Reddenings of Cepheids

The aim of this work is to derive precise reddenings for 31 Cepheids using multiphase high-resolution spectroscopic observations and literature-derived colors. Each individual reddening value was determined as a difference between the observed (B - V) value and a calculated (B - V) value based on Castelli stellar model atmospheres and atmosphere parameters (effective temperature and gravity) previously determined through high-resolution spectroscopic analysis. This procedure was repeated for all pulsational phases at which spectra were obtained (typically 11 spectra for each star). After that, the mean reddening value for a given Cepheid was obtained. The reddening values derived were compared to values based on the use of distances and multiband photometry, reaching the general conclusion that reddening derived in this manner agrees with those from other methods.

Neuropsychological predictors of response to randomized treatment in obsessive-compulsive disorder

Objective: To identify neuropsychological predictors of treatment response to cognitive-behavioral therapy (CBT) and fluoxetine in treatment-naive adults with obsessive-compulsive disorder (OCD). Method: Thirty-eight adult outpatients with OCD underwent neuropsychological assessment, including tasks of intellectual function, executive functioning and visual and verbal memory, before randomization to a 12-week clinical trial of either CBT or fluoxetine. Neuropsychological measures were used to identify predictors of treatment response in OCD. Results: Neuropsychological measures that predicted a better treatment response to either CBT or fluoxetine were higher verbal IQ (Wechsler Abbreviated Scale of Intelligence) (p = 0.008); higher verbal memory on the California Verbal Learning Test (p = 0.710); shorter time to complete part D (Dots) (p<0.001), longer time to complete part W (Words) (p = 0.025) and less errors on part C (Colors) (p<0.001) in the Victoria Stroop Test (VST). Fewer perseverations on the California Verbal Learning Test, a measure of mental flexibility, predicted better response to CBT, but worse response to fluoxetine (p = 0.002). Conclusion: In general, OCD patients with better cognitive and executive abilities at baseline were more prone to respond to either CBT or fluoxetine. Our finding that neuropsychological measures of mental flexibility predicted response to treatment in opposite directions for CBT and fluoxetine suggests that OCD patients with different neuropsychological profiles may respond preferentially to one type of treatment versus the other. Further studies with larger samples of OCD patients are necessary to investigate the heuristic value of such findings in a clinical context. (C) 2012 Elsevier Inc. All rights reserved.

Gamma Irradiation of in-Shell and Blanched Peanuts Protects against Mycotoxic Fungi and Retains Their Nutraceutical Components during Long-Term Storage

Peanut samples were irradiated (0.0, 5.2, 7.2 or 10.0 kGy), stored for a year (room temperature) and examined every three months. Mycotoxic fungi (MF) were detected in non-irradiated blanched peanuts. A dose of 5.2 kGy was found suitable to prevent MF growth in blanched samples. No MF was detected in in-shell peanuts, with or without irradiation. The colors of the control in-shell and blanched samples were, respectively, 44.72 and 60.21 (L *); 25.20 and 20.38 (Chroma); 53.05 and 86.46 (degrees Hue). The water activities (Aw) were 0.673 and 0.425. The corresponding fatty acids were 13.33% and 12.14% (C16:0), 44.94% and 44.92% (C18:1,omega 9) and 37.10% and 37.63% (C18: 2,omega 6). The total phenolics (TP) were 4.62 and 2.52 mg GAE/g, with antioxidant activities (AA) of 16.97 and 10.36 mu mol TEAC/g. Storage time negatively correlated with Aw (in-shell peanuts) or L *, linoleic acid, TP and AA (in-shell and blanched peanuts) but positively correlated with Aw (blanched peanuts), and with oleic acid (in-shell and blanched peanuts). Irradiation positively correlated with antioxidant activity (blanched peanuts). No correlation was found between irradiation and AA (in-shell samples) or fatty acids and TP (in-shell and blanched peanuts). Irradiation protected against MF and retained both the polyunsaturated fatty acids and polyphenols in the samples.

Galaxy interactions I. Major and minor mergers

Aims. We study galaxy pair samples selected from the Sloan Digital Sky Survey (SDSS-DR7) and we perform an analysis of minor and major mergers with the aim of investigating the dependence of galaxy properties on interactions. Methods. We build a galaxy pair catalog requiring r(p) < 25 kpc h(-1) and Delta V < 350 km s(-1) within redshift z < 0.1. By visual inspection of SDSS images we remove false identifications and we classify the interactions into three categories: pairs undergoing merging, M; pairs with evident tidal features, T; and non disturbed, N. We also divide the pair sample into minor and major interactions according to the luminosity ratio of the galaxy members. We study star formation activity through colors, the 4000 angstrom break, and star formation rates. Results. We find that similar to 10% of the pairs are classified as M. These systems show an excess of young stellar populations as inferred from the D-n(4000) spectral index, colors, and star formation rates of the member galaxies, an effect which we argue is directly related to the ongoing merging process. We find similar to 30% of the pairs exhibiting tidal features (T pairs) with member galaxies showing evidence of old stellar populations. This can be associated either to the disruptive effect of some tidal interactions, or to the longer time-scale of morphological disturbance with respect to the bursts of the tidal induced star formation. Regardless of the color distribution, we find a prominent blue peak in the strongest mergers, while pairs with tidal signs under a minor merger show a strong red peak. Therefore, our results show that galaxy interactions are important in driving the evolution of galaxy bimodality. By adding stellar masses and star formation rates of the two members of the pairs, we explore the global efficiency of star formation of the pairs as a whole. We find that, at a given total stellar mass, major mergers are significantly more efficient (a factor approximate to 2) in forming new stars, with respect to both minor mergers or a control sample of non-interacting galaxies. We conclude that the characteristics of the interactions and the ratio of luminosity galaxy pair members involved in a merger are important parameters in setting galaxy properties.

