about
A giant outburst two years before the core-collapse of a massive star.A very faint core-collapse supernova in M85.A low-energy core-collapse supernova without a hydrogen envelope.An accreting pulsar with extreme properties drives an ultraluminous x-ray source in NGC 5907.A study of the Type II-P supernova 2003gd in M74PESSTO: survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient ObjectsSN 2012ec: mass of the progenitor from PESSTO follow-up of the photospheric phaseLow luminosity Type II supernovae – II. Pointing towards moderate mass precursorsThe broad-lined Type Ic supernova 2003jd★SN 2009ib: a Type II-P supernova with an unusually long plateauSN 2009N: linking normal and subluminous Type II-P SNeGALEXSpectroscopy of SN 2005ay Suggests Ultraviolet Spectral Uniformity among Type II-P SupernovaeWhat brakes the Crab pulsar?Aqueye+: a new ultrafast single photon counter for optical high time resolution astrophysicsOptical phase coherent timing of the Crab nebula pulsar with Iqueye at the ESO New Technology TelescopeAqueye Plus: a very fast single photon counter for astronomical photometry to quantum limits equipped with an Optical Vortex coronagraphAqueye optical observations of the Crab Nebula pulsarThe optical light curve of the Large Magellanic Cloud pulsar B0540−69 in 2009Iqueye: a single-photon counting very high-speed photometer for the ESO 3.5m NTTComparison of progenitor mass estimates for the Type IIP SN 2012AProspects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946Massive stars exploding in a He-rich circumstellar medium – IV. Transitional Type Ibn supernovaeThe Type IIP supernova 2012aw in M95: hydrodynamical modeling of the photospheric phase from accurate spectrophotometric monitoringSN 2009E: a faint clone of SN 1987ASN 2009jf: a slow-evolving stripped-envelope core-collapse supernova★SN 1998A: explosion of a blue supergiantThe Large Observatory for x-ray timingLOFT: the Large Observatory For X-ray TimingThe LOFT mission concept: a status updateScience with e-ASTROGAMSNe 2013K and 2013am: observed and physical properties of two slow, normal Type IIP eventsThe Large Observatory for X-ray Timing (LOFT)A variable Quasi-Periodic Oscillation in M82 X-1. Timing and spectral analysis of XMM-Newton and RossiXTE observationsUltraluminous X-ray sources: X-ray timing and new optical observationsSpectral variability in Swift and Chandra observations of the ultraluminous source NGC 55 ULX1Ultraluminous X-ray sources: a deeper insight into their spectral evolutionThe two ultraluminous X-ray sources in the galaxy NGC 925Discovery of a 0.42-s pulsar in the ultraluminous X-ray source NGC 7793 P13Periodic signals from the Circinus region: two new cataclysmic variables and the ultraluminous X-ray source candidate GC X-1Discovery of a 6.4 h black hole binary in NGC 4490
P50
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P50
description
onderzoeker
@nl
researcher
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հետազոտող
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name
L. Zampieri
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L. Zampieri
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Luca Zampieri
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Luca Zampieri
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L. Zampieri
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L. Zampieri
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Luca Zampieri
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Luca Zampieri
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L. Zampieri
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L. Zampieri
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L. Zampieri
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Luca Zampieri
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Luca Zampieri
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P1153
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P31
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0000-0002-6516-1329
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