Effect of fungicides and alternative products in control of anthracnose and black spot of guava

This work aimed to evaluate the efficiency of fungicides in controlling in vitro and in vivo the causal agents of anthracnose (Colletotrichum gloeosporioides and C. acutatum) and black spot (Guignardia psidii) and evaluate the effect of alternative products to control these diseases. Inhibition of mycelial growth of the pathogens was evaluated for ten fungicides at concentrations of 1, 10 and 100 mg L-1 of active ingredient in potato-dextrose-agar medium. The effectiveness of the fungicides azoxystrobin + difenoconazole, cyproconazole, pyraclostrobin, tebuconazole and tebuconazole + trifloxystrobin in controlling disease incidence and severity of anthracnose, through applications in the field, was measured in fruits collected at three stages of maturation, according to the skin color ( dark green, light green and yellowish green). In postharvest dipping of fruits, the products evaluated were citric acid, peracetic acid, salicylic acid, sodium bicarbonate, chlorine dioxide, Ecolife (R) and chitosan. The fungicides azoxystrobin + difenoconazole, pyraclostrobin, tebuconazole and trifloxystrobin + tebuconazole were highly effective in inhibiting the in vitro mycelial growth of G. psidii and moderately to highly effective in inhibiting C. acutatum and C. gloeosporioides. In field conditions, the fungicide azoxystrobin + difenoconazole was effective in controlling anthracnose and black spot in fruit at three maturity stage ( skin color yellowish green). The alternative products tested were ineffective in the curative control of anthracnose and early blight at postharvest of guava.

Milky Way demographics with the VVV survey I. The 84-million star colour-magnitude diagram of the Galactic bulge

Context. The Milky Way (MW) bulge is a fundamental Galactic component for understanding the formation and evolution of galaxies, in particular our own. The ESO Public Survey VISTA Variables in the Via Lactea is a deep near-IR survey mapping the Galactic bulge and southern plane. Particularly for the bulge area, VVV is covering similar to 315 deg(2). Data taken during 2010 and 2011 covered the entire bulge area in the JHKs bands. Aims. We used VVV data for the whole bulge area as a single and homogeneous data set to build for the first time a single colour-magnitude diagram (CMD) for the entire Galactic bulge. Methods. Photometric data in the JHK(s) bands were combined to produce a single and huge data set containing 173 150 467 sources in the three bands, for the similar to 315 deg(2) covered by VVV in the bulge. Selecting only the data points flagged as stellar, the total number of sources is 84 095 284. Results. We built the largest colour-magnitude diagrams published up to date, containing 173.1+ million sources for all data points, and more than 84.0 million sources accounting for the stellar sources only. The CMD has a complex shape, mostly owing to the complexity of the stellar population and the effects of extinction and reddening towards the Galactic centre. The red clump (RC) giants are seen double in magnitude at b similar to -8 degrees-10 degrees, while in the inner part (b similar to -3 degrees) they appear to be spreading in colour, or even splitting into a secondary peak. Stellar population models show the predominance of main-sequence and giant stars. The analysis of the outermost bulge area reveals a well-defined sequence of late K and M dwarfs, seen at (J - K-s) similar to 0.7-0.9 mag and K-s greater than or similar to 14 mag. Conclusions. The interpretation of the CMD yields important information about the MW bulge, showing the fingerprint of its structure and content. We report a well-defined red dwarf sequence in the outermost bulge, which is important for the planetary transit searches of VVV. The double RC in magnitude seen in the outer bulge is the signature of the X-shaped MW bulge, while the spreading of the RC in colour, and even its splitting into a secondary peak, are caused by reddening effects. The region around the Galactic centre is harder to interpret because it is strongly affected by reddening and extinction.

