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Dark matter constraints from a joint analysis of dwarf Spheroidal galaxy observations with VERITAS
(2017)
We present constraints on the annihilation cross section of weakly interacting massive particles dark matter based on the joint statistical analysis of four dwarf galaxies with VERITAS. These results are derived from an optimized photon weighting statistical technique that improves on standard imaging atmospheric Cherenkov telescope (IACT) analyses by utilizing the spectral and spatial properties of individual photon events. We report on the results of similar to 230 hours of observations of five dwarf galaxies and the joint statistical analysis of four of the dwarf galaxies. We find no evidence of gamma-ray emission from any individual dwarf nor in the joint analysis. The derived upper limit on the dark matter annihilation cross section from the joint analysis is 1.35 x 10(-23) cm(3) s(-1) at 1 TeV for the bottom quark (b (b) over bar) final state, 2.85 x 10(-24) cm(3) s(-1) at 1 TeV for the tau lepton (tau+tau(-)) final state and 1.32 x 10-25 cm(3) s(-1) at 1 TeV for the gauge boson (gamma gamma) final state.
Aims. We present an extensive study of the BL Lac object Mrk 501 based on a data set collected during the multi-instrument campaign spanning from 2009 March 15 to 2009 August 1, which includes, among other instruments, MAGIC, VERITAS, Whipple 10 m, and Fermi-LAT to cover the gamma-ray range from 0.1 GeV to 20 TeV; RXTE and Swift to cover wavelengths from UV to hard X-rays; and GASP-WEBT, which provides coverage of radio and optical wavelengths. Optical polarization measurements were provided for a fraction of the campaign by the Steward and St. Petersburg observatories. We evaluate the variability of the source and interband correlations, the gamma-ray flaring activity occurring in May 2009, and interpret the results within two synchrotron self-Compton (SSC) scenarios. Methods. The multiband variability observed during the full campaign is addressed in terms of the fractional variability, and the possible correlations are studied by calculating the discrete correlation function for each pair of energy bands where the significance was evaluated with dedicated Monte Carlo simulations. The space of SSC model parameters is probed following a dedicated grid-scan strategy, allowing for a wide range of models to be tested and offering a study of the degeneracy of model-to-data agreement in the individual model parameters, hence providing a less biased interpretation than the "single-curve SSC model adjustment" typically reported in the literature. Results. We find an increase in the fractional variability with energy, while no significant interband correlations of flux changes are found on the basis of the acquired data set. The SSC model grid-scan shows that the flaring activity around May 22 cannot be modeled adequately with a one-zone SSC scenario (using an electron energy distribution with two breaks), while it can be suitably described within a two (independent) zone SSC scenario. Here, one zone is responsible for the quiescent emission from the averaged 4.5-month observing period, while the other one, which is spatially separated from the first, dominates the flaring emission occurring at X-rays and very-high-energy (> 100 GeV, VHE) gamma-rays. The flaring activity from May 1, which coincides with a rotation of the electric vector polarization angle (EVPA), cannot be satisfactorily reproduced by either a one-zone or a two-independent-zone SSC model, yet this is partially affected by the lack of strictly simultaneous observations and the presence of large flux changes on sub-hour timescales (detected at VHE gamma rays). Conclusions. The higher variability in the VHE emission and lack of correlation with the X-ray emission indicate that, at least during the 4.5-month observing campaign in 2009, the highest energy (and most variable) electrons that are responsible for the VHE gamma rays do not make a dominant contribution to the similar to 1 keV emission. Alternatively, there could be a very variable component contributing to the VHE gamma-ray emission in addition to that coming from the SSC scenario. The studies with our dedicated SSC grid-scan show that there is some degeneracy in both the one-zone and the two-zone SSC scenarios probed, with several combinations of model parameters yielding a similar model-to-data agreement, and some parameters better constrained than others. The observed gamma-ray flaring activity, with the EVPA rotation coincident with the first gamma-ray flare, resembles those reported previously for low frequency peaked blazars, hence suggesting that there are many similarities in the flaring mechanisms of blazars with different jet properties.
