activity
20092026
most citedYoung Radio Pulsars in Galactic Globular Clusters

77 citations · 321 across the 12 of their papers we have counts for

collaborators

10 papers

astro-ph.HE2026

A pulsar escaping an ancient open cluster via tidal stripping

Lei Zhang, Xiaoting Fu, Di Li +21

Open clusters are the primary birthplaces of stars in the Milky Way disk, yet their neutron star progeny are rarely found within them, presumably due to supernova-induced kicks tha…

astro-ph.HE2019★ 9 cited

The dynamics of Galactic centre pulsars: constraining pulsar distances and intrinsic spin-down

B. B. P. Perera, E. D. Barr, M. B. Mickaliger +11

Through high-precision radio timing observations, we show that five recycled pulsars in the direction of the Galactic Centre (GC) have anomalous spin period time derivative ($\dot…

astro-ph.HE2013★ 57 cited

The Galactic centre pulsar population

Jayanth Chennamangalam, D. R. Lorimer

The recent discovery of a magnetar in the Galactic centre region has allowed Spitler et al. to characterize the interstellar scattering in that direction. They find that the tempor…

astro-ph.IM2013★ 12 cited

Jumping the energetics queue: Modulation of pulsar signals by extraterrestrial civilizations

Jayanth Chennamangalam, Andrew P. V. Siemion, D. R. Lorimer +1

It has been speculated that technological civilizations evolve along an energy consumption scale first formulated by Kardashev, ranging from human-like civilizations that consume e…

astro-ph.GA2013★ 32 cited

An empirical Bayesian analysis applied to the globular cluster pulsar population

P. J. Turk, D. R. Lorimer

We describe an empirical Bayesian approach to determine the most likely size of an astronomical population of sources of which only a small subset are observed above some limiting…

astro-ph.SR2012

Constraining the luminosity function parameters and population size of radio pulsars in globular clusters

Jayanth Chennamangalam, D. R. Lorimer, Ilya Mandel +1

The luminosity distribution of Galactic radio pulsars is believed to be log-normal in form. Applying this functional form to populations of pulsars in globular clusters, we employ…