THE INFRARED COLORS OF THE SUN

Solar infrared colors provide powerful constraints on the stellar effective temperature scale, but they must be measured with both accuracy and precision in order to do so. We fulfill this requirement by using line-depth ratios to derive in a model-independent way the infrared colors of the Sun, and we use the latter to test the zero point of the Casagrande et al. effective temperature scale, confirming its accuracy. Solar colors in the widely used Two Micron All Sky Survey (2MASS) JHK(s) and WISE W1-4 systems are provided: (V - J)(circle dot) = 1.198, (V - H)(circle dot) = 1.484, (V - K-s)(circle dot) = 1.560, (J - H)(circle dot) = 0.286, (J - K-s)(circle dot) = 0.362, (H - K-s)(circle dot) = 0.076, (V - W1)(circle dot) = 1.608, (V - W2)(circle dot) = 1.563, (V - W3)(circle dot) = 1.552, and (V - W4)(circle dot) = 1.604. A cross-check of the effective temperatures derived implementing 2MASS or WISE magnitudes in the infrared flux method confirms that the absolute calibration of the two systems agrees within the errors, possibly suggesting a 1% offset between the two, thus validating extant near-and mid-infrared absolute calibrations. While 2MASS magnitudes are usually well suited to derive T-eff, we find that a number of bright, solar-like stars exhibit anomalous WISE colors. In most cases, this effect is spurious and can be attributed to lower-quality measurements, although for a couple of objects (3%+/- 2% of the total sample) it might be real, and may hint at the presence of warm/hot debris disks.

Sviluppo di algoritmi avanzati di analisi e diagnosi combustione in tempo reale per motori endotermici alternativi

Increasingly stringent exhaust emission limits and higher fuel economy are the main drivers of the engine development process. As a consequence, the complexity of the propulsion units and its subsystems increase, due to the extensive use of sensors and actuators needed to obtain a precise control over the combustion phase. Since engine calibration process consumes most of the development time, new tools and methodologies are needed to shorten the development time and increase the performance attainable. Real time combustion analysis, based on the in-cylinder pressure signal, can significantly improve the calibration of the engine control strategies and the development of new algorithms, giving instantaneous feedback on the engine behavior. A complete combustion analysis and diagnosis system has been developed, capable of evaluating the most important indicators about the combustion process, such as indicated mean effective pressure, heat release, mass fraction burned and knock indexes. Such a tool is built on top of a flexible, modular and affordable hardware platform, capable of satisfying the requirements needed for accuracy and precision, but also enabling the use directly on-board the vehicle, due to its small form factor.

Methodological improvement of 3D fluoroscopic analysis for the robust quantification of 3D kinematics of human joints

3D video-fluoroscopy is an accurate but cumbersome technique to estimate natural or prosthetic human joint kinematics. This dissertation proposes innovative methodologies to improve the 3D fluoroscopic analysis reliability and usability. Being based on direct radiographic imaging of the joint, and avoiding soft tissue artefact that limits the accuracy of skin marker based techniques, the fluoroscopic analysis has a potential accuracy of the order of mm/deg or better. It can provide fundamental informations for clinical and methodological applications, but, notwithstanding the number of methodological protocols proposed in the literature, time consuming user interaction is exploited to obtain consistent results. The user-dependency prevented a reliable quantification of the actual accuracy and precision of the methods, and, consequently, slowed down the translation to the clinical practice. The objective of the present work was to speed up this process introducing methodological improvements in the analysis. In the thesis, the fluoroscopic analysis was characterized in depth, in order to evaluate its pros and cons, and to provide reliable solutions to overcome its limitations. To this aim, an analytical approach was followed. The major sources of error were isolated with in-silico preliminary studies as: (a) geometric distortion and calibration errors, (b) 2D images and 3D models resolutions, (c) incorrect contour extraction, (d) bone model symmetries, (e) optimization algorithm limitations, (f) user errors. The effect of each criticality was quantified, and verified with an in-vivo preliminary study on the elbow joint. The dominant source of error was identified in the limited extent of the convergence domain for the local optimization algorithms, which forced the user to manually specify the starting pose for the estimating process. To solve this problem, two different approaches were followed: to increase the optimal pose convergence basin, the local approach used sequential alignments of the 6 degrees of freedom in order of sensitivity, or a geometrical feature-based estimation of the initial conditions for the optimization; the global approach used an unsupervised memetic algorithm to optimally explore the search domain. The performances of the technique were evaluated with a series of in-silico studies and validated in-vitro with a phantom based comparison with a radiostereometric gold-standard. The accuracy of the method is joint-dependent, and for the intact knee joint, the new unsupervised algorithm guaranteed a maximum error lower than 0.5 mm for in-plane translations, 10 mm for out-of-plane translation, and of 3 deg for rotations in a mono-planar setup; and lower than 0.5 mm for translations and 1 deg for rotations in a bi-planar setups. The bi-planar setup is best suited when accurate results are needed, such as for methodological research studies. The mono-planar analysis may be enough for clinical application when the analysis time and cost may be an issue. A further reduction of the user interaction was obtained for prosthetic joints kinematics. A mixed region-growing and level-set segmentation method was proposed and halved the analysis time, delegating the computational burden to the machine. In-silico and in-vivo studies demonstrated that the reliability of the new semiautomatic method was comparable to a user defined manual gold-standard. The improved fluoroscopic analysis was finally applied to a first in-vivo methodological study on the foot kinematics. Preliminary evaluations showed that the presented methodology represents a feasible gold-standard for the validation of skin marker based foot kinematics protocols.

