The Indian Pulsar Timing Array: First data release
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Published:2022
Issue:
Volume:39
Page:
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ISSN:1323-3580
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Container-title:Publications of the Astronomical Society of Australia
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language:en
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Short-container-title:Publ. Astron. Soc. Aust.
Author:
Tarafdar PratikORCID, Nobleson KORCID, Rana PrernaORCID, Singha JaikhombaORCID, Krishnakumar M. A.ORCID, Joshi Bhal ChandraORCID, Paladi Avinash KumarORCID, Kolhe NeelORCID, Batra Neelam DhandaORCID, Agarwal NikitaORCID, Bathula AdarshORCID, Dandapat SubhajitORCID, Desai ShantanuORCID, Dey LankeswarORCID, Hisano ShinnosukeORCID, Ingale PrathameshORCID, Kato RyoORCID, Kharbanda DivyanshORCID, Kikunaga TomonosukeORCID, Marmat PiyushORCID, Pandian B. ArulORCID, Prabu T.ORCID, Srivastava AmanORCID, Surnis MayureshORCID, Susarla Sai ChaitanyaORCID, Susobhanan AbhimanyuORCID, Takahashi KeitaroORCID, Arumugam P.ORCID, Bagchi ManjariORCID, Banik SarmisthaORCID, De KishalayORCID, Girgaonkar RaghavORCID, Gopakumar A.ORCID, Gupta YashwantORCID, Maan YogeshORCID, Manoharan P. K.ORCID, Naidu Arun, Pathak DhruvORCID
Abstract
Abstract
We present the pulse arrival times and high-precision dispersion measure estimates for 14 millisecond pulsars observed simultaneously in the 300
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500 MHz and 1260
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1460 MHz frequency bands using the upgraded Giant Metrewave Radio Telescope. The data spans over a baseline of 3.5 years (2018-2021), and is the first official data release made available by the Indian Pulsar Timing Array collaboration. This data release presents a unique opportunity for investigating the interstellar medium effects at low radio frequencies and their impact on the timing precision of pulsar timing array experiments. In addition to the dispersion measure time series and pulse arrival times obtained using both narrowband and wideband timing techniques, we also present the dispersion measure structure function analysis for selected pulsars. Our ongoing investigations regarding the frequency dependence of dispersion measures have been discussed. Based on the preliminary analysis for five millisecond pulsars, we do not find any conclusive evidence of chromaticity in dispersion measures. Data from regular simultaneous two-frequency observations are presented for the first time in this work. This distinctive feature leads us to the highest precision dispersion measure estimates obtained so far for a subset of our sample. Simultaneous multi-band upgraded Giant Metrewave Radio Telescope observations in 300
$-$
500 MHz and 1260
$-$
1460 MHz are crucial for high-precision dispersion measure estimation and for the prospect of expanding the overall frequency coverage upon the combination of data from the various Pulsar Timing Array consortia in the near future. Parts of the data presented in this work are expected to be incorporated into the upcoming third data release of the International Pulsar Timing Array.
Publisher
Cambridge University Press (CUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
41 articles.
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