128 research outputs found
Expression of mesenchymal stem cell marker CD90 on dermal sheath cells of the anagen hair follicle in canine species
The dermal sheath (DS) of the hair follicle is comprised by fibroblast-like cells and extends along the follicular epithelium, from the bulb up to the infundibulum. From this structure, cells with stem characteristics were isolated: they have a mesenchymal origin and express CD90 protein, a typical marker of mesenchymal stem cells. It is not yet really clear in which region of hair follicle these cells are located but some experimental evidence suggests that dermal stem cells are localized prevalently in the lower part of the anagen hair follicle
The presence and localization of apelin in the sheep abomasum: impact of diets characterized by different chemical composition
The apelinergic system is a complex system including the apelin peptide (AP), initially isolated in 1998 from bovine stomach homogenates and its receptor, named APJ receptor. The apelin peptide is extensively expressed in several human and laboratory animal organs (heart, lung, brain, mammary gland). Between the different roles hypothesize for apelin there are also the control of blood pressure and the stimulation of drinking behavior in rats. Recently its expression was also evidenced in the basal glandular portion of the stomach in laboratory animals, allowing to hypothesize its intervention in the control of acid secretion. No data concerning its presence and distribution in the abomasums of the sheep are present at the moment. So, we decided to test the presence and distribution of apelin in the abomasums of the sheep and the possible existence of a variability as a consequence of the different water content of the diet.The experiment was conducted using 50 sheep fed on Apennine semi-natural pasture for two experimental periods: in the first period the animals were fed for 45 days on the pasture at the maximum of its flowering; in the second one the animals were fed on the same pasture until its maximum dryness but the half of them daily received adiet integration of cereals. At the end of each experimental period, some animals were regularly slaughtered at the local abattoir, the abomasum specimens were immediately removed and some of them processed for routine tissue-embedding preparation while other for molecular biology.
The immunohistochemical reaction was visualized on 5 µm serial sections, using a primary rabbit polyclonal antibody (anti-AP), the avidin-biotin-complex and the DAB as the chromogen.
The immunohistochemical study showed a peculiar immunoreaction for AP in the abomasum of the animals examined. In particular, a immunopositive reaction for AP was evident in the cells of the basal third of the tubular glands and they were mainly of the closed type, with an oval or round shape and contained many perinuclear granules. The immunopositive reactions didn’t evidence any difference both in the localization and in the number of the positive cells, between the different groups. Immuno-positivity for AP was not observed in any other histological structure or in the sections utilized as negative controls.These results allow us to conclude that AP is present in the glandular tissue of the abomasums of the sheep, as observed in laboratory animals, with a peculiar cytoplasmatic localization and to hypothesize that AP is involved in the control of gastric secretion, probably via APJ receptor. The AP expression in the stomach doesn’t seem to be influenced by the water content of the diets with a positivity that appears to be localized in the same glandular portion between the different animal groups
The Circumgalactic Medium in Massive Halos
This chapter presents a review of the current state of knowledge on the cool
(T ~ 1e4 K) halo gas content around massive galaxies at z ~ 0.2-2. Over the
last decade, significant progress has been made in characterizing the cool
circumgalactic gas in massive halos of Mh ~ 1e12-1e14 Msun at intermediate
redshifts using absorption spectroscopy. Systematic studies of halo gas around
massive galaxies beyond the nearby universe are made possible by large
spectroscopic samples of galaxies and quasars in public archives. In addition
to accurate and precise constraints for the incidence of cool gas in massive
halos, detailed characterizations of gas kinematics and chemical compositions
around massive quiescent galaxies at z ~ 0.5 have also been obtained. Combining
all available measurements shows that infalling clouds from external sources
are likely the primary source of cool gas detected at d >~ 100 kpc from massive
quiescent galaxies. The origin of the gas closer in is currently less certain,
but SNe Ia driven winds appear to contribute significantly to cool gas found at
d < 100 kpc. In contrast, cool gas observed at d <~ 200 kpc from luminous
quasars appears to be intimately connected to quasar activities on parsec
scales. The observed strong correlation between cool gas covering fraction in
quasar host halos and quasar bolometric luminosity remains a puzzle. Combining
absorption-line studies with spatially-resolved emission measurements of both
gas and galaxies is the necessary next step to address remaining questions.Comment: 29 pages, 7 figures, invited review to appear in "Gas Accretion onto
Galaxies", Astrophysics and Space Science Library, eds. A. Fox & R. Dave, to
be published by Springe
Perfluoroalkyl substances, sex hormones, and insulin-like growth factor-1 at 6–9 Years of age : a cross-sectional analysis within the C8 health project
Background: Exposure to some perfluoroalkyl substances (PFAS), such as perfluorohexane sulfonate
(PFHxS), perfluorooctanoate (PFOA), perfluorooctane sulfonate (PFOS), and perfluorononanoic acid
(PFNA), may alter levels of sex hormones and insulin-like growth factor-1 (IGF-1) in animals. Human
studies on this topic are scarce and none have been conducted in young children.