Quantifying the OH radical by global scale NMHC measurements from the NOAA - ESRL cooperative flask sampling network

Summary PhD Thesis Jan Pollmann: This thesis focuses on global scale measurements of light reactive non-methane hydrocarbon (NMHC), in the volatility range from ethane to toluene with a special focus on ethane, propane, isobutane, butane, isopentane and pentane. Even though they only occur at the ppt level (nmol mol-1) in the remote troposphere these species can yield insight into key atmospheric processes. An analytical method was developed and subsequently evaluated to analyze NMHC from the NOAA – ERSL cooperative air sampling network. Potential analytical interferences through other atmospheric trace gases (water vapor and ozone) were carefully examined. The analytical parameters accuracy and precision were analyzed in detail. It was proven that more than 90% of the data points meet the Global Atmospheric Watch (GAW) data quality objective. Trace gas measurements from 28 measurement stations were used to derive the global atmospheric distribution profile for 4 NMHC (ethane, propane, isobutane, butane). A close comparison of the derived ethane data with previously published reports showed that northern hemispheric ethane background mixing ratio declined by approximately 30% since 1990. No such change was observed for southern hemispheric ethane. The NMHC data and trace gas data supplied by NOAA ESRL were used to estimate local diurnal averaged hydroxyl radical (OH) mixing ratios by variability analysis. Comparison of the variability derived OH with directly measured OH and modeled OH mixing ratios were found in good agreement outside the tropics. Tropical OH was on average two times higher than predicted by the model. Variability analysis was used to assess the effect of chlorine radicals on atmospheric oxidation chemistry. It was found that Cl is probably not of significant relevance on a global scale.