GAUDY JUVENILE PLUMAGES OF CINEREOUS MOURNER (LANIOCERA HYPOPYRRA) AND BRAZILIAN LANIISOMA (LANIISOMA ELEGANS)

We describe the juvenile plumages of the Cinereous Mourner (Laniocera hypopyrra) and the Brazilian Laniisoma (Laniisoma elegans). Both L. hypopyrra and L. elegans possess a dramatically conspicuous plumage as juveniles in contrast to the generally cryptic plumage pattern exhibited by most juvenile birds. They are predominantly covered by cinnamon-orange feathers with black terminal spots, contrasting with the nest and the predominant colors of their environment. This colorful plumage presumably makes them more at risk from predation by visually oriented animals (e.g., raptors and primates), during one of the most vulnerable phases of their life, and strongly suggests these plumages function as a true, or false (mimicry), signal of 'unprofitability'. Previous knowledge concerning the phylogenetic relationships between these two genera, and the juvenile plumage patterns of other species placed in the Tityridae indicate this shared character in L. hypopyrra and L. elegans represents a synapomorphy within this clade, thereby providing additional evidence of their relationship. Received 13 December 2011. Accepted 1 May 2012.

Microclimate under different shading screens in greenhouses cultivated with bromeliads

This study had as its objective the evaluation of the influence of shading screens of different colors on the different microclimate variables in a greenhouse covered with transparent low-density polyethylene (LDPE). The experiment was conducted with five treatments: thermo-reflective screen (T1); a control - without screen (T2); red screen (T3); blue screen (T4); and black screen (T5), all of them with 70% of shading. An automatic micrometeorological station was installed in each treatment, measuring air temperature (T), relative humidity (RH), incoming solar radiation (Rg), photosynthetically active radiation (PAR) and net radiation (Rn) continuously. The control (T2) and red screen (T3) treatments promoted the highest solar radiation transmissivity, respectively 56.3 and 27%. The black screen (T5) had the lowest solar radiation transmissivity (10.4%). For PAR and Rn the same tendency was observed. The highest temperature was observed under blue screen (T4) treatment, which was 1.3 °C higher than external condition. Blue screen (T4) treatment also presented the highest relative humidity difference between inside and outside conditions.

Utilization of fringe projection technique for evaluation of wound dimensions and of healing progress.

Background: The methods used for evaluating wound dimensions, especially the chronic ones, are invasive and inaccurate. The fringe projection technique with phase shift is a non-invasive, accurate and low-cost optical method. Objective: The aim is to validate the technique through the determination of dimensions of objects of known topography and with different geometries and colors to simulate the wounds and tones of skin color. Taking into account the influence of skin wound optical factors, the technique will be used to evaluate actual patients’ wound dimensions and to study its limitations in this application. Methods: Four sinusoidal fringe patterns, displaced ¼ of period each, were projected onto the objects surface. The object dimensions were obtained from the unwrapped phase map through the observation of the fringe deformations caused by the object topography and using phase shift analysis. An object with simple geometry was used for dimensional calibration and the topographic dimensions of the others were determined from it. After observing the compatibility with the data and validating the method, it was used for measuring the dimensions of real patients’ wounds. Results and Conclusions: The discrepancies between actual topography and dimensions determined with Fringe Projection Technique and for the known object were lower than 0.50 cm. The method was successful in obtaining the topography of real patient’s wounds. Objects and wounds with sharp topographies or causing shadow or reflection are difficult to be evaluated with this technique.

