TY - JOUR A1 - Wech, Tobias A1 - Ankenbrand, Markus Johannes A1 - Bley, Thorsten Alexander A1 - Heidenreich, Julius Frederik T1 - A data-driven semantic segmentation model for direct cardiac functional analysis based on undersampled radial MR cine series JF - Magnetic Resonance in Medicine N2 - Purpose Image acquisition and subsequent manual analysis of cardiac cine MRI is time-consuming. The purpose of this study was to train and evaluate a 3D artificial neural network for semantic segmentation of radially undersampled cardiac MRI to accelerate both scan time and postprocessing. Methods A database of Cartesian short-axis MR images of the heart (148,500 images, 484 examinations) was assembled from an openly accessible database and radial undersampling was simulated. A 3D U-Net architecture was pretrained for segmentation of undersampled spatiotemporal cine MRI. Transfer learning was then performed using samples from a second database, comprising 108 non-Cartesian radial cine series of the midventricular myocardium to optimize the performance for authentic data. The performance was evaluated for different levels of undersampling by the Dice similarity coefficient (DSC) with respect to reference labels, as well as by deriving ventricular volumes and myocardial masses. Results Without transfer learning, the pretrained model performed moderately on true radial data [maximum number of projections tested, P = 196; DSC = 0.87 (left ventricle), DSC = 0.76 (myocardium), and DSC =0.64 (right ventricle)]. After transfer learning with authentic data, the predictions achieved human level even for high undersampling rates (P = 33, DSC = 0.95, 0.87, and 0.93) without significant difference compared with segmentations derived from fully sampled data. Conclusion A 3D U-Net architecture can be used for semantic segmentation of radially undersampled cine acquisitions, achieving a performance comparable with human experts in fully sampled data. This approach can jointly accelerate time-consuming cine image acquisition and cumbersome manual image analysis. KW - undersampling KW - cardiovascular magnetic resonance (CMR) KW - deep learning KW - radial KW - semantic segmentation Y1 - 2022 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-257616 VL - 87 IS - 2 ER - TY - CHAP A1 - Bezan, Sarah T1 - A Darwinism of the Muck and Mire: Decomposing the Eco- and Zoopoetics of Stephen Collis’ and Jordan Scott’s decomp T2 - Texts, Animals, Environments: Zoopoetics and Ecopoetics N2 - No abstract available. KW - Animal Studies KW - Cultural Animal Studies KW - Cultural Studies KW - Ecocriticism KW - Environmental Humanities KW - Human-Animal Studies KW - Literary Studies Y1 - 2019 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-178074 UR - https://www.rombach-verlag.de/buecher/suchergebnis/rombach/buch/details/texts-animals-environments.html PB - Rombach Druck- und Verlagshaus CY - Freiburg i. Br. ER - TY - JOUR A1 - Beer, Katharina A1 - Joschinski, Jens A1 - Sastre, Alazne Arrazola A1 - Krauss, Jochen A1 - Helfrich-Förster, Charlotte T1 - A damping circadian clock drives weak oscillations in metabolism and locomotor activity of aphids (Acyrthosiphon pisum) JF - Scientific Reports N2 - Timing seasonal events, like reproduction or diapause, is crucial for the survival of many species. Global change causes phenologies worldwide to shift, which requires a mechanistic explanation of seasonal time measurement. Day length (photoperiod) is a reliable indicator of winter arrival, but it remains unclear how exactly species measure day length. A reference for time of day could be provided by a circadian clock, by an hourglass clock, or, as some newer models suggest, by a damped circadian clock. However, damping of clock outputs has so far been rarely observed. To study putative clock outputs of Acyrthosiphon pisum aphids, we raised individual nymphs on coloured artificial diet, and measured rhythms in metabolic activity in light-dark illumination cycles of 16:08 hours (LD) and constant conditions (DD). In addition, we kept individuals in a novel monitoring setup and measured locomotor activity. We found that A. pisum is day-active in LD, potentially with a bimodal distribution. In constant darkness rhythmicity of locomotor behaviour persisted in some individuals, but patterns were