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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7873
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dc.contributor.authorSusobhanan, Abhimanyu-
dc.contributor.authorMaan, Yogesh-
dc.contributor.authorJoshi, Bhal Chandra-
dc.contributor.authorPrabu, T.-
dc.contributor.author+ 19 Co- Authors-
dc.date.accessioned2022-01-12T10:18:38Z-
dc.date.available2022-01-12T10:18:38Z-
dc.date.issued2021-04-14-
dc.identifier.citationPublications of the Astronomical Society of Australia, 2021, Vol. 38, e017, p11en_US
dc.identifier.issn1323-3580-
dc.identifier.issn1448-6083 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/7873-
dc.descriptionOpen Accessen_US
dc.description.abstractWe introduce pinta, a pipeline for reducing the upgraded GiantMetre-wave Radio Telescope (uGMRT) raw pulsar timing data, developed for the Indian Pulsar Timing Array experiment. We provide a detailed description of the workflow and usage of pinta, as well as its computational performance and RFI mitigation characteristics. We also discuss a novel and independent determination of the relative time offsets between the different back-end modes of uGMRT and the interpretation of the uGMRT observation frequency settings and their agreement with results obtained from engineering tests. Further, we demonstrate the capability of pinta to generate data products which can produce high-precision TOAs using PSR J1909−3744 as an example. These results are crucial for performing precision pulsar timing with the uGMRT.en_US
dc.language.isoenen_US
dc.publisherCambridge University Press on behalf of the Astronomical Society of Australiaen_US
dc.relation.urihttps://doi.org/10.1017/pasa.2021.12en_US
dc.relation.urihttps://arxiv.org/abs/2007.02930en_US
dc.rights2021 The Author(s)en_US
dc.subjectastronomy data analysis – pulsarsen_US
dc.titlepinta: The uGMRT data processing pipeline for the Indian Pulsar Timing Arrayen_US
dc.typeArticleen_US
Appears in Collections:Research Papers(EEG)

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