24 resultados para Alexander I, Pope, d. 115 or 6.
Resumo:
We report the first in situ measurements of neutral deuterium originating in the local interstellar medium (LISM) in Earth’s orbit. These measurements were performed with the IBEX-Lo camera on NASA’s interstellar boundary explorer (IBEX) satellite. All data from the spring observation periods of 2009 through 2011 have been analysed. In the three years of the IBEX mission time, the observation geometry and orbit allowed for a total observation time of 115.3 days for the LISM. However, the effects of the spinning spacecraft and the stepping through 8 energy channels mean that we are only observing the interstellar wind for a total time of 1.44 days, in which 2 counts for interstellar deuterium were collected. We report here a conservative number, because a possibility of systematic error or additional noise, though eliminated in our analysis to the best of our knowledge, only supports detection at a 1-sigma level. From these observations, we derive a ratio D/H = (5.8 ± 4.4) × 10-4 at 1 AU. After modelling the transport and loss of D and H from the termination shock to Earth’s orbit, we find that our result of D/HLISM = (1.6 ± 1.2) × 10-5 agrees with D/HLIC = (1.6 ± 0.4) × 10-5 for the local interstellar cloud. This weak interstellar signal is extracted from a strong terrestrial background signal consisting of sputter products from the sensor’s conversion surface. As reference, we accurately measure the terrestrial D/H ratio in these sputtered products and then discriminate this terrestrial background source. Because of the diminishing D and H signal at Earth’s orbit during the rising solar activity due to photoionisation losses and increased photon pressure, our result demonstrates that in situ measurements of interstellar deuterium in the inner heliosphere are only possible during solar minimum conditions.
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The awakening of national consciousness went hand in hand in Bohemia with an anxiety about national disappearance. In this context, the recourse to Pan-Slavism was for the Czechs a way to encourage themselves through the idea of belonging to a great Slavic world, while the Slavic Congress organized in Prague in 1848 was an attempt to realize this ideal. The Congress was a failure from the political point of view, but it did have some socio-cultural repercussions: notably, it served as a pretext for the advancement of women's issues in Bohemia. It is indeed in the wake of the Congress that Honorata z Wiśniowskich Zapová, a Polish women settled in Prague after her marriage to a Czech intellectual, founded, under the guise of collaboration between all Slavic women, the first women's association, as well as a (very short-lived) Czech-Polish institute, where Czech, as well as Polish girls, could get a quality education in their mother tongue. Honorata was undoubtedly the source of the polonophilia wind that seemed to blow over the Czech emancipation movement in the second half of the nineteenth century. In particular, Karolina Světlá showed in her Memoirs a great recognition for Honorata's efforts in matters of emancipation and education, and explicitly took up the challenge launched by the latter in founding another women's association and in inaugurating a school for underprivileged girls. But the tribute Světlá paid to Honorata is even more evident in her literary work, where Poland and the Polish woman (who often wears Honorata's features) play a significant role (see for example her short novel Sisters or her story A Few Days in the Life of a Prague Dandy). Světlá was probably the Czech feminist writer who, in her activities and in her work, relied most strongly on the Polish woman as a model for the Czech woman. However, she wasn't alone. In general, it was a characteristic of the Czech feminist movement of the second half of the nineteenth century to have recourse to the Polish woman and to Poland as a landmark for comparison and as a goal to be achieved.
