimodality has been previously found in A stars, but rarely in OB binaries, which up to this point have been assumed to be mostly compact with a tail of wider companions. We also do not find a substantial population of equal-mass binaries. The observed distribution of mass ratios declines steeply with mass, and like the direct star counts, indicates that our companions follow a standard power law initial mass function. Again, this is in contrast to earlier findings of flat mass ratio distributions in OB associations. We excluded collision as a dominant formation mechanism but find no clear preference for core accretion or competitive accretion.Marie Skłodowska-Curie Grant AgreementFCT-PortugalERC Starting Gran

The GRAVITY+ Project: Towards All-sky, Faint-Science, High-Contrast Near-Infrared Interferometry at the VLTI

The GRAVITY instrument has been revolutionary for near-infrared interferometry by pushing sensitivity and precision to previously unknown limits. With the upgrade of GRAVITY and the Very Large Telescope Interferometer (VLTI) in GRAVITY+, these limits will be pushed even further, with vastly improved sky coverage, as well as faint-science and high-contrast capabilities. This upgrade includes the implementation of wide-field off-axis fringe-tracking, new adaptive optics systems on all Unit Telescopes, and laser guide stars in an upgraded facility. GRAVITY+ will open up the sky to the measurement of black hole masses across cosmic time in hundreds of active galactic nuclei, use the faint stars in the Galactic centre to probe General Relativity, and enable the characterisation of dozens of young exoplanets to study their formation, bearing the promise of another scientific revolution to come at the VLTI.Comment: Published in the ESO Messenge

Les systèmes turbidiques du Golfe d'Oman et de la marge est-africaine : architecture, évolution des apports au Quaternaire terminal et impact de la distribution sédimentaire sur les propriétés géoacoustiques des fonds

Ce travail présente une analyse des systèmes turbiditiques actuels du Golfe d’Oman et de la marge est-africaine (océan Indien occidental), auparavant méconnus. Il se base sur une base de données acoustique (bathymétrie, imagerie multifaisceaux, sismique THR et multitraces) et sédimentologique (carottes küllenberg et calypso) issues de campagnes successives réalisées par le SHOM et l’IFP. L’architecture des systèmes de dépôts profonds et les processus associés ont révélé une grande diversité selon le contexte géodynamique et physiographique des marges étudiées (marge passive, marge transformante, marge active). Les différents systèmes étudiés illustrent notamment le rôle du contexte tectonique régional sur la répartition et la morphologie des dépocentres à plusieurs échelles d’observation. L'analyse détaillée des faciès et séquences sédimentaires a permis de mettre en évidence le fonctionnement sédimentaire des différents systèmes en lien avec les conditions physiographiques et environnementales régionales (influence des crues liées à la mousson sur le transfert sédimentaire). A travers la reconstruction des transferts sédimentaires dans ces systèmes turbiditiques, nous discutons de l’impact relatif des différents facteurs forçant la sédimentation gravitaire sous-marine à haute-fréquence (eustatisme, climat, et tectonique). Pour cela, une étude stratigraphique détaillée a été réalisée sur la base de différents outils (datation radiocarbone, géochimie élémentaire, biostratigraphie) permettant de contraindre dans le temps les séries sédimentaires gravitaires. L’évolution des apports sédimentaires et des processus de dépôt au cours du Quaternaire terminal, en relation avec les modifications paléo-environnementales continentales, a permis d’identifier l’impact, l’importance relative et les interactions entre les forçages externes sur le développement à haute-fréquence (103-104ans) de systèmes de dépôt gravitaires, dans divers contextes géodynamiques. Les connaissances acquises sur la sédimentation du Golfe d’Oman ont finalement permis d’alimenter une base de données sédimentologique conséquente. L’intégration de cette base dans un modèle numérique géoacoustique (« simulateur ») développé par le SHOM a permis d’évaluer quantitativement l’impact des variations sédimentaires à différentes échelles (distribution spatiale, lithologie, stratification, processus de dépôt) sur la propagation du signal acoustique pour différentes gammes de fréquence (de 300 Hz jusqu’à 3 kHz) et angles d’émission (de 0 à 90°). Ces travaux constituent une base pour la réalisation d’un modèle géoacoustique régional robuste.This study focuses on the Late Quaternary turbidite systems of the Gulf of Oman and the East-African margin (western Indian Ocean), previously poorly studied. It is based upon a compilation of acoustic data (bathymetry, multibeam imagery, 3.5 kHz and multi-channel seismic) and sedimentological data (küllenberg and calypso piston cores) recovered during several cruises leaded by the SHOM and IFP institutes. Turbidite system architecture and sedimentary processes revealed a strong variability primarily related to the physiographic, hydro-climatic and geodynamic context of each margin. High-resolution stratigraphy has been achieved using a combination of radiocarbon dating, XRF geochemistry, biostratigraphy). This allowed to investigate the impact, the interaction and the relative importance of the external forcings on deep water sedimentation (i.e. tectonics, climate and eustasy) at high- frequency (103 -104 yrs) in different tectonic setting (active & passive margins). Finally, integration of the sedimentological data set in a geoacoustic numerical modelling leaded to a first quantitative estimation of the regional relationship between sea-floor properties (lithology, depositional environment, stratification) and propagation of acoustic signal at 300 Hz- 3kHz frequencies and 0-90°. This work constitutes a basis for future geoacoustic modelling in the area

