activity
20002025
most citedFormation of Double Neutron Star Systems

698 citations · 4.2k across the 62 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 8 cited

On the vanishing orbital X-ray variability of the eclipsing binary millisecond pulsar 47 Tuc W

Pavan R. Hebbar, Craig O. Heinke, D. Kandel +2

Redback millisecond pulsars (MSPs) typically show pronounced orbital variability in their X-ray emission due to our changing view of the intrabinary shock (IBS) between the pulsar…

astro-ph.HE2020★ 19 cited

Giant pulses from J1823-3021A observed with the MeerKAT telescope

F. Abbate, M. Bailes, S. J. Buchner +11

The millisecond pulsar J1823-3021A is a very active giant pulse emitter in the globular cluster NGC 6624. New observations with the MeerKAT radio telescope have revealed 14350 gian…

astro-ph.SR2020★ 36 cited

Precise mass measurements for the double neutron star system J1829+2456

Henryk T. Haniewicz, Robert D. Ferdman, Paulo C. C. Freire +4

PSR J1829+2456 is a radio pulsar in a relativistic binary system with another neutron star. It has a rotational period of 41 ms and a mildly eccentric () 28-hr orbit. We…

astro-ph.IM2020★ 178 cited

The MeerKAT Telescope as a Pulsar Facility: System verification and early science results from MeerTime

M. Bailes, A. Jameson, F. Abbate +72

We describe system verification tests and early science results from the pulsar processor (PTUSE) developed for the newly-commissioned 64-dish SARAO MeerKAT radio telescope in Sout…

physics.ins-det2020

MADMAX Status Report

S. Beurthey, N. Böhmer, P. Brun +42

In this report we present the status of the MAgnetized Disk and Mirror Axion eXperiment (MADMAX), the first dielectric haloscope for the direct search of dark matter axions in the…

astro-ph.HE2020★ 25 cited

Shapiro delay in PSR~J18112405

C. Ng, L. Guillemot, P. C. C. Freire +5

This paper presents the first detection of Shapiro delay from the binary millisecond pulsar PSR J1811-2405. We report a 11- measurement of the orthometric amplitude, h=6.8(6…