about
Observation of the Suppression of the Flux of Cosmic Rays above 4 × 10 19 eVCorrelation of the highest-energy cosmic rays with nearby extragalactic objects.Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory.Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nucleiAn evaluation of the exposure in nadir observation of the JEM-EUSO missionThe camera of the ASTRI SST-2M prototype for the Cherenkov Telescope ArrayCharacteristics and Performance of the GAW Experiment for a Large Field of View Cerenkov Gamma-ray TelescopeMeasurement of the Proton-Air Cross Section ats=57 TeVwith the Pierre Auger ObservatoryMeasurement of the Depth of Maximum of Extensive Air Showers above1018 eVUpper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger ObservatoryAuxiliary instruments for the absolute calibration of the ASTRI SST-2M prototype for the Cherenkov Telescope ArrayIllumination technique for the relative calibration of the ASTRI SST-2M cameraUVSiPM: A light detector instrument based on a SiPM sensor working in single photon countingPerformance and applications of the UVscope instrumentThe UVscope instrument in the framework of ground-based cosmic ray fluorescence observatoriesExtensive air showers and diffused Cherenkov light detection: The ULTRA experimentImproved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger ObservatoryCalibration aspects of the JEM-EUSO missionErratum to: Ultra high energy photons and neutrinos with JEM-EUSOErratum: Muons in air showers at the Pierre Auger Observatory: Measurement of atmospheric production depth [Phys. Rev. D90, 012012 (2014)]Erratum to: Performances of JEM-EUSO: angular reconstructionPerformances of JEM–EUSO: energy and X max reconstructionScience of atmospheric phenomena with JEM-EUSOSpace experiment TUS on board the Lomonosov satellite as pathfinder of JEM-EUSOThe EUSO-Balloon pathfinderThe JEM-EUSO mission: An introductionMonitoring of persistent accreting pulsating neutron stars observed during the INTEGRAL Core ProgramThe populations of hard X-ray andγ-ray sources: a correlation study and new possible identificationsSearch for gamma ray bursts with the ARGO-YBJ detector in scaler modeSoftware timing calibration of the ARGO-YBJ detectorScaler mode technique for the ARGO-YBJ detectorBroadband Spectrum of Cygnus X‐1 in Two Spectral States withBeppoSAXThe broad band spectral properties of binary X-ray pulsarsThe pulsed light curves of Her X–1 as observed by BeppoSAXA Swift view on IGR J19149+1036Orbital period of Swift J1816.7–1613 revealed by the Swift Burst Alert TelescopeFinding a 61.0 d orbital period for the HMXB 4U 1036−56 with the Swift-BAT monitoringThe 54-day orbital period of AX J1820.5–1434 unveiled bySwiftSwift observations of the high-mass X-ray binary IGR J16283-4838 unveil a 288 day orbital periodSwiftdiscovery of the orbital period of the high mass X-ray binary IGR J015712−7259 in the Small Magellanic Cloud
P50
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P50
description
researcher, ORCID id # 0000-0001-7341-6603
@en
wetenschapper
@nl
name
Alberto Segreto
@ast
Alberto Segreto
@en
Alberto Segreto
@es
Alberto Segreto
@nl
type
label
Alberto Segreto
@ast
Alberto Segreto
@en
Alberto Segreto
@es
Alberto Segreto
@nl
prefLabel
Alberto Segreto
@ast
Alberto Segreto
@en
Alberto Segreto
@es
Alberto Segreto
@nl
P1153
55854061800
P21
P31
P496
0000-0001-7341-6603