The star formation rate in the inner Milky Way Galaxy

The present star formation rate (SFR) in the inner Galaxy is puzzling for the chemical evolution models (CEM). No static CEM is able to reproduce the peak of the SFR in the 4 kpc ring. The main reason is probably a shortage of gas, which could be due to the dynamical effects produced by the galactic bar, not considered by these models. We developed a CEM that includes radial gas flows in order to mimic the effects of the galactic bar in the first 5 kpc of the galactic disk. In this model, the star formation (SF) is a two-step process: first, the diffuse gas forms molecular clouds. Then, stars form from cloud-cloud collisions or by the interaction between massive stars and the molecular gas. The former is called spontaneous and the latter induced SF. The mass in the different phases of each region changes by the processes associated with the stellar formation and death by: the SF due to spontaneous fragmentation of gas in the halo; formation of gas clouds in the disk from the diffuse gas; induced SF in the disk due to the interaction between massive stars and gas clouds; and finally, the restitution of the diffuse gas associated to these process of cloud and star formation. In the halo, the star formation rate for the diffuse gas follows a Schmidt law with a power n = 1.5. In the disk, the stars form in two steps: first, molecular clouds are formed from the diffuse gas also following a Schmidt law with n=1.5 and a proportionality factor. Including a specific pattern of radial gas flows, the CEM is able to reproduce with success the peak in the SFR at 4 kpc (fig. 1).

Analisi, progettazione e valutazione dell'efficacia dello spot pubblicitario. Una semiotica per la ricerca di mercato

