Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 490, Issue 4, Pages 4666-4687Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz2857
Keywords
stars: neutron; pulsars: general; gravitational waves; methods: data analysis
Categories
Funding
- NSF [1430284, 1458952]
- National Science Foundation (NSF) [AST-1744119]
- Commonwealth Government
- ERC [227947]
- STFC
- CNRS/INSU, France
- Simons Foundation
- NANOGrav Physics Frontiers Center (NSF) [1430284]
- Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav) [CE170100004]
- Australian Research Council [FL150100148]
- European Research Council [610058]
- NSFC [U15311243]
- TianShanChuangXinTuanDui
- Max-Planck Partner Group
- Youth Innovation Promotion Association of Chinese Academy of Sciences
- Chinese Academy of Science
- Chinese Academy of Sciences [XDB23000000]
- National Natural Science Foundation of China [11743002, 11873067]
- National Aeronautics and Space Administration
- JPL RTD program
- NSERC
- Canadian Institute for Advanced Research
- [XDB23010200]
- [2017YFA0402600]
- STFC [ST/N000633/1, ST/K000845/1, ST/P000649/1, ST/S000305/1, ST/H002006/1] Funding Source: UKRI
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In 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.
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