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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/8706
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dc.contributor.authorSusobhanan, Abhimanyu-
dc.contributor.authorPaladi, Avinash Kumar-
dc.contributor.authorDesmecht, Réka-
dc.contributor.authorAmarnath-
dc.contributor.authorBagchi, Manjari-
dc.contributor.authorChakraborty, Manoneeta-
dc.contributor.authorChowdhury, Shaswata-
dc.contributor.authorDas, Suruj Jyoti-
dc.contributor.authorDeb, Debabrata-
dc.contributor.authorDesai, Shantanu-
dc.contributor.authorDwivedi, Churchil-
dc.contributor.authorGrover, Himanshu-
dc.contributor.authorJose, Jibin-
dc.contributor.authorJoshi, Bhal Chandra-
dc.contributor.authorKala, Shubham-
dc.contributor.authorKareem, Fazal-
dc.contributor.authorMeena, Kuldeep-
dc.contributor.authorMondal, Sushovan-
dc.contributor.authorNobleson, K-
dc.contributor.authorPandian, B Arul-
dc.contributor.authorRai, Kaustubh-
dc.contributor.authorShukla, Adya-
dc.contributor.authorSingh, Manpreet-
dc.contributor.authorSrivastava, Aman-
dc.contributor.authorSurnis, Mayuresh-
dc.contributor.authorTahbildar, Hemanga-
dc.contributor.authorTakahashi, Keitaro-
dc.contributor.authorTarafdar, Pratik-
dc.contributor.authorVara, Kunjal-
dc.contributor.authorVyasraj, Vaishnavi-
dc.contributor.authorZuraiq, Zenia-
dc.date.accessioned2026-04-15T05:10:40Z-
dc.date.available2026-04-15T05:10:40Z-
dc.date.issued2026-03-09-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2026, Vol. 547 (4), AR No. stag444en_US
dc.identifier.issn1365-2966-
dc.identifier.urihttp://hdl.handle.net/2289/8706-
dc.descriptionOpen Access. Also available at arXiv.org (one of the alternative locations)en_US
dc.description.abstractIn the wideband paradigm of pulsar timing, the time of arrival of a pulsar pulse is measured simultaneously with the corresponding dispersion measure from a frequency-resolved integrated pulse profile. We present a new method for performing wideband measurements that rigorously accounts for measurement noise. We demonstrate this method using observations of PSR J2124−3358 made as part of the Indian Pulsar Timing Array experiment using the upgraded Giant Metre-wave Radio Telescope, and show that our method produces more realistic measurement uncertainty estimates compared to the existing wideband measurement method.en_US
dc.language.isoenen_US
dc.publisherMonthly Notices of the Royal Astronomical Societyen_US
dc.relation.urihttps://doi.org/10.48550/arXiv.2512.01288en_US
dc.relation.urihttps://doi.org/10.1093/mnras/stag444en_US
dc.rights© The Author(s) 2026en_US
dc.subjectmethods: data analysisen_US
dc.subjectpulsars: generalen_US
dc.titleRevisiting wideband pulsar timing measurementsen_US
dc.typeArticleen_US
dc.additionalCollection: RAS Journalsen_US
Appears in Collections:Research Papers (A&A)

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