Objectives: To investigate the relationship between levels of PFAS and estradiol, total testosterone and
IGF-1 in 2,292 children (aged 6-9 years) from the C8 Health Project living near a chemical plant in the
Mid-Ohio Valley (USA) with local contamination from PFOA.
Methods: Serum samples were collected in 2005-2006 and analyzed for PFAS, sex hormones and
IGF-1. Results from regression models were expressed as the adjusted percentage difference (95% CI)
per sex-specific interquartile range (IQR) increment of each PFAS serum concentration. Analyses by
PFAS quartiles were also conducted.
Results: Median concentrations of PFHxS, PFOA, PFOS, and PFNA were 8, 35, 22, and 1.7 ng/mL in
boys and 7, 30, 21, and 1.7 ng/mL in girls. In boys, PFOA concentrations were significantly associated
with testosterone levels (-4.9% [-8.7, -0.8%]); PFOS with estradiol (-4.0% [-7.7, -0.1%]), testosterone
(-5.8% [-9.4, -2.0%]), and IGF-1 (-5.9% [-8.3, -3.3%]); and PFNA with IGF-1 (-3.5% [-6.0, -1.0%]). In
girls, significant associations were found between PFOS and testosterone (-6.6% [-10.1, -2.8%]) and
IGF-1 (-5.6% [-8.2, -2.9%]); and PFNA and IGF-1 (-3.8% [-6.4, -1.2%]). In both sexes, the magnitudes
of the associations decreased monotonically across quartiles for testosterone and PFOS, and for IGF-1
and both PFOS and PFNA.
Conclusions: To our knowledge, this is the first study suggesting that PFAS are associated with lowe
A multi-disciplinary perspective on emergent and future innovations in peer review [version 2; referees: 2 approved]
Peer review of research articles is a core part of our scholarly communication system. In spite of its importance, the status and purpose of peer review is often contested. What is its role in our modern digital research and communications infrastructure? Does it perform to the high standards with which it is generally regarded? Studies of peer review have shown that it is prone to bias and abuse in numerous dimensions, frequently unreliable, and can fail to detect even fraudulent research. With the advent of web technologies, we are now witnessing a phase of innovation and experimentation in our approaches to peer review. These developments prompted us to examine emerging models of peer review from a range of disciplines and venues, and to ask how they might address some of the issues with our current systems of peer review. We examine the functionality of a range of social Web platforms, and compare these with the traits underlying a viable peer review system: quality control, quantified performance metrics as engagement incentives, and certification and reputation. Ideally, any new systems will demonstrate that they out-perform and reduce the biases of existing models as much as possible. We conclude that there is considerable scope for new peer review initiatives to be developed, each with their own potential issues and advantages. We also propose a novel hybrid platform model that could, at least partially, resolve many of the socio-technical issues associated with peer review, and potentially disrupt the entire scholarly communication system. Success for any such development relies on reaching a critical threshold of research community engagement with both the process and the platform, and therefore cannot be achieved without a significant change of incentives in research environments
Galaxy counterparts of intervening high-z sub-DLAs/DLAs and MgII absorbers towards gamma-ray bursts
We present the first search for galaxy counterparts of intervening high-z
(2<z< 3.6) sub-DLAs and DLAs towards GRBs. Our final sample comprises of five
intervening sub-DLAs and DLAs in four GRB fields. To identify candidate galaxy
counterparts of the absorbers we use deep optical and near-infrared imaging,
and low-, mid- and high-resolution spectroscopy acquired with 6 to 10-m class
telescopes, the Hubble and the Spitzer space telescopes. Furthermore, we use
the spectroscopic information and spectral-energy-distribution fitting
techniques to study them in detail. Our main result is the detection and
spectroscopic confirmation of the galaxy counterpart of the intervening DLA at
z=3.096 in the field of GRB 070721B (z_GRB=3.6298) as proposed by other
authors. We also identify good candidates for the galaxy counterparts of the
two strong MgII absorbers at z=0.6915 and 1.4288 towards GRB 050820A
(z_GRB=2.615). The properties of the detected DLA galaxy are typical for
Lyman-break galaxies (LBGs) at similar redshifts; a young, highly starforming
galaxy that shows evidence for a galactic outflow. This supports the hypothesis
that a DLA can be the gaseous halo of an LBG. In addition, we report a redshift
coincidence of different objects associated with metal lines in the same field,
separated by 130-161 kpc. The high detection rate of three correlated
structures on a length scale as small as ~150 kpc in two pairs of lines of