Resumo:
1944/1945 wurde in Cham-Hagendorn eine Wassermühle ausgegraben, die dank ihrer aussergewöhnlich guten Holzerhaltung seit langem einen prominenten Platz in der Forschung einnimmt. 2003 und 2004 konnte die Kantonsarchäologie Zug den Platz erneut archäologisch untersuchen. Dabei wurden nicht nur weitere Reste der Wassermühle, sondern auch Spuren älterer und jüngerer Anlagen geborgen: eine ältere und eine jüngere Schmiedewerkstatt (Horizont 1a/Horizont 3) sowie ein zweiphasiges Heiligtum (Horizonte 1a/1b). All diese Anlagen lassen sich nun in das in den neuen Grabungen erkannte stratigraphische Gerüst einhängen (s. Beil. 2). Dank der Holzerhaltung können die meisten Phasen dendrochronologisch datiert werden (s. Abb. 4.1/1a): Horizont 1a mit Schlagdaten zwischen 162(?)/173 und 200 n. Chr., Horizont 1b um 215/218 n. Chr. und Horizont 2 um 231 n. Chr. Ferner konnten in den neuen Grabungen Proben für mikromorphologische und archäobotanische Untersuchungen entnommen werden (Kap. 2.2; 3.11). In der vorliegenden Publikation werden der Befund und die Baustrukturen vorgelegt, (Kap. 2), desgleichen sämtliche stratifizierten Funde und eine umfassende Auswahl der 1944/1945 geborgenen Funde (Kap. 3). Dank anpassender Fragmente, sog. Passscherben, lassen sich diese zum Teil nachträglich in die Schichtenabfolge einbinden. Die mikromorphologischen und die archäobotanischen Untersuchungen (Kap. 2.2; 3.11) zeigen, dass der Fundplatz in römischer Zeit inmitten einer stark vom Wald und dem Fluss Lorze geprägten Landschaft lag. In unmittelbarer Nähe können weder eine Siedlung noch einzelne Wohnbauten gelegen haben. Die demnach nur gewerblich und sakral genutzten Anlagen standen an einem Bach, der vermutlich mit jenem Bach identisch ist, der noch heute das Groppenmoos entwässert und bei Cham-Hagendorn in die Lorze mündet (s. Abb. 2.4/1). Der antike Bach führte wiederholt Hochwasser ─ insgesamt sind fünf grössere Überschwemmungsphasen auszumachen (Kap. 2.2; 2.4). Wohl anlässlich eines Seehochstandes durch ein Überschwappen der Lorze in den Bach ausgelöst, müssen diese Überschwemmungen eine enorme Gewalt entwickelt haben, der die einzelnen Anlagen zum Opfer fielen. Wie die Untersuchung der Siedlungslandschaft römischer Zeit rund um den Zugersee wahrscheinlich macht (Kap. 6 mit Abb. 6.2/2), drften die Anlagen von Cham-Hagendorn zu einer in Cham-Heiligkreuz vermuteten Villa gehören, einem von fünf grösseren Landgütern in diesem Gebiet. Hinweise auf Vorgängeranlagen fehlen, mit denen die vereinzelten Funde des 1. Jh. n. Chr. (Kap. 4.5) in Verbindung gebracht werden könnten. Diese drften eher von einer der Überschwemmungen bachaufwärts weggerissen und nach Cham-Hagendorn eingeschwemmt worden sein. Die Nutzung des Fundplatzes (Horizont 1a; s. Beil. 6) setzte um 170 n. Chr. mit einer Schmiedewerkstatt ein (Kap. 2.5.1). Der Fundanfall, insbesondere die Schmiedeschlacken (Kap. 3.9) belegen, dass hier nur hin und wieder Geräte hergestellt und repariert wurden (Kap. 5.2). Diese Werkstatt war vermutlich schon aufgelassen und dem Verfall preisgegeben, als man 200 n. Chr. (Kap. 4.2.4) auf einer Insel zwischen dem Bach und einem Lorzearm ein Heiligtum errichtete (Kap. 5.3). Beleg für den sakralen Status dieser Insel ist in erster Linie mindestens ein eigens gepflanzter Pfirsichbaum, nachgewiesen mit Pollen, einem Holz und über 400 Pfirsichsteinen (Kap. 3.11). Die im Bach verlaufende Grenze zwischen dem sakralen Platz und der profanen Umgebung markierte man