Il lavoro di ricerca tenta di inquadrare sotto nuove prospettive una problematica ormai classica all’interno della semiotica della pubblicità: l’analisi dello spot. I punti chiave del lavoro – e la pretesa di una certa differenza rispetto a lavori con oggetti affini – consistono sostanzialmente in tre aspetti. Innanzitutto, vi è un ritorno alle origini flochiane nella misura in cui non solo il contesto complessivo e le finalità che la ricerca si propone sono fortemente ancorati all’interno di obiettivi di marketing, ma tutto lo studio nella sua interezza nasce dal dialogo concreto tra metodologia di analisi semiotica e prassi concreta all’interno degli istituti di ricerca di mercato. La tesi non presenta quindi una collezione di analisi di testi pubblicitari condotte in modo autoriferito, quanto piuttosto di “messe alla prova” della metodologia, funzionali alla definizione di disegni di ricerca per la marketing research. Questo comporta un dialogo piuttosto stretto con metodologie affini (sociologia qualitativa e quantitativa, psicologia motivazionale, ecc.) nella convinzione che la priorità accordata all’oggetto di analisi sia sovraordinata rispetto all’ortodossia degli strumenti metodologici. In definitiva, lo spot è sempre e comunque analizzato all’interno di una prospettiva brand-centrica che ha ben in mente la semiotica della situazione di consumo rispetto alla quale lo spot agisce da leva di valorizzazione per l’acquisto. In secondo luogo, gli oggetti analizzati sono piuttosto vari e differenziati: non solo lo spot nella sua versione audiovisiva definitiva (il “girato”), ma anche storyboard, animatic, concept (di prodotto e di comunicazione). La prospettiva generativa greimasiana va a innestarsi su problematiche legate (anche) alla genesi dello spot, alla sua progettazione e riprogettazione/ottimizzazione. La tesi mostra quindi come una semiotica per le consulenze di marketing si diriga sul proprio oggetto ponendogli domande ben circoscritte e finalizzate a un obiettivo specifico, sostanzialmente derivato dal brief contenente le intenzioni comunicazionali del cliente-azienda. Infine, pur rimanendo all’interno di una teoria semiotica generativa (sostanzialmente greimasiana e post greimasiana), la ricerca adotta una prospettiva intrinsecamente multidisciplinare che se da un lato guarda a problematiche legate al marketing, al branding e alla comunicazione pubblicitaria e d’impresa tout court, dall’altro ritorna alle teorie dell’audiovisivo, mostrando affinità e differenze rispetto a forme audiovisive standard (il “film”) e a mutuazioni da nuove estetiche (la neotelevisione, il videoclip, ecc). La tesi si mostra solidamente convinta del fatto che per parlare di efficacia discorsiva sia imprescindibile approfondire le tematiche riguardanti il sincretismo espressivo e le specifiche modalità di manifestazione stilistica. In questo contesto, il lavoro si compone di quattro grandi aree tematiche. Dopo una breve introduzione sull’attualità del tema “spot” e sulla prospettiva analiticometodologica adottata (§ 1.), nel secondo capitolo si assume teoreticamente che i contenuti dello spot derivino da una specifica (e di volta in volta diversa) creolizzazione tra domini tematici derivanti dalla marca, dal prodotto (inteso tanto come concept di prodotto, quanto come prodotto già “vestito” di una confezione) e dalle tendenze socioculturali. Le tre dimensioni vengono valutate in relazione all’opposizione tra heritage, cioè continuità rispetto al passato e ai concorrenti e vision, cioè discontinuità rispetto alla propria storia comunicazionale e a quella dei concorrenti. Si esplorano inoltre altri fattori come il testimonial-endorser che, in quanto elemento già intrinsecamente foriero di elementi di valorizzazione, va a influire in modo rilevante sul complesso tematico e assiologico della pubblicità. Essendo la sezione della tesi che prende in considerazione il piano specificatamente contenutistico dello spot, questa parte diventa quindi anche l’occasione per ritornare sul modello delle assiologie del consumo di Jean-Marie Floch, approntando alcune critiche e difendendo invece un modello che – secondo la prospettiva qui esposta – contiene punti di attualità ineludibili rispetto a schematizzazioni che gli sono successive e in qualche modo debitrici. Segue una sezione (§ 3.) specificatamente dedicata allo svolgimento e dis-implicazione del sincretismo audiovisivo e quindi – specularmente alla precedente, dedicata alle forme e sostanze del contenuto – si concentra sulle dinamiche espressive. Lo spot viene quindi analizzato in quanto “forma testuale” dotata di alcune specificità, tra cui in primis la brevità. Inoltre vengono approfondite le problematiche legate all’apporto di ciascuna specifica sostanza: il rapporto tra visivo e sonoro, lo schermo e la sua multiprospetticità sempre più evidente, il “lavoro” di punteggiatura della musica, ecc. E su tutto il concetto dominante di montaggio, intrinsecamente unito a quello di ritmo. Il quarto capitolo ritorna in modo approfondito sul rapporto tra semiotica e ricerca di mercato, analizzando sia i rapporti di reciproca conoscenza (o non conoscenza), sia i nuovi spazi di intervento dell’analisi semiotica. Dopo aver argomentato contro un certo scetticismo circa l’utilità pragmatica dell’analisi semiotica, lo studio prende in esame i tradizionali modelli di valutazione e misurazione dell’efficacia pubblicitaria (pre- e post- test) cercando di semiotizzarne il portato. Ne consegue la proposta di disegni di ricerca semiotici modulari: integrabili tra loro e configurabili all’interno di progetti semio-quali-quantitativi. Dopo aver ridefinito le possibilità di un’indagine semiotica sui parametri di efficacia discorsiva, si procede con l’analisi di un caso concreto (§ 5.): dato uno spot che si è dimostrato efficace agli occhi dell’azienda committente, quali possono essere i modi per replicarne i fattori di successo? E come spiegare invece quelli di insuccesso delle campagne successive che – almeno teoricamente – erano pensate per capitalizzare l’efficacia della prima? Non si tratta quindi di una semiotica ingenuamente chiamata a “misurare” l’efficacia pubblicitaria, che evidentemente la marketing research analizza con strumenti quantitativi assodati e fondati su paradigmi di registrazione di determinati parametri sul consumatore (ricordo spontaneo e sollecitato, immagine di marca risultante nella mente di user e prospect consumer, intenzione d’acquisto stimolata). Piuttosto l’intervento qui esposto si preoccupa più funzionalmente a spiegare quali elementi espressivi, discorsivi, narrativi, siano stati responsabili (e quindi prospetticamente potranno condizionare in positivo o in negativo in futuro) la ricezione dello spot. L’analisi evidenzia come elementi apparentemente minimali, ancorati a differenti livelli di pertinenza siano in grado di determinare una notevole diversità negli effetti di senso. Si tratta quindi di un problema di mancata coerenza tra intenzioni comunicative e testo pubblicitario effettivamente realizzato. La risoluzione di tali questioni pragmatiche conduce ad approfondimenti teoricometodologici su alcuni versanti particolarmente interessanti. In primo luogo, ci si interroga sull’apporto della dimensione passionale nella costruzione dell’efficacia e nel coinvolgimento dello spettatore/consumatore. Inoltre – e qui risiede uno dei punti di maggior sintesi del lavoro di tesi – si intraprende una proficua discussione dei modelli di tipizzazione dei generi pubblicitari, intesi come forme discorsive. Si fanno quindi dialogare modelli diversi ma in qualche misura coestensivi e sovrapponibili come quelli di Jean Marie Floch, Guido Ferraro, Cosetta Saba e Chiara Giaccardi. Si perviene così alla costruzione di un nuovo modello sintetico, idealmente onnipervasivo e trasversale alle prospettive analizzate.

