Entrapment of HETS recombinant protein onto PLGA and alginate NPs improves the immunogenicity of the protein against E. coli O157:H7.

Enterohemorrhagic Escherichia coli (EHEC) are known as the gastrointestinal pathogens and major causes of enterohemorrhagic colitis since decades ago. There is no efficient approved vaccine against EHEC O157 and non-O157. In the present study, a recombinant candidate vaccine against enterohemorrhagic E. coli (EHEC) O157:H7 entrapped in the sodium alginate and PLGA nanoparticles and the efficiency of the immunization of these formulations were investigated. nanoparticles due to their properties like controlled cargoes release, adjuvanticity, cargo protection, increased bioavailability, etc have been noticed for drug delivery. A chimeric protein composed of HcpA, EspA, Tir and Stx2B antigens was designed, recombinantly expressed, purified and entrapped in nanoparticles. BALB/c mice were administrated with nano-formulated and free proteins. IgG titer, EHEC fecal shedding and the ability of the immune sera to neutralize Stx toxin and inhibit the bacterial attachment to Caco-2 cells were analyzed. Fecal shedding analysis demonstrated that the colonization of the bacteria in the intestine of the mice was reduced significantly (P > 0.01). Immune mice were able to tolerate up to 200 LD50 of the active Stx toxin. About 80% of the bacterial binding capacity to Caco-2 cells was declined, especially in groups immunized with nano-formulations. Considering the importance of EHEC, especially O157 serotype, on public health and the other hand, the lack of an efficient vaccine in this regard, delivery of HETS candidate vaccine with NPs can be applied to prevent the infection by the pathogen.

The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment.

The carriers of the diffuse interstellar bands (DIBs) are largely unidentified molecules ubiquitously present in the interstellar medium (ISM). After decades of study, two strong and possibly three weak near-infrared DIBs have recently been attributed to the [Formula: see text] fullerene based on observational and laboratory measurements. There is great promise for the identification of the over 400 other known DIBs, as this result could provide chemical hints towards other possible carriers. In an effort to systematically study the properties of the DIB carriers, we have initiated a new large-scale observational survey: the ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES). The main objective is to build on and extend existing DIB surveys to make a major step forward in characterising the physical and chemical conditions for a statistically significant sample of interstellar lines-of-sight, with the goal to reverse-engineer key molecular properties of the DIB carriers. EDIBLES is a filler Large Programme using the Ultraviolet and Visual Echelle Spectrograph at the Very Large Telescope at Paranal, Chile. It is designed to provide an observationally unbiased view of the presence and behaviour of the DIBs towards early-spectral type stars whose lines-of-sight probe the diffuse-to-translucent ISM. Such a complete dataset will provide a deep census of the atomic and molecular content, physical conditions, chemical abundances and elemental depletion levels for each sightline. Achieving these goals requires a homogeneous set of high-quality data in terms of resolution (R ~ 70 000 - 100 000), sensitivity (S/N up to 1000 per resolution element), and spectral coverage (305-1042 nm), as well as a large sample size (100+ sightlines). In this first paper the goals, objectives and methodology of the EDIBLES programme are described and an initial assessment of the data is provided.