zusätzlich mit einer Pfahlreihe (Kap. 2.5.3). In diese war ein schmaler Langbau integriert (Kap. 2.5.2), der an die oft an Temenosmauern antiker Heiligtümer angebauten Portiken erinnert und wohl auch die gleiche Funktion wie diese gehabt hatte, nämlich das Aufbewahren von Weihegaben und Kultgerät (Kap. 5.3). Das reiche Fundmaterial, das sich in den Schichten der ersten Überschwemmung fand (s. Abb. 5./5), die um 205/210 n. Chr. dieses Heiligtum zerstört hatte, insbesondere die zahlreiche Keramik (Kap. 3.2.4), und die zum Teil auffallend wertvollen Kleinfunde (Kap. 3.3.3), drften zum grössten Teil einst in diesem Langbau untergebracht gewesen sein. Ein als Glockenklöppel interpretiertes, stratifiziertes Objekt spricht dafür, dass die fünf grossen, 1944/1945 als Stapel aufgefundenen Eisenglocken vielleicht auch dem Heiligtum zuzuweisen sind (Kap. 3.4). In diesen Kontext passen zudem die überdurchschnittlich häufig kalzinierten Tierknochen (Kap. 3.10). Nach der Überschwemmung befestigte man für 215 n. Chr. (Kap. 4.2.4) das unterspülte Bachufer mit einer Uferverbauung (Kap. 2.6.1). Mit dem Bau eines weiteren, im Bach stehenden Langbaus (Kap. 2.6.2) stellte man 218 n. Chr. das Heiligtum auf der Insel in ähnlicher Form wieder her (Horizont 1b; s. Beil. 7). Von der Pfahlreihe, die wiederum die sakrale Insel von der profanen Umgebung abgrenzte, blieben indes nur wenige Pfähle erhalten. Dennoch ist der sakrale Charakter der Anlage gesichert. Ausser dem immer noch blühenden Pfirsichbaum ist es ein vor dem Langbau aufgestelltes Ensemble von mindestens 23 Terrakottafigurinen (s. Abb. 3.6/1), elf Veneres, zehn Matres, einem Jugendlichen in Kapuzenmantel und einem kindlichen Risus (Kap. 3.6; s. auch Kap. 2.6.3). In den Sedimenten der zweiten Überschwemmung, der diese Anlage um 225/230 n. Chr. zum Opfer gefallen war, fanden sich wiederum zahlreiche Keramikgefässe (Kap. 3.2.4) und zum Teil wertvolle Kleinfunde wie eine Glasperle mit Goldfolie (Kap. 3.8.2) und eine Fibel aus Silber (Kap. 3.3.3), die wohl ursprünglich im Langbau untergebracht waren (Kap. 5.3.2 mit Abb. 5/7). Weitere Funde mit sicherem oder möglichem sakralem Charakter finden sich unter den 1944/1945 geborgenen Funden (s. Abb. 5/8), etwa ein silberner Fingerring mit Merkurinschrift, ein silberner Lunula-Anhänger, eine silberne Kasserolle (Kap. 3.3.3), eine Glasflasche mit Schlangenfadenauflage (Kap. 3.8.2) und einige Bergkristalle (Kap. 3.8.4). Im Bereich der Terrakotten kamen ferner mehrere Münzen (Kap. 3.7) zum Vorschein, die vielleicht dort niedergelegt worden waren. Nach der zweiten Überschwemmung errichtete man um 231 n. Chr. am Bach eine Wassermühle (Horizont 2; Kap. 2.7; Beil. 8; Abb. 2.7/49). Ob das Heiligtum auf der Insel wieder aufgebaut oder aufgelassen wurde, muss mangels Hinweisen offen bleiben. Für den abgehobenen Zuflusskanal der Wassermühle verwendete man mehrere stehen gebliebene Pfähle der vorangegangenen Anlagen der Horizonte 1a und 1b. Obwohl die Wassermühle den 28 jährlichen Überschwemmungshorizonten (Kap. 2.2) und den Funden (Kap. 4.3.2; 4.4.4; 45) zufolge nur bis um 260 n. Chr., während gut einer Generation, bestand, musste sie mindestens zweimal erneuert werden – nachgewiesen sind drei Wasserräder, drei Mühlsteinpaare und vermutlich drei Podeste, auf denen jeweils das Mahlwerk ruhte. Grund für diese Umbauten war wohl der weiche, instabile Untergrund, der zu Verschiebungen geführt hatte, so dass das Zusammenspiel von Wellbaum bzw. Sternnabe und