The second set of pulsar discoveries by CHIME/FRB/Pulsar: 14 rotating radio transients and 7 pulsars

Author:

Dong Fengqiu Adam1ORCID,Crowter Kathryn1,Meyers Bradley W12,Pleunis Ziggy3ORCID,Stairs Ingrid1,Tan Chia Min45ORCID,Yu Tinyau Timothy1,Boyle Patrick J45,Cook Amanda M36,Fonseca Emmanuel78,Gaensler B M36,Good Deborah C910,Kaspi Victoria45,McKee James W1112ORCID,Patel Chitrang45,Pearlman Aaron B45

Affiliation:

1. Department of Physics and Astronomy, University of British Columbia , 6224 Agricultural Road, Vancouver, BC V6T 1Z1 , Canada

2. International Centre for Radio Astronomy Research, Curtin University , Bentley, WA 6102 , Australia

3. Dunlap Institute for Astronomy & Astrophysics, University of Toronto , 50 St. George Street, Toronto, ON M5S 3H4 , Canada

4. Department of Physics, McGill University , 3600 rue University, Montréal, QC H3A 2T8 , Canada

5. McGill Space Institute, McGill University , 3550 rue University, Montréal, QC H3A 2A7 , Canada

6. David A. Dunlap Institute Department of Astronomy & Astrophysics, University of Toronto , 50 St. George Street, Toronto, ON M5S 3H4 , Canada

7. Department of Physics and Astronomy, West Virginia University , Morgantown, WV 26506-6315 , USA

8. Center for Gravitational Waves and Cosmology , Chestnut Ridge Research Building, Morgantown, WV 26505 , USA

9. Department of Physics, University of Connecticut , 196A Auditorium Rd Unit 3046, Storrs, CT 06269 , USA

10. Center for Computational Astrophysics, Flatiron Institute , 162 5th Avenue, New York, New York, 10010 , USA

11. E.A. Milne Centre for Astrophysics, University of Hull , Cottingham Road, Kingston-upon-Hull HU6 7RX , UK

12. Centre of Excellence for Data Science, Artificial Intelligence and Modelling (DAIM), University of Hull , Cottingham Road, Kingston-upon-Hull HU6 7RX , UK

Abstract

ABSTRACT The Canadian Hydrogen Mapping Experiment (CHIME) is a radio telescope located in British Columbia, Canada. The large field of view allows CHIME/FRB to be an exceptional pulsar and rotating radio transient (RRAT) finding machine, despite saving only the metadata of incoming Galactic events. We have developed a pipeline to search for pulsar/RRAT candidates using density-based spatial clustering of applications with noise (dbscan), a clustering algorithm. Follow-up observations are then scheduled with the more sensitive CHIME/Pulsar instrument capable of near-daily high-time resolution spectra observations. We have developed the CHIME/Pulsar Single Pulse Pipeline to automate the processing of CHIME/Pulsar search-mode data. We report the discovery of 21 new Galactic sources, with 14 RRATs, 6 isolated long-period pulsars, and 1 binary system. Owing to CHIME/Pulsar’s observations, we have obtained timing solutions for 8 of the 14 RRATs along with all the regular pulsars and the binary system. Notably, we report that the binary system is in a long orbit of 412 d with a minimum companion mass of 0.1303 solar masses and no evidence of an optical companion within 10″ of the pulsar position. This highlights that working synergistically with CHIME/FRB’s large survey volume CHIME/Pulsar can obtain arc second localizations for low-burst rate RRATs through pulsar timing. We find that the properties of our newly discovered RRATs are consistent with those of the presently known population. They tend to have lower burst rates than those found in previous surveys, which is likely due to survey bias rather than the underlying population.

Funder

Canada Foundation for Innovation

University of Toronto

Canadian Institute for Advanced Research

McGill University

McGill Space Institute

Trottier Family Foundation

University of British Columbia

Natural Sciences and Engineering Research Council of Canada

CITA

Canada Research Chairs

CRC

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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