1,478 research outputs found
Poloxomer 188 Has a Deleterious Effect on Dystrophic Skeletal Muscle Function
Duchenne muscular dystrophy (DMD) is an X-linked, fatal muscle wasting disease for which there is currently no cure and limited palliative treatments. Poloxomer 188 (P188) is a tri-block copolymer that has been proposed as a potential treatment for cardiomyopathy in DMD patients. Despite the reported beneficial effects of P188 on dystrophic cardiac muscle function, the effects of P188 on dystrophic skeletal muscle function are relatively unknown. Mdx mice were injected intraperitoneally with 460 mg/kg or 30 mg/kg P188 dissolved in saline, or saline alone (control). The effect of single-dose and 2-week daily treatment was assessed using a muscle function test on the Tibialis Anterior (TA) muscle in situ in anaesthetised mice. The test comprises a warm up, measurement of the force-frequency relationship and a series of eccentric contractions with a 10% stretch that have previously been shown to cause a drop in maximum force in mdx mice. After 2 weeks of P188 treatment at either 30 or 460 mg/kg/day the drop in maximum force produced following eccentric contractions was significantly greater than that seen in saline treated control mice (Pâ=â0.0001). Two week P188 treatment at either dose did not significantly change the force-frequency relationship or maximum isometric specific force produced by the TA muscle. In conclusion P188 treatment increases susceptibility to contraction-induced injury following eccentric contractions in dystrophic skeletal muscle and hence its suitability as a potential therapeutic for DMD should be reconsidered
Targeting FLT3 in primary MLL-gene-rearranged infant acute lymphoblastic leukemia
Acute lymphoblastic leukemia (ALL) in infants is characterized by
rearrangements of the mixed lineage leukemia (MLL) gene, drug resistance,
and a poor treatment outcome. Therefore, novel therapeutic strategies are
needed to improve prognosis. Recently, we showed that FLT3 is highly
expressed in MLL rearranged ALL (MLL). Here we demonstrate FLT3 expression
in infants with MLL (n = 41) to be significantly higher compared to both
infant (n = 8; P < .001) and noninfant patients with ALL (n = 23; P =
.001) carrying germline MLL genes. Furthermore, leukemic cells from
infants with MLL were significantly more sensitive to the Fms-like
tyrosine kinase 3 (FLT3) inhibitor PKC412 (N-benzoyl staurosporine) than
noninfant ALL cells, and at least as sensitive as internal tandem
duplication-positive (ITD+) AML cells. Surprisingly, activation loop
mutations only occurred in about 3% (1 of 36) of the cases and no
FLT3/ITDs were observed. However, measuring FLT3 phosphorylation in
infants with MLL expressing varying levels of wild-type FLT3 revealed that
high-level FLT3 expression is associated with ligand-independent FLT3
activation. This suggests that infant MLL cells displaying activated FLT3
as a result of overexpression can be targeted by FLT3 inhibitors such as
PKC412. However, at concentrations of PKC412 minimall
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger
Observatory and is used to detect the radio emission of cosmic-ray air showers.
These observations are compared to the data of the surface detector stations of
the Observatory, which provide well-calibrated information on the cosmic-ray
energies and arrival directions. The response of the radio stations in the 30
to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of
the incoming electric field. For the latter, the energy deposit per area is
determined from the radio pulses at each observer position and is interpolated
using a two-dimensional function that takes into account signal asymmetries due
to interference between the geomagnetic and charge-excess emission components.
The spatial integral over the signal distribution gives a direct measurement of
the energy transferred from the primary cosmic ray into radio emission in the
AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air
shower arriving perpendicularly to the geomagnetic field. This radiation energy
-- corrected for geometrical effects -- is used as a cosmic-ray energy
estimator. Performing an absolute energy calibration against the
surface-detector information, we observe that this radio-energy estimator
scales quadratically with the cosmic-ray energy as expected for coherent
emission. We find an energy resolution of the radio reconstruction of 22% for
the data set and 17% for a high-quality subset containing only events with at
least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO
Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory
A measurement of the cosmic-ray spectrum for energies exceeding
eV is presented, which is based on the analysis of showers
with zenith angles greater than detected with the Pierre Auger
Observatory between 1 January 2004 and 31 December 2013. The measured spectrum
confirms a flux suppression at the highest energies. Above
eV, the "ankle", the flux can be described by a power law with
index followed by
a smooth suppression region. For the energy () at which the
spectral flux has fallen to one-half of its extrapolated value in the absence
of suppression, we find
eV.Comment: Replaced with published version. Added journal reference and DO
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
We measure the energy emitted by extensive air showers in the form of radio
emission in the frequency range from 30 to 80 MHz. Exploiting the accurate
energy scale of the Pierre Auger Observatory, we obtain a radiation energy of
15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV
arriving perpendicularly to a geomagnetic field of 0.24 G, scaling
quadratically with the cosmic-ray energy. A comparison with predictions from
state-of-the-art first-principle calculations shows agreement with our
measurement. The radiation energy provides direct access to the calorimetric
energy in the electromagnetic cascade of extensive air showers. Comparison with
our result thus allows the direct calibration of any cosmic-ray radio detector
against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI.
