Multi-band Extension of the Wideband Timing Technique
The wideband timing technique enables the high-precision simultaneous estimation of pulsar Times of Arrival (ToAs) and Dispersion Measures (DMs) while effectively modeling frequency-dependent profile evolution. We present two novel independent methods that extend the standard wideband technique to h...
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creator | Paladi, Avinash Kumar Dwivedi, Churchil Rana, Prerna Nobleson, K Susobhanan, Abhimanyu Joshi, Bhal Chandra Tarafdar, Pratik Deb, Debabrata Arumugam, Swetha Gopakumar, A Krishnakumar, M A Neelam Dhanda Batra Debnath, Jyotijwal Fazal Kareem Arumugam, Paramasivan Bagchi, Manjari Bathula, Adarsh Dandapat, Subhajit Desai, Shantanu Gupta, Yashwant Hisano, Shinnosuke Kharbanda, Divyansh Kikunaga, Tomonosuke Kolhe, Neel Maan, Yogesh Manoharan, P K Singha, Jaikhomba Srivastava, Aman Surnis, Mayuresh Takahashi, Keitaro |
description | The wideband timing technique enables the high-precision simultaneous estimation of pulsar Times of Arrival (ToAs) and Dispersion Measures (DMs) while effectively modeling frequency-dependent profile evolution. We present two novel independent methods that extend the standard wideband technique to handle simultaneous multi-band pulsar data incorporating profile evolution over a larger frequency span to estimate DMs and ToAs with enhanced precision. We implement the wideband likelihood using the libstempo python interface to perform wideband timing in the tempo2 framework. We present the application of these techniques to the dataset of fourteen millisecond pulsars observed simultaneously in Band 3 (300 - 500 MHz) and Band 5 (1260 - 1460 MHz) of the upgraded Giant Metrewave Radio Telescope (uGMRT) with a large band gap of 760 MHz as a part of the Indian Pulsar Timing Array (InPTA) campaign. We achieve increased ToA and DM precision and sub-microsecond root mean square post-fit timing residuals by combining simultaneous multi-band pulsar observations done in non-contiguous bands for the first time using our novel techniques. |
doi_str_mv | 10.48550/arxiv.2304.13072 |
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We present two novel independent methods that extend the standard wideband technique to handle simultaneous multi-band pulsar data incorporating profile evolution over a larger frequency span to estimate DMs and ToAs with enhanced precision. We implement the wideband likelihood using the libstempo python interface to perform wideband timing in the tempo2 framework. We present the application of these techniques to the dataset of fourteen millisecond pulsars observed simultaneously in Band 3 (300 - 500 MHz) and Band 5 (1260 - 1460 MHz) of the upgraded Giant Metrewave Radio Telescope (uGMRT) with a large band gap of 760 MHz as a part of the Indian Pulsar Timing Array (InPTA) campaign. We achieve increased ToA and DM precision and sub-microsecond root mean square post-fit timing residuals by combining simultaneous multi-band pulsar observations done in non-contiguous bands for the first time using our novel techniques.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2304.13072</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Broadband ; Evolution ; Millisecond pulsars ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Radio telescopes</subject><ispartof>arXiv.org, 2023-11</ispartof><rights>2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,786,887,27932</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2304.13072$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stad3122$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Paladi, Avinash Kumar</creatorcontrib><creatorcontrib>Dwivedi, Churchil</creatorcontrib><creatorcontrib>Rana, Prerna</creatorcontrib><creatorcontrib>Nobleson, K</creatorcontrib><creatorcontrib>Susobhanan, Abhimanyu</creatorcontrib><creatorcontrib>Joshi, Bhal Chandra</creatorcontrib><creatorcontrib>Tarafdar, Pratik</creatorcontrib><creatorcontrib>Deb, Debabrata</creatorcontrib><creatorcontrib>Arumugam, Swetha</creatorcontrib><creatorcontrib>Gopakumar, A</creatorcontrib><creatorcontrib>Krishnakumar, M A</creatorcontrib><creatorcontrib>Neelam Dhanda Batra</creatorcontrib><creatorcontrib>Debnath, Jyotijwal</creatorcontrib><creatorcontrib>Fazal Kareem</creatorcontrib><creatorcontrib>Arumugam, Paramasivan</creatorcontrib><creatorcontrib>Bagchi, Manjari</creatorcontrib><creatorcontrib>Bathula, Adarsh</creatorcontrib><creatorcontrib>Dandapat, Subhajit</creatorcontrib><creatorcontrib>Desai, Shantanu</creatorcontrib><creatorcontrib>Gupta, Yashwant</creatorcontrib><creatorcontrib>Hisano, Shinnosuke</creatorcontrib><creatorcontrib>Kharbanda, Divyansh</creatorcontrib><creatorcontrib>Kikunaga, Tomonosuke</creatorcontrib><creatorcontrib>Kolhe, Neel</creatorcontrib><creatorcontrib>Maan, Yogesh</creatorcontrib><creatorcontrib>Manoharan, P K</creatorcontrib><creatorcontrib>Singha, Jaikhomba</creatorcontrib><creatorcontrib>Srivastava, Aman</creatorcontrib><creatorcontrib>Surnis, Mayuresh</creatorcontrib><creatorcontrib>Takahashi, Keitaro</creatorcontrib><title>Multi-band Extension of the Wideband Timing Technique</title><title>arXiv.org</title><description>The wideband timing technique enables the high-precision simultaneous estimation of pulsar Times of Arrival (ToAs) and Dispersion Measures (DMs) while effectively modeling frequency-dependent profile evolution. We present two novel independent methods that extend the standard wideband technique to handle simultaneous multi-band pulsar data incorporating profile evolution over a larger frequency span to estimate DMs and ToAs with enhanced precision. We implement the wideband likelihood using the libstempo python interface to perform wideband timing in the tempo2 framework. We present the application of these techniques to the dataset of fourteen millisecond pulsars observed simultaneously in Band 3 (300 - 500 MHz) and Band 5 (1260 - 1460 MHz) of the upgraded Giant Metrewave Radio Telescope (uGMRT) with a large band gap of 760 MHz as a part of the Indian Pulsar Timing Array (InPTA) campaign. 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We present two novel independent methods that extend the standard wideband technique to handle simultaneous multi-band pulsar data incorporating profile evolution over a larger frequency span to estimate DMs and ToAs with enhanced precision. We implement the wideband likelihood using the libstempo python interface to perform wideband timing in the tempo2 framework. We present the application of these techniques to the dataset of fourteen millisecond pulsars observed simultaneously in Band 3 (300 - 500 MHz) and Band 5 (1260 - 1460 MHz) of the upgraded Giant Metrewave Radio Telescope (uGMRT) with a large band gap of 760 MHz as a part of the Indian Pulsar Timing Array (InPTA) campaign. 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subjects | Broadband Evolution Millisecond pulsars Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Radio telescopes |
title | Multi-band Extension of the Wideband Timing Technique |
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