The AO327 Drift Survey Catalog and Data Release of Pulsar Detections
The AO327 drift survey for radio pulsars and transients used the Arecibo telescope from 2010 until its collapse in 2020. AO327 collected ∼3100 hr of data at 327 MHz with a time resolution of 82 μ s and a frequency resolution of 24 kHz. While the main motivation for such surveys is the discovery of n...
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IOP Publishing
2024-01-01
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Online Access: | https://doi.org/10.3847/1538-4365/ad19da |
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author | J. S. Deneva M. McLaughlin T. E. E. Olszanski E. F. Lewis D. Pang P. C. C. Freire M. Bagchi K. Stovall |
author_facet | J. S. Deneva M. McLaughlin T. E. E. Olszanski E. F. Lewis D. Pang P. C. C. Freire M. Bagchi K. Stovall |
author_sort | J. S. Deneva |
collection | DOAJ |
description | The AO327 drift survey for radio pulsars and transients used the Arecibo telescope from 2010 until its collapse in 2020. AO327 collected ∼3100 hr of data at 327 MHz with a time resolution of 82 μ s and a frequency resolution of 24 kHz. While the main motivation for such surveys is the discovery of new pulsars and new, even unforeseen, types of radio transients, they also serendipitously collect a wealth of data on known pulsars. We present an electronic catalog of data and data products of 206 pulsars whose periodic emission was detected by AO327 and are listed in the Australia Telescope National Facility catalog of all published pulsars. The AO327 data products include dedispersed time series at full time resolution, average (“folded”) pulse profiles, Gaussian pulse profile templates, and an absolute phase reference that allows phase aligning the AO327 pulse profiles in a physically meaningful manner with profiles from data taken with other instruments. We also provide machine-readable tables with uncalibrated flux measurements at 327 MHz and pulse widths at 50% and 10% of the pulse peak determined from the fitted Gaussian profile templates. The AO327 catalog data set can be used in applications like population analysis of radio pulsars, pulse profile evolution studies in time and frequency, cone and core emission of the pulsar beam, scintillation, pulse intensity distributions, and others. It also constitutes a ready-made resource for teaching signal-processing and pulsar astronomy techniques. |
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spelling | doaj.art-7a59c60c110c4ecfb53b4242ef24aaf42024-02-26T10:06:44ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492024-01-0127112310.3847/1538-4365/ad19daThe AO327 Drift Survey Catalog and Data Release of Pulsar DetectionsJ. S. Deneva0https://orcid.org/0000-0003-1226-0793M. McLaughlin1https://orcid.org/0000-0001-7697-7422T. E. E. Olszanski2E. F. Lewis3https://orcid.org/0000-0002-2972-522XD. Pang4P. C. C. Freire5https://orcid.org/0000-0003-1307-9435M. Bagchi6https://orcid.org/0000-0001-8640-8186K. Stovall7https://orcid.org/0000-0002-7261-594XGeorge Mason University , 4400 University Dr., Fairfax, VA 22030, USAWest Virginia University , P.O. Box 6315, Morgantown, WV 26506, USAWest Virginia University , P.O. Box 6315, Morgantown, WV 26506, USAWest Virginia University , P.O. Box 6315, Morgantown, WV 26506, USAWest Virginia University , P.O. Box 6315, Morgantown, WV 26506, USAMax-Planck-Institut für Radioastronomie , Bonn, GermanyThe Institute of Mathematical Sciences , Chennai 600113, India; Homi Bhabha National Institute , Mumbai 400094, IndiaUniversity of New Mexico , Albuquerque, NM 87131, USAThe AO327 drift survey for radio pulsars and transients used the Arecibo telescope from 2010 until its collapse in 2020. AO327 collected ∼3100 hr of data at 327 MHz with a time resolution of 82 μ s and a frequency resolution of 24 kHz. While the main motivation for such surveys is the discovery of new pulsars and new, even unforeseen, types of radio transients, they also serendipitously collect a wealth of data on known pulsars. We present an electronic catalog of data and data products of 206 pulsars whose periodic emission was detected by AO327 and are listed in the Australia Telescope National Facility catalog of all published pulsars. The AO327 data products include dedispersed time series at full time resolution, average (“folded”) pulse profiles, Gaussian pulse profile templates, and an absolute phase reference that allows phase aligning the AO327 pulse profiles in a physically meaningful manner with profiles from data taken with other instruments. We also provide machine-readable tables with uncalibrated flux measurements at 327 MHz and pulse widths at 50% and 10% of the pulse peak determined from the fitted Gaussian profile templates. The AO327 catalog data set can be used in applications like population analysis of radio pulsars, pulse profile evolution studies in time and frequency, cone and core emission of the pulsar beam, scintillation, pulse intensity distributions, and others. It also constitutes a ready-made resource for teaching signal-processing and pulsar astronomy techniques.https://doi.org/10.3847/1538-4365/ad19daPulsarsNeutron starsCatalogsSurveys |
spellingShingle | J. S. Deneva M. McLaughlin T. E. E. Olszanski E. F. Lewis D. Pang P. C. C. Freire M. Bagchi K. Stovall The AO327 Drift Survey Catalog and Data Release of Pulsar Detections The Astrophysical Journal Supplement Series Pulsars Neutron stars Catalogs Surveys |
title | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections |
title_full | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections |
title_fullStr | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections |
title_full_unstemmed | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections |
title_short | The AO327 Drift Survey Catalog and Data Release of Pulsar Detections |
title_sort | ao327 drift survey catalog and data release of pulsar detections |
topic | Pulsars Neutron stars Catalogs Surveys |
url | https://doi.org/10.3847/1538-4365/ad19da |
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