9.8k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- West Virginia UniversityUS118 papers
- University of Wisconsin–MilwaukeeUS108 papers
- Goddard Space Flight CenterUS107 papers
- Eötvös Loránd UniversityHU95 papers
- California Institute of TechnologyUS92 papers
- Cornell UniversityUS87 papers
- Rochester Institute of TechnologyUS83 papers
- Swinburne University of TechnologyAU80 papers
- University of TorontoCA80 papers
- Columbia UniversityUS78 papers
- Montana State UniversityUS78 papers
- University of Washington BothellUS77 papers
14 papers · 1 filter
Design and Commissioning of an LWA Swarm Station: The Long Wavelength Array -- North Arm
C. A. Taylor, J. Dowell, G. B. Taylor +9
Modern radio interferometers are designed with increasingly sprawling geographical footprints, offering enhanced sensitivity and resolution. However, managing such extensive facili…
A radio technosignature search towards Proxima Centauri resulting in a signal-of-interest
Shane Smith, Danny C Price, Sofia Z Sheikh +15
The detection of life beyond Earth is an ongoing scientific endeavour, with profound implications. One approach, known as the search for extraterrestrial intelligence (SETI), seeks…
Analysis of the Breakthrough Listen signal of interest blc1 with a technosignature verification framework
Sofia Z. Sheikh, Shane Smith, Danny C. Price +15
The aim of the search for extraterrestrial intelligence (SETI) is to find technologically-capable life beyond Earth through their technosignatures. On 2019 April 29, the Breakthrou…
A pulsar-based timescale from the International Pulsar Timing Array
G. Hobbs, L. Guo, R. N. Caballero +56
We have constructed a new timescale, TT(IPTA16), based on observations of radio pulsars presented in the first data release from the International Pulsar Timing Array (IPTA). We us…
Template bank for spinning compact binary mergers in the second observation run of Advanced LIGO and the first observation run of Advanced Virgo
Debnandini Mukherjee, Sarah Caudill, Ryan Magee +25
We describe the methods used to construct the aligned-spin template bank of gravitational waveforms used by the GstLAL-based inspiral pipeline to analyze data from the second obser…
Noise Budget and Interstellar Medium Mitigation Advances in the NANOGrav Pulsar Timing Array
T. Dolch, S. Chatterjee, J. M. Cordes +9
Gravitational wave (GW) detection with pulsar timing arrays (PTAs) requires accurate noise characterization. The noise of our Galactic-scale GW detector has been systematically eva…
Thermal modelling of Advanced LIGO test masses
Haoyu Wang, Carl Blair, Miguel Dovale Álvarez +8
High-reflectivity fused silica mirrors are at the epicentre of current advanced gravitational wave detectors. In these detectors, the mirrors interact with high power laser beams.…
Statistical Analyses for NANOGrav 5-year Timing Residuals
Y. Wang, J. M. Cordes, F. A. Jenet +11
In pulsar timing, timing residuals are the differences between the observed times of arrival and the predictions from the timing model. A comprehensive timing model will produce fe…
From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release
L. Lentati, R. M. Shannon, W. A. Coles +80
We analyse the stochastic properties of the 49 pulsars that comprise the first International Pulsar Timing Array (IPTA) data release. We use Bayesian methodology, performing model…
The International Pulsar Timing Array: First Data Release
J. P. W. Verbiest, L. Lentati, G. Hobbs +89
The highly stable spin of neutron stars can be exploited for a variety of (astro-)physical investigations. In particular arrays of pulsars with rotational periods of the order of m…
Analytical model for ring heater thermal compensation in the Advanced Laser Interferometer Gravitational-wave Observatory
Joshua Ramette, Marie Kasprzack, Aidan Brooks +3
Advanced laser interferometer gravitational-wave detectors use high laser power to achieve design sensitivity. A small part of this power is absorbed in the interferometer cavity m…
The NANOGrav Nine-Year Data Set: Noise Budget for Pulsar Arrival Times on Intraday Timescales
M. T. Lam, J. M. Cordes, S. Chatterjee +21
The use of pulsars as astrophysical clocks for gravitational wave experiments demands the highest possible timing precision. Pulse times of arrival (TOAs) are limited by stochastic…
Single-Source Gravitational Wave Limits from the J1713+0747 24-hr Global Campaign
T. Dolch, J. A. Ellis, S. Chatterjee +34
Dense, continuous pulsar timing observations over a 24-hr period provide a method for probing intermediate gravitational wave (GW) frequencies from 10 microhertz to 20 millihertz.…
The NANOGrav Nine-year Data Set: Observations, Arrival Time Measurements, and Analysis of 37 Millisecond Pulsars
Z. Arzoumanian, A. Brazier, S. Burke-Spolaor +41
We present high-precision timing observations spanning up to nine years for 37 millisecond pulsars monitored with the Green Bank and Arecibo radio telescopes as part of the North A…