The crafting of hope: Contextualising add-ons in the treatment trajectories of IVF patients

The proliferation and popularity of additional treatments in IVF, also known as add-ons, has generated widespread discussion and controversy in the UK, where concerns have addressed the lack of evidence to support the efficacy and safety of these treatments, their cost, and their connection to a wider context of privatisation of fertility treatment. Drawing on 42 interviews with IVF patients, this article explores the role of hope in the appeal of add-ons from the patient perspective. The analysis is presented in two parts: firstly, we investigate the role of hope in patients’ decision-making on treatment, contextualising add-ons in the broader trajectory of their IVF experience; secondly, we examine how patients navigate the offer of add-ons, focusing on the role of hope in how they rationalise their decisions on whether to include them in their fertility treatment. Our analysis shows how patients craft their hope to navigate the increasing number of available options in their quest to find the treatment(s) that will “work” for them. We suggest that the imperative for patients to explore all options is intensified with the emergence of add-ons, which produces a novel context and version of a “hope technology”

Using interview excerpts to facilitate focus group discussion

The use of interviews and focus groups is well-established in the social science methods literature. However, discussion on how research can combine these two methods in creative ways is less common. While researchers are generally aware of the potential of focus groups for further probing issues that emerge in one-on-one interviews, few studies detail how this might be achieved in practice. In this article, we describe and reflect on a focus group elicitation strategy that uses individual interview excerpts to facilitate discussion in group settings. In our reflection, we draw on a study that investigated the sharing of embryo images in fertility treatment. The article contributes to the methods literature firstly, by reflecting on the novel use of individual interview material in focus groups and secondly, by discussing the re-enactment of interview excerpts as an effective audio elicitation tool to be used in the later stages of research

Numerical study of halo concentrations in dark-energy cosmologies

We study the concentration parameters, their mass dependence and redshift evolution, of dark-matter halos in different dark-energy cosmologies with constant and time-variable equation of state, and compare them with "standard'' Lambda-CDM and OCDM models. We find that previously proposed algorithms for predicting halo concentrations can be well adapted to dark-energy models. When centred on the analytically expected values, halo concentrations show a log-normal distribution with a uniform standard deviation of ~0.2. The dependence of averaged halo concentrations on mass and redshift permits a simple fit of the form (1+z) c=c0 (M/M0)^a, with a~-0.1 throughout. We find that the cluster concentration depends on the dark energy equation of state at the cluster formation redshift z_{coll} through the linear growth factor D_+(z_{coll}). As a simple correction accounting for dark-energy cosmologies, we propose scaling c0 from Lambda-CDM with the ratio of linear growth factors, c0 -> c0 D_+(z_{coll})/D_{+,Lambda-CDM}(z_{coll}).Comment: 11 pages, submitted to Astronomy & Astrophysic

Winds as the origin of radio emission in z=2.5z=2.5 radio-quiet extremely red quasars

Most active galactic nuclei (AGNs) are radio-quiet, and the origin of their radio emission is not well-understood. One hypothesis is that this radio emission is a by-product of quasar-driven winds. In this paper, we present the radio properties of 108 extremely red quasars (ERQs) at $z=2-4$. ERQs are among the most luminous quasars ($L_{bol} \sim 10^{47-48}$ erg/s) in the Universe, with signatures of extreme ($\gg 1000$ km/s) outflows in their [OIII]$\lambda$5007 \AA\ emission, making them the best subjects to seek the connection between radio and outflow activity. All ERQs but one are unresolved in the radio on $\sim 10$ kpc scales, and the median radio luminosity of ERQs is $\nu L_\nu [{\rm 6\,GHz}] = 10^{41.0}$ erg/s, in the radio-quiet regime, but one to two orders of magnitude higher than that of other quasar samples. The radio spectra are steep, with a mean spectral index $\langle \alpha \rangle = -1.0$. In addition, ERQs neatly follow the extrapolation of the low-redshift correlation between radio luminosity and the velocity dispersion of [OIII]-emitting ionized gas. Uncollimated winds, with a power of one per cent of the bolometric luminosity, can account for all these observations. Such winds would interact with and shock the gas around the quasar and in the host galaxy, resulting in acceleration of relativistic particles and the consequent synchrotron emission observed in the radio. Our observations support the picture in which ERQs are signposts of extremely powerful episodes of quasar feedback, and quasar-driven winds as a contributor of the radio emission in the intermediate regime of radio luminosity $\nu L_\nu = 10^{39}-10^{42}$ erg/s.Comment: accepted by MNRA

Identificação de minerais do grupo das zeólitas por espectroscopia de reflectância, para aplicação como remineralizadores de solo.