Therapeutisches drug monitoring bei antidepressiver Pharmakotherapie

Therapeutisches Drug Monitoring (TDM) umfasst die Messung von Medikamentenspiegeln im Blut und stellt die Ergebnisse in Zusammenhang mit dem klinischen Erscheinungsbild der Patienten. Dabei wird angenommen, dass die Konzentrationen im Blut besser mit der Wirkung korrelieren als die Dosis. Dies gilt auch für Antidepressiva. Voraussetzung für eine Therapiesteuerung durch TDM ist die Verfügbarkeit valider Messmethoden im Labor und die korrekte Anwendung des Verfahrens in der Klinik. Ziel dieser Arbeit war es, den Einsatz von TDM für die Depressionsbehandlung zu analysieren und zu verbessern. Im ersten Schritt wurde für das neu zugelassene Antidepressivum Duloxetin eine hochleistungsflüssig-chromatographische (HPLC) Methode mit Säulenschaltung und spektrophotometrischer Detektion etabliert und an Patienten für TDM angewandt. Durch Analyse von 280 Patientenproben wurde herausgefunden, dass Duloxetin-Konzentrationen von 60 bis 120 ng/ml mit gutem klinischen Ansprechen und einem geringen Risiko für Nebenwirkungen einhergingen. Bezüglich seines Interaktionspotentials erwies sich Duloxetin im Vergleich zu anderen Antidepressiva als schwacher Inhibitor des Cytochrom P450 (CYP) Isoenzyms 2D6. Es gab keinen Hinweis auf eine klinische Relevanz. Im zweiten Schritt sollte eine Methode entwickelt werden, mit der möglichst viele unterschiedliche Antidepressiva einschließlich deren Metaboliten messbar sind. Dazu wurde eine flüssigchromatographische Methode (HPLC) mit Ultraviolettspektroskopie (UV) entwickelt, mit der die quantitative Analyse von zehn antidepressiven und zusätzlich zwei antipsychotischen Substanzen innerhalb von 25 Minuten mit ausreichender Präzision und Richtigkeit (beide über 85%) und Sensitivität erlaubte. Durch Säulenschaltung war eine automatisierte Analyse von Blutplasma oder –serum möglich. Störende Matrixbestandteile konnten auf einer Vorsäule ohne vorherige Probenaufbereitung abgetrennt werden. Das kosten- und zeiteffektive Verfahren war eine deutliche Verbesserung für die Bewältigung von Proben im Laboralltag und damit für das TDM von Antidepressiva. Durch Analyse des klinischen Einsatzes von TDM wurden eine Reihe von Anwendungsfehlern identifiziert. Es wurde deshalb versucht, die klinische Anwendung des TDM von Antidepressiva durch die Umstellung von einer weitgehend händischen Dokumentation auf eine elektronische Bearbeitungsweise zu verbessern. Im Rahmen der Arbeit wurde untersucht, welchen Effekt man mit dieser Intervention erzielen konnte. Dazu wurde eine Labor-EDV eingeführt, mit der der Prozess vom Probeneingang bis zur Mitteilung der Messergebnisse auf die Stationen elektronisch erfolgte und die Anwendung von TDM vor und nach der Umstellung untersucht. Die Umstellung fand bei den behandelnden Ärzten gute Akzeptanz. Die Labor-EDV erlaubte eine kumulative Befundabfrage und eine Darstellung des Behandlungsverlaufs jedes einzelnen Patienten inklusive vorhergehender Klinikaufenthalte. Auf die Qualität der Anwendung von TDM hatte die Implementierung des Systems jedoch nur einen geringen Einfluss. Viele Anforderungen waren vor und nach der Einführung der EDV unverändert fehlerhaft, z.B. wurden häufig Messungen vor Erreichen des Steady State angefordert. Die Geschwindigkeit der Bearbeitung der Proben war im Vergleich zur vorher händischen Ausführung unverändert, ebenso die Qualität der Analysen bezüglich Richtigkeit und Präzision. Ausgesprochene Empfehlungen hinsichtlich der Dosierungsstrategie der angeforderten Substanzen wurden häufig nicht beachtet. Verkürzt wurde allerdings die mittlere Latenz, mit der eine Dosisanpassung nach Mitteilung des Laborbefundes erfolgte. Insgesamt ist es mit dieser Arbeit gelungen, einen Beitrag zur Verbesserung des Therapeutischen Drug Monitoring von Antidepressiva zu liefern. In der klinischen Anwendung sind allerdings Interventionen notwendig, um Anwendungsfehler beim TDM von Antidepressiva zu minimieren.

