about
Giant magnetized outflows from the centre of the Milky WayThe Sky Polarization ObservatoryBaR-SPOrt: the instrument to be accommodated at Dome CThe BaR-SPOrt experiment: measuring the CMBP E-mode power spectrum from Dome CThe BaR-SPOrt experimentAdvanced Diagnostics for the Study of Linearly Polarized Emission. II. Application to Diffuse Interstellar Radio Synchrotron EmissionThe jet/wind outflow in Centaurus A: a local laboratory for AGN feedbackA new perspective on turbulent Galactic magnetic fields through comparison of linear polarization decomposition techniquesLimiting magnetic fields in the cosmic web with diffuse radio emissionA Southern-Sky Total Intensity Source Catalogue at 2.3 GHz from S-Band Polarisation All-Sky Survey DataMagnetic field disorder and Faraday effects on the polarization of extragalactic radio sourcesA radio-polarisation and rotation measure study of the Gum nebula and its environmentGalactic interstellar turbulence across the southern sky seen through spatial gradients of the polarization vectorDetection of a radio bridge in Abell 3667BaR-SPOrt: Balloon-Borne Radiometers for Sky Polarization ObservationsSPOrt: an experiment aimed at measuring the large-scale cosmic microwave background polarizationThe Sky Polarization Observatory (SPOrt) ProgrammeThe BaR-SPOrt experimentThe SPOrt experimentImaging of SNR IC443 and W44 with the Sardinia Radio Telescope at 1.5 and 7 GHzThe Sardinia Radio Telescope. From a technological project to a radio observatorySardinia Radio Telescope wide-band spectral-polarimetric observations of the galaxy cluster 3C 129Sardinia Radio Telescope: General Description, Technical Commissioning and First LightCommissioning of the Sardinia Radio Telescope in Italy: Results and perspectivesThe sardinia radio telescope: Overview and statusSearch for Ammonia Radio Emission in Comet 9P/Tempel~1 after the Deep Impact EventThe 999thSwiftgamma-ray burst: Some like it thermalStatus report of the SRT radiotelescope control software: the DISCOS projectRules of thumb to increase the software quality through testingDiving into the Sardinia Radio Telescope minor servo systemThe control software for the Sardinia Radio TelescopeSETI-Italia 2003 status report and first results of a KL transform algorithm for ETI signal detectionResults of the first Italian planetary radar experimentObservations of a nearby filament of galaxy clusters with the Sardinia Radio TelescopeSArdinia Roach2-based Digital Architecture for Radio Astronomy (SARDARA)Sardinia Radio Telescope observations of Abell 194The Parkes Galactic Meridian Survey: observations and CMB polarization foreground analysis1.4-GHz polarimetric observations of the two fields imaged by the DASI experimentDeep 1.4-GHz observations of diffuse polarized emissionPolarized diffuse emission at 2.3 GHz in a high Galactic latitude area
P50
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P50
description
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
Sergio Poppi
@ast
Sergio Poppi
@en
Sergio Poppi
@es
Sergio Poppi
@nl
type
label
Sergio Poppi
@ast
Sergio Poppi
@en
Sergio Poppi
@es
Sergio Poppi
@nl
prefLabel
Sergio Poppi
@ast
Sergio Poppi
@en
Sergio Poppi
@es
Sergio Poppi
@nl
P106
P1153
6602635190
P21
P31
P496
0000-0002-4698-2607