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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2023
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| Online Access: | https://arxiv.org/abs/2312.07471 |
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| _version_ | 1866910544237166592 |
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| author | McEwen, A. E. Swiggum, J. K. Kaplan, D. L. Tan, C. M. Meyers, B. W. Fonseca, E. Agazie, G. Y. Chawla, P. Crowter, K. DeCesar, M. E. Dolch, T. Dong, F. A. Fiore, W. Fonseca, E. Good, D. C. Istrate, A. G. Kaspi, V. M. Kondratiev, V. I. van Leeuwen, J. Levin, L. Lewis, E. F. Lynch, R. S. Masui, K. W. McKee, J. W. McLaughlin, M. A. Noori, H. Al Parent, E. Ransom, S. M. Siemens, X. Spiewak, R. Stairs, I. H. |
| author_facet | McEwen, A. E. Swiggum, J. K. Kaplan, D. L. Tan, C. M. Meyers, B. W. Fonseca, E. Agazie, G. Y. Chawla, P. Crowter, K. DeCesar, M. E. Dolch, T. Dong, F. A. Fiore, W. Fonseca, E. Good, D. C. Istrate, A. G. Kaspi, V. M. Kondratiev, V. I. van Leeuwen, J. Levin, L. Lewis, E. F. Lynch, R. S. Masui, K. W. McKee, J. W. McLaughlin, M. A. Noori, H. Al Parent, E. Ransom, S. M. Siemens, X. Spiewak, R. Stairs, I. H. |
| contents | The Green Bank North Celestial Cap survey is one of the largest and most sensitive searches for pulsars and transient radio objects. Observations for the survey have finished; priorities have shifted toward long-term monitoring of its discoveries. In this study, we have developed a pipeline to handle large datasets of archival observations and connect them to recent, high-cadence observations taken using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope. This pipeline handles data for 128 pulsars and has produced measurements of spin, positional, and orbital parameters that connect data over observation gaps as large as 2000 days. We have also measured glitches in the timing residuals for five of the pulsars included and proper motion for 19 sources (13 new). We include updates to orbital parameters for 19 pulsars, including 9 previously unpublished binaries. For two of these binaries, we provide updated measurements of post-Keplerian binary parameters, which result in much more precise estimates of the total masses of both systems. For PSR J0509+3801, the much improved measurement of the Einstein delay yields much improved mass measurements for the pulsar and its companion, 1.399(6)\Msun and 1.412(6)\Msun, respectively. For this system, we have also obtained a measurement of the orbital decay due to the emission of gravitational waves: $\dot{P}_{\rm B} = -1.37(7)\times10^{-12}$, which is in agreement with the rate predicted by general relativity for these masses. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2312_07471 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | The Green Bank North Celestial Cap Survey IX: Timing Follow-up for 128 Pulsars McEwen, A. E. Swiggum, J. K. Kaplan, D. L. Tan, C. M. Meyers, B. W. Fonseca, E. Agazie, G. Y. Chawla, P. Crowter, K. DeCesar, M. E. Dolch, T. Dong, F. A. Fiore, W. Fonseca, E. Good, D. C. Istrate, A. G. Kaspi, V. M. Kondratiev, V. I. van Leeuwen, J. Levin, L. Lewis, E. F. Lynch, R. S. Masui, K. W. McKee, J. W. McLaughlin, M. A. Noori, H. Al Parent, E. Ransom, S. M. Siemens, X. Spiewak, R. Stairs, I. H. High Energy Astrophysical Phenomena The Green Bank North Celestial Cap survey is one of the largest and most sensitive searches for pulsars and transient radio objects. Observations for the survey have finished; priorities have shifted toward long-term monitoring of its discoveries. In this study, we have developed a pipeline to handle large datasets of archival observations and connect them to recent, high-cadence observations taken using the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope. This pipeline handles data for 128 pulsars and has produced measurements of spin, positional, and orbital parameters that connect data over observation gaps as large as 2000 days. We have also measured glitches in the timing residuals for five of the pulsars included and proper motion for 19 sources (13 new). We include updates to orbital parameters for 19 pulsars, including 9 previously unpublished binaries. For two of these binaries, we provide updated measurements of post-Keplerian binary parameters, which result in much more precise estimates of the total masses of both systems. For PSR J0509+3801, the much improved measurement of the Einstein delay yields much improved mass measurements for the pulsar and its companion, 1.399(6)\Msun and 1.412(6)\Msun, respectively. For this system, we have also obtained a measurement of the orbital decay due to the emission of gravitational waves: $\dot{P}_{\rm B} = -1.37(7)\times10^{-12}$, which is in agreement with the rate predicted by general relativity for these masses. |
| title | The Green Bank North Celestial Cap Survey IX: Timing Follow-up for 128 Pulsars |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2312.07471 |