The VIMOS-VLT Deep Survey: the evolution of type-1 AGN

Quasars and AGN play an important role in many aspects of the modern cosmology. Of particular interest is the issue of the interplay between AGN activity and formation and evolution of galaxies and structures. Studies on nearby galaxies revealed that most (and possibly all) galaxy nuclei contain a super-massive black hole (SMBH) and that between a third and half of them are showing some evidence of activity (Kormendy and Richstone, 1995). The discovery of a tight relation between black holes mass and velocity dispersion of their host galaxy suggests that the evolution of the growth of SMBH and their host galaxy are linked together. In this context, studying the evolution of AGN, through the luminosity function (LF), is fundamental to constrain the theories of galaxy and SMBH formation and evolution. Recently, many theories have been developed to describe physical processes possibly responsible of a common formation scenario for galaxies and their central black hole (Volonteri et al., 2003; Springel et al., 2005a; Vittorini et al., 2005; Hopkins et al., 2006a) and an increasing number of observations in different bands are focused on collecting larger and larger quasar samples. Many issues remain however not yet fully understood. In the context of the VVDS (VIMOS-VLT Deep Survey), we collected and studied an unbiased sample of spectroscopically selected faint type-1 AGN with a unique and straightforward selection function. Indeed, the VVDS is a large, purely magnitude limited spectroscopic survey of faint objects, free of any morphological and/or color preselection. We studied the statistical properties of this sample and its evolution up to redshift z 4. Because of the contamination of the AGN light by their host galaxies at the faint magnitudes explored by our sample, we observed that a significant fraction of AGN in our sample would be missed by the UV excess and morphological criteria usually adopted for the pre-selection of optical QSO candidates. If not properly taken into account, this failure in selecting particular sub-classes of AGN could, in principle, affect some of the conclusions drawn from samples of AGN based on these selection criteria. The absence of any pre-selection in the VVDS leads us to have a very complete sample of AGN, including also objects with unusual colors and continuum shape. The VVDS AGN sample shows in fact redder colors than those expected by comparing it, for example, with the color track derived from the SDSS composite spectrum. In particular, the faintest objects have on average redder colors than the brightest ones. This can be attributed to both a large fraction of dust-reddened objects and a significant contamination from the host galaxy. We have tested these possibilities by examining the global spectral energy distribution of each object using, in addition to the U, B, V, R and I-band magnitudes, also the UV-Galex and the IR-Spitzer bands, and fitting it with a combination of AGN and galaxy emission, allowing also for the possibility of extinction of the AGN flux. We found that for 44% of our objects the contamination from the host galaxy is not negligible and this fraction decreases to 21% if we restrict the analysis to a bright subsample (M1450 <-22.15). Our estimated integral surface density at IAB < 24.0 is 500 AGN per square degree, which represents the highest surface density of a spectroscopically confirmed sample of optically selected AGN. We derived the luminosity function in B-band for 1.0 < z < 3.6 using the 1/Vmax estimator. Our data, more than one magnitude fainter than previous optical surveys, allow us to constrain the faint part of the luminosity function up to high redshift. A comparison of our data with the 2dF sample at low redshift (1 < z < 2.1) shows that the VDDS data can not be well fitted with the pure luminosity evolution (PLE) models derived by previous optically selected samples. Qualitatively, this appears to be due to the fact that our data suggest the presence of an excess of faint objects at low redshift (1.0 < z < 1.5) with respect to these models. By combining our faint VVDS sample with the large sample of bright AGN extracted from the SDSS DR3 (Richards et al., 2006b) and testing a number of different evolutionary models, we find that the model which better represents the combined luminosity functions, over a wide range of redshift and luminosity, is a luminosity dependent density evolution (LDDE) model, similar to those derived from the major Xsurveys. Such a parameterization allows the redshift of the AGN density peak to change as a function of luminosity, thus fitting the excess of faint AGN that we find at 1.0 < z < 1.5. On the basis of this model we find, for the first time from the analysis of optically selected samples, that the peak of the AGN space density shifts significantly towards lower redshift going to lower luminosity objects. The position of this peak moves from z 2.0 for MB <-26.0 to z 0.65 for -22< MB <-20. This result, already found in a number of X-ray selected samples of AGN, is consistent with a scenario of “AGN cosmic downsizing”, in which the density of more luminous AGN, possibly associated to more massive black holes, peaks earlier in the history of the Universe (i.e. at higher redshift), than that of low luminosity ones, which reaches its maximum later (i.e. at lower redshift). This behavior has since long been claimed to be present in elliptical galaxies and it is not easy to reproduce it in the hierarchical cosmogonic scenario, where more massive Dark Matter Halos (DMH) form on average later by merging of less massive halos.

A high energy perspective of the co-evolution of black holes and their host galaxies