OH- und HO 2-Radikale über dem tropischen Regenwald

Beständig werden Spurenstoffe in die Atmosphäre emittiert, die ihren Ursprung in biogenen oder anthropogenen Quellen haben. Daß es dennoch im allgemeinen nicht zu einer Anreicherung bis hin zu toxischen Konzentrationen kommt, liegt an dem Vermögen der Atmosphäre sich durch Oxidationsprozesse selbst zu reinigen. Eine wichtige Aufgabe kommt dabei dem Hydroxylradikal OH zu, welches tagsüber die Oxidationskapazität der Atmosphäre bestimmt. Hierbei spielen die tropischen Regionen mit einer der höchsten OH-Produktionsraten eine zentrale Rolle. Gleichzeitig sind die tropischen Regenwälder eine bedeutende globale Quelle für Kohlenwasserstoffe, die durch Reaktion mit OH-Radikalen dessen Konzentration und damit die Oxidationskapazität der Atmosphäre herabsetzen. Während der GABRIEL-Meßkampagne 2005 im äquatorialen Südamerika wurde der Einfluß der Regenwaldemissionen auf das HOx-Budget (HOx = OH+HO2) untersucht. Zu diesem Zweck wurde das Radikalmeßinstrument HORUS entwickelt. Im Rahmen dieser Arbeit wurden unterschiedliche Komponenten des Gerätes optimiert, der Meßaufbau ins Flugzeug integriert und Methoden zur Kalibrierung entwickelt. Bei der internationalen Vergleichskampagne HOxComp2005 zeigte HORUS seine Eignung zur Messung von troposphärischen OH- und HO2-Radikalen.rnrnDie durchgeführten HOx-Messungen während der GABRIEL-Meßkampagne sind die ersten ihrer Art, die über einem tropischen Regenwald stattgefunden haben. Im Gegensatz zu den Vorhersagen globaler Modelle wurden unerwartet hohe OH- und HO2-Konzentrationen in der planetaren Grenzschicht des tropischen Regenwalds beobachtet. Der Vergleich der berechneten OH-Produktions- und Verlustraten, die aus dem umfangreichen Datensatz von GABRIEL ermittelt wurden, zeigte, daß hierbei eine wichtige OH-Quelle unberücksichtigt blieb. Mit Hilfe des Boxmodells MECCA, in welchem die gemessenen Daten als Randbedingungen in die Simulationen eingingen, wurden die modellierten OH- und HO2- Konzentrationen im Gleichgewichtszustand den beobachteten Konzentrationen gegenübergestellt. Luftmassen der freien Troposphäre und der maritimen Grenzschicht zeigten eine gute Übereinstimmung zwischen Messung und Modell. Über dem tropischen Regenwald jedoch wurden die beobachteten HOx-Konzentrationen in der planetaren Grenzschicht durch das Modell, vor allem am Nachmittag, signifikant unterschätzt. Dabei lag die Diskrepanz zwischen den beobachteten und simulierten Konzentrationen bei einem mittleren Wert von OHobs/OHmod = 12.2 ± 3.5 und HO2obs/HO2mod = 4.1 ± 1.4. Die Abweichung zwischen Messung und Modell korrelieren hierbei mit der Isoprenkonzentration. Während für niedrige Isoprenmischungsverhältnisse, wie sie über dem Ozean oder in Höhen > 3 km vorherrschten, die Beobachtungen mit den Simulationen innerhalb eines Faktors 1.6±0.7 übereinstimmten, nahm die Unterschätzung durch das Modell für steigende Isoprenmischungsverhältnisse > 200 pptV über dem tropischen Regenwald zu.rnrnDer kondensierte chemische Mechanismus von MECCA wurde mit der ausführlichen Isoprenchemie des ”Master Chemical Mechanism“ überprüft, welches vergleichbare HOx-Konzentrationen lieferte. OH-Simulationen, durchgeführt mit der gemessenen HO2-Konzentration als zusätzliche Randbedingung, zeigten, daß die Konversion zwischen HO2 und OH innerhalb des Modells nicht ausreichend ist. Durch Vernachlässigung der gesamten Isoprenchemie konnte dagegen eine Übereinstimmung zwischen Modell und Messung erreicht werden. Eine OH-Quelle in der gleichen Größenordnung wie die OH-Senke durch Isopren, ist somit zur Beschreibung der beobachteten OH-Konzentration notwendig. Reaktionsmechanismen, die innerhalb der Isoprenchemie die gleiche Anzahl an OH-Radikalen erzeugen wie sie verbrauchen, könnten eine mögliche Ursache sein. Unterschiedliche zusätzliche Reaktionen wurden in die Isoprenabbaumechanismen des Modells implementiert, die zur Erhöhung der OH-Quellstärke führen sollten. Diese bewirkten eine Zunahme der simulierten HO2-Konzentrationen um einen maximalen Faktor von 5 für OH und 2 für HO2. Es wird eine OH-Zyklierungswahrscheinlichkeit r von bis zu 94% gefordert, wie sie für die GABRIEL-Messungen erreicht wurde. Die geringe OH-Zyklierungswahrscheinlichkeit von 38% des Modells zeigte, daß wichtige Zyklierungsvorgänge im chemischen Mechanismus bislang nicht berücksichtigt werden. Zusätzliche Zyklierungsreaktionen innerhalb des Isoprenmechanismus, die auch unter niedrigen NO-Konzentrationen zur Rückbildung von OHRadikalen führen, könnten eine Erklärung für die über dem Regenwald beobachteten hohen OH-Konzentration liefern.rn

Development of an LC-MS/MS method for the quantitation of 55 compounds prescribed in combined cardiovascular therapy