The gaseous halo of the Milky Way

In the last decade, sensitive observations have revealed that disc galaxies are surrounded by multiphase gaseous halos produced by the circulation of gas from the discs to the environment and vice-versa. This Thesis is a study of the gaseous halo of the Milky Way carried out via the modelling of the HI emission and the available absorption-line data. We fitted simple kinematical models to the HI LAB Survey and found that the Galaxy has a massive (~3x10^8 Mo) HI halo extending a few kiloparsecs above the plane. This layer rotates more slowly than the disc and shows a global inflow motion, a kinematics similar to that observed in the HI halos of nearby galaxies. We built a dynamical model of the galactic fountain to reproduce the properties of this layer. In this model, fountain clouds are ejected from the disc by SN feedback and - as suggested by hydrodynamical simulations - triggers the cooling of coronal gas, which is entrained by the cloud wakes and accretes onto the disc when the clouds fall back. For a proper choice of the parameters, the model reproduces well the HI data and predicts an accretion of coronal gas onto the disc at a rate of 2 Mo/yr. We extended this model to the warm-hot component of the halo, showing that most of the ion absorption features observed towards background sources are consistent with being produced in the turbulent wakes that lag behind the fountain clouds. Specifically, the column densities, positions, and velocities of the absorbers are well reproduced by our model. Finally, we studied the gas content of galaxies extracted from a cosmological N-body+SPH simulation, and found that an HI halo with the forementioned properties is not observed, probably due ti the relatively low resolution of the simulations.

Resolved stellar populations in milky way and andromeda's new satellites

This thesis concerns the study of the variable stars and resolved stellar populations in four recently discovered dSphs, namely, Hercules and Ursa Major I (UMa I), which are UFD satellites of the MW; Andromeda XIX (And XIX) and Andromeda XXI (And XXI), which are satellites of M31. The main aim is to obtain detailed informations on the properties (age, metallicity, distance, and Oosterhoff type) of the stellar populations in these galaxies, to compare them with those of other satellites around the MW and M31, both ''classical'' dSphs and UFDs. The observables used to achieve these goals are the pulsating variables, especially the RR Lyrae stars, and the color magnitude diagram (CMD) of the resolved stellar populations. In particular, for UMa I, we combined B, V time-series observations from four different ground-based telescopes (Cassini, TLS, TT1 and Subaru) and for Hercules, we used archival data acquired with the Advanced Camera for Surveys (ACS) on board the HST. We used, instead B and V times-series photometry obtained with the Large Binocular Telescope (LBT) for And XIX and And XXI .

Late Infiltration of Post-orthodontic White Spot Lesions

White spot lesion (WSL) infiltration has been recommended immediately after debonding of orthodontic brackets. It is however not clear if established inactive WSLs can also be masked through infiltrationOrthodontic treatment of a 19-year-old patient had to be terminated prematurely due to development of multiple WSLs of varying severity. Three months after debonding, the patient presented for lesion infiltration. After etching with 15% HCl gel and re-wetting of the dried surfaces it seemed that a good outcome could be expected. Lesion infiltration led to complete masking of less severe WSLs. The visual appearance of moderate and severe WSLs was improved but they were still visible after treatment.Inactive WSLs may not represent an increased caries risk, but patients are often bothered esthetically. Infiltration by repeated etching might be a viable approach even for inactive WSLs. Controlled clinical trials are needed to investigate the long-term performance of this technique.

Spot drug-eluting stenting for long coronary stenoses: long-term results of a randomized clinical study

Preliminary results of a randomized trial have suggested that total lesion coverage with drug-eluting stents (DES) is not necessary in the presence of diffuse disease of nonuniform severity. In the present study, we report long-term results of this trial.

