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Sökning: WFRF:(Chelli A.)

  • Resultat 1-8 av 8
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1.
  • Kattge, Jens, et al. (författare)
  • TRY plant trait database - enhanced coverage and open access
  • 2020
  • Ingår i: Global Change Biology. - : Wiley-Blackwell. - 1354-1013 .- 1365-2486. ; 26:1, s. 119-188
  • Tidskriftsartikel (refereegranskat)abstract
    • Plant traits-the morphological, anatomical, physiological, biochemical and phenological characteristics of plants-determine how plants respond to environmental factors, affect other trophic levels, and influence ecosystem properties and their benefits and detriments to people. Plant trait data thus represent the basis for a vast area of research spanning from evolutionary biology, community and functional ecology, to biodiversity conservation, ecosystem and landscape management, restoration, biogeography and earth system modelling. Since its foundation in 2007, the TRY database of plant traits has grown continuously. It now provides unprecedented data coverage under an open access data policy and is the main plant trait database used by the research community worldwide. Increasingly, the TRY database also supports new frontiers of trait-based plant research, including the identification of data gaps and the subsequent mobilization or measurement of new data. To support this development, in this article we evaluate the extent of the trait data compiled in TRY and analyse emerging patterns of data coverage and representativeness. Best species coverage is achieved for categorical traits-almost complete coverage for 'plant growth form'. However, most traits relevant for ecology and vegetation modelling are characterized by continuous intraspecific variation and trait-environmental relationships. These traits have to be measured on individual plants in their respective environment. Despite unprecedented data coverage, we observe a humbling lack of completeness and representativeness of these continuous traits in many aspects. We, therefore, conclude that reducing data gaps and biases in the TRY database remains a key challenge and requires a coordinated approach to data mobilization and trait measurements. This can only be achieved in collaboration with other initiatives.
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  • Malbet, F., et al. (författare)
  • High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)
  • 2012
  • Ingår i: Experimental Astronomy. - : Springer Science and Business Media LLC. - 0922-6435 .- 1572-9508. ; 34:2, s. 385-413
  • Tidskriftsartikel (refereegranskat)abstract
    • A complete census of planetary systems around a volume-limited sample of solar-type stars (FGK dwarfs) in the Solar neighborhood (d a parts per thousand currency signaEuro parts per thousand 15 pc) with uniform sensitivity down to Earth-mass planets within their Habitable Zones out to several AUs would be a major milestone in extrasolar planets astrophysics. This fundamental goal can be achieved with a mission concept such as NEAT-the Nearby Earth Astrometric Telescope. NEAT is designed to carry out space-borne extremely-high-precision astrometric measurements at the 0.05 mu as (1 sigma) accuracy level, sufficient to detect dynamical effects due to orbiting planets of mass even lower than Earth's around the nearest stars. Such a survey mission would provide the actual planetary masses and the full orbital geometry for all the components of the detected planetary systems down to the Earth-mass limit. The NEAT performance limits can be achieved by carrying out differential astrometry between the targets and a set of suitable reference stars in the field. The NEAT instrument design consists of an off-axis parabola single-mirror telescope (D = 1 m), a detector with a large field of view located 40 m away from the telescope and made of 8 small movable CCDs located around a fixed central CCD, and an interferometric calibration system monitoring dynamical Young's fringes originating from metrology fibers located at the primary mirror. The mission profile is driven by the fact that the two main modules of the payload, the telescope and the focal plane, must be located 40 m away leading to the choice of a formation flying option as the reference mission, and of a deployable boom option as an alternative choice. The proposed mission architecture relies on the use of two satellites, of about 700 kg each, operating at L2 for 5 years, flying in formation and offering a capability of more than 20,000 reconfigurations. The two satellites will be launched in a stacked configuration using a Soyuz ST launch vehicle. The NEAT primary science program will encompass an astrometric survey of our 200 closest F-, G- and K-type stellar neighbors, with an average of 50 visits each distributed over the nominal mission duration. The main survey operation will use approximately 70% of the mission lifetime. The remaining 30% of NEAT observing time might be allocated, for example, to improve the characterization of the architecture of selected planetary systems around nearby targets of specific interest (low-mass stars, young stars, etc.) discovered by Gaia, ground-based high-precision radial-velocity surveys, and other programs. With its exquisite, surgical astrometric precision, NEAT holds the promise to provide the first thorough census for Earth-mass planets around stars in the immediate vicinity of our Sun.
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3.
  • Cockell, C.S., et al. (författare)
  • Darwin - an experimental astronomy mission to search for extrasolar planets
  • 2009
  • Ingår i: Experimental Astronomy. - 0922-6435 .- 1572-9508. ; 23:1, s. 435-461
  • Tidskriftsartikel (refereegranskat)abstract
    • As a response to ESA call for mission concepts for its Cosmic Vision 2015–2025 plan, we propose a mission called Darwin. Its primary goal is the study of terrestrial extrasolar planets and the search for life on them. In this paper, we describe different characteristics of the instrument.
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  • Wincup, C, et al. (författare)
  • ANTI-RITUXIMAB ANTIBODIES DEMONSTRATE NEUTRALISING CAPACITY, ASSOCIATE WITH LOWER CIRCULATING DRUG LEVELS AND EARLY RELAPSE IN PATIENTS UNDERGOING TREATMENT FOR SYSTEMIC LUPUS ERYTHEMATOSUS
  • 2022
  • Ingår i: ANNALS OF THE RHEUMATIC DISEASES. - : BMJ. - 0003-4967 .- 1468-2060. ; 81, s. 1344-1345
  • Konferensbidrag (övrigt vetenskapligt/konstnärligt)abstract
    • A major limitation of biologic therapy is formation of anti-drug antibodies (ADA). We previously found ADA to rituximab (RTX) are more prevalent in patients undergoing treatment for systemic lupus erythematosus (SLE) than rheumatoid arthritis and vasculitis (1). In addition, we demonstrated that ADA to RTX predict subsequent infusion related reactions (2). However, little is known regarding the long-term dynamics of ADA to RTX in patients undergoing treatment for SLE.ObjectivesIn this study we evaluated the longitudinal impact of ADA positivity with particular focus on; 1) Risk factors for development of ADA. 2) Impact of ADA on treatment response. 3) Influence of ADA on RTX drug kinetics over time. 4) The capacity of ADA to neutralise RTX.MethodsPatients with SLE undergoing treatment with RTX were recruited to this study (n=35). Serum samples were collected at the following intervals post-treatment; 1-3 months (defined as ‘early’ post-treatment), 6 months, 12 months, 36 months (n=114).Clinical and laboratory data was collected pre-treatment and at each follow-up time point. Response to treatment was assessed by improvement in SLEDAI-2K score from baseline and also according to BILAG as previously described (3).ADA were detected using an electrochemiluminescent immunoassay. Serum RTX levels were measured by ELISA. ADA status was defined according to the following patterns over time; persistently negative, persistently positive (0-15 AU/ml) and persistently high positive (≥16 AU/ml, upper quartile). A complement dependent cytotoxic assay was used to determine neutralising capability of ADA in a subgroup of positive samples (n=38).ResultsADA to RTX were found to be persistently positive in 64.3% of patients over the 36-month follow-up period and there was no significant difference in baseline disease activity (BILAG / SLEDAI-2K) between those who were subsequently ADA positive vs negative. ADA positive patients had a younger age at diagnosis of SLE when compared with ADA negative (mean 22.50 ± 9.10 vs 37.29 ± 11.31 years, p=0.002, Figure 1 A). Multivariate logistic regression found a 22% decrease in risk of ADA positivity for each addition year after diagnosis (p=0.03).Figure 1.ADA positive patients had a significantly lower C3 level at baseline (mean 0.61 ± 0.23 g/L vs 0.87 ± 0.30 g/L, p=0.026), which remained lower at each subsequent time point post-treatment up to 12 months post-treatment (Figure 1B).At 1-3 months post-RTX, patients who were ADA positive had a significantly lower circulating drug level than ADA negative (p<0.001, Figure 1 C).In terms of clinical response, ADA positive patients had an initial significant improvement in disease activity (SLEDAI-2K) by 3 months (p<0.001). However, response was not maintained at 12 months (Figure 1 D). In comparison, ADA negative patients showed a significant improvement in SLEDAI-2K at 6 months and this was maintained across the 36-month follow-up period (Figure 1 E).BILAG defined relapse was more common at six months post-treatment in ADA positive patients (22%) and ADA highly positive patients (33%) than those who were ADA negative (in which there were no cases of relapse within the first six months, Figure 1 F). At 12-months post-RTX, a higher rate of BILAG defined Major Response was seen in those who were ADA negative (80%) when compared with ADA positive (44%) and high positive (36%) as shown in Figure 1 G.Finally, antibodies derived from all ADA positive samples (38/38) were found to neutralise RTX in vitro.ConclusionADA to RTX were common and persisted over the 36-month period of this study. ADA associated with earlier serum drug elimination, increased relapse rates and demonstrated neutralising capacity suggesting that ADA could be a significant limitation to sustained response to treatment in clinical practice.References[1]Faustini F et al. Arthritis research & therapy. 2021;23(1):211[2]Wincup C et al. Annals of the rheumatic diseases. 2019;78(8):1140-2[3]Md Yusof MY et al Annals of the rheumatic diseases. 2017;76(11):1829-36Disclosure of InterestsNone declared
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7.
  • Wittkowski, M., et al. (författare)
  • CalVin 3 - A New Release of the ESO Calibrator Selection Tool for the VLT Interferometer
  • 2011
  • Ingår i: The Messenger. - : ESO. ; 145, s. 7-9
  • Tidskriftsartikel (refereegranskat)abstract
    • Interferometric observations require frequent measurements of calibration stars of known diameter to estimate the instrumental transfer function. ESO offers the preparation tool CalVin to select suitable calibrators from an underlying list of calibrators. The latest version 3, first released in January 2011, offers major improvements in the number of available calibrators, the functionality of the search tool, as well as in terms of performance and ease of use. It has been developed in a collaboration between ESO and the French Jean-Marie Mariotti Center (JMMC).
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