0000000000054642

AUTHOR

André Schulz

0000-0002-9381-2651

showing 12 related works from this author

Distinctive body perception mechanisms in high versus low symptom reporters: A neurophysiological model for medically-unexplained symptoms.

2020

Abstract Objective The neurophysiological processes involved in the generation of medically-unexplained symptoms (MUS) remain unclear. This study tested three assumptions of the perception-filter model contributing to MUS: (I.) increased bodily signal strength (II.) decreased filter function, (III.) increased perception. Methods In this cross-sectional, observational study, trait MUS were assessed by a web-based survey (N = 486). The upper and lower decile were identified as extreme groups of high (HSR; n = 29; 26 women; Mage = 26.0 years) and low symptom reporters (LSR; n = 29; 21 women; Mage = 28.4 years). Mean heart rate (HR) and heart rate variability (HRV), and cortisol awakening respo…

medicine.medical_specialtyCortisol awakening responseHeartbeatbusiness.industrymedia_common.quotation_subjectMedically unexplainedBody perceptionAudiologyNeurophysiology03 medical and health sciencesPsychiatry and Mental healthClinical Psychology0302 clinical medicinePerceptionHeart ratemedicineHeart rate variability030212 general & internal medicinebusiness030217 neurology & neurosurgerymedia_commonJournal of psychosomatic research
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Making sense of what you sense: Disentangling interoceptive awareness, sensibility and accuracy.

2016

Garfinkel and Critchley (2013) recently proposed a three level model of interoception. Only few studies, however, have empirically tested this theoretical model thus far. The present study aimed at investigating (1) the central assumptions of this model, i.e. that Accuracy, Sensibility and Awareness are distinguishable facets of interoception and that Interoceptive Accuracy is the basic level of interoception, and (2) whether cardiovascular activation (as indexed by heart rate) is differentially related to the three facets of interoception. Analyses were conducted on a total sample of N=159 healthy participants (118 female [74.2%]; mean age=23.9years, SD=3.3, range=19-45) who performed eith…

AdultMaleHeartbeat050105 experimental psychologyThree levelDevelopmental psychologyInteroceptionCorrelation03 medical and health sciencesYoung Adult0302 clinical medicineHeart RatePhysiology (medical)Humans0501 psychology and cognitive sciencesSensibilityGeneral Neuroscience05 social sciencesMean ageAwarenessMiddle AgedNeuropsychology and Physiological PsychologyBasic levelInteroceptionFemalePsychology030217 neurology & neurosurgeryCognitive psychologyInternational journal of psychophysiology : official journal of the International Organization of Psychophysiology
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High blood pressure responders show largest increase in heartbeat perception accuracy after post-learning stress following a cardiac interoceptive le…

2020

Mental disorders with physical symptoms, e.g. somatic symptom disorder, are characterized by altered interoceptive accuracy (IAc), which can be explained by individual differences in interoceptive learning (IL). We investigated if stress facilitates IL. Seventy-three healthy participants performed a heartbeat counting task (HCT: T1) and a heartbeat perception training (HBPT). After exposure to a socially-evaluated cold pressor stress test (SECPT; n = 48) or a control condition (n = 25), two more HCTs were performed (T2: 30 min after SECPT; T3: 24 h later). After the HBPT, all participants showed an increase in IAc. We separated the stress group into high vs. low systolic blood pressures (SB…

MalePituitary-Adrenal SystemSocial SciencesBlood PressureSomatic symptom disorderMEMORY CONSOLIDATIONCortisolInteroception0302 clinical medicineHeart RatePsychologyANXIETYBRAINPsychology BiologicalPsychology ExperimentalGeneral Neuroscience05 social sciencesCold pressor testPerceptual learningNeuropsychology and Physiological PsychologyHypertensionCardiologyAnxietyFemaleMemory consolidationSENSITIVITYmedicine.symptomLife Sciences & BiomedicineBehavioral SciencesDECLARATIVE MEMORYHypothalamo-Hypophyseal SystemAWARENESSmedicine.medical_specialtyHeartbeatINDUCED CORTISOL ELEVATIONSStress050105 experimental psychologyYoung Adult03 medical and health sciencesStress PhysiologicalInternal medicinemedicineHumansAutonomic nervous system0501 psychology and cognitive sciencesMEDICALLY UNEXPLAINED SYMPTOMSScience & Technologybusiness.industryPanic disordermedicine.diseasePANIC DISORDERREACTIVITYAutonomic nervous systemBlood pressureHeartbeat perceptionSymptom perceptionbusiness030217 neurology & neurosurgeryBiological Psychology
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Subclinical levels of anxiety but not depression are associated with planning performance in a large population-based sample

