Pulsar Cyclic Spectroscopy in the Partial-deconvolution Regime: Benefits and Limitations

Journal article

Open access

Peer reviewed

Jacob E. Turner, Timothy Dolch, Paul B. Demorest, Ryan S. Lynch, Daniel R. Stinebring, Cody Jessup, Nathaniel Jones and Christopher Scheithauer

The Astrophysical journal, Vol.989(2), p.228

20/08/2025

Abstract

Interstellar medium

Millisecond pulsars

Pulsar timing method

Pulsars

url

https://doi.org/10.3847/1538-4357/adec73View

Published (Version of record) Open

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Title: Pulsar Cyclic Spectroscopy in the Partial-deconvolution Regime: Benefits and Limitations
Creators - without role: Jacob E. Turner - Green Bank Observatory , P.O. Box 2, Green Bank, WV 24944, USA
Timothy Dolch - Eureka Scientific
Paul B. Demorest - National Radio Astronomy Observatory
Ryan S. Lynch - Green Bank Observatory , P.O. Box 2, Green Bank, WV 24944, USA
Daniel R. Stinebring - Oberlin College
Cody Jessup - Montana State University
Nathaniel Jones - Hillsdale College Department of Physics, 33 E. College Street, Hillsdale, MI 49242, USA
Christopher Scheithauer - Hillsdale College
Publication Details: The Astrophysical journal, Vol.989(2), p.228
Publisher: The American Astronomical Society
Number of pages: 