Thanks to the Chandra and XMM–Newton surveys, the hard X-ray sky is now probed down to a flux limit where the bulk of the X-ray background is almost completely resolved into discrete sources, at least in the 2–8 keV band. Extensive programs of multiwavelength follow-up observations showed that the large majority of hard X–ray selected sources are identified with Active Galactic Nuclei (AGN) spanning a broad range of redshifts, luminosities and optical properties. A sizable fraction of relatively luminous X-ray sources hosting an active, presumably obscured, nucleus would not have been easily recognized as such on the basis of optical observations because characterized by “peculiar” optical properties. In my PhD thesis, I will focus the attention on the nature of two classes of hard X-ray selected “elusive” sources: those characterized by high X-ray-to-optical flux ratios and red optical-to-near-infrared colors, a fraction of which associated with Type 2 quasars, and the X-ray bright optically normal galaxies, also known as XBONGs. In order to characterize the properties of these classes of elusive AGN, the datasets of several deep and large-area surveys have been fully exploited. The first class of “elusive” sources is characterized by X-ray-to-optical flux ratios (X/O) significantly higher than what is generally observed from unobscured quasars and Seyfert galaxies. The properties of well defined samples of high X/O sources detected at bright X–ray fluxes suggest that X/O selection is highly efficient in sampling high–redshift obscured quasars. At the limits of deep Chandra surveys (∼10−16 erg cm−2 s−1), high X/O sources are generally characterized by extremely faint optical magnitudes, hence their spectroscopic identification is hardly feasible even with the largest telescopes. In this framework, a detailed investigation of their X-ray properties may provide useful information on the nature of this important component of the X-ray source population. The X-ray data of the deepest X-ray observations ever performed, the Chandra deep fields, allows us to characterize the average X-ray properties of the high X/O population. The results of spectral analysis clearly indicate that the high X/O sources represent the most obscured component of the X–ray background. Their spectra are harder (G ∼ 1) than any other class of sources in the deep fields and also of the XRB spectrum (G ≈ 1.4). In order to better understand the AGN physics and evolution, a much better knowledge of the redshift, luminosity and spectral energy distributions (SEDs) of elusive AGN is of paramount importance. The recent COSMOS survey provides the necessary multiwavelength database to characterize the SEDs of a statistically robust sample of obscured sources. The combination of high X/O and red-colors offers a powerful tool to select obscured luminous objects at high redshift. A large sample of X-ray emitting extremely red objects (R−K >5) has been collected and their optical-infrared properties have been studied. In particular, using an appropriate SED fitting procedure, the nuclear and the host galaxy components have been deconvolved over a large range of wavelengths and ptical nuclear extinctions, black hole masses and Eddington ratios have been estimated. It is important to remark that the combination of hard X-ray selection and extreme red colors is highly efficient in picking up highly obscured, luminous sources at high redshift. Although the XBONGs do not present a new source population, the interest on the nature of these sources has gained a renewed attention after the discovery of several examples from recent Chandra and XMM–Newton surveys. Even though several possibilities were proposed in recent literature to explain why a relatively luminous (LX = 1042 − 1043erg s−1) hard X-ray source does not leave any significant signature of its presence in terms of optical emission lines, the very nature of XBONGs is still subject of debate. Good-quality photometric near-infrared data (ISAAC/VLT) of 4 low-redshift XBONGs from the HELLAS2XMMsurvey have been used to search for the presence of the putative nucleus, applying the surface-brightness decomposition technique. In two out of the four sources, the presence of a nuclear weak component hosted by a bright galaxy has been revealed. The results indicate that moderate amounts of gas and dust, covering a large solid angle (possibly 4p) at the nuclear source, may explain the lack of optical emission lines. A weak nucleus not able to produce suffcient UV photons may provide an alternative or additional explanation. On the basis of an admittedly small sample, we conclude that XBONGs constitute a mixed bag rather than a new source population. When the presence of a nucleus is revealed, it turns out to be mildly absorbed and hosted by a bright galaxy.

Perturbative and non perturbative effects in the Standard Model and orbifolded ADS/CFT based theories

We study some perturbative and nonperturbative effects in the framework of the Standard Model of particle physics. In particular we consider the time dependence of the Higgs vacuum expectation value given by the dynamics of the StandardModel and study the non-adiabatic production of both bosons and fermions, which is intrinsically non-perturbative. In theHartree approximation, we analyze the general expressions that describe the dissipative dynamics due to the backreaction of the produced particles. Then, we solve numerically some relevant cases for the Standard Model phenomenology in the regime of relatively small oscillations of the Higgs vacuum expectation value (vev). As perturbative effects, we consider the leading logarithmic resummation in small Bjorken x QCD, concentrating ourselves on the Nc dependence of the Green functions associated to reggeized gluons. Here the eigenvalues of the BKP kernel for states of more than three reggeized gluons are unknown in general, contrary to the large Nc limit (planar limit) case where the problem becomes integrable. In this contest we consider a 4-gluon kernel for a finite number of colors and define some simple toy models for the configuration space dynamics, which are directly solvable with group theoretical methods. In particular we study the depencence of the spectrum of thesemodelswith respect to the number of colors andmake comparisons with the planar limit case. In the final part we move on the study of theories beyond the Standard Model, considering models built on AdS5 S5/Γ orbifold compactifications of the type IIB superstring, where Γ is the abelian group Zn. We present an appealing three family N = 0 SUSY model with n = 7 for the order of the orbifolding group. This result in a modified Pati–Salam Model which reduced to the StandardModel after symmetry breaking and has interesting phenomenological consequences for LHC.

