0000000001303857

AUTHOR

G. Muller

showing 5 related works from this author

Prognostic significance of central venous-to-arterial carbon dioxide difference during the first 24 hours of septic shock in patients with and withou…

2017

IF 6.238; International audience; Objective: To investigate the prognostic significance of central venous-to-arterial carbon dioxide difference (cv-art CO2 gap) during septic shock in patients with and without impaired cardiac function.Methods: We performed a prospective cohort study in 10 French intensive care units. Patients suffering from septic shock were assigned to the impaired cardiac function group (‘cardiac group’, n=123) if they had atrial fibrillation (AF) and/or left ventricular ejection fraction (LVEF) 0.9 kPa at 12 h had a higher risk of day 28 mortality (hazard ratio=3.18; P=0.0049). Among the 59 patients in the cardiac group with mean arterial pressure (MAP) ≥65 mm Hg, centr…

Cardiac function curveAdultMalemedicine.medical_specialtyMean arterial pressureAdolescentCentral Venous Pressurecentral venous-arterial CO2 difference030204 cardiovascular system & hematologyVentricular Function Left03 medical and health sciencesYoung Adult0302 clinical medicine[ SDV.MHEP ] Life Sciences [q-bio]/Human health and pathologyInternal medicineIntensive caremedicineHumansArterial PressureProspective StudiesAgedEjection fractionbusiness.industrySeptic shockCentral venous pressure030208 emergency & critical care medicineCarbon DioxideMiddle Agedmedicine.diseasePrognosisShock Septic3. Good healthSurgeryAnesthesiology and Pain MedicineBlood pressureblood gas analysisCardiologyArterial bloodseptic shockFemalebusiness[SDV.MHEP]Life Sciences [q-bio]/Human health and pathology
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Infarctus du myocarde au cours de l’artérite à cellules géantes : étude de cohorte

2020

Introduction Le risque d’evenement cardiovasculaire est accru au cours de l’arterite a cellules geantes (ACG), en particulier dans les premiers mois suivant le diagnostic de la vascularite [1] . L’objectif de ce travail etait de decrire les caracteristiques des infarctus du myocarde (IDM) survenant chez des patients atteints d’ACG et de les comparer avec des IDM survenant chez des patients ne presentant pas d’ACG au moment de leur IDM. Patients et methodes Les patients atteints d’ACG ont ete identifies parmi la liste des biopsies d’artere temporale (BAT) qui montraient des lesions d’ACG et qui avaient ete analysees entre le 1er janvier 2001 et le 31 decembre 2016 dans les deux laboratoires …

03 medical and health sciences0302 clinical medicine010102 general mathematicsGastroenterologyInternal Medicine030212 general & internal medicine0101 mathematics01 natural sciencesLa Revue de Médecine Interne
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Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

2016

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Hadronic interaction[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsCOLLISIONSAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesGeneral Physics and AstronomyCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciencesCalibrationHigh Energy PhysicsUHE Cosmic Rays010306 general physicsParticle PhysicsCosmic raysGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryEnergyMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaInteraction modelASTROFÍSICAHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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CCDC 139657: Experimental Crystal Structure Determination

2001

Related Article: P.Lahuerta, E.Moreno, A.Monge, G.Muller, J.Perez-Prieto, M.Sanau, S.-E.Stiriba|2000|Eur.J.Inorg.Chem.||2481|doi:10.1002/1099-0682(200012)2000:12<2481::AID-EJIC2481>3.0.CO;2-M

Space GroupCrystallographyCrystal SystemCrystal StructureCell Parametersbis((mu~2~-Trifluoroacetato-OO')-(trifluoroacetato-O)-(((1S2S5R)-2-hydroxy-5-(isopropenyl)-2-methylcyclohexyl)diphenylphosphine-PO)-rhodium(ii)) chloroform solvateExperimental 3D Coordinates
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CCDC 139658: Experimental Crystal Structure Determination

2001

Related Article: P.Lahuerta, E.Moreno, A.Monge, G.Muller, J.Perez-Prieto, M.Sanau, S.-E.Stiriba|2000|Eur.J.Inorg.Chem.||2481|doi:10.1002/1099-0682(200012)2000:12<2481::AID-EJIC2481>3.0.CO;2-M

bis((mu~2~-Trifluoroacetato-OO')-(trifluoroacetato-O)-(((1R2R5S)-2-hydroxy-5-(isopropenyl)-2-methylcyclohexyl)diphenylphosphine-PO)-rhodium(ii)) dihydrateSpace GroupCrystallographyCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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