# Lubrano, P.

Overview
Works: 8 works in 8 publications in 1 language and 15 library holdings
Publication Timeline
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Most widely held works by P Lubrano
A measurement of electron-tau universality from decays of intermediate vector bosons at the CERN $$\bar pp$$ collider by UA2 Collaboration( )

1 edition published in 1991 in English and held by 2 WorldCat member libraries worldwide

Measurement of the transverse momentum distributions ofW andZ bosons at the CERN $$\bar pp$$ collider by UA 2 Collaboration( )

1 edition published in 1990 in English and held by 2 WorldCat member libraries worldwide

Search for top quark production at the CERN $$\bar pp$$ collider by UA 2 Collaboration( )

1 edition published in 1990 in English and held by 2 WorldCat member libraries worldwide

Fermi-LAT observations of LIGO/Virgo event GW170817 by M Ajello( )

1 edition published in 2018 in English and held by 2 WorldCat member libraries worldwide

<> by The NA62 collaboration( )

1 edition published in 2019 in English and held by 2 WorldCat member libraries worldwide

A measurement of two-jet decays of theW andZ bosons at the CERN $$\bar p$$ p collider by UA2 Collaboration( )

1 edition published in 1991 in English and held by 2 WorldCat member libraries worldwide

Measurement ofW andZ production cross sections at the CERN $$\bar p$$ p collider by UA2 Collaboration( )

1 edition published in 1990 in English and held by 2 WorldCat member libraries worldwide

FERMI-LAT SEARCH FOR PULSAR WIND NEBULAE AROUND GAMMA-RAY PULSARS by M Ackermann( )

1 edition published in 2011 in English and held by 1 WorldCat member library worldwide

The high sensitivity of the Fermi-LAT (Large Area Telescope) offers the first opportunity to study faint and extended GeV sources such as pulsar wind nebulae (PWNe). After one year of observation the LAT detected and identified three PWNe: the Crab Nebula, Vela-X, and the PWN inside MSH 15-52. In the meantime, the list of LAT detected pulsars increased steadily. These pulsars are characterized by high energy loss rates ((E) over dot) from similar to 3 x 10(33) erg s( -1) to 5 x 10(38) erg s( -1) and are therefore likely to power a PWN. This paper summarizes the search for PWNe in the off-pulse windows of 54 LAT-detected pulsars using 16 months of survey observations. Ten sources show significant emission, seven of these likely being of magnetospheric origin. The detection of significant emission in the off-pulse interval offers new constraints on the gamma-ray emitting regions in pulsar magnetospheres. The three other sources with significant emission are the Crab Nebula, Vela-X, and a new PWN candidate associated with the LAT pulsar PSR J1023-5746, coincident with the TeV source HESS J1023-575. We further explore the association between the HESS and the Fermi source by modeling its spectral energy distribution. Flux upper limits derived for the 44 remaining sources are used to provide new constraints on famous PWNe that have been detected at keV and/or TeV energies

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