Übersetzungsrad nicht mehr funktionierte und das ganze System zerbrach. Die Analyse von Pollen aus dem Gehhorizont hat als Mahlgut Getreide vom Weizentyp nachgewiesen (Kap. 3.11.4). Das Abzeichen eines Benefiziariers (Kap. 3.3.2 mit Abb. 3.3/23,B71) könnte dafür sprechen, dass das verarbeitete Getreide zumindest zum Teil für das römische Militär bestimmt war (s. auch Kap. 6.2.3). Ein im Horizont 2 gefundener Schreibgriffel und weitere stili sowie eine Waage für das Wägen bis zu 35-40 kg schweren Waren aus dem Fundbestand von 1944/1945 könnten davon zeugen, dass das Getreide zu wägen und zu registrieren war (Kap. 3.4.2). Kurz nach 260 n. Chr. fiel die Wassermühle einem weiteren Hochwasser zum Opfer. Für den folgenden Horizont 3 (Beil. 9) brachte man einen Kiesboden ein und errichtete ein kleines Gebäude (Kap. 2.8). Hier war wohl wiederum eine Schmiede untergebracht, wie die zahlreichen Kalottenschlacken belegen (Kap. 3.9), die im Umfeld der kleinen Baus zum Vorschein kamen. Aufgrund der Funde (Kap. 4.4.4; 4.5) kann diese Werkstatt nur kurze Zeit bestanden haben, höchstens bis um 270 n. Chr., bevor sie einem weiteren Hochwasser zum Opfer fiel. Von der jüngsten Anlage, die wohl noch in römische Zeit datiert (Horizont 4; Beil. 10), war lediglich eine Konstruktion aus grossen Steinplatten zu fassen (Kap. 2.9.1). Wozu sie diente, muss offen bleiben. Auch der geringe Fundanfall spricht dafür, dass die Nutzung des Platzes, zumindest für die römische Zeit, allmählich ein Ende fand (Kap. 4.5). Zu den jüngsten Strukturen gehören mehrere Gruben (Kap. 2.9.2), die vielleicht der Lehmentnahme dienten. Mangels Funden bleibt ihre Datierung indes ungewiss. Insbesondere wissen wir nicht, ob sie noch in römische Zeit datieren oder jünger sind. Spätestens mit der fünften Überschwemmung, die zur endgültigen Verlandung führte und wohl schon in die frühe Neuzeit zu setzen ist, wurde der Platz aufgelassen und erst mit dem Bau der bestehenden Fensterfabrik Baumgartner wieder besetzt.
Resumo:
Firn and polar ice cores offer the only direct palaeoatmospheric archive. Analyses of past greenhouse gas concentrations and their isotopic compositions in air bubbles in the ice can help to constrain changes in global biogeochemical cycles in the past. For the analysis of the hydrogen isotopic composition of methane (δD(CH4) or δ2H(CH4)) 0.5 to 1.5 kg of ice was hitherto used. Here we present a method to improve precision and reduce the sample amount for δD(CH4) measurements in (ice core) air. Pre-concentrated methane is focused in front of a high temperature oven (pre-pyrolysis trapping), and molecular hydrogen formed by pyrolysis is trapped afterwards (post-pyrolysis trapping), both on a carbon-PLOT capillary at −196 °C. Argon, oxygen, nitrogen, carbon monoxide, unpyrolysed methane and krypton are trapped together with H2 and must be separated using a second short, cooled chromatographic column to ensure accurate results. Pre- and post-pyrolysis trapping largely removes the isotopic fractionation induced during chromatographic separation and results in a narrow peak in the mass spectrometer. Air standards can be measured with a precision better than 1‰. For polar ice samples from glacial periods, we estimate a precision of 2.3‰ for 350 g of ice (or roughly 30 mL – at standard temperature and pressure (STP) – of air) with 350 ppb of methane. This corresponds to recent tropospheric air samples (about 1900 ppb CH4) of about 6 mL (STP) or about 500 pmol of pure CH4.