Outdoor bronze conservation: assessment of protective treatments by accelerated aging and of treatment removal procedures by laser cleaning

Outdoor bronzes exposed to the environment form naturally a layer called patina, which may be able to protect the metallic substrate. However, since the last century, with the appearance of acid rains, a strong change in the nature and properties of the copper based patinas occurred [1]. Studies and general observations have established that bronze corrosion patinas created by acid rain are not only disfiguring in terms of loss of detail and homogeneity, but are also unstable [2]. The unstable patina is partially leached away by rainwater. This leaching is represented by green streaking on bronze monuments [3]. Because of the instability of the patina, conservation techniques are usually required. On a bronze object exposed to the outdoor environment, there are different actions of the rainfall and other atmospheric agents as a function of the monument shape. In fact, we recognize sheltered and unsheltered areas as regards exposure to rainwater [4]. As a consequence of these different actions, two main patina types are formed on monuments exposed to the outdoor environment. These patinas have different electrochemical, morphological and compositional characteristics [1]. In the case of sheltered areas, the patina contains mainly copper products, stratified above a layer strongly enriched in insoluble Sn oxides, located at the interface with the uncorroded metal. Moreover, different colors of the patina result from the exposure geometry. The surface color may be pale green for unsheltered areas, and green and mat black for sheltered areas [4]. Thus, in real outdoor bronze monuments, the corrosion behavior is strongly influenced by the exposure geometry. This must be taken into account when designing conservation procedures, since the patina is in most cases the support on which corrosion inhibitors are applied. Presently, for protecting outdoor bronzes against atmospheric corrosion, inhibitors and protective treatments are used. BTA and its derivatives, which are the most common inhibitors used for copper and its alloy, were found to be toxic for the environment and human health [5, 6]. Moreover, it has been demonstrated that BTA is efficient when applied on bare copper but not as efficient when applied on bare bronze [7]. Thus it was necessary to find alternative compounds. Silane-based inhibitors (already successfully tested on copper and other metallic substrates [8]), were taken into consideration as a non-toxic, environmentally friendly alternative to BTA derivatives for bronze protection. The purpose of this thesis was based on the assessment of the efficiency of a selected compound, to protect the bronze against corrosion, which is the 3-mercapto-propyl-trimethoxy-silane (PropS-SH). It was selected thanks to the collaboration with the Corrosion Studies Centre “Aldo Daccò” at the Università di Ferrara. Since previous studies [9, 10, 11] demonstrated that the addition of nanoparticles to silane-based inhibitors leads to an increase of the protective efficiency, we also wanted to evaluate the influence of the addition of CeO2, La2O3, TiO2 nanoparticles on the protective efficiency of 3-mercapto-propyl-trimethoxy-silane, applied on pre-patinated bronze surfaces. This study is the first section of the thesis. Since restorers have to work on patinated bronzes and not on bare metal (except for contemporary art), it is important to be able to recreate the patina, under laboratory conditions, either in sheltered or unsheltered conditions to test the coating and to obtain reliable results. Therefore, at the University of Bologna, different devices have been designed to simulate the real outdoor conditions and to create a patina which is representative of real application conditions of inhibitor or protective treatments. In particular, accelerated ageing devices by wet & dry (simulating the action of stagnant rain in sheltered areas [12]) and by dropping (simulating the leaching action of the rain in unsheltered areas [1]) tests were used. In the present work, we used the dropping test as a method to produce pre-patinated bronze surfaces for the application of a candidate inhibitor as well as for evaluating its protective efficiency on aged bronze (unsheltered areas). In this thesis, gilded bronzes were also studied. When they are exposed to the outside environment, a corrosion phenomenon appears which is due to the electrochemical couple gold/copper where copper is the anode. In the presence of an electrolyte, this phenomenon results in the formation of corrosion products than will cause a blistering of the gold (or a break-up and loss of the film in some cases). Moreover, because of the diffusion of the copper salts to the surface, aggregates and a greenish film will be formed on the surface of the sample [13]. By coating gilded samples with PropS-SH and PropS-SH containing nano-particles and carrying out accelerated ageing by the dropping test, a discussion is possible on the effectiveness of this coating, either with nano-particles or not, against the corrosion process. This part is the section 2 of this thesis. Finally, a discussion about laser treatment aiming at the assessment of reversibility/re-applicability of the PropS-SH coating can be found in section 3 of this thesis. Because the protective layer loses its efficiency with time, it is necessary to find a way of removing the silane layer, before applying a new one on the “bare” patina. One request is to minimize the damages that a laser treatment would create on the patina. Therefore, different laser fluences (energy/surface) were applied on the sample surface during the treatment process in order to find the best range of fluence. In particular, we made a characterization of surfaces before and after removal of PropS-SH (applied on a naturally patinated surface, and subsequently aged by natural exposure) with laser methods. The laser removal treatment was done by the CNR Institute of Applied Physics “Nello Carrara” of Sesto Fiorentino in Florence. In all the three sections of the thesis, a range of non-destructive spectroscopic methods (Scanning Electron Microscopy with Energy Dispersive Spectroscopy (SEM-EDS), μ-Raman spectroscopy, X-Ray diffractometry (XRD)) were used for characterizing the corroded surfaces. AAS (Atomic Absorption Spectroscopy) was used to analyze the ageing solutions from the dropping test in sections 1 and 2.

