Searching a Thousand Radio Pulsars for Gamma-ray Emission

Cutoff Flux UL OP ph cm −2 s −1 For regions with no significant detection, the 95% confidence- level photon flux upper limit assuming a PLSuperExpCutoff spec- tral model with

To search for gamma-ray pulsations in LAT data, it is necessary to assume a certain “phase model” (i.e. a rotation ephemeris) relating the arrival time of every photon to a

In this Letter, we report the discovery of PSR J1208 −6238, a very young, highly magnetized gamma-ray pulsar with sim- ilar properties to those of PSR J1119 −6127, including a

compare our best-fit values to this and do not use it to limit the likelihood analysis. Both the OG and TPC model match the observed gamma-ray light curve well, but neither

Of the remaining three pulsars, detected only through tim- ing analysis, the most notable is certainly PSR J2043+2740 which, with an age in excess of one million years, would be

We have tested gtbary and gtpphase with giant radio pulses from the Crab pulsar B0531+21 and from the millisecond pulsar B1937+21, recorded at the Nançay radio telescope, X-ray

Combined unabsorbed SED using the gamma-ray fluxes from Fermi-LAT (blue) and AGILE/GRID (red), the XMM-Newton (ma- genta), RXTE (light blue), and INTEGRAL (cyan) average X-ray

The majority of the GBM-measured TGFs can be best fit if the source altitude is below 15 km and 70% of events best fit by leader models cannot be satisfactorily modeled unless a