Les systèmes turbidiques du Golfe d'Oman et de la marge est-africaine : architecture, évolution des apports au Quaternaire terminal et impact de la distribution sédimentaire sur les propriétés géoacoustiques des fonds

Ce travail présente une analyse des systèmes turbiditiques actuels du Golfe d’Oman et de la marge est-africaine (océan Indien occidental), auparavant méconnus. Il se base sur une base de données acoustique (bathymétrie, imagerie multifaisceaux, sismique THR et multitraces) et sédimentologique (carottes küllenberg et calypso) issues de campagnes successives réalisées par le SHOM et l’IFP. L’architecture des systèmes de dépôts profonds et les processus associés ont révélé une grande diversité selon le contexte géodynamique et physiographique des marges étudiées (marge passive, marge transformante, marge active). Les différents systèmes étudiés illustrent notamment le rôle du contexte tectonique régional sur la répartition et la morphologie des dépocentres à plusieurs échelles d’observation. L'analyse détaillée des faciès et séquences sédimentaires a permis de mettre en évidence le fonctionnement sédimentaire des différents systèmes en lien avec les conditions physiographiques et environnementales régionales (influence des crues liées à la mousson sur le transfert sédimentaire). A travers la reconstruction des transferts sédimentaires dans ces systèmes turbiditiques, nous discutons de l’impact relatif des différents facteurs forçant la sédimentation gravitaire sous-marine à haute-fréquence (eustatisme, climat, et tectonique). Pour cela, une étude stratigraphique détaillée a été réalisée sur la base de différents outils (datation radiocarbone, géochimie élémentaire, biostratigraphie) permettant de contraindre dans le temps les séries sédimentaires gravitaires. L’évolution des apports sédimentaires et des processus de dépôt au cours du Quaternaire terminal, en relation avec les modifications paléo-environnementales continentales, a permis d’identifier l’impact, l’importance relative et les interactions entre les forçages externes sur le développement à haute-fréquence (103-104ans) de systèmes de dépôt gravitaires, dans divers contextes géodynamiques. Les connaissances acquises sur la sédimentation du Golfe d’Oman ont finalement permis d’alimenter une base de données sédimentologique conséquente. L’intégration de cette base dans un modèle numérique géoacoustique (« simulateur ») développé par le SHOM a permis d’évaluer quantitativement l’impact des variations sédimentaires à différentes échelles (distribution spatiale, lithologie, stratification, processus de dépôt) sur la propagation du signal acoustique pour différentes gammes de fréquence (de 300 Hz jusqu’à 3 kHz) et angles d’émission (de 0 à 90°). Ces travaux constituent une base pour la réalisation d’un modèle géoacoustique régional robuste.This study focuses on the Late Quaternary turbidite systems of the Gulf of Oman and the East-African margin (western Indian Ocean), previously poorly studied. It is based upon a compilation of acoustic data (bathymetry, multibeam imagery, 3.5 kHz and multi-channel seismic) and sedimentological data (küllenberg and calypso piston cores) recovered during several cruises leaded by the SHOM and IFP institutes. Turbidite system architecture and sedimentary processes revealed a strong variability primarily related to the physiographic, hydro-climatic and geodynamic context of each margin. High-resolution stratigraphy has been achieved using a combination of radiocarbon dating, XRF geochemistry, biostratigraphy). This allowed to investigate the impact, the interaction and the relative importance of the external forcings on deep water sedimentation (i.e. tectonics, climate and eustasy) at high- frequency (103 -104 yrs) in different tectonic setting (active & passive margins). Finally, integration of the sedimentological data set in a geoacoustic numerical modelling leaded to a first quantitative estimation of the regional relationship between sea-floor properties (lithology, depositional environment, stratification) and propagation of acoustic signal at 300 Hz- 3kHz frequencies and 0-90°. This work constitutes a basis for future geoacoustic modelling in the area