Untersuchung zum Beitrag des ON-Kanals zu zeitlichen und chromatischen Verarbeitungsmechanismen in der Retina

Ziel der vorliegenden Arbeit war es, mithilfe von Dressurexperimenten in Kombination mit dem Einsatz von Neuropharmaka die Bedeutung des retinalen ON-Kanals für zwei visuelle Leistungen des Goldfisches – das kontrastabhängige zeitliche Auflösungsvermögen sowie die Wellenlängenunterscheidungsfähigkeit - zu untersuchen. Da die Tiere nach der pharmakologischen Blockade keinerlei verändertes Verhalten zeigten, kann davon ausgegangen werden, dass der retinale ON-Kanal weder für die Prozessierung des kontrastabhängigen zeitlichen Auflösungsvermögens noch für die Wellenlängenunterscheidungsfähigkeit eine maßgebliche Rolle spielt. Aus den Versuchen zur Wellenlängenunterscheidungsfähigkeit kann des Weiteren abgeleitet werden, dass der ON-Kanal auch für die spektrale Empfindlichkeit der Tiere bei der gegebenen Beleuchtungs- und Dressurbedingungen (L+-Dressur) keine Bedeutung zu haben scheint. Nach den Versuchen zum kontrastabhängigen zeitlichen Auflösungsvermögen kann festgehalten werden, dass das zeitliche Auflösungsvermögen des Goldfisches sich mit abnehmendem Stimuluskontrast verändert: Der für die Tiere wahrnehmbare Flickerfrequenzbereich wird mit abnehmendem Kontrast geringer. Die Flimmerfusionsfrequenz wird im oberen Frequenzbereich früher erreicht; im unteren Flickerfrequenzbereich tritt mit abnehmendem Kontrast auch eine untere Grenze des zeitlichen Auflösungsvermögens auf. Des Weiteren zeigen die Ergebnisse aus den Verhaltensversuchen zu den kontrastabhängigen zeitlichen Übertragungseigenschaften eine gute Vergleichbarkeit zu elektrophysiologisch gewonnenen Antworten von ON bzw. OFF-Bipolarzellen. Ebenso ähneln sich die Kurvenverläufe zum kontrastabhängigen zeitlichen Auflösungsvermögen und die aus den Versuchen zur kontrastabhängigen Ganzfeldbewegungswahrnehmung – einer visuellen Leistung, deren Prozessierung eines ON-Kanal-Beitrages bedarf. Diese Ergebnisse deuten darauf hin, dass das zeitliche Auflösungsvermögen wie auch die Ganzfeldbewegungswahrnehmung hauptsächlich von retinalen Verarbeitungsprozessen abhängen.

