Genomic and toxigenic heterogeneity of bacillus cereus sensu lato Isolated from ready-to-eat foods and powdered milk in day care centers in Colombia

Bacillus cereus sensu lato (s.l.) is a group of bacteria commonly found in diverse environments, including foods, with potential to cause emesis and diarrhea. In Colombia, it is one of the main foodborne pathogens. The aim of this study was to determine the genomic and toxigenic heterogeneity of B. cereus s.l. isolated from ready-to-eat foods and powdered milk collected in day care centers of Medellin, Colombia. Of 112 B. cereus s.l. isolates obtained, 94% were beta-hemolytic. Toxigenic heterogeneity was established by the presence of nheABC, hblCDAB, cytK2, entFM, and cesB toxigenic genes. The nheABC operon and entFM gene were most frequently detected in the isolates, whereas the cesB gene was not found. According to the toxin genes content, nine toxigenic profiles were identified. A 44% of isolates had profiles with all genes for nonhemolytic enterotoxin, hemolysin BL, and enterotoxin FM production (profiles II and IV). Pulsed-field gel electrophoresis analysis indicated a high genomic heterogeneity among the B. cereus s.l., with 68 isolates grouping into 16 clusters and 33 placed separately in the dendrogram. This study provides useful information on the safety of ready-to-eat foods and powdered milk in day care centers where children, a susceptible population, are exposed and it should incentive for more studies to understand the distribution of different toxin-encoding genes among B. cereus s.l. isolates, enabling detailed risk assessment

Study of star-forming galaxies in SDSS up to redshift 0.4: I. Metallicity evolution

The chemical composition of the gas in galaxies versus cosmic time provides a very important tool for understanding galaxy evolution. Although there are many studies at high redshift, they are rather scarce at lower redshifts. However, low redshift studies can provide important clues about the evolution of galaxies, furnishing the required link between local and high redshift universe. In this work we focus on the metallicity of the gas of star-forming galaxies at low redshift, looking for signs of chemical evolution. To analyze the metallicity contents star-forming galaxies of similar luminosities and masses at different redshifts. With this purpose, we present a study of the metallicity of relatively massive (log(M_star/M_sun)>10.5) star forming galaxies from SDSS--DR5 (Sloan Digital Sky Survey--Data Release 5), using different redshift intervals from 0.04 to 0.4. We used data processed with the STARLIGHT spectral synthesis code, correcting the fluxes for dust extinction, estimating metallicities using the R_23 method, and segregating the samples with respect to the value of the [NII]6583/[OII]3727 line ratio in order to break the R_23 degeneracy selecting the upper branch. We analyze the luminosity and mass-metallicity relations, and the effect of the Sloan fiber diameter looking for possible biases. By dividing our redshift samples in intervals of similar magnitude and comparing them, significant signs of metallicity evolution are found. Metallicity correlates inversely with redshift: from redshift 0 to 0.4 a decrement of ~0.1 dex in 12+log(O/H) is found.Comment: 11 pages, 9 figures, Accepted for publication in A&

Quyca Muysca: Urban Coloniality of Nature, Cuerpo-Territorio [Body-Territory], and Muysca Resurgence

This dissertation investigates the territorial dimensions of the Muysca community of Suba’s process of Indigenous resurgence through the ethical and methodological framework of Participatory Action Research (PAR). In drawing on the meanings and embodied practices attributed to, and associated with, territory by members of the Muysca community, I argue that the Muysca Indigenous resurgence movement both challenges processes of urban coloniality while also cultivating novel expressions of urban indigeneity. Building on three years of prior engagement with the community, in addition to twelve months of ethnographic research guided by PAR, in Bogota, Colombia, I analyzed archival material and employed ethnographic techniques such as in-depth participant observation, semi-structured interviews, participatory mapping, and visual methodologies. Informed by critical feminism, decolonial thought, and urban political ecology, I mobilize the Indigenous notion of cuerpo-territorio [body-territory] to analyze the Muysca urban experience in two interrelated aspects. First, I argue that encounters between the Muysca and the state are characterized by continuously being immersed within regimes of authenticity that structure how the Muysca interact and negotiate with governmental institutions toward territorial recognition and sovereignty. I particularly explore how the Muysca have embraced performance as an instrument mediating between the institutionalized demands for diacritic markers and the Muysca identity revitalization. Second, I present the notion of body-territory to highlight the relationship between the Muysca bodies and Suba. By examining Muysca meanings of territory, this study reconceptualizes space as an extension of the Muysca body. It presents the effects of urban coloniality on the Muysca, focusing on urban development, environmental degradation, urban planning policies, and the erasure of Muysca socioecological epistemologies. Nevertheless, I present how the Muysca of Suba contest this logic by engaging in everyday bodily practices of resurgence, such as the conservation of urban gardens called Muysca Tâ, the occupation of sacred natural places, and the revitalization of their language, Muysc cubun. In illustrating how the concept of body-territory provides an ontological foundation for approaching the experiential, semantic, performative, and contested aspects of the Muysca of Suba’s territorial struggles, this dissertation provides a novel lens through which to better understand urban indigeneity in the Global South