mostly complex with several predominant periods. Metabolic activity, on the other hand, damped quickly. A damped circadian clock, potentially driven by multiple oscillator populations, is the most likely explanation of our results. KW - circadian mechanisms KW - behavioural ecology KW - damped circadian clock KW - Acyrthosiphon pisum Y1 - 2017 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-170020 VL - 7 IS - 14906 ER - TY - JOUR A1 - Reuss, Heiko A1 - Kiesel, Andrea A1 - Kunde, Wilfried A1 - Wühr, Peter T1 - A cue from the unconscious - masked symbols prompt spatial anticipation JF - Frontiers in Psychology N2 - Anticipating where an event will occur enables us to instantaneously respond to events that occur at the expected location. Here we investigated if such spatial anticipations can be triggered by symbolic information that participants cannot consciously see. In two experiments involving a Posner cueing task and a visual search task, a central cue informed participants about the likely location of the next target stimulus. In half of the trials, this cue was rendered invisible by pattern masking. In both experiments, visible cues led to cueing effects, that is, faster responses after valid compared to invalid cues. Importantly, even masked cues caused cueing effects, though to a lesser extent. Additionally, we analyzed effects on attention that persist from one trial to the subsequent trial. We found that spatial anticipations are able to interfere with newly formed spatial anticipations and influence orienting of attention in the subsequent trial. When the preceding cue was visible, the corresponding spatial anticipation persisted to an extent that prevented a noticeable effect of masked cues. The effects of visible cues were likewise modulated by previous spatial anticipations, but were strong enough to also exert an impact on attention themselves. Altogether, the results suggest that spatial anticipations can be formed on the basis of unconscious stimuli, but that interfering influences like still active spatial anticipations can suppress this effect. KW - masked priming KW - unconscious processing KW - anticipation KW - endogenous shifts of attention KW - spatial cueing Y1 - 2012 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-123971 VL - 3 ER - TY - JOUR A1 - Reymus, M. A1 - Stawarczyk, B. A1 - Winkler, A. A1 - Ludwig, J. A1 - Kess, S. A1 - Krastl, G. A1 - Krug, R. T1 - A critical evaluation of the material properties and clinical suitability of in‐house printed and commercial tooth replicas for endodontic training JF - International Endodontic Journal N2 - Aim To assess the suitability of several 3D‐printed resins for the manufacturing of tooth replicas for endodontic training in comparison with commercially available replicas by analysing the properties of the materials and comparing them with real teeth during endodontic training. Methodology Tooth replicas were 3D‐printed using four resins (NextDent Model, NextDent C&B, V‐Print ee and Vero White Plus) and compared with two commercially available products (VDW and Smile Factory) as well as extracted human teeth. Martens hardness, indentation modulus and radiopacity were investigated on these tooth replicas. Experienced dentists evaluated the suitability of the replicas for endodontic training by comparing them with real teeth in terms of appearance, anatomy, radiopacity, similarity to dentine during access opening, canal gauging and canal instrumentation. Data were analysed using the Kolmogorov–Smirnov and Mann–Whitney U‐test. Results The greatest hardness values were recorded for human dentine (P < 0.001), followed by V‐Print ee and the commercial tooth replica of Smile Factory. The greatest radiopacity was associated with VOC and dentine (P < 0.001) in comparison with the other materials tested. The appearance of the in‐house printed tooth replicas was subjectively evaluated by the dentists as being more realistic than the commercially available products. No differences between the replicas was detected during mechanical instrumentation of root canals. Conclusion None of the tooth replicas were able to simulate human dentine from the perspectives evaluated. V‐Print ee had radiopacity comparable with dentine, but its hardness was not comparable with dentine. KW - 3D