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A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context and by addressing the suitability of planets for the presence of life. EChO—the Exoplanet Characterisation Observatory—is a mission concept specifically geared for this purpose. EChO will provide simultaneous, multi-wavelength spectroscopic observations on a stable platform that will allow very long exposures. The use of passive cooling, few moving parts and well established technology gives a low-risk and potentially long-lived mission. EChO will build on observations by Hubble, Spitzer and ground-based telescopes, which discovered the first molecules and atoms in exoplanetary atmospheres. However, EChO’s configuration and specifications are designed to study a number of systems in a consistent manner that will eliminate the ambiguities affecting prior observations. EChO will simultaneously observe a broad enough spectral region—from the visible to the mid-infraredto constrain from one single spectrum the temperature structure of the atmosphere, the abundances of the major carbon and oxygen bearing species, the expected photochemically-produced species and magnetospheric signatures. The spectral range and resolution are tailored to separate bands belonging to up to 30 molecules and retrieve the composition and temperature structure of planetary atmospheres. The target list for EChO includes planets ranging from Jupiter-sized with equilibrium temperatures T eq up to 2,000 K, to those of a few Earth masses, with T eq \u223c 300 K. The list will include planets with no Solar System analog, such as the recently discovered planets GJ1214b, whose density lies between that of terrestrial and gaseous planets, or the rocky-iron planet 55 Cnc e, with day-side temperature close to 3,000 K. As the number of detected exoplanets is growing rapidly each year, and the mass and radius of those detected steadily decreases, the target list will be constantly adjusted to include the most interesting systems. We have baselined a dispersive spectrograph design covering continuously the 0.4–16 μm spectral range in 6 channels (1 in the visible, 5 in the InfraRed), which allows the spectral resolution to be adapted from several tens to several hundreds, depending on the target brightness. The instrument will be mounted behind a 1.5 m class telescope, passively cooled to 50 K, with the instrument structure and optics passively cooled to \u223c45 K. EChO will be placed in a grand halo orbit around L2. This orbit, in combination with an optimised thermal shield design, provides a highly stable thermal environment and a high degree of visibility of the sky to observe repeatedly several tens of targets over the year. Both the baseline and alternative designs have been evaluated and no critical items with Technology Readiness Level (TRL) less than 4–5 have been identified. We have also undertaken a first-order cost and development plan analysis and find that EChO is easily compatible with the ESA M-class mission framework.