Improved sensitivity of an interferon-gamma release assay (T-SPOT.TB™) in combination with tuberculin skin test for the diagnosis of latent tuberculosis in the presence of HIV co-infection

Background Interferon-gamma release assays (IGRA) are more specific than the tuberculin skin test (TST) for the diagnosis of Mycobacterium tuberculosis infection. Data on sensitivity are controversial in HIV infection. Methods IGRA (T-SPOT.TB) was performed using lymphocytes stored within 6 months before culture-confirmed tuberculosis was diagnosed in HIV-infected individuals in the Swiss HIV Cohort Study. Results 64 individuals (69% males, 45% of non-white ethnicity, median age 35 years (interquartile range [IQR] 31-42), 28% with prior AIDS) were analysed. Median CD4 cell count was 223 cells/μl (IQR 103-339), HIV-RNA was 4.7 log10 copies/mL (IQR 4.3-5.2). T-SPOT.TB resulted positive in 25 patients (39%), negative in 18 (28%) and indeterminate in 21 (33%), corresponding to a sensitivity of 39% (95% CI 27-51%) if all test results were considered, and 58% (95% CI 43-74%) if indeterminate results were excluded. Sensitivity of IGRA was independent of CD4 cell count (p = 0.698). Among 44 individuals with available TST, 22 (50%) had a positive TST. Agreement between TST and IGRA was 57% (kappa = 0.14, p = 0.177), and in 34% (10/29) both tests were positive. Combining TST and IGRA (at least one test positive) resulted in an improved sensitivity of 67% (95% CI 52-81%). In multivariate analysis, older age was associated with negative results of TST and T-SPOT.TB (OR 3.07, 95% CI 1,22-7.74, p = 0.017, per 10 years older). Conclusions T-SPOT.TB and TST have similar sensitivity to detect latent TB in HIV-infected individuals. Combining TST and IGRA may help clinicians to better select HIV-infected individuals with latent tuberculosis who qualify for preventive treatment.

Mitral isthmus ablation with and without temporary spot occlusion of the coronary sinus: a randomized clinical comparison of acute outcomes

To evaluate the safety and outcomes of mitral isthmus (MI) linear ablation with temporary spot occlusion of the coronary sinus (CS). Background: CS blood flow cools local tissue precluding transmurality and bidirectional block across MI lesion.

TUNING, AVO, AND FLAT-SPOT EFFECTS IN A SEISMIC ANALYSIS OF NORTH SEA BLOCK F3

Reflection seismic data from the F3 block in the Dutch North Sea exhibits many large-amplitude reflections at shallow horizons, typically categorized as “brightspots ” (Schroot and Schuttenhelm, 2003), mainly because of their bright appearance. In most cases, these bright reflections show a significant “flatness” contrasting with local structural trends. While flatspots are often easily identified in thick reservoirs, we have often occasionally observed apparent flatspot tuning effects at fluid contacts near reservoir edges and in thin reservoir beds, while only poorly understanding them. We conclude that many of the shallow large-amplitude reflections in block F3 are dominated by flatspots, and we investigate the thin-bed tuning effects that such flatspots cause as they interact with the reflection from the reservoir’s upper boundary. There are two possible effects to be considered: (1) the “wedge-model” tuning effects of the flatspot and overlying brightspots, dimspots, or polarity-reversals; and (2) the stacking effects that result from possible inclusion of post-critical flatspot reflections in these shallow sands. We modeled the effects of these two phenomena for the particular stratigraphic sequence in block F3. Our results suggest that stacking of post-critical flatspot reflections can cause similar large-amplitude but flat reflections, in some cases even causing an interface expected to produce a ‘dimspot’ to appear as a ‘brightspot’. Analysis of NMO stretch and muting shows the likely exclusion of critical offset data in stacked output. If post-critical reflections are included in stacking, unusual results will be observed. In the North Sea case, we conclude the tuning effect was the primary reason causing for the brightness and flatness of these reflections. However, it is still important to note that care should be taken while applying muting on reflections with wide range of incidence angles and the inclusion of critical offset data may cause some spurious features in the stacked section.