Mending Identity: The Revitalization Process of the Muisca of Suba

For over five centuries, the Muiscas have faced direct colonial aggression against their traditional belief systems and sacred practices that have been historically demonized and driven to the brink of extinction. Despite such circumstances, however, the Muisca community has thrived to the present day, and since the turn of the twentieth century has begun to undergo a process of re-identification as an indigenous community in an attempt to revitalize their ethnic identity and practices. These efforts of re-indigenization have challenged their historically coerced identities, actively engaging in returning to traditional practices and beliefs, demand cultural and spiritual liberties, and regain their proper rights to sacred lands, which have also been devastated for centuries. Based on an ethnographic study conducted in Colombia, this thesis examines how rituals in sacred places are of central importance to this community within the re-indigenization process that is currently underway in the Muisca community

Lindane and Endosulfan Sulfate Isomers in Crassostrea virginica (Gmelin, 1791) Oyster Populations in Lagoon Systems from Central Gulf of Mexico

The aim of this study was to determine Lindane and Endosulfan Sulfate isomers in Crassostrea virginica oyster populations (Gmelin, 1791) in the Mandinga and Alvarado lagoon systems located in the central Gulf of Mexico. Samples were taken from the main oyster banks of each lagoon system, during the three representative seasons of the region, wet, dry and north winds. By means of free diving, 30 commercial size oysters (7 ± 3 cm) were collected in four oyster banks or stations of the Mandinga lagoon system, totaling 360 organisms, while in the Alvarado lagoon system there were a total of 90 oysters during the annual cycle. Concentration of lindane and endosulfan sulfate isotopes in C. virginica was performed with a gas chromatograph (Thermo Electron Model Trace GC Ultra 115V, Thermo Fisher Scientific Inc©, Monterrey, Nuevo León, México) with an Electron capture detector. Results showed that in the Alvarado Lagoon system mean concentrations of C. virginica oysters for lindane pesticide were 4.11 ± 3.83 ng⋅g-1, whereas for the Mandinga lagoon system, were 8.69 ± 5.15 ng⋅g-1. Endosulfan sulfate showed the highest average concentration in the Mandinga lagoon system with 24.68 ± 1.20 ng ⋅g-1. In addition, the endosulfan sulfate presents differences in its spatial distribution; high concentration levels in the Mandinga lagoon system whereas the lindane heterogeneity at all sampling points in both lagoons. Values of concentrations and relationships between compounds suggest recent contributions that could correspond to the excessive fluctuations of water discharged into the lagoon caused by the atypical rains of the year of sampling. It was concluded that endosulfan sulfate and lindane show concentration in all the points of sampling in both lagoons

Embedding products in symmetric products of continua

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Study of the Largest Multiwavelength Campaign of the Microquasar GRS 1915+105

We present the results from a multiwavelength campaign of GRS 1915+105 performed from 2000 April 16 to 25. This is one of the largest coordinated set of observations ever performed for this source, covering the wide energy band in radio (13.3-0.3 cm), near-infrared (J-H-K), X-rays and Gamma-rays (from 1 keV to 10 MeV). During the campaign GRS 1915+105 was predominantly in the "plateau" (or low/hard) state but sometimes showed soft X-ray oscillations: before April 20.3, rapid, quasi-periodic (~= 45 min) flare-dip cycles were observed. The radio flares observed on April 17 shows frequency- dependent peak delay, consistent with an expansion of synchrotron-emitting region starting at the transition from the hard-dip to the soft-flare states in X-rays. On the other hand, infrared flares on April 20 appear to follow (or precede) the beginning of X-ray oscillations with an inconstant time delay of ~= 5-30 min. This implies that the infrared emitting region is located far from the black hole by >~ 10E13 cm, while its size is <~ 10E12 cm constrained from the time variability. We find a good correlation between the quasi-steady flux level in the near-infrared band and in the X-ray band. From this we estimate that the reprocessing of X-rays, probably occurring in the outer parts of the accretion disk, accounts for about 20-30% of the observed K magnitude in the plateau state. The OSSE spectrum in the 0.05-10 MeV band is represented by a single power law with a photon index of 3.1 extending to ~1 MeV with no cutoff. The power-law slope above ~30 keV is found to be very similar between different states in spite of large flux variations in soft X-rays, implying that the electron energy distribution is not affected by the change of the state in the accretion disk.Comment: 31 pages, 11 figures. Accepted for publication in ApJ, vol. 571, 2002. Minor corrections. Figure 2 is revised (numbers on the top axis are corrected). References are update