This paper reports an LC-MS/MS method with positive electrospray ionization for the screening of commonly prescribed cardiovascular drugs in human plasma, including compounds with antihypertensive (57), antidiabetic (12), hypolipemiant (5), anticoagulant (2) and platelet anti-aggregation (2) effects. Sample treatment consisted of a simple protein precipitation with MeOH/0.1 M ZnSO₄ (4:1, v/v) solution after the addition of internal standard, followed by evaporation and reconstitution. Analytes separation was performed on a Polar-RP column (150 m x 2 mm, 4 μm) using a gradient elution of 15 min. The MS system was operated in MRM mode, monitoring one quantitation and one confirmation transition for each analyte. The recovery of the protein precipitation step ranged from 50 to 70% for most of the compounds, while some were considerably affected by matrix effects. Since several analytes fulfilled the linearity, accuracy and precision values required by the ICH guidelines, the method proved to be suitable for their quantitative analysis. The limits of quantitation varied from 0.38 to 9.1 μg/L and the limits of detection from 0.12 to 5.34 μg/L. The method showed to be suitable for the detection of plasma samples of patients under cardiovascular treatment with the studied drugs, and for 55 compounds reliable quantitative results could be obtained.

Highly accurate isotope composition measurements by a miniature laser ablation mass spectrometer designed for in situ investigations on planetary surface

An experimental procedure for precise and accurate measurements of isotope abundances by a miniature laser ablation mass spectrometer for space research is described. The measurements were conducted on different untreated NIST standards and galena samples by applying pulsed UV laser radiation (266 nm, 3 ns and 20 Hz) for ablation, atomisation, and ionisation of the sample material. Mass spectra of released ions are measured by a reflectron-type time-of-flight mass analyser. A computer controlled performance optimiser was used to operate the system at maximum ion transmission and mass resolution. At optimal experimental conditions, the best relative accuracy and precision achieved for Pb isotope compositions are at the per mill level and were obtained in a range of applied laser irradiances and a defined number of accumulated spectra. A similar relative accuracy and precision was achieved in the study of Pb isotope compositions in terrestrial galena samples. The results for the galena samples are similar to those obtained with a thermal ionisation mass spectrometer (TIMS). The studies of the isotope composition of other elements yielded relative accuracy and precision at the per mill level too, with characteristic instrument parameters for each element. The relative accuracy and precision of the measurements is degrading with lower element/isotope concentration in a sample. For the elements with abundances below 100 ppm these values drop to the percent level. Depending on the isotopic abundances of Pb in minerals, 207Pb/206Pb ages with accuracy in the range of tens of millions of years can be achieved.

High-Resolution Chemical Depth Profiling of Solid Material Using a Miniature Laser Ablation/Ionization Mass Spectrometer

High-resolution chemical depth profiling measurements of copper films are presented. The 10 μm thick copper test samples were electrodeposited on a Si-supported Cu seed under galvanostatic conditions in the presence of particular plating additives (SPS, Imep, PEI, and PAG) used in the semiconductor industry for the on-chip metallization of interconnects. To probe the trend of these plating additives toward inclusion into the deposit upon growth, quantitative elemental mass spectrometric measurements at trace level concentration were conducted by using a sensitive miniature laser ablation ionization mass spectrometer (LIMS), originally designed and developed for in situ space exploration. An ultrashort pulsed laser system (τ ∼ 190 fs, λ = 775 nm) was used for ablation and ionization of sample material. We show that with our LIMS system, quantitative chemical mass spectrometric analysis with an ablation rate at the subnanometer level per single laser shot can be conducted. The measurement capabilities of our instrument, including the high vertical depth resolution coupled with high detection sensitivity of ∼10 ppb, high dynamic range ≥10(8), measurement accuracy and precision, is of considerable interest in various fields of application, where investigations with high lateral and vertical resolution of the chemical composition of solid materials are required, these include, e.g., wafers from semiconductor industry or studies on space weathered samples in space research.

Validation of an enzyme-linked immunosorbent assay (ELISA) for the measurement of canine S100A12.