Plasmonic nanorods and nanoparticle-assemblies

Die vorliegenden Dissertation beschäftigt sich mit plasmonischen Nanopartikeln, deren Wechselwirkung mit Licht in einer Plasmonenschwingung resultiert. Suspensionen dieser Partikel zeigen kräftige Farben, da sich die Resonanzfrequenz der Plasmonenschwingung im sichtbaren Bereich des elektromagnetischen Spektrum befindet. Durch die Veränderung interner (Material, Größe, Form) oder externer Parameter (Brechungsindex der Umgebung, Abstand zu anderen plasmonischen Partikeln) lässt sich die Farbe der Partikel verändern, eine Verschiebung der Resonanzfrequenz kann beobachtet werden. Ihre Sensitivität gegenüber äußeren Bedingungen ist der Grund, weshalb plasmonische Nanopartikel als Sensoren eingesetzt werden können. Wichtig ist hierbei nicht nur, dass die Partikel eine hohe Sensitivität zeigen, sondern auch die Möglichkeit, reproduzierbar Partikel zu synthetisieren, die experimentellen Anforderungen entsprechen. In der vorliegenden Arbeit wird das Wachstum von reinen Gold- und mit Silber beschichteten Goldnanostäbchen untersucht. Des Weiteren werden plasmonische Nanopartikel als Orientierungs-, Brechungsindex- und Abstandssensoren verwendet. Die Synthese von Goldnanostäbchen erfolgt auf nasschemischen Weg, ihr anisotropes Wachstum aus isotropen Keimen wird durch zahlreiche Faktoren beeinflusst. In diesem Zusammenhang wurde ein Wachstumsmodell entwickelt, das neben dem Vorhandensein eines Stabilisators auch die Rolle von Bromid- und Silberionen herausstellt, die durch selektive Adsorption das Wachstum bestimmter Kristallflächen inhibieren. Zudem konnte gezeigt werden, dass die Potentialdifferenz zwischen Reduktions- und Oxidationsmittel klein sein muss, um ein langsames selektives Wachstum zu gewährleisten. rnDurch das Aufwachsen einer dünnen Silberschicht auf Goldnanostäbchen verbessert sich deren Qualität im Bezug auf die heterogene Linienbreite. Der “Plasmonic Focusing Effect”, die Änderung der Steigung des linearen Zusammenhangs von Plasmonenresonanz und Aspektverhältnis, konnte theoretisch berechnet und experimentell verifiziert werden. Durch die Aufnahme zeitaufgelöster Spektren und die Untersuchung des Verlaufs der Reaktion wurden sowohl Reaktionsordnung, als auch Aktivierungsenergie ermittelt. Das so gefundene kinetische Model erlaubt zudem die Vorhersage des Reaktionsprodukts zu verschiedenen Zeiten. rnEinzelne Goldnanostäbchen wurden in einer Gelmatrix bei verschiedenen Temperaturen untersucht, die Aufnahme der zeitlichen Variation der polarisationsabhängigen Streuintensität konnte genutzt werden, um den Kollaps des Gels zu charakterisieren. Neben der Verwendung einzelner plasmonischer Nanopartikel wurden auch Dimere, bestehend aus zwei Goldnanokugeln, untersucht. Nach der Kalibrierung der Resonanzfrequenz gegenüber des Abstandes der beiden Partikel durch externe Methoden (Lichtstreuung, Cryo- Elektronenmikroskopie) wurde der so gefundene exponentielle Zusammenhang verwendet, um sowohl den Brechungsindex der Umgebung, als auch den Abstand der beiden Goldnanokugeln zu bestimmen. Des Weiteren wurden Goldnanopartikeldimere benutzt, um ein als Linker verwendetes thermoresponsives Elastin-Polymer bei verschiedenen Temperaturen zu charakterisieren. Neben Aggregaten aus zwei Goldnanokugeln wurden auch so genannte “core-satellite” Strukturen synthetisiert, die um einen großen Goldnanopartikelkern viele kleine Goldnanopartikel tragen. Diese Partikel haben eine theoretisch vorhergesagte höhere Sensitivität gegenüber Brechungsindexänderungen, was in ersten Experimenten gezeigt werden konnte.

Dressurexperimente zur Unterscheidungsfähigkeit zwischen weißem Licht und Spektralfarben beim Goldfisch

Der Goldfisch besitzt, im Gegensatz zum Menschen, ein tetrachromatisches Farbensehsystem, das außerordentlich gut untersucht ist. Die Farben gleicher Helligkeit lassen sich hier in einem dreidimensionalen Tetraeder darstellen. Ziel der vorliegenden Arbeit war es herauszufinden, wie gut der Goldfisch Farben, die dem Menschen ungesättigt erscheinen und im Inneren des Farbtetraeders liegen, unterscheiden kann. Des Weiteren stellte sich die Frage, ob sowohl „Weiß“ (ohne UV) als auch Xenonweiß (mit UV) vom Fisch als „unbunt“ oder „neutral“ wahrgenommenen werden. Um all dies untersuchen zu können, musste ein komplexer Versuchsaufbau entwickelt werden, mit dem den Fischen monochromatische und mit Weiß gemischte Lichter gleicher Helligkeit, sowie Xenonweiß gezeigt werden konnte. Die Fische erlernten durch operante Konditionierung einen Dressurstimulus (monochromatisches Licht der Wellenlängen 660 nm, 599 nm, 540 nm, 498 nm oder 450 nm) von einem Vergleichsstimulus (Projektorweiß) zu unterscheiden. Im Folgenden wurde dem Vergleichstimulus in 10er-Schritten immer mehr der jeweiligen Dressurspektralfarbe beigemischt, bis die Goldfische keine sichere Wahl für den Dressurstimulus mehr treffen konnten. Die Unterscheidungsleistung der Goldfische wurde mit zunehmender Beimischung von Dressurspektralfarbe zum Projektorweiß immer geringer und es kristallisierte sich ein Bereich in der Grundfläche des Tetraeders heraus, in dem die Goldfische keine Unterscheidung mehr treffen konnten. Um diesen Bereich näher zu charakterisieren, bekamen die Goldfische Mischlichter, bei denen gerade keine Unterscheidung mehr zum Projektorweiß möglich war, in Transfertests gezeigt. Da die Goldfische diese Mischlichter nicht voneinander unterscheiden konnten, läßt sich schließen, dass es einen größeren Bereich gibt, der, ebenso wie Weiß (ohne UV) für den Goldfisch „neutral“ erscheint. Wenn nun Weiß (ohne UV) für den Goldfisch „neutral“ erscheint, sollte es dem Xenonweiß ähnlich sein. Die Versuche zeigten allerdings, dass die Goldfische die Farben Weiß (ohne UV) und Xenonweiß als verschieden wahrnehmen. Betrachtet man die Sättigung für die Spektralfarben, so zeigte sich, dass die Spektralfarbe 540 nm für den Goldfisch am gesättigsten, die Spektralfarbe 660 nm am ungesättigsten erscheint.