Printing KW - dental education KW - replica KW - undergraduate training Y1 - 2020 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-218085 VL - 53 IS - 10 SP - 1446 EP - 1454 ER - TY - JOUR A1 - Staiger, Christine A1 - Cadot, Sidney A1 - Kooter, Raul A1 - Dittrich, Marcus A1 - Müller, Tobias A1 - Klau, Gunnar W. A1 - Wessels, Lodewyk F. A. T1 - A Critical Evaluation of Network and Pathway-Based Classifiers for Outcome Prediction in Breast Cancer JF - PLoS One N2 - Recently, several classifiers that combine primary tumor data, like gene expression data, and secondary data sources, such as protein-protein interaction networks, have been proposed for predicting outcome in breast cancer. In these approaches, new composite features are typically constructed by aggregating the expression levels of several genes. The secondary data sources are employed to guide this aggregation. Although many studies claim that these approaches improve classification performance over single genes classifiers, the gain in performance is difficult to assess. This stems mainly from the fact that different breast cancer data sets and validation procedures are employed to assess the performance. Here we address these issues by employing a large cohort of six breast cancer data sets as benchmark set and by performing an unbiased evaluation of the classification accuracies of the different approaches. Contrary to previous claims, we find that composite feature classifiers do not outperform simple single genes classifiers. We investigate the effect of (1) the number of selected features; (2) the specific gene set from which features are selected; (3) the size of the training set and (4) the heterogeneity of the data set on the performance of composite feature and single genes classifiers. Strikingly, we find that randomization of secondary data sources, which destroys all biological information in these sources, does not result in a deterioration in performance of composite feature classifiers. Finally, we show that when a proper correction for gene set size is performed, the stability of single genes sets is similar to the stability of composite feature sets. Based on these results there is currently no reason to prefer prognostic classifiers based on composite features over single genes classifiers for predicting outcome in breast cancer. KW - modules KW - protein-interaction networks KW - expression signature KW - classification KW - set KW - metastasis KW - stability KW - survival KW - database KW - markers Y1 - 2012 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-131323 VL - 7 IS - 4 ER - TY - JOUR A1 - Karak, Suvendu A1 - Stepanenko, Vladimir A1 - Addicoat, Matthew A. A1 - Keßler, Philipp A1 - Moser, Simon A1 - Beuerle, Florian A1 - Würthner, Frank T1 - A Covalent Organic Framework for Cooperative Water Oxidation JF - Journal of the American Chemical Society N2 - The future of water-derived hydrogen as the “sustainable energy source” straightaway bets on the success of the sluggish oxygen-generating half-reaction. The endeavor to emulate the natural photosystem II for efficient water oxidation has been extended across the spectrum of organic and inorganic combinations. However, the achievement has so far been restricted to homogeneous catalysts rather than their pristine heterogeneous forms. The poor structural understanding and control over the mechanistic pathway often impede the overall development. Herein, we have synthesized a highly crystalline covalent organic framework (COF) for chemical and photochemical water oxidation. The interpenetrated structure assures the catalyst stability, as the catalyst’s performance remains unaltered after several cycles. This COF exhibits the highest ever accomplished catalytic activity for such an organometallic crystalline solid-state material where the rate of oxygen evolution is as high as ∼26,000 μmol L\(^{–1}\) s\(^{–1}\) (second-order rate constant k ≈ 1650 μmol L s\(^{–1}\) g\(^{–2}\)). The catalyst also proves its exceptional activity (k ≈ 1600 μmol L s\(^{–1}\) g\(^{–2}\)) during light-driven water oxidation under very dilute conditions. The cooperative interaction between metal centers in the crystalline network offers 20–30-fold superior activity during chemical as well as photocatalytic water oxidation as