sight is intriguing. The absorbers in each of these are most likely not part of
the same gravitationally bound structure. They more likely represent groups of
galaxies.Comment: A&A, accepted; 20 pages in journal format; 12 pages main text, 1 page
references, 1 page appendix, 14 figures, 8 tables. Note, Tables 1 and 4 look
different than in the journal but are identica
Roles of type II thioesterases and their application for secondary metabolite yield improvement
L'Italia come modello per l'Europa e per il mondo nelle politiche sanitarie per il trattamento dell'epatite cronica da HCV
The World Health Organization foresees the
elimination of HCV infection by 2030. In light of this and the curre
nt, nearly worldwide, restriction in direct-acting agents
(DAA) accessibility due to their high price, we aimed to evaluate
the cost-effectiveness of two alternative DAA treatment
policies: Policy 1 (universal): treat all patients, regardless of the fibrosis stage; Policy 2 (prioritized): treat only priori
tized
patients and delay treatment of the
remaining patients until reaching stage F3. T
he model was based on patient’s data
from the PITER cohort. We demonstrated that extending HC
V treatment of patients in any fibrosis stage improves health
outcomes and is cost-effective
A multi-disciplinary perspective on emergent and future innovations in peer review
Peer review of research articles is a core part of our scholarly communication system. In spite of its importance, the status and purpose of peer review is often contested. What is its role in our modern digital research and communications infrastructure? Does it perform to the high standards with which it is generally regarded? Studies of peer review have shown that it is prone to bias and abuse in numerous dimensions, frequently unreliable, and can fail to detect even fraudulent research. With the advent of web technologies, we are now witnessing a phase of innovation and experimentation in our approaches to peer review. These developments prompted us to examine emerging models of peer review from a range of disciplines and venues, and to ask how they might address some of the issues with our current systems of peer review. We examine the functionality of a range of social Web platforms, and compare these with the traits underlying a viable peer review system: quality control, quantified performance metrics as engagement incentives, and certification and reputation. Ideally, any new systems will demonstrate that they out-perform and reduce the biases of existing models as much as possible. We conclude that there is considerable scope for new peer review initiatives to be developed, each with their own potential issues and advantages. We also propose a novel hybrid platform model that could, at least partially, resolve many of the socio-technical issues associated with peer review, and potentially disrupt the entire scholarly communication system. Success for any such development relies on reaching a critical threshold of research community engagement with both the process and the platform, and therefore cannot be achieved without a significant change of incentives in research environments
Geomorphological controls on the evolution of Adriatic historical cities (Central Italy), determined using contemporary maps and art.
The geomorphological analysis of historically urbanized areas provides an irreplaceable scientific basis to understand how geomorphological factors
conditioned urbanization and it also gives us a baseline for comparison with the modern environment. Recently the mass digitization and resulting online access to old maps and art prints have vastly increased the amount of usable materials available for integrated analysis. This paper considers three urbanized historical sites on the Adriatic coast (Central Italy): Rimini, Pesaro, and Fano, which owe their urban development to particular geomorphological and environmental conditions modified over the centuries from the Roman age to present time. The focus here is on the evolution of the shoreline and the geomorphic variables associated with river mouths. These factors are fundamental for determining the development of the city, both as basic boundary elements – and therefore includes defence and protection – and also for development of the harbours. The studied areas are characterized by very detailed and precise contemporaneous cartographic documentation and artistic representations. The integrated analysis of
these sites represents another important tool for urban planning, not to mention a primary data source for historical urban planning. Perhaps a deeper understanding of the rates of geomorphological change in a historical time frame can lead to smarter plans that do not assume a fixed unchanging nature for the physical elements upon which older plans rested
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