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19982021
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 24.6k across the 209 of their papers we have counts for

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Showing astro-ph.IMShow all

24 papers · 1 filter

astro-ph.IM2020★ 14 cited

Revisiting profile instability of J1022+1001

Prajwal V. Padmanabh, Ewan D. Barr, David J. Champion +4

Millisecond pulsars in timing arrays can act as probes for gravitational wave detection and improving the solar system ephemerides among several other applications. However, the st…

astro-ph.IM2020★ 1 cited

On the prospects of imaging Sagittarius A* from space

Freek Roelofs, Heino Falcke, Christiaan Brinkerink +8

Very Long Baseline Interferometry (VLBI) at sub-millimeter waves has the potential to image the shadow of the black hole in the Galactic Center, Sagittarius A* (Sgr A*), and thereb…

astro-ph.IM2019★ 229 cited

An ultra-wide bandwidth (704 to 4032 MHz) receiver for the Parkes radio telescope

G. Hobbs, R. N. Manchester, A. Dunning +69

We describe an ultra-wide-bandwidth, low-frequency receiver ("UWL") recently installed on the Parkes radio telescope. The receiver system provides continuous frequency coverage fro…

astro-ph.IM2019★ 55 cited

TeraHertz Exploration and Zooming-in for Astrophysics (THEZA): ESA Voyage 2050 White Paper

Leonid I. Gurvits, Zsolt Paragi, Viviana Casasola +32

This paper presents the ESA Voyage 2050 White Paper for a concept of TeraHertz Exploration and Zooming-in for Astrophysics (THEZA). It addresses the science case and some implement…

astro-ph.IM2019★ 1.1k cited

First M87 Event Horizon Telescope Results. II. Array and Instrumentation

The Event Horizon Telescope Collaboration

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comp…

astro-ph.IM2018

RFI Flagging Implications for Short-Duration Transients

Y. Cendes, P. Prasad, A. Rowlinson +24

With their wide fields of view and often relatively long coverage of any position in the sky in imaging survey mode, modern radio telescopes provide a data stream that is naturally…

astro-ph.IM2018

LOFT-e: Localisation Of Fast Transients with e-MERLIN

C. R. H. Walker, R. P. Breton, P. A. Harrison +8

The majority of fast radio bursts (FRBs) are poorly localised, hindering their potential scientific yield as galactic, intergalactic, and cosmological probes. LOFT-e, a digital bac…

astro-ph.IM2018★ 28 cited

MeerTime - the MeerKAT Key Science Program on Pulsar Timing

M. Bailes, E. Barr, N. D. R. Bhat +28

The MeerKAT telescope represents an outstanding opportunity for radio pulsar timing science with its unique combination of a large collecting area and aperture efficiency (effectiv…

astro-ph.IM2017★ 17 cited

VOEvent Standard for Fast Radio Bursts

Emily Petroff, Leon Houben, Keith Bannister +13

Fast radio bursts are a new class of transient radio phenomena currently detected as millisecond radio pulses with very high dispersion measures. As new radio surveys begin searchi…

astro-ph.IM2017★ 92 cited

A search for optical bursts from the repeating fast radio burst FRB 121102

Liam K Hardy, Vik S Dhillon, Laura G Spitler +14

We present a search for optical bursts from the repeating fast radio burst FRB 121102 using simultaneous observations with the high-speed optical camera ULTRASPEC on the 2.4-m Thai…

astro-ph.IM2017★ 37 cited

Pulsar Timing and its Application for Navigation and Gravitational Wave Detection

Werner Becker, Michael Kramer, Alberto Sesana

Pulsars are natural cosmic clocks. On long timescales they rival the precision of terrestrial atomic clocks. Using a technique called pulsar timing, the exact measurement of pulse…

astro-ph.IM2015★ 74 cited

The noise properties of 42 millisecond pulsars from the European Pulsar Timing Array and their impact on gravitational wave searches