compared to its amorphous polymeric counterpart. KW - water oxidation KW - sustainable energy source KW - covalent organic framework KW - catalyst KW - crystalline KW - catalysis KW - nanoparticles Y1 - 2022 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-287591 UR - https://pubs.acs.org/doi/10.1021/jacs.2c07282 SN - 0002-7863 VL - 144 IS - 38 ER - TY - THES A1 - Lewandowska, Natalia Ewelina T1 - A Correlation Study of Radio Giant Pulses and Very High Energy Photons from the Crab Pulsar T1 - Eine Korrelationsstudie zwischen Riesenpulsen im Radiobereich und Photonen im Gammabereich vom Pulsar im Krebsnebel N2 - Pulsars (in short for Pulsating Stars) are magnetized, fast rotating neutron stars. The basic picture of a pulsar describes it as a neutron star which has a rotation axis that is not aligned with its magnetic field axis. The emission is assumed to be generated near the magnetic poles of the neutron star and emitted along the open magnetic field lines. Consequently, the corresponding beam of photons is emitted along the magnetic field line axis. The non-alignment of both, the rotation and the magnetic field axis, results in the effect that the emission of the pulsar is only seen if its beam points towards the observer. The emission from a pulsar is therefore perceived as being pulsed although its generation is not. This rather simple geometrical model is commonly referred to as Lighthouse Model and has been widely accepted. However, it does not deliver an explanation of the precise mechanisms behind the emission from pulsars (see below for more details). Nowadays more than 2000 pulsars are known. They are observed at various wavelengths. Multiwavelength studies have shown that some pulsars are visible only at certain wavelengths while the emission from others can be observed throughout large parts of the electromagnetic spectrum. An example of the latter case is the Crab pulsar which is also the main object of interest in this thesis. Originating from a supernova explosion observed in 1054 A.D. and discovered in 1968, the Crab pulsar has been the central subject of numerous studies. Its pulsed emission is visible throughout the whole electromagnetic spectrum which makes it a key figure in understanding the possible mechanisms of multiwavelength emission from pulsars. The Crab pulsar is also well known for its radio emission strongly varying on long as well as on short time scales. While long time scale behaviour from a pulsar is usually examined through the use of its average profile (a profile resulting from averaging of a large number of individual pulses resulting from single rotations), short time scale behaviour is examined via its single pulses. The short time scale anomalous behaviour of its radio emission is commonly referred to as Giant Pulses and represents the central topic of this thesis. While current theoretical approaches place the origin of the radio emission from a pulsar like the Crab near its magnetic poles (Polar Cap Model) as already indicated by the Lighthouse model, its emission at higher frequencies, especially its gamma-ray emission, is assumed to originate further away in the geometrical region surrounding a pulsar which is commonly referred to as a pulsar magnetosphere (Outer Gap Model). Consequently, the respective emission regions are usually assumed not to be connected. However, past observational results from the Crab pulsar represent a contradiction to this assumption. Radio giant pulses from the Crab pulsar have been observed to emit large amounts of energy on very short time scales implying small emission regions on the surface of the pulsar. Such energetic events might also leave a trace in the gamma-ray emission of the Crab pulsar. The aim of this thesis is to search for this connection in the form of a correlation study between radio giant pulses and gamma-photons from the Crab pulsar. To make such a study possible, a multiwavelength observational campaign was organized for which radio observations were independently applied for, coordinated and carried out with the Effelsberg radio telescope and the Westerbork Synthesis Radio Telescope and gamma-ray observations with the Major Atmospheric Imaging Cherenkov telescopes. The corresponding radio and gamma-ray data sets were reduced and the correlation