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OBJECTIVE To evaluate the effectiveness of 200 mg of daily vaginal natural progesterone to prevent preterm birth in women with preterm labour. DESIGN Multicentre, randomised, double-blind, placebo-controlled trial. SETTING Twenty-nine centres in Switzerland and Argentina. POPULATION A total of 385 women with preterm labour (24(0/7) to 33(6/7) weeks of gestation) treated with acute tocolysis. METHODS Participants were randomly allocated to either 200 mg daily of self-administered vaginal progesterone or placebo within 48 hours of starting acute tocolysis. MAIN OUTCOME MEASURES Primary outcome was delivery before 37 weeks of gestation. Secondary outcomes were delivery before 32 and 34 weeks, adverse effects, duration of tocolysis, re-admissions for preterm labour, length of hospital stay, and neonatal morbidity and mortality. The study was ended prematurely based on results of the intermediate analysis. RESULTS Preterm birth occurred in 42.5% of women in the progesterone group versus 35.5% in the placebo group (relative risk [RR] 1.2; 95% confidence interval [95% CI] 0.93-1.5). Delivery at <32 and <34 weeks did not differ between the two groups (12.9 versus 9.7%; [RR 1.3; 95% CI 0.7-2.5] and 19.7 versus 12.9% [RR 1.5; 95% CI 0.9-2.4], respectively). The duration of tocolysis, hospitalisation, and recurrence of preterm labour were comparable between groups. Neonatal morbidity occurred in 44 (22.8%) cases on progesterone versus 35 (18.8%) cases on placebo (RR: 1.2; 95% CI 0.82-1.8), whereas there were 4 (2%) neonatal deaths in each study group. CONCLUSION There is no evidence that the daily administration of 200 mg vaginal progesterone decreases preterm birth or improves neonatal outcome in women with preterm labour.
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OBJECTIVE Vitamin D (D) status is reported to correlate negatively with insulin production and insulin sensitivity in patients with type 2 diabetes mellitus (T2DM). However, few placebo-controlled intervention data are available. We aimed to assess the effect of large doses of parenteral D3 on glycosylated haemoglobin (HbA(₁c)) and estimates of insulin action (homeostasis model assessment insulin resistance: HOMA-IR) in patients with stable T2DM. MATERIALS AND METHODS We performed a prospective, randomised, double-blind, placebo-controlled pilot study at a single university care setting in Switzerland. Fifty-five patients of both genders with T2DM of more than 10 years were enrolled and randomised to either 300,000 IU D or placebo, intramuscularly. The primary endpoint was the intergroup difference in HbA(₁c) levels. Secondary endpoints were: changes in insulin sensitivity, albuminuria, calcium/phosphate metabolism, activity of the renin-aldosterone axis and changes in 24-hour ambulatory blood pressure values. RESULTS After 6 months of D supply, there was a significant intergroup difference in the change in HbA(₁c) levels (relative change [mean ± standard deviation] +2.9% ± 1.5% in the D group vs +6.9% ± 2.1% the in placebo group, p = 0.041) as HOMA-IR decreased by 12.8% ± 5.6% in the D group and increased by 10% ± 5.4% in the placebo group (intergroup difference, p = 0.032). Twenty-four-hour urinary albumin excretion decreased in the D group from 200 ± 41 to 126 ± 39, p = 0.021). There was no significant intergroup difference for the other secondary endpoints. CONCLUSIONS D improved insulin sensitivity (based on HOMA-IR) and affected the course of HbA(₁c) positively compared with placebo in patients with T2DM.
Resumo:
Compared with the coronary setting, knowledge about antithrombotic therapies after endovascular treatment (EVT) is inadequate in patients with peripheral artery disease (PAD). Based on a review of trials and guidelines, which is summarized in this article, there is scant evidence that antithrombotic drugs improve outcome after peripheral EVT. To address this knowledge gap, the randomized, open-label, multinational edoxaban in patients with Peripheral Artery Disease (ePAD) study (ClinicalTrials.gov identifier NCT01802775) was designed to explore the safety and efficacy of a combined regimen of antiplatelet therapy with clopidogrel and anticoagulation with edoxaban, a selective and direct factor Xa inhibitor, both combined with aspirin. As of July 2014, 203 patients (144 men; mean age 67 years) from 7 countries have been enrolled. These patients have been allocated to once-daily edoxaban [60 mg for 3 months (or 30 mg in the presence of factors associated with increased exposure)] or clopidogrel (75 mg/d for 3 months). All patients received aspirin (100 mg/d) for the 6-month duration of the study. The primary safety endpoint is major or clinically relevant nonmajor bleeding; the primary efficacy endpoint is restenosis or reocclusion at the treated segment(s) measured at 1, 3, and 6 months using duplex ultrasound scanning. All outcomes will be assessed and adjudicated centrally in a masked fashion. The ePAD study is the first of its kind to investigate a combined regimen of antiplatelet therapy and anticoagulation through factor Xa inhibition with edoxaban.