A utilização de zeólitas para melhorar a qualidade do solo destinado à agricultura ganha espaço em todo o mundo. A elevada capacidade de troca catiônica das zeólitas favorece a conservação de nutrientes no solo e, a alta capacidade de retenção de água em seus retículos cristalinos faz destes minerais excelentes condicionadores de solo. A ausência de depósitos de zeólitas em exploração no Brasil torna os basaltos da Formação Serra Geral da Bacia do Paraná um alvo com grande potencial para a prospecção por zeólitas naturais. Pesquisas da CPRM destacam a significativa presença de zeólitas especialmente no contato entre os derrames inferiores da Formação Serra Geral e os arenitos eólicos da Formação Botucatu no Rio Grande do Sul. A espectroscopia de reflectância é uma ferramenta capaz de contribuir para a identificação de zeólitas em campo ou laboratório, utilizando-se de análises rápidas e de baixo custo. O conhecimento prévio do comportamento espectral das zeólitas é de grande utilidade na prospecção de alvos potenciais na Formação Serra Geral (pilhas de lobos e brechas de topo de derrames basálticos). Nestas ambiências foram reconhecidas macroscopicamente heulandita, escolecita, estilbita, laumontita e mordenita. O presente trabalho apresenta os resultados de leituras em amostras representativas das paragêneses que caracterizam os diferentes blocos determinados pelo Projeto Agrominerais Bacia do Paraná no Rio Grande do Sul-CPRM, com uso do espectrorradiômetro FieldSpec 3 Hi-Res© - ASD, de resolução espectral entre 0,35 e 2,5 μm. Foram identificadas curvas espectrais referentes à estilbita, heulandita, laumontita, mordenita e possivelmente analcima e clinoptilolita, localmente associadas à calcita. Por meio de assinaturas espectrais poderão ser construídos padrões para as zeólitas, para classificação de imagens de satélite, devendo-se considerar a relação entre a dimensão dos alvos e as resoluções espaciais e espectrais dos sensores orbitais e aeroportados disponíveis para o imageamento da área de pesquisa

Astrophysical and Cosmological Information from Large-scale sub-mm Surveys of Extragalactic Sources

We present a quantitative analysis of the astrophysical and cosmological information that can be extracted from the many important wide-area, shallow surveys that will be carried out in the next few years. Our calculations combine the predictions of the physical model by Granato et al. (2004) for the formation and evolution of spheroidal galaxies with up-to-date phenomenological models for the evolution of starburst and normal late-type galaxies and of radio sources. We compute the expected number counts and the redshift distributions of these source populations separately and then focus on proto-spheroidal galaxies. For the latter objects we predict the counts and redshift distributions of strongly lensed sources at 250, 350, 500, and 850 micron, the angular correlation function of sources detected in the surveys considered, the angular power spectra due to clustering of sources below the detection limit in Herschel and Planck surveys. An optimal survey for selecting strongly lensed proto-spheroidal galaxies is described, and it is shown how they can be easily distinguished from the other source populations. We also discuss the detectability of the imprints of the 1-halo and 2-halo regimes on angular correlation functions and clustering power spectra, as well as the constraints on cosmological parameters that can be obtained from the determinations of these quantities. The novel data relevant to derive the first sub-millimeter estimates of the local luminosity functions of starburst and late-type galaxies, and the constraints on the properties of rare source populations, such as blazars, are also briefly described.Comment: 16 pages, 10 figures. Accepted for publication on MNRA

Neurophysiological Profile of Antismoking Campaigns

Over the past few decades, antismoking public service announcements (PSAs) have been used by governments to promote healthy behaviours in citizens, for instance, against drinking before the drive and against smoke. Effectiveness of such PSAs has been suggested especially for young persons. By now, PSAs efficacy is still mainly assessed through traditional methods (questionnaires and metrics) and could be performed only after the PSAs broadcasting, leading to waste of economic resources and time in the case of Ineffective PSAs. One possible countermeasure to such ineffective use of PSAs could be promoted by the evaluation of the cerebral reaction to the PSA of particular segments of population (e.g., old, young, and heavy smokers). In addition, it is crucial to gather such cerebral activity in front of PSAs that have been assessed to be effective against smoke (Effective PSAs), comparing results to the cerebral reactions to PSAs that have been certified to be not effective (Ineffective PSAs). &e eventual differences between the cerebral responses toward the two PSA groups will provide crucial information about the possible outcome of new PSAs before to its broadcasting. &is study focused on adult population, by investigating the cerebral reaction to the vision of different PSA images, which have already been shown to be Effective and Ineffective for the promotion of an antismoking behaviour. Results showed how variables as gender and smoking habits can influence the perception of PSA images, and how different communication styles of the antismoking campaigns could facilitate the comprehension of PSA’s message and then enhance the related impac

The Ventasso Horse: genetic characterization by microsatellites markers

The genetic structure of Ventasso Horse (VH) was investigated using 12 microsatellites. The analyses were carried out on 117 VH individuals and the results were compared with those obtained analysing 11 other breeds reared in Italy. All microsatellites were polymorphic in VH and in the other breeds. A total of 124 alleles (from 6 to 19 alleles per microsatellite) were detected. Average heterozygosity was 0.743 in VH and ranged from 0.613 to 0.759 in the other breeds. The mean FST value had an average value of 0.0932. Genetic distances were calculated using Nei's standard genetic distance (Ds). The smallest Ds values were found between VH and Anglo-Arab, Thoroughbred, Maremmano and Lipizzan horse breeds. Phylogenetic trees constructed using neighbour-joining method showed two clear separate clusters: the first includes Bardigiano, Haflinger and Italian Heavy Draught Horse, the second contains the other 9 breeds

The active optics software for the VST telescope

The VST (VLT Survey Telescope) active optics software must basically provide the analysis of the image coming from the wavefront sensor (a 10x10 subpupils Shack Hartmann device) and the calculation of primary mirror forces and secondary mirror displacements to correct the aberrations of the optical system, instrinsic or originated for thermal and gravity reasons. After the telescope commissioning the VST will be operated by ESO. In this framework, INAF-OAC staff was committed to design and realize the software in a VLT-compliant way. This will smoothen the integration, operation and maintenance of the telescope in the Paranal observatory