Supplemental material in the ancillary file
Mineral Detection of Neutrinos and Dark Matter 2024. Proceedings
The second "Mineral Detection of Neutrinos and Dark Matter" (MDvDM'24)
meeting was held January 8-11, 2024 in Arlington, VA, USA, hosted by Virginia
Tech's Center for Neutrino Physics. This document collects contributions from
this workshop, providing an overview of activities in the field. MDvDM'24 was
the second topical workshop dedicated to the emerging field of mineral
detection of neutrinos and dark matter, following a meeting hosted by IFPU in
Trieste, Italy in October 2022. Mineral detectors have been proposed for a wide
variety of applications, including searching for dark matter, measuring various
fluxes of astrophysical neutrinos over gigayear timescales, monitoring nuclear
reactors, and nuclear disarmament protocols; both as paleo-detectors using
natural minerals that could have recorded the traces of nuclear recoils for
timescales as long as a billion years and as detectors recording nuclear recoil
events on laboratory timescales using natural or artificial minerals.
Contributions to this proceedings discuss the vast physics potential, the
progress in experimental studies, and the numerous challenges lying ahead on
the path towards mineral detection. These include a better understanding of the
formation and annealing of recoil defects in crystals; identifying the best
classes of minerals and, for paleo-detectors, understanding their geology;
modeling and control of the relevant backgrounds; developing, combining, and
scaling up imaging and data analysis techniques; and many others. During the
last years, MDvDM has grown rapidly and gained attention. Small-scale
experimental efforts focused on establishing various microscopic readout
techniques are underway at institutions in North America, Europe and Asia. We
are looking ahead to an exciting future full of challenges to overcome,
surprises to be encountered, and discoveries lying ahead of us.Comment: Summary and proceedings of the MDvDM'24 conference, Jan 8-11 202
Pathways to cellular supremacy in biocomputing
Synthetic biology uses living cells as the substrate for performing human-defined computations. Many current implementations of cellular computing are based on the âgenetic circuitâ metaphor, an approximation of the operation of silicon-based computers. Although this conceptual mapping has been relatively successful, we argue that it fundamentally limits the types of computation that may be engineered inside the cell, and fails to exploit the rich and diverse functionality available in natural living systems. We propose the notion of âcellular supremacyâ to focus attention on domains in which biocomputing might offer superior performance over traditional computers. We consider potential pathways toward cellular supremacy, and suggest application areas in which it may be found.A.G.-M. was supported by the SynBio3D project of the UK Engineering and Physical Sciences Research Council (EP/R019002/1) and the European CSA on biological standardization BIOROBOOST (EU grant number 820699). T.E.G. was supported by a Royal Society University Research Fellowship (grant UF160357) and BrisSynBio, a BBSRC/ EPSRC Synthetic Biology Research Centre (grant BB/L01386X/1). P.Z. was supported by the EPSRC Portabolomics project (grant EP/N031962/1). P.C. was supported by SynBioChem, a BBSRC/EPSRC Centre for Synthetic Biology of Fine and Specialty Chemicals (grant BB/M017702/1) and the ShikiFactory100 project of the European Unionâs Horizon 2020 research and innovation programme under grant agreement 814408
The WSES/SICG/ACOI/SICUT/AcEMC/SIFIPAC guidelines for diagnosis and treatment of acute left colonic diverticulitis in the elderly
Acute left colonic diverticulitis (ALCD) in the elderly presents with unique epidemiological features when compared with younger patients. The clinical presentation is more nuanced in the elderly population, having higher in-hospital and postoperative mortality. Furthermore, geriatric comorbidities are a risk factor for complicated diverticulitis. Finally, elderly patients have a lower risk of recurrent episodes and, in case of recurrence, a lower probability of requiring urgent surgery than younger patients. The aim of the present work is to study age-related factors that may support a unique approach to the diagnosis and treatment of this problem in the elderly when compared with the WSES guidelines for the management of acute left-sided colonic diverticulitis. During the 1 degrees Pisa Workshop of Acute Care & Trauma Surgery held in Pisa (Italy) in September 2019, with the collaboration of the World Society of Emergency Surgery (WSES), the Italian Society of Geriatric Surgery (SICG), the Italian Hospital Surgeons Association (ACOI), the Italian Emergency Surgery and Trauma Association (SICUT), the Academy of Emergency Medicine and Care (AcEMC) and the Italian Society of Surgical Pathophysiology (SIFIPAC), three panel members presented a number of statements developed for each of the four themes regarding the diagnosis and management of ALCD in older patients, formulated according to the GRADE approach, at a Consensus Conference where a panel of experts participated. The statements were subsequently debated, revised, and finally approved by the Consensus Conference attendees. The current paper is a summary report of the definitive guidelines statements on each of the following topics: diagnosis, management, surgical technique and antibiotic therapy.Peer reviewe
- âŠ