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Introduction: In team sports the ability to use peripheral vision is essential to track a number of players and the ball. By using eye-tracking devices it was found that players either use fixations and saccades to process information on the pitch or use smooth pursuit eye movements (SPEM) to keep track of single objects (Schütz, Braun, & Gegenfurtner, 2011). However, it is assumed that peripheral vision can be used best when the gaze is stable while it is unknown whether motion changes can be equally well detected when SPEM are used especially because contrast sensitivity is reduced during SPEM (Schütz, Delipetkose, Braun, Kerzel, & Gegenfurtner, 2007). Therefore, peripheral motion change detection will be examined by contrasting a fixation condition with a SPEM condition. Methods: 13 participants (7 male, 6 female) were presented with a visual display consisting of 15 white and 1 red square. Participants were instructed to follow the red square with their eyes and press a button as soon as a white square begins to move. White square movements occurred either when the red square was still (fixation condition) or moving in a circular manner with 6 °/s (pursuit condition). The to-be-detected white square movements varied in eccentricity (4 °, 8 °, 16 °) and speed (1 °/s, 2 °/s, 4 °/s) while movement time of white squares was constant at 500 ms. 180 events should be detected in total. A Vicon-integrated eye-tracking system and a button press (1000 Hz) was used to control for eye-movements and measure detection rates and response times. Response times (ms) and missed detections (%) were measured as dependent variables and analysed with a 2 (manipulation) x 3 (eccentricity) x 3 (speed) ANOVA with repeated measures on all factors. Results: Significant response time effects were found for manipulation, F(1,12) = 224.31, p < .01, ηp2 = .95, eccentricity, F(2,24) = 56.43; p < .01, ηp2 = .83, and the interaction between the two factors, F(2,24) = 64.43; p < .01, ηp2 = .84. Response times increased as a function of eccentricity for SPEM only and were overall higher than in the fixation condition. Results further showed missed events effects for manipulation, F(1,12) = 37.14; p < .01, ηp2 = .76, eccentricity, F(2,24) = 44.90; p < .01, ηp2 = .79, the interaction between the two factors, F(2,24) = 39.52; p < .01, ηp2 = .77 and the three-way interaction manipulation x eccentricity x speed, F(2,24) = 3.01; p = .03, ηp2 = .20. While less than 2% of events were missed on average in the fixation condition as well as at 4° and 8° eccentricity in the SPEM condition, missed events increased for SPEM at 16 ° eccentricity with significantly more missed events in the 4 °/s speed condition (1 °/s: M = 34.69, SD = 20.52; 2 °/s: M = 33.34, SD = 19.40; 4 °/s: M = 39.67, SD = 19.40). Discussion: It could be shown that using SPEM impairs the ability to detect peripheral motion changes at the far periphery and that fixations not only help to detect these motion changes but also to respond faster. Due to high temporal constraints especially in team sports like soccer or basketball, fast reaction are necessary for successful anticipation and decision making. Thus, it is advised to anchor gaze at a specific location if peripheral changes (e.g. movements of other players) that require a motor response have to be detected. In contrast, SPEM should only be used if a single object, like the ball in cricket or baseball, is necessary for a successful motor response. References: Schütz, A. C., Braun, D. I., & Gegenfurtner, K. R. (2011). Eye movements and perception: A selective review. Journal of Vision, 11, 1-30. Schütz, A. C., Delipetkose, E., Braun, D. I., Kerzel, D., & Gegenfurtner, K. R. (2007). Temporal contrast sensitivity during smooth pursuit eye movements. Journal of Vision, 7, 1-15.