about
An ultraluminous X-ray source powered by an accreting neutron star.A precise measurement of the magnetic field in the corona of the black hole binary V404 Cygni.The reflection component from Cygnus X-1 in the soft state measured by NuSTAR and SuzakuThe nuclear spectroscopic telescope array (NuSTAR) high-energy X-ray missionXIPE: the x-ray imaging polarimetry explorerA Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-NewtonLense-Thirring precession in ULXs as a possible means to constrain the neutron star equation of stateAn iron K component to the ultrafast outflow in NGC 1313 X-1An extremely luminous and variable ultraluminous X-ray source in the outskirts of Circinus observed with NuSTARThe Large Observatory for X-ray Timing (LOFT)Distorted cyclotron line profile in Cep X-4 as observed by NuSTARCalibration of the NuSTAR high-energy focusing X-ray telescopeNuSTARDISCOVERY OF A CYCLOTRON LINE IN THE BE/X-RAY BINARY RX J0520.5–6932 DURING OUTBURSTTiming and flux evolution of the Galactic Center magnetar Sgr J1745-2900NuSTAR results and future plans for magnetar and rotation-powered pulsar observationsA Hard Look at the Neutron Stars and Accretion Disks in 4U 1636-53, GX 17+2, and 4U 1705-44 withNuStarAn XMM-Newton and NuSTAR Study of IGR J18214-1318: A Non-pulsating High-mass X-Ray Binary with a Neutron StarLiving on a Flare: Relativistic Reflection in V404 Cyg Observed byNuSTARduring Its Summer 2015 OutburstNustar and XMM-Newton observations of the neutron star X-ray binary 1RXS J180408.9-34205NuSTARdetection of 4s Hard X-ray Lags from the Accreting Pulsar GS 0834-430NuSTARANDINTEGRALOBSERVATIONS OF A LOW/HARD STATE OF 1E1740.7-2942Constraints on the neutron star and inner accretion flow in Serpens X-1 using NuSTARNuSTARDETECTION OF HARD X-RAY PHASE LAGS FROM THE ACCRETING PULSAR GS 0834–430Magnetic field strength of a neutron-star-powered ultraluminous X-ray sourceEvidence for Pulsar-like Emission Components in the Broadband ULX SampleSuper-Eddington accretion on to the neutron star NGC 7793 P13: Broad-band X-ray spectroscopy and ultraluminous X-ray sourcesNo Time for Dead Time: Use the Fourier Amplitude Differences to Normalize Dead-time-affected PeriodogramsAn elevation of 0.1 light-seconds for the optical jet base in an accreting Galactic black hole systemSpectral and Timing Properties of IGR J17091–3624 in the Rising Hard State During Its 2016 OutburstSingle-dish and VLBI observations of Cygnus X-3 during the 2016 giant flare episodeImaging of SNR IC443 and W44 with the Sardinia Radio Telescope at 1.5 and 7 GHzThe Slowest Spinning X-Ray Pulsar in an Extragalactic Globular ClusterThe Broadband Spectral Variability of Holmberg IX X-1High-resolution spectral imaging of SNR W44 and IC443 at 22 GHz with the Sardinia Radio TelescopeDetection of very low-frequency, quasi-periodic oscillations In the 2015 outburst of V404 CygniSpectral changes in the hyperluminous pulsar in NGC 5907 as a function of super-orbital phaseThe Sardinia Radio Telescope (SRT): A large modern radio telescope for observations from meter to mm wavelengthsThe Sardinia Radio Telescope. From a technological project to a radio observatoryULX spectra revisited: Accreting, highly magnetized neutron stars as the engines of ultraluminous X-ray sourcesSardinia Radio Telescope wide-band spectral-polarimetric observations of the galaxy cluster 3C 129
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description
researcher, ORCID id # 0000-0002-4576-9337
@en
wetenschapper
@nl
name
Matteo Bachetti
@ast
Matteo Bachetti
@en
Matteo Bachetti
@es
Matteo Bachetti
@nl
type
label
Matteo Bachetti
@ast
Matteo Bachetti
@en
Matteo Bachetti
@es
Matteo Bachetti
@nl
altLabel
M. Bachetti
@en
prefLabel
Matteo Bachetti
@ast
Matteo Bachetti
@en
Matteo Bachetti
@es
Matteo Bachetti
@nl
P106
P21
P31
P496
0000-0002-4576-9337