analysis thereafter consisted of three different approaches: 1) The search for a clustering in the differences of the times of arrival of radio giant pulses and gamma-photons; 2) The search for a linear correlation between radio giant pulses and gamma-photons using the Pearson correlation approach; 3) A search for an increase of the gamma-ray flux around occurring radio giant pulses. In the last part of the correlation study an increase of the number of gamma-photons centered on a radio giant pulse by about 17% (in contrast with the number of gamma-photons when no radio giant pulse occurs in the same time window) was discovered. This finding suggests that a new theoretical approach for the emission of young pulsars like the Crab pulsar, is necessary. N2 - Pulsare (Kurzform von Pulsating Stars) sind stark magnetisierte, rotierende Neutronensterne. Nach dem Standardmodell ist ein Pulsar ein Neutronenstern mit einer Rotationsachse, die nicht entlang der Achse seines Magnetfelds ausgerichtet ist. Es wird angenommen, dass die Pulsarstrahlung in der Nähe der Pole des Neutronensterns an offenen Magnetfeldlinien entsteht. Der dadurch entstehende Photonenstrahl wird entlang der Magnetfeldachse emittiert. Die unterschiedlichen Ausrichtungen der Rotations- und Magnetfeldachse führen dazu, dass die Strahlung des Pulsars von einem Beobachter nur wahrgenommen wird, wenn der Photonenstrahl die Sichtlinie des Beobachters überstreicht. Durch diesen Effekt wird beim Beobachter der Anschein erweckt die Pulsarstrahlung sei gepulst, obwohl sie kontinuerlich produziert wird. Dieses vereinfachte geometrische Model, in der Literatur oftmals als Leuchtturm Modell bezeichnet, ist heutzutage weitestgehend akzeptiert. Es liefert dennoch keine Erklärung für die genaue Entstehung der Pulsarstrahlung (siehe weiter unten). Heutzutage sind mehr als 2000 Pulsare bekannt und werden mittlerweile nicht nur bei Radiowellenlängen untersucht. Multiwellenlängenstudien haben zu der Entdeckung geführt, dass einige Pulsar nur in bestimmten Wellenlängenbereichen sichtbar sind, während die Strahlung von anderen Pulsaren in weiten Teilen des elektromagnetischen Spektrums nachgewiesen werden kann. Ein Beispiel für letzteren Fall ist der Crab Pulsar, das Objekt das die vorliegende Arbeit hauptsächlich betrachtet. Entstanden in einer Supernova, die im Jahre 1054 n.Chr. beobachtet wurde, wurde er 1968 als stellarer Überrest dieser Explosion entdeckt und seitdem im Rahmen zahlreicher Studien untersucht. Seine gepulste Strahlung kann im gesamten elektromagnetischen Spektrum nachgewiesen werden. Diese Eigenschaft macht ihn zu einem Schlüsselobjekt für die Erforschung möglicher Emissionsmechanismen der Strahlung von Pulsaren. Eine weitere Besonderheit des Crab Pulsars liegt auch in dem anomalen Verhalten seiner Radiostrahlung auf kurzen Zeitskalen. Während das Langzeitverhalten eines Pulsars mittels seines mittleren Pulsprofiles (eines Profils resultierend aus der Mittelung vieler Einzelpulse aus einzelnen Rotationen) untersucht wird, wird das Kurzzeitverhalten mittels einzelner Pulse untersucht. Als anomales Verhalten der Radiostrahlung des Crab Pulsars auf diesen kurzen Zeitskalen sind die sogenannten Riesenpulse (Giant Pulses) von Interesse. Einzelpulse dieser Art sind der zentrale zu untersuchende Aspekt der vorliegenden Arbeit. Gängige theoretische Modelle gehen davon aus, dass die Radiostrahlung eines Pulsars in der Nähe der Pole entsteht (Polar Cap Model), wie zuvor vom Leuchtturm Model impliziert wurde, während die hochfrequente Strahlung, wie z.B. die gamma-Strahlung, weiter außen in der Magnetosphäre, die den Pulsar umgibt, entsteht (Outer Gap Model). Ausgehend von diesen beiden theoretischen Ansätzen, wird angenommen, dass die entsprechenden Entstehungsregionen nicht miteinander verbunden sind. Die bisherigen Beobachtungen des Crab Pulsars widersprechen jedoch dieser Annahme. Untersuchungen der Riesenpulse des Crab Pulsars im Radiobereich haben ergeben, dass diese Einzelpulse große Energiemengen binnen sehr kurzen Zeitskalen freisetzen. Dieses Phänomen deutet auf sehr kleine Emissionsregionen auf der Oberfläche des Pulsars hin. Eine Freisetzung dieser Energiemengen könnte auch Spuren im Bereich der hochenergetischen gamma-Strahlung hinterlassen. Das Ziel der vorliegenden Arbeit ist daher eine