Das prolongierte Weaning von Patienten mit neurologischen oder neurochirurgischen Erkrankungen weist Besonderheiten auf, denen die Deutsche Gesellschaft für Neurorehabilitation e. V. in einer eigenen Leitlinie Rechnung trägt.
Im Hinblick auf Definitionen (z. B. Weaningerfolg und -versagen), Weaningkategorien, Pathophysiologie des Weaningversagens und allgemeine Weaningstrategien wird ausdrücklich auf die aktuelle S2k-Leitlinie der Deutschen Gesellschaft für Pneumologie und Beatmungsmedizin e. V. verwiesen.
In der neurologisch-neurochirurgischen Frührehabilitation werden Patienten mit zentralen Störungen der Atmungsregulation (z. B. Hirnstammläsionen), des Schluckaktes (neurogene Dysphagien), mit neuromuskulären Problemen (z. B. Critical-illness-Polyneuropathie, Guillain-Barre-Syndrom, Querschnittlähmungen, Myasthenia gravis) und/oder kognitiven Störungen (z. B. Bewusstseins- und Vigilanzstörungen, schwere Kommunikationsstörungen) versorgt, deren Betreuung bei der Entwöhnung von der Beatmung neben intensivmedizinischer Kompetenz auch neurologische bzw. neurochirurgische und neurorehabilitative Expertise erfordert. In Deutschland wird diese Kompetenz in Zentren der neurologisch-neurochirurgischen Frührehabilitation vorgehalten, und zwar als Krankenhausbehandlung.
Der Leitlinie liegt eine systematische Recherche von Leitliniendatenbanken und Medline zugrunde. Unter Moderation durch die Arbeitsgemeinschaft der Wissenschaftlichen Medizinischen Fachgesellschaften (AWMF) erfolgte die Konsensfindung mittels nominalen Gruppenprozesses und Delphi-Verfahren.
In der vorliegenden Leitlinie der DGNR wird auf die strukturellen und inhaltlichen Besonderheiten der neurologisch-neurochirurgischen Frührehabilitation sowie vorhandene Studien zum Weaning in Frührehabilitationseinrichtungen eingegangen.
Adressaten der Leitlinie sind Neurologen, Neurochirurgen, Anästhesisten, Palliativmediziner, Logopäden, Intensivpflegekräfte, Ergotherapeuten, Physiotherapeuten und Neuropsychologen. Ferner richtet sich diese Leitlinie zur Information an Fachärzte für Physikalische Medizin und Rehabilitation (PMR), Pneumologen, Internisten, Atmungstherapeuten, den Medizinischen Dienst der Krankenkassen (MDK) und des Spitzenverbands Bund der Krankenkassen e. V. (MDS). Das wesentliche Ziel dieser Leitlinie ist es, den aktuellen Wissensstand zum Thema „Prolongiertes Weaning in der neurologisch-neurochirurgischen Frührehabilitation“ zu vermitteln.
We present a search for magnetically broadened gamma-ray emission around active galactic nuclei (AGNs), using VERITAS observations of seven hard-spectrum blazars. A cascade process occurs when multi-TeV gamma-rays from an AGN interact with extragalactic background light (EBL) photons to produce electron-positron pairs, which then interact with cosmic microwave background photons via inverse-Compton scattering to produce gamma-rays. Due to the deflection of the electron- positron pairs, a non-zero intergalactic magnetic field (IGMF) would potentially produce detectable effects on the angular distribution of the cascade emission. In particular, an angular broadening compared to the unscattered emission could occur. Through non-detection of angularly broadened emission from 1ES 1218 vertical bar 304, the source with the largest predicted cascade fraction, we exclude a range of IGMF strengths around 10(-14) G at the 95% confidence level. The extent of the exclusion range varies with the assumptions made about the intrinsic spectrum of 1ES. 1218+304 and the EBL model used in the simulation of the cascade process. All of the sources are used to set limits on the flux due to extended emission.