activity
20242026
collaborators

41 papers

astro-ph.HE2026

Exploring the optical properties of redback pulsars: The case of J1717+4308A in the globular cluster M92

Jianxing Chen, Greta Ettorre, Cristina Pallanca +13

Binary millisecond pulsars (MSPs) in globular clusters (GCs) are key for binary and stellar evolution studies under extreme conditions. The identification of their optical companio…

astro-ph.IM2026

Overview of the Canadian Hydrogen Observatory and Radio Transient Detector (CHORD) Project

The CHORD Collaboration, Kevin Bandura, Leonid Belostotski +49

The Canadian Hydrogen Observatory and Radio-transient Detector (CHORD) is a next-generation wideband radio interferometer currently being constructed and commissioned at the Domini…

astro-ph.HE2026

Pulsars in Globular Clusters With the SKAO

M. Bagchi, F. Abbate, V. Balakrishnan +14

Globular clusters (GCs) are highly efficient factories of radio pulsars: per unit of stellar mass, they contain about 1000 times more pulsars than in the Galactic field. Thus far,…

astro-ph.HE2026

Testing Gravity with Binary Pulsars in the SKA Era

V. Venkatraman Krishnan, L. Shao, V. Balakrishnan +21

Binary (and trinary) radio pulsars are natural laboratories in space for understanding gravity in the strong field regime, with many unique and precise tests carried out so far, in…

astro-ph.HE2026

Understanding Pulsar Wind Nebulae with the SKA

Joseph D. Gelfand, C. -Y. Ng, B. Posselt +9

Produced by the interaction between the ``pulsar wind'' powered by the rotational energy of a neutron star and its surroundings, the study of pulsar wind nebulae (PWNe) provides vi…

astro-ph.HE2026

Detection of relativistic orbital deformation from improved timing of PSR J17571854

Jaikhomba Singha, Vivek Venkatraman Krishnan, Marisa Geyer +12

PSR~J17571854, a 21.5\,ms pulsar, is a highly relativistic double neutron star (DNS) system in a tight eccentric () 4.4\,hr orbit. With extremely large gravitational w…