R. N. Caballero, K. J. Lee, L. Lentati +36

The sensitivity of Pulsar Timing Arrays to gravitational waves depends on the noise present in the individual pulsar timing data. Noise may be either intrinsic or extrinsic to the…

astro-ph.IM2015

Pulsar Science with the SKA

Michael Kramer, Ben Stappers

The SKA will be transformational for many areas of science, but in particular for the study of neutron stars and their usage as tools for fundamental physics in the form of radio p…

astro-ph.IM2014★ 109 cited

LOFAR Sparse Image Reconstruction

H. Garsden, J. N. Girard, J. L. Starck +77

Context. The LOw Frequency ARray (LOFAR) radio telescope is a giant digital phased array interferometer with multiple antennas distributed in Europe. It provides discrete sets of F…

astro-ph.IM2013★ 31 cited

High-Angular-Resolution and High-Sensitivity Science Enabled by Beamformed ALMA

Vincent Fish, Walter Alef, James Anderson +66

An international consortium is presently constructing a beamformer for the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile that will be available as a facility instrum…

astro-ph.IM2013★ 2.7k cited

LOFAR: The LOw-Frequency ARray

M. P. van Haarlem, M. W. Wise, A. W. Gunst +197

LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR…

astro-ph.IM2013★ 41 cited

A coherent acceleration search of the Parkes multi-beam pulsar survey - techniques and the discovery and timing of 16 pulsars

R. P. Eatough, M. Kramer, A. G. Lyne +1

A fully coherent acceleration search algorithm has been applied to the Parkes multi- beam pulsar survey of the Galactic plane to search for previously undiscovered relativistic bin…

astro-ph.IM2013★ 11 cited

Pathway to the Square Kilometre Array - The German White Paper -

F. Aharonian, T. G. Arshakian, B. Allen +69

The Square Kilometre Array (SKA) is the most ambitious radio telescope ever planned. With a collecting area of about a square kilometre, the SKA will be far superior in sensitivity…

astro-ph.IM2012★ 48 cited

The optimal schedule for pulsar timing array observations

K. J. Lee, C. G. Bassa, R. Karuppusamy +3

In order to maximize the sensitivity of pulsar timing arrays to a stochastic gravitational wave background, we present computational techniques to optimize observing schedules. The…

astro-ph.IM2011★ 35 cited

Very High Angular Resolution Science with the Square Kilometre Array

L. E. H. Godfrey, H. Bignall, S. Tingay +7

Preliminary specifications for the Square Kilometre Array (SKA) call for 25% of the total collecting area of the dish array to be located at distances greater than 180 km from the…

astro-ph.IM2010★ 1 cited

LOFAR, LEAP and beyond: Using next generation telescopes for pulsar astrophysics

Michael Kramer, Ben Stappers

Radio astronomy has benefited greatly from advances in technology and will continue to do so in the future. In fact, we are experiencing a revolution in the way radio astronomy is…

astro-ph.IM2010

Early Pulsar Observations with LOFAR

Jason Hessels, Ben Stappers, Anastasia Alexov +10

This contribution to the proceedings of "A New Golden Age for Radio Astronomy" is simply intended to give some of the highlights from pulsar observations with LOFAR at the time of…

astro-ph.IM2010★ 126 cited

Selection of radio pulsar candidates using artificial neural networks

R. P. Eatough, N. Molkenthin, M. Kramer +4

Radio pulsar surveys are producing many more pulsar candidates than can be inspected by human experts in a practical length of time. Here we present a technique to automatically id…

astro-ph.IM2009★ 10 cited

A new technique for timing the double pulsar system

P. C. C. Freire, N. Wex, M. Kramer +5

In 2004, McLaughlin et al. discovered a phenomenon in the radio emission of PSR J0737-3039B (B) that resembles drifting sub-pulses. The repeat rate of the sub-pulses is equal to th…