Spatial and temporal variation in settlement, growth and condition of the rockfish species Sebastes caurinus and Sebastes carnatus in the Channel Islands region, Santa Barbara, CA

Survival during the early life stages of marine species, including nearshore temperate reef fishes, is typically very low, and small changes in mortality rates, due to physiological and environmental conditions, can have marked effects on survival of a cohort and, on a larger scale, on the success of a recruitment season. Moreover, trade offs between larval growth and accumulation of energetic resources prior to settlement are likely to influence growth and survival until this critical period and afterwards. Rockfish recruitment rates are notoriously variable between years and across geographic locations. Monitoring of rates of onshore delivery of pelagic juveniles (defined here as settlement) of two species of nearshore rockfishes, Sebastes caurinus and Sebastes carnatus, was done between 2003-2009 years using artificial collectors placed at San Miguel and Santa Cruz Island, off Southern California coast. I investigated spatiotemporal variation in settlement rate, lipid content, pelagic larval duration and larval growth of the newly settled fishes; I assessed relationships between birth date, larval growth, early life-history characteristics and lipid content at settlement, considering also interspecific differences; finally, I attempt to relate interannual patterns of settlement and of early life history traits to easily accessible, local and regional indices of ocean conditions including in situ ocean temperature and regional upwelling, sea surface temperature (SST) and Chlorophyll-a (Chl-a) concentration. Spatial variations appeared to be of low relevance, while significant interannual differences were detected in settlement rate, pelagic larval duration and larval growth. The amount of lipid content of the newly settled fishes was highly variable in space and time, but did not differ between the two species and did not show any relationships with early life history traits, indicating that no trade off involved these physiological processes or they were masked by high individual variability in different periods of larval life. Significant interspecific differences were found in the timing of parturition and settlement and in larval growth rates, with S. carnatus growing faster and breeding and settling later than S. caurinus. The two species exhibited also different patterns of correlations between larval growth rates and larval duration. S. carnatus larval duration was longer when the growth in the first two weeks post-hatch was faster, while S. caurinus had a shorter larval duration when grew fast in the middle and in the end of larval life, suggesting different larval strategies. Fishes with longer larval durations were longer in size at settlement and exhibited longer planktonic phase in periods of favourable environmental conditions. Ocean conditions had a low explanatory power for interannual variation in early life history traits, but a very high explanatory power for settlement fluctuations, with regional upwelling strength being the principal indicator. Nonetheless, interannual variability in larval duration and growth were related to great phenological changes in upwelling happened during the period of this study and that caused negative consequences at all trophic levels along the California coast. Despite the low explanatory power of the environmental variables used in this study on the variation of larval biological traits, environmental processes were differently related with early life history characteristics analyzed to species, indicating possible species-specific susceptibility to ocean conditions and local environmental adaptation, which should be further investigated. These results have implications for understanding the processes influencing larval and juvenile survival, and consequently recruitment variability, which may be dependent on biological characteristics and environmental conditions.

Analysis of the spectrum of the spin-1 biquadratic antiferromagnetic chain

In questo elaborato vengono discusse le catene di spin-1, modelli quantistici definiti su un reticolo unidimensionale con interazione tra siti primi vicini. Fra la ricca varietà di tipologie esistenti è stato scelto di porre attenzione primariamente sul modello antiferromagnetico con interazione puramente biquadratica. Vengono presentati diversi metodi di classificazione degli autostati di tale modello, a partire dalle simmetrie che ne caratterizzano l’Hamiltoniana. La corrispondenza con altri modelli noti, quali il modello XXZ di spin 1/2, la catena di Heisenberg SU (3) ed i modelli di Potts, è utile ad individuare strutture simmetriche nascoste nel formalismo di spin-1, le quali consentono di ricavare informazioni sullo spettro energetico. Infine, vengono presentati risultati numerici accompagnati da alcune considerazioni sulle modifiche dello spettro quando si aggiunge un termine bilineare alla Hamiltoniana biquadratica.

The molecular gas content of star-forming galaxies in the ALPINE fields.

In this thesis, I aim to study the evolution with redshift of the gas mass fraction of a sample of 53 sources (from z ∼ 0.5 to z > 5) serendipitously detected in ALMA band 7 as part of the ALMA Large Program to INvestigate C II at Early Times (ALPINE). First, I used SED-fitting software CIGALE, which is able to implement energy balancing between the optical and the far infrared part, to produce a best-fit template of my sources and to have an estimate of some physical properties, such as the star formation rate (SFR), the total infrared luminosity and the total stellar mass. Then, using the tight correlation found by Scoville et al. (2014) between the ISM molecular gas mass and the rest-frame 850 μm luminosity, I used the latter, extrapolating it from the best-fit template using a code that I wrote in Python, as a tracer for the molecular gas. For my sample, I then derived the most important physical properties, such as molecular gas mass, gas mass fractions, specific star formation rate and depletion timescales, which allowed me to better categorize them and find them a place within the evolutionary history of the Universe. I also fitted our sources, via another code I wrote again in Python, with a general modified blackbody (MBB) model taken from the literature (Gilli et al. (2014), D’Amato et al. (2020)) to have a direct method of comparison with similar galaxies. What is evident at the end of the paper is that the methods used to derive the physical quantities of the sources are consistent with each other, and these in turn are in good agreement with what is found in the literature.

Determination of microplastics in the digestive content of pelagic fish of commercial interest

The study aimed to determine the amount of microplastics (MPs) found in the digestive content of some pelagic tuna fish species of commercial interest caught along the Spanish coasts. In total, 601 individuals belonging to eight tuna species, and one species of the Corypheanidae family, were examined for the presence of MPs in their stomachs. Fish were collected from 9 different locations along the Spanish coasts by commercial fishers. A total of 170 MPs were extracted from the fish stomach of 75 individuals. The number of particles present in the stomach ranged from 1 to 20 (mean 0.3± 1.2 SD MPs per individual). The species with the highest amount of MPs was Auxix rochei whereas the species that did not present any MPs was Coryphaena hippurus, the only species not belonging to the tuna group. In terms of location, the highest ratio of MPs (71%) was found in the fish collected from Azohia, and the lowest in Mazagon (7%). In general, the fish that ingested more MPs were those caught from sites that were closer to the coasts (Canarias Islands stations and Azohia). No correlation between the number of ingested MPs and the size and weight of the fish were detected nor for the whole sample nor for each species separately. Analyzing the MPs in terms of colour, green colour MPs were the most dominant (52%) followed by blue colour (25%). Analyzing the MPs in terms of size, 11 categories were considered and the most dominant size was 0-0.5 micron. Fibers were excluded from the analysis because no protocol was adopted to prevent their contamination. Furthermore, 100% of the MPs found were fragments. The data did not show a high presence of MPs in the analyzed study areas. A bias could probably be due to the method used, allowing to loose a certain quantity of very small microplastics, and also to ethological and biological factors of the species, as documented by other studies: very often MPs do not accumulate in the stomach and are expelled from the individual.