2 citations · 2 across the 3 of their papers we have counts for
6 papers
Population synthesis of Galactic middle-aged pulsar wind nebulae I. Detection prospects for current and future instruments
A. De Sarkar, D. F. Torres, B. Olmi +2
Pulsar wind nebulae (PWNe) constitute the largest population of Galactic very-high-energy (VHE; GeV) -ray sources and are key laboratories for studying particle accel…
Population synthesis of Galactic middle-aged pulsar wind nebulae II. Observational signatures of superefficiency
D. F. Torres, A. De Sarkar, B. Olmi +2
Pulsar wind nebulae (PWNe) interacting with the host supernova remnants (SNRs) can enter the reverberation phase in which reverse-shock-driven compression amplifies the magnetic fi…
Temporal evolution of the periodic GeV signal from 4FGL J1913.2+0512 and analysis of the SS 433 / W50 lobes
Ãmer Faruk Ãoban, Diego F. Torres, Jian Li +3
SS 433 is a microquasar whose relativistic jets precess every ~162 days, providing a laboratory for jet-interstellar medium interactions. We present a comprehensive analysis of 16…
The dispersion in pulsar -ray efficiency
Daniel Ãñiguez-Pascual, Daniele Viganò, Diego F. Torres
The observational efficiency of pulsars, defined as the ratio of the observationally derived isotropic-equivalent luminosity, , where is the average…
Synchro-curvature description of γ-ray light curves and spectra of pulsars: concurrent fitting
Daniel Ãñiguez-Pascual, Diego F. Torres, Daniele Viganò
We present a concurrent fitting of spectra and light curves of the whole population of detected gamma-ray pulsars. Using a synchro-curvature model we compare our theoretical output…
Spatio-spectral-temporal Modelling of Two Young Pulsar Wind Nebulae
A. Kundu, Jagdish C. Joshi, C. Venter +5
Recent observations of a few young pulsar wind nebulae (PWNe) have revealed their morphologies in some detail. Given the availability of spatio-spectral-temporal data, we use our m…