Elektrophysiologische Charakterisierung der Neurone im Tectum opticum des Goldfisches hinsichtlich Farbe und Bewegung

Die vorliegende Arbeit verfolgte mehrere Ziele. Die Hauptaufgabe war es, farbsensitive und bewegungssensitive Neurone im Tectum opticum des Goldfisches zu finden und diese hinsichtlich ihres Antwortverhaltens zu charakterisieren. Aus Verhaltensversuchen ist bekannt, dass sowohl das Ganzfeldbewegungssehen als auch das Objektbewegungssehen „farbenblind“ ist, da die Verarbeitung dieser Sehleistungen jeweils nur von einem Zapfentyp getrieben wird. Es sollte untersucht werden, ob sich diese Farbenblindheit auch auf Ebene der tectalen bewegungsempfindlichen Neurone finden lässt. Schließlich sollten die Ableitorte im Tectum opticum kartiert werden, um festzustellen, ob es jeweils bestimmte örtlich abgegrenzte Areale für Farbe einerseits und für Bewegung andererseits gibt.rnDie Aktivität von tectalen Units wurde durch extrazelluläre Ableitungen registriert. Um farbspezifische Neurone zu identifizieren und zu charakterisieren, wurden 21 verschiedene Farbpapiere (HKS-Standard) aus dem gesamten Farbenkreis (ausgenommen UV) präsentiert. Auf jedes Farbpapier folgte ein neutrales Graupapier. Des Weiteren wurde eine Schwarz-Weiß-Grau-Sequenz gezeigt, um das Antwortverhalten der Units auf Helligkeitswechsel zu prüfen. Jeder Stimulus wurde für fünf Sekunden präsentiert und die gesamte Stimulussequenz wurde mindestens dreimal wiederholt. Zur Identifizierung bewegungssensitiver Neurone wurde ein sich exzentrisch bewegendes schwarz-weißes Zufallspunktmuster präsentiert. Um die „Farbenblindheit“ des Bewegungssehens zu testen, wurden zwei rot-grüne Zufallspunktmuster präsentiert, die den L-Zapfen des Goldfisches unterschiedlich stark modulierten. Den meisten Units wurden sowohl die Farb- als auch die Bewegungsstimuli gezeigt.rnEs konnten 69 Units abgeleitet werden. Von diesen antworteten 34 sowohl auf Farbstimuli als auch auf Helligkeitsreize, 19 Units reagierten ausschließlich auf Farbstimuli, 15 Units zeigten sich nur für den Bewegungsstimulus sensitiv und zwei Units beantworteten ausschließlich Helligkeitswechsel. Die farbempfindlichen Units konnten in 14 Gruppen eingeteilt werden: sechs Gruppen im Rotbereich (22 Units), fünf Gruppen im Blau-Grünbereich (21 Units), eine Gruppe im Gelbbereich (zwei Units), eine Gruppe, die alle Farbstimuli mit Erhöhung der Aktivität (sechs Units) und eine Gruppe, die alle Farbstimuli mit Erniedrigung der Aktivität (eine Unit) beantwortete. Es wurden zwei Arten von Gegenfarbzellen gefunden: Rot-ON/Blau-und-Grün-OFF (12 Units) und Rot-OFF/Blau-und-Grün-ON (sieben Units). Es wurden verschiedene zeitliche Antwortmuster gefunden. Während einige Units nur Reizwechsel beantworteten, zeigten die meisten Units ein tonisches Antwortverhalten. Manche Units beantworteten jeden Stimuluswechsel phasisch und darüber hinaus bestimmte Stimuli tonisch. Die meisten tectalen Neurone zeigten eine Grundaktivität. Alle Units, denen sowohl der Farb- als auch der Bewegungsstimulus gezeigt wurden, antworteten nur auf eine Stimulusart. rnDiese Ergebnisse lassen folgende Schlüsse zu: Die Verarbeitung von Farbe und Bewegung im Tectum opticum des Goldfischs wird über zwei unterschiedlichen Verarbeitungswegen geleistet, da alle Units entweder auf Farb- oder auf Bewegungsstimuli antworten. Das Bewegungssehen wird im Goldfisch durch nur einen Zapfentyp (M- oder L-Zapfen) vermittelt und ist somit “farbenblind”, da alle bewegungssensitiven Units die Aktivität einstellten, wenn der Stimulus nur noch einen Zapfentyp modulierte. Es scheint spezifische Areale für „Farbe“ und „Bewegung“ im Tectum opticum des Goldfisches zu geben, da bewegungssensitive Units bevorzugt im posterio-medialen Bereich in einer Tiefe zwischen 200-400 µm gefunden und farbspezifische Units vor allem im anterio-medialen Bereich entdeckt wurden.