2017

BackgroundMajor depression and anxiety disorders are known to negatively influence cognitive performance. Moreover, there is evidence for greater cognitive decline in older adults with generalized anxiety disorder. Except for clinical studies, complex executive planning functions and subclinical levels of anxiety have not been examined in a population-based sample with a broad age range.MethodsPlanning performance was assessed using the Tower of London task in a population-based sample of 4240 participants aged 40–80 years from the Gutenberg Health Study (GHS) and related to self-reported anxiety and depression by means of multiple linear regression analysis.ResultsHigher anxiety ratings we…

Male050103 clinical psychologymedicine.medical_specialtyGeneralized anxiety disorderPopulationAnxietyNeuropsychological TestsExecutive Function03 medical and health sciencesCognition0302 clinical medicineGermanyHumansMedicineCognitive Dysfunction0501 psychology and cognitive sciencesProspective StudiesEffects of sleep deprivation on cognitive performanceCognitive declineeducationPsychiatryProblem SolvingApplied PsychologyDepression (differential diagnoses)AgedSubclinical infectioneducation.field_of_studyDepressionbusiness.industry05 social sciencesCognitionMiddle Agedmedicine.disease030227 psychiatryPsychiatry and Mental healthCross-Sectional StudiesLinear ModelsAnxietyFemalemedicine.symptombusinessPsychomotor PerformanceClinical psychologyPsychological Medicine
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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PHQ-2 and GAD-2 scores predict mortality in patients undergoing oral anticoagulation

2015

Psychiatry and Mental healthClinical Psychologymedicine.medical_specialtybusiness.industryInternal medicinemedicineIn patientbusinessOral anticoagulationJournal of Psychosomatic Research
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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Muons in air showers at the Pierre Auger Observatory

2015

We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies large…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCosmic-ray interactionsAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayextensive atmospherical showers muon density muon number Pierre Auger Observatory cosmic radiation UHEHadronic interaction models7. Clean energyAugerSettore FIS/04 - Fisica Nucleare e SubnucleareNuclear physicsAltitudeSettore FIS/05 - Astronomia e AstrofisicaObservatoryNERGY COSMIC-RAYS DETECTOR MODEL.Extensive air showerscosmic radiation UHEDETECTORScalingCosmic raysZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryMuonNERGY COSMIC-RAYSSettore FIS/01 - Fisica Sperimentaleenergy cosmic-rays; detector; modelAstrophysics::Instrumentation and Methods for AstrophysicsFísica[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ObservatoryASTROFÍSICAextensive atmospherical showersmuon numberMODELmuon densityExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaPhysical Review D
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Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory

2015

Energy-dependent patterns in the arrival directions of cosmic rays are searched for using data of the Pierre Auger Observatory. We investigate local regions around the highest-energy cosmic rays with E ≥ 6×1019 eV by analyzing cosmic rays with energies above E ≥ 5×1018 eV arriving within an angular separation of approximately 15∘. We characterize the energy distributions inside these regions by two independent methods, one searching for angular dependence of energy-energy correlations and one searching for collimation of energy along the local system of principal axes of the energy distribution. No significant patterns are found with this analysis. The comparison of these measurements with …