Untersuchung einer möglichen Verbindung zwischen den Radiopulsen des Crab Pulsars im Radiobereich und seiner gamma-Strahlung in der Form einer Korrelationsstudie. Um eine solche Studie zu ermöglichen, wurde eine Multiwellenlängen Beobachtungskampagne organisiert. Im Rahmen dieser Kampagne wurden selbstständig Radiobeobachtungen am Effelsberger Radioteleskop und am Westerbork Synthesis Radio Telescope und gamma-Beobachtungen an den Major Atmospheric Imaging Cherenkov Teleskopen erfolgreich beantragt, koordiniert und (teilweise selbstständig vor Ort) ausgeführt. Die daraus entstehenden Datensätze wurden entsprechend bearbeitet und in der resultierenden Korrelationsanalyse wurden die folgenden Aspekte untersucht: 1) Eine Anhäufung in den Ankunftszeiten von Riesenpulsen und gamma-Photonen; 2) Eine Suche nach einer linearen Korrelation zwischen Riesenpulsen und gamma-Photonen mittels der Pearson Korrelation; 3) Eine Suche nach einer Erhöhung des Flusses von gamma-Photonen in der zeitlichen Umgebung eines Riesenpulses im Radiobereich. Im letzten Teil der Analyse konnte eine Erhöhung der Anzahl von gamma-Photonen, die zeitlich auf einem Riesenpuls zentriert sind, von ungefähr 17% (im Vergleich zu der entsprechenden Anzahl im gleichen Zeitfenster, wenn kein Riesenpuls vorhanden ist) nachgewiesen werden. Dieses Ergebnis gibt einen wichtigen Impuls für die Überarbeitung der bereits vorhandenen Emissionsmodelle von jungen Pulsaren wie dem Crab Pulsar. KW - Pulsar KW - Crab-Nebel KW - Gammaastronomie KW - Radioastronomie KW - crab pulsar KW - giant pulses KW - neutron star KW - correlation KW - radio astronomy KW - gamma astronomy KW - Radiofrequenzstrahlung KW - Gammastrahlenastronomie KW - Korrelation Y1 - 2015 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-123533 ER - TY - JOUR A1 - Jain, M. A1 - Vélez, J. I. A1 - Acosta, M. T. A1 - Palacio, L. G. A1 - Balog, J. A1 - Roessler, E. A1 - Pineda, D. A1 - Londoño, A. C. A1 - Palacio, J. D. A1 - Arbelaez, A. A1 - Lopera, F. A1 - Elia, J. A1 - Hakonarson, H. A1 - Seitz, C. A1 - Freitag, C. M. A1 - Palmason, H. A1 - Meyer, J. A1 - Romanos, M. A1 - Walitza, S. A1 - Hemminger, U. A1 - Warnke, A. A1 - Romanos, J. A1 - Renner, T. A1 - Jacob, C. A1 - Lesch, K.-P. A1 - Swanson, J. A1 - Castellanos, F. X. A1 - Bailey-Wilson, J. E. A1 - Arcos-Burgos, M. A1 - Muenke, M. T1 - A cooperative interaction between LPHN3 and 11q doubles the risk for ADHD JF - Molecular Psychiatry N2 - In previous studies of a genetic isolate, we identified significant linkage of attention deficit hyperactivity disorder (ADHD) to 4q, 5q, 8q, 11q and 17p. The existence of unique large size families linked to multiple regions, and the fact that these families came from an isolated population, we hypothesized that two-locus interaction contributions to ADHD were plausible. Several analytical models converged to show significant interaction between 4q and 11q (P<1 × 10−8) and 11q and 17p (P<1 × 10−6). As we have identified that common variants of the LPHN3 gene were responsible for the 4q linkage signal, we focused on 4q–11q interaction to determine that single-nucleotide polymorphisms (SNPs) harbored in the LPHN3 gene interact with SNPs spanning the 11q region that contains DRD2 and NCAM1 genes, to double the risk of developing ADHD. This interaction not only explains genetic effects much better than taking each of these loci effects by separated but also differences in brain metabolism as depicted by proton magnetic resonance spectroscopy data and pharmacogenetic response to stimulant medication. These findings not only add information about how high order genetic interactions might be implicated in conferring susceptibility to develop ADHD but also show that future studies of the effects of genetic interactions on ADHD clinical information will help to shape predictive models of individual outcome. KW - ADHD KW - genetic interaction KW - LPHN3 KW - NCAM1 KW - DRD2 Y1 - 2012 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-125128 VL - 17 ER - TY - JOUR A1 - Hünig, Siegfried A1 - Wehner, Ingeborg T1 - A convenient synthesis of 2,2',6,6'-Tetramethyl-4,4'-bipyridine and its oxidation to 2,2',6,6'-Tetracarboxy-4,4'-bipyridine N2 - No abstract available Y1 - 1989 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:bvb:20-opus-32005 ER -