Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7913
Title: Low-frequency wideband timing of InPTA pulsars observed with the uGMRT
Authors: Nobleson, K.
Agarwal, Nikita
Girgaonkar, Raghav
Pandian, Arul
Chandra Joshi, Bhal
Krishnakumar, M.A.
Susobhanan, Abhimanyu
Desai, Shantanu
Prabu, T.
Bathula, Adarsh
Pennucci, Timothy T.
Banik, Sarmistha
Bagchi, Manjari
Dhanda Batra, Neelam
Choudhary, Arpita
Dandapat, Subhajit
Dey, Lankeswar
Gupta, Yashwant
Hisano, Shinnosuke
Kato, Ryo
Kharbanda, Divyansh
Kikunaga, Tomonosuke
Kolhe, Neel
Maan, Yogesh
Marmat, Piyush
Arumugam, P.
Manoharan, P.K.
Pathak, Dhruv
Singha, Jaikhomba
Surnis, Mayuresh P.
Susarla, Sai Chaitanya
Takahashi, Keitaro
Keywords: pulsars
gravitational waves
Issue Date: May-2022
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of Royal Astronomical Society, 2022, Vol. 512, p1234
Abstract: High-precision measurements of the pulsar dispersion measure (DM) are possible using telescopes with low-frequency wideband receivers. We present an initial study of the application of the wideband timing technique, which can simultaneously measure the pulsar times of arrivals (ToAs) and DMs, for a set of five pulsars observed with the upgraded Giant Metrewave Radio Telescope (uGMRT) as part of the Indian Pulsar Timing Array (InPTA) campaign. We have used the observations with the 300–500 MHz band of the uGMRT for this purpose. We obtain high precision in DM measurements with precisions of the order 10−6 cm−3 pc. The ToAs obtained have sub-μs precision and the rms of the post-fit ToA residuals are in the sub-μs range. We find that the uncertainties in the DMs and ToAs obtained with this wideband technique, applied to low-frequency data, are consistent with the results obtained with traditional pulsar timing techniques and comparable to high-frequency results from other PTAs. This work opens up an interesting possibility of using low-frequency wideband observations for precision pulsar timing and gravitational wave detection with similar precision as high-frequency observations used conventionally.
Description: Restricted Access
URI: http://hdl.handle.net/2289/7913
ISSN: 0035-8711
1365-2966 (Online)
Alternative Location: https://arxiv.org/abs/2112.06908
https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.1234N/abstract
https://inspirehep.net/literature/1989650
https://doi.org/10.1093/mnras/stac532
Copyright: 2022 The Author(s)
Appears in Collections:Research Papers(EEG)

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