AstrofísicaPhysics and Astronomy (miscellaneous)Raycosmic radiation anisotropy cosmic radiation propagation cosmic radiation deflectionAstronomymagnetic fieldpAstrophysicsanisotropy [cosmic radiation]01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareAugerPierre//purl.org/becyt/ford/1 [https]ObservatoryJetsQuantum Chromodynamicscosmic radiation: VHEenergy: correlationPatternsMonte Carlo010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic radiation: propagationEnergyCOSMIC cancer databaseAngular distance[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleSearchAstrophysics::Instrumentation and Methods for Astrophysicscosmic radiation anisotropyPierre Auger Observatorycosmic radiation: deflectionRadiación cósmicaAugerSurface Detector ArrayCosmicArrivalComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaPrincipal axis theorem[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Regular Article - Experimental PhysicsAstrophysics::High Energy Astrophysical PhenomenaPhysics and Astronomy (miscellaneous) Engineering (miscellaneous).FOS: Physical sciencesCosmic ray530cosmic radiation: anisotropyParticle detectorSettore FIS/05 - Astronomia e AstrofisicaVHE [cosmic radiation]statistical analysisSpectrum0103 physical sciencesthrustddc:530Engineering (miscellaneous)AstrophysiqueCiencias ExactasPierre Auger Observatoryair: showerscosmic radiation propagationPhysics and Astronomy (miscellaneous); Engineering (miscellaneous)010308 nuclear & particles physicsturbulence[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstroparticles//purl.org/becyt/ford/1.3 [https]ASTROFÍSICAGalactic Magnetic-fieldcorrelation [energy]DirectionExperimental High Energy Physicscosmic radiation deflectionpropagation [cosmic radiation]direct detectiongalaxyObservatory[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]deflection [cosmic radiation]showers [air]Model
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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

2015

We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up t…

acceleration of particles; astroparticle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Upper LimitAstronomyCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias Físicas01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareSettore FIS/05 - Astronomia e AstrofisicaObservatorySpectrum0103 physical sciencesacceleration of particles astroparticle physicsSurface Detector010303 astronomy & astrophysicsacceleration of particleAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleArrayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicAstronomy and AstrophysicsASTROFÍSICANucleiSpace and Planetary Scienceastroparticle physicsExperimental High Energy Physicsacceleration of particles; astroparticle physics; Nuclear and High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCatalogSkyAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Cardiac modulation of startle is altered in depersonalization-/derealization disorder: Evidence for impaired brainstem representation of baro-afferen…

2016

Patients with depersonalization-/derealization disorder (DPD) show altered heartbeat-evoked brain potentials, which are considered psychophysiological indicators of cortical representation of visceral-afferent neural signals. The aim of the current investigation was to clarify whether the impaired CNS representation of visceral-afferent neural signals in DPD is restricted to the cortical level or is also present in sub-cortical structures. We used cardiac modulation of startle (CMS) to assess baro-afferent signal transmission at brainstem level in 22 DPD and 23 healthy control individuals. The CMS paradigm involved acoustic startle stimuli (105dB(A), 50ms) elicited 0, 100, 200, 300, 400 and…

AdultMaleStartle responseReflex StartleVisceral AfferentsBaroreflexDepersonalization-derealization disorder03 medical and health sciences0302 clinical medicineHeart RateHeart ratemedicineDerealizationHumansEvoked PotentialsBiological PsychiatryCardiac cyclemedicine.diagnostic_testBrainHeartBaroreflexmedicine.disease030227 psychiatryPeripheralPsychiatry and Mental healthAcoustic StimulationDepersonalizationFemaleBrainstemPsychologyNeuroscience030217 neurology & neurosurgeryBrain StemPsychiatry research
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The energy spectrum of cosmic rays beyond the turn-down around 1017 eV as measured with the surface detector of the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina – Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia – the Australian Research Council; Be…

Physics and Astronomy (miscellaneous)AstronomyAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesFluxCosmic rayAstrophysics7. Clean energy01 natural sciencesdetector: fluorescenceAugercosmic rayssurface [detector]Observatory0103 physical sciencescalorimeterddc:530High Energy Physicscosmic radiation: UHEspectrum [cosmic radiation]010303 astronomy & astrophysicsEngineering (miscellaneous)Engineering & allied operationsHigh Energy Astrophysical Phenomena (astro-ph.HE)fluorescence [detector]Pierre Auger ObservatoryPhysicsastro-ph.HEcosmic radiation: energy spectrumcosmic radiation: spectrumdetector: surface010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugerCalorimeterfluxobservatoryspectralddc:620[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomenaenergy spectrum [cosmic radiation]Energy (signal processing)RAIOS CÓSMICOSultra-high energy cosmic rays energy spectrum features.
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