Gravitational Waves From Known Pulsars: Results From The Initial Detector Era

We present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo. We do not see evidence for gravitational wave emission from any of the targeted sources but produce upper limits on the emission amplitude. We highlight the results from seven young pulsars with large spin-down luminosities. We reach within a factor of five of the canonical spin-down limit for all seven of these, whilst for the Crab and Vela pulsars we further surpass their spin-down limits. We present new or updated limits for 172 other pulsars (including both young and millisecond pulsars). Now that the detectors are undergoing major upgrades, and, for completeness, we bring together all of the most up-to-date results from all pulsars searched for during the operations of the first-generation LIGO, Virgo and GEO600 detectors. This gives a total of 195 pulsars including the most recent results described in this paper.United States National Science FoundationScience and Technology Facilities Council of the United KingdomMax-Planck-SocietyState of Niedersachsen/GermanyAustralian Research CouncilInternational Science Linkages program of the Commonwealth of AustraliaCouncil of Scientific and Industrial Research of IndiaIstituto Nazionale di Fisica Nucleare of ItalySpanish Ministerio de Economia y CompetitividadConselleria d'Economia Hisenda i Innovacio of the Govern de les Illes BalearsNetherlands Organisation for Scientific ResearchPolish Ministry of Science and Higher EducationFOCUS Programme of Foundation for Polish ScienceRoyal SocietyScottish Funding CouncilScottish Universities Physics AllianceNational Aeronautics and Space AdministrationOTKA of HungaryLyon Institute of Origins (LIO)National Research Foundation of KoreaIndustry CanadaProvince of Ontario through the Ministry of Economic Development and InnovationNational Science and Engineering Research Council CanadaCarnegie TrustLeverhulme TrustDavid and Lucile Packard FoundationResearch CorporationAlfred P. Sloan FoundationAstronom

Rescue intracranial stenting in acute ischemic stroke (study).

BACKGROUND AND PURPOSE: In cases of acute ischemic stroke that are caused by intracranial large vessel occlusion, rescue intracranial stenting has recently become a treatment option to achieve recanalization in patients when mechanical thrombectomy fails. However, there have been few studies to date that support this beneficial treatment. Our goal is to analyze whether the use of rescue intracranial stenting would improve non-poor prognosis in patients 3 months posttreatment. METHODS: This was a retrospective analysis of a prospective cohort of patients with acute ischemic stroke who were treated with rescue stenting at our hospital. Inclusion criteria for the study consisted of evidence of intracranial large vessel occlusion, absence of intracranial hemorrhage, and severe stenosis or reocclusion after mechanical thrombectomy. Tandem occlusions, failure to follow up after discharge, and a severe combined illness concomitant with acute ischemic stroke were excluded. The primary outcome was the non-poor outcome rate at 3 months and postprocedural symptomatic intracerebral hemorrhage. RESULTS: The posttreatment outcomes of 85 eligible patients who received rescue intracranial stenting between August 2019 and May 2021 are reported. In total, 82 of these patients (96.5%) had successful recanalization and 4 (4.7%) experienced symptomatic intracerebral hemorrhage. In total, 47 (55.3%) patients had non-poor and 35 (41.2%) good outcomes at 3 months after treatment with rescue intracranial stenting. The use of dual antiplatelet therapy was associated with new infarcts (relative risk = 0.1; 95% confidence interval 0.01-0.7) and symptomatic intracerebral hemorrhage (relative risk = 0.1; 95% confidence interval 0.01-0.9). CONCLUSION: Our study suggests that despite the occurrence of postprocedural symptomatic intracerebral hemorrhage in a low proportion of cases, rescue intracranial stenting could be an important alternative treatment after mechanical thrombectomy failure

Proneural and mesenchymal glioma stem cells display major differences in splicing and lncRNA profiles

Therapy resistance and recurrence in high-grade gliomas are driven by their populations of glioma stem cells (GSCs). Thus, detailed molecular characterization of GSCs is needed to develop more effective therapies. We conducted a study to identify differences in the splicing profile and expression of long non-coding RNAs in proneural and mesenchymal GSC cell lines. Genes related to cell cycle, DNA repair, cilium assembly, and splicing showed the most differences between GSC subgroups. We also identified genes distinctly associated with survival among patients of mesenchymal or proneural subgroups. We determined that multiple long non-coding RNAs with increased expression in mesenchymal GSCs are associated with poor survival of glioblastoma patients. In summary, our study established critical differences between proneural and mesenchymal GSCs in splicing profiles and expression of long non-coding RNA. These splicing isoforms and lncRNA signatures may contribute to the uniqueness of GSC subgroups, thus contributing to cancer phenotypes and explaining differences in therapeutic responses.This study was supported by a grant from Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), Brazil to PAFG and LOFP and by NIH 7R21CA175875-03. This study was partially supported by grants from Serrapilheira foundation and Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP; 2018/15579-8) to PAFG. GDAG and BRC were supported by fellowships from FAPESP (2017/19541-2) and (2013/25483-4 and 2013/07159-5), respectively. PRA was supported by CPRIT Training Grant - RP14010

Evidence of a J/ψΛJ/\psi\Lambda structure and observation of excited Ξ−\Xi^- states in the Ξb−→J/ψΛK−\Xi^-_b \to J/\psi\Lambda K^- decay

First evidence of a structure in the $J/\psi{\Lambda}$ invariant mass distribution is obtained from an amplitude analysis of $\Xi_b^-{\rightarrow}J/\psi{\Lambda}K^-$ decays. The observed structure is consistent with being due to a charmonium pentaquark with strangeness with a significance of $3.1\sigma$ including systematic uncertainties and look-elsewhere effect. Its mass and width are determined to be $4458.8\pm2.9^{+4.7}_{-1.1}$ MeV and $17.3\pm6.5^{+8.0}_{-5.7}$ MeV, respectively, where the quoted uncertainties are statistical and systematic. The structure is also consistent with being due to two resonances. In addition, the narrow excited $\Xi^-$ states, $\Xi(1690)^-$ and $\Xi(1820)^-$, are seen for the first time in a $\Xi^-_b$ decay, and their masses and widths are measured with improved precision. The analysis is performed using $pp$ collision data corresponding to a total integrated luminosity of 9 fb$^{-1}$, collected with the LHCb experiment at centre-of-mass energies of 7, 8 and 13 TeV