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The International Pulsar Timing Array: Second Data ReleaseIn this paper, we describe the International Pulsar Timing Array second data release, which includes recent pulsar timing data obtained by three regional consortia: the European Pulsar Timing Array, the North American Nanohertz Observatory for Gravitational Waves, and the
Parkes Pulsar Timing Array. We analyse and where possible combine high-precision timing data for 65 millisecond pulsars which are regularly observed by these groups. A basic noise analysis, including the processes which are both correlated and uncorrelated in time, provides noise models and timing ephemerides for the pulsars. We find that the timing precisions of pulsars are generally improved compared to the previous data release, mainly due to the addition of new data in the combination. The main purpose of this work is to create the most up-to-date IPTA data release. These data are publicly available for searches for low-frequency gravitational waves and other pulsar science.
Document ID
20210010388
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
B B P Perara ORCID
(University of Manchester Manchester, Manchester, United Kingdom)
M E DeCesar
(Lafayette College Easton, Pennsylvania, United States)
P B Demorest
(National Radio Astronomy Observatory Charlottesville, Virginia, United States)
M Kerr ORCID
(United States Naval Research Laboratory Washington D.C., District of Columbia, United States)
L Lentati
(Cavendish Laboratory Cambridge, UK)
D J Nice
(Lafayette College Easton, Pennsylvania, United States)
S Oslowski ORCID
(Swinburne University of Technology Melbourne, Victoria, Australia)
S M Ransom ORCID
(National Radio Astronomy Observatory Charlottesville, Virginia, United States)
M J Keith
(University of Manchester Manchester, Manchester, United Kingdom)
Z Arzoumanian
(Goddard Institute for Space Studies New York, New York, United States)
M Bailes
(Swinburne University of Technology Melbourne, Victoria, Australia)
P T Baker
(West Virginia University Morgantown, West Virginia, United States)
C G Bassa
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
NDR Bhat
(Curtin University Perth, Western Australia, Australia)
A Brazier
(Cornell University Ithaca, New York, United States)
M Burgay ORCID
(Osservatorio Astronomico di Cagliari Cagliari, Italy)
S Burke-Spolaor
(West Virginia University Morgantown, West Virginia, United States)
R N Caballero
(Peking University Beijing, Beijing, China)
D J Champion ORCID
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
S Chatterjee
(Cornell University Ithaca, New York, United States)
S Chen
(PSL Research University Paris, France)
I Cognard
( CNRS-Universite d’ Orleans)
J M Cordes
(Cornell University Ithaca, New York, United States)
K Crowter
(University of British Columbia Vancouver, British Columbia, Canada)
S Dai
(Australia Telescope National Facility Parkes, New South Wales, Australia)
G Desvignes
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
T Dolch
(Hillsdale College Hillsdale, Michigan, United States)
R D Ferdman
(University of East Anglia Norwich, Norfolk, United Kingdom)
E C Ferrara
(University of Maryland, College Park College Park, Maryland, United States)
E Fonseca
(McGill University Montreal, Quebec, Canada)
J M Goldstein ORCID
(University of Birmingham Birmingham, United Kingdom)
E Graikou
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
L Guillemot
( CNRS-Universite d’ Orleans)
J S Hazboun
(University of Washington Bothell Bothell, Washington, United States)
G Hobbs ORCID
(Australia Telescope National Facility Parkes, New South Wales, Australia)
H Hu ORCID
(Max Planck Institute for Radio Astronomy Bonn, Germany)
K Islo
(University of Wisconsin–Milwaukee Milwaukee, Wisconsin, United States)
G H Janssen
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
R Karuppusam
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
M Kramer
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
M T Lam
(West Virginia University Morgantown, West Virginia, United States)
K J Lee
(Peking University Beijing, Beijing, China)
K Liu
(Netherlands Institute for Radio Astronomy Dwingeloo, Netherlands)
J Luo
(University of Toronto Toronto, Ontario, Canada)
A G Lyne
(University of Manchester Manchester, Manchester, United Kingdom)
R N Manchester
(Australia Telescope National Facility Parkes, New South Wales, Australia)
J W McKee ORCID
(Australia Telescope National Facility Parkes, New South Wales, Australia)
M A McLaughlin
(West Virginia University Morgantown, West Virginia, United States)
C M F Mingarelli ORCID
(Flatiron Institute New York, New York, United States)
A P Parthasarathy
(Swinburne University of Technology Melbourne, Victoria, Australia)
T T Pennucci
(Hungarian Academy of Sciences Budapest, Hungary)
D Perrodin
(Osservatorio Astronomico di Cagliari Cagliari, Italy)
A Possenti
(Osservatorio Astronomico di Cagliari Cagliari, Italy)
D J Reardon ORCID
(Swinburne University of Technology Melbourne, Victoria, Australia)
C J Russell ORCID
(CSIRO Scientific Computing Canberra, Australian Capital Territory, Australia)
S A Sanidas
(University of Manchester Manchester, Manchester, United Kingdom)
A Sesana
(University of Milano-Bicocca Milan, Italy)
G Shaifullah ORCID
(University of Milano-Bicocca Milan, Italy)
R M Shannon
(Swinburne University of Technology Melbourne, Victoria, Australia)
X Siemens
(University of Wisconsin–Milwaukee Milwaukee, Wisconsin, United States)
J Simon
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
R Spiewak ORCID
(University of Manchester Manchester, Manchester, United Kingdom)
I H Stairs
(University of British Columbia Vancouver, British Columbia, Canada)
B W Stappers
(University of Manchester Manchester, Manchester, United Kingdom)
J K Swiggum
(University of Wisconsin–Milwaukee Milwaukee, Wisconsin, United States)
S R Taylor
(California Institute of Technology Pasadena, California, United States)
G Theureau
(CNRS-Universite d’Orleans)
C Tiburzi
(University of British Columbia Vancouver, British Columbia, Canada)
M Vallisneri
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
A Vecchio
(University of Birmingham Birmingham, United Kingdom)
J B Wang
(Chinese Academy of Sciences Beijing, Beijing, China)
S B Zhang
(Chinese Academy of Sciences Beijing, Beijing, China)
L Zhang
(Chinese Academy of Sciences Beijing, Beijing, China)
W W Zhu
(Chinese Academy of Sciences Beijing, Beijing, China)
X J Zhu ORCID
(Monash University Melbourne, Victoria, Australia)
Date Acquired
February 19, 2021
Publication Date
October 12, 2019
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford
Volume: 490
Issue: 4
Issue Publication Date: December 1, 2019
ISSN: 0035-8711
e-ISSN: 1365-2966
Subject Category
Astronomy
Funding Number(s)
WBS: 273493
CONTRACT_GRANT: 80GSFC17M0002
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
neutron
pulsars
gravitational waves
data analysis
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