BACKGROUND Canine S100 calcium-binding protein A12 (cS100A12) shows promise as biomarker of inflammation in dogs. A previously developed cS100A12-radioimmunoassay (RIA) requires radioactive tracers and is not sensitive enough for fecal cS100A12 concentrations in 79% of tested healthy dogs. An ELISA assay may be more sensitive than RIA and does not require radioactive tracers. OBJECTIVE The purpose of the study was to establish a sandwich ELISA for serum and fecal cS100A12, and to establish reference intervals (RI) for normal healthy canine serum and feces. METHODS Polyclonal rabbit anti-cS100A12 antibodies were generated and tested by Western blotting and immunohistochemistry. A sandwich ELISA was developed and validated, including accuracy and precision, and agreement with cS100A12-RIA. The RI, stability, and biologic variation in fecal cS100A12, and the effect of corticosteroids on serum cS100A12 were evaluated. RESULTS Lower detection limits were 5 μg/L (serum) and 1 ng/g (fecal), respectively. Intra- and inter-assay coefficients of variation were ≤ 4.4% and ≤ 10.9%, respectively. Observed-to-expected ratios for linearity and spiking recovery were 98.2 ± 9.8% (mean ± SD) and 93.0 ± 6.1%, respectively. There was a significant bias between the ELISA and the RIA. The RI was 49-320 μg/L for serum and 2-484 ng/g for fecal cS100A12. Fecal cS100A12 was stable for 7 days at 23, 4, -20, and -80°C; biologic variation was negligible but variation within one fecal sample was significant. Corticosteroid treatment had no clinically significant effect on serum cS100A12 concentrations. CONCLUSIONS The cS100A12-ELISA is a precise and accurate assay for serum and fecal cS100A12 in dogs.

Assessment of the performance of 3m 3500 organic vapor monitors over extended sampling durations

The purpose of this study was to assess the accuracy and precision of airborne volatile organic compound (VOC) concentrations measured using passive air samplers (3M 3500 organic vapor monitors) over extended sampling durations (9 and 15 days). A total of forty-five organic vapor monitor samples were collected at a State of Texas air monitoring site during two different sampling periods (July/August and November 2008). The results of this study indicate that for most of the tested compounds, there was no significant difference between long-term (9 or 15 days) sample concentrations and the means of parallel consecutive short-term (3 days) sample concentrations. Biases of 9 or 15-day measurements vs. consecutive 3-day measurements showed considerable variability. Those compounds that had percent bias values of <10% are suggested as acceptable for long-term sampling (9 and 15 days). Of the twenty-one compounds examined, 10 compounds are classified as acceptable for long-term sampling; these include m,p-xylene, 1,2,4-trimethylbenzene, n-hexane, ethylbenzene, benzene, toluene, o-xylene, d-limonene, dimethylpentane and methyl tertbutyl ether. The ratio of sampling procedure variability relative to variability within days was approximately 1.89 for both sampling periods for the 3-day vs. 9-day comparisons and approximately 2.19 for both sampling periods for the 3-day vs. 15-day comparisons. Considerably higher concentrations of most VOCs were measured during the November sampling period compared to the July/August period. These differences may be a result of varying meteorological conditions during these two time periods, e.g., the differences in wind direction, and wind speed. Further studies are suggested to further evaluate the accuracy and precision of 3M 3500 organic vapor monitors over extended sampling durations. ^

Rare earth elements determined in Antarctic ice by inductively coupled plasma

Inductively coupled plasma mass spectrometry (ICP-MS) is a suitable tool for multi-element analysis at low concentration levels. Rare earth element (REE) determinations in standard reference materials and small volumes of molten ice core samples from Antarctica have been performed with an ICP-time of flight-MS (ICP-TOF-MS) system. Recovery rates for REE in e.g. SPS-SW1 amounted to not, vert, similar ~103%, and the relative standard deviations were 3.4% for replicate analysis at REE concentrations in the lower ng/l range. Analyses of REE concentrations in Antarctic ice core samples showed that the ICP-TOF-MS technique meets the demands of restricted sample mass. The data obtained are in good agreement with ICP-Quadrupole-MS (ICP-Q-MS) and ICP-Sector Field-MS (ICP-SF-MS) results. The ICP-TOF-MS system determines accurately and precisely REE concentrations exceeding 5 ng/l while between 0.5 and 5 ng/l accuracy and precision are element dependent.

Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra

Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100 000 Milky Way stars using the FLAMES spectrograph at the VLT, down to V = 19 mag, systematically covering all the main components of the Milky Way and providing the first homogeneous overview of the distributions of kinematics and chemical element abundances in the Galaxy. Observations of young open clusters, in particular, are giving new insights into their initial structure, kinematics, and their subsequent evolution. Aims. This paper describes the analysis of UVES and GIRAFFE spectra acquired in the fields of young clusters whose population includes pre-main sequence (PMS) stars. The analysis is applied to all stars in such fields, regardless of any prior information on membership, and provides fundamental stellar atmospheric parameters, elemental abundances, and PMS-specific parameters such as veiling, accretion, and chromospheric activity. Methods. When feasible, different methods were used to derive raw parameters (e.g. line equivalent widths) fundamental atmospheric parameters and derived parameters (e.g. abundances). To derive some of these parameters, we used methods that have been extensively used in the past and new ones developed in the context of the Gaia-ESO survey enterprise. The internal precision of these quantities was estimated by inter-comparing the results obtained by these different methods, while the accuracy was estimated by comparison with independent external data, such as effective temperature and surface gravity derived from angular diameter measurements, on a sample of benchmarks stars. A validation procedure based on these comparisons was applied to discard spurious or doubtful results and produce recommended parameters. Specific strategies were implemented to resolve problems of fast rotation, accretion signatures, chromospheric activity, and veiling. Results. The analysis carried out on spectra acquired in young cluster fields during the first 18 months of observations, up to June 2013, is presented in preparation of the first release of advanced data products. These include targets in the fields of the ρ Oph, Cha I, NGC 2264, γ Vel, and NGC 2547 clusters. Stellar parameters obtained with the higher resolution and larger wavelength coverage from UVES are reproduced with comparable accuracy and precision using the smaller wavelength range and lower resolution of the GIRAFFE setup adopted for young stars, which allows us to provide stellar parameters with confidence for the much larger GIRAFFE sample. Precisions are estimated to be ≈120 K rms in Teff, ≈0.3 dex rms in log g, and ≈0.15 dex rms in [Fe/H] for the UVES and GIRAFFE setups.

Use of the EM algorithm to detect QTL affecting multiple-traits in an across half-sib family analysis

QTL detection experiments in livestock species commonly use the half-sib design. Each male is mated to a number of females, each female producing a limited number of progeny. Analysis consists of attempting to detect associations between phenotype and genotype measured on the progeny. When family sizes are limiting experimenters may wish to incorporate as much information as possible into a single analysis. However, combining information across sires is problematic because of incomplete linkage disequilibrium between the markers and the QTL in the population. This study describes formulae for obtaining MLEs via the expectation maximization (EM) algorithm for use in a multiple-trait, multiple-family analysis. A model specifying a QTL with only two alleles, and a common within sire error variance is assumed. Compared to single-family analyses, power can be improved up to fourfold with multi-family analyses. The accuracy and precision of QTL location estimates are also substantially improved. With small family sizes, the multi-family, multi-trait analyses reduce substantially, but not totally remove, biases in QTL effect estimates. In situations where multiple QTL alleles are segregating the multi-family analysis will average out the effects of the different QTL alleles.

Estimating nutrient intake in comparative studies of animals: an example using dietary carotenoid content in birds

Many different methods of reporting animal diets have been used in ecological research. These vary greatly in level of accuracy and precision and therefore complicate attempts to measure and compare diets, and quantitites of nutrients in those diets, across a wide range of taxa. For most birds, the carotenoid content of the diet has not been directly measured. Here, therefore, I use an avian example to show how different methods of measuring the quantities of various foods in the diet affect the relative rankings of higher taxa (families, subfamilies, and tribes), and species within these taxa, with regard to the carotenoid contents of their diets. This is a timely example, as much recent avian literature has focused on the way dietary carotenoids may be traded off among aspects of survival, fitness and signalling. I assessed the mean dietary carotenoid contents of representatives of thirty higher taxa of birds using four different carotenoid intake indices varying in precision, including trophic levels, a coarse-scale and a fine-scale categorical index, and quantitative estimates of dietary carotenoids. This last method was used as the benchmark. For comparisons among taxa, all but the trophic level index were significantly correlated with each other. However, for comparisons of species within taxa, the fine-scale index outperformed the coarse-scale index, which in turn outperformed the trophic level index. In addition, each method has advantages and disadvantages, as well as underlying assumptions that must be considered. Examination and comparison of several possible methods of diet assessment appears to highlight these so that the best possible index is used given available data, and it is recommended that such a step be taken prior to the inclusion of estimated nutrient intake in any statistical analysis. Although applied to avian carotenoids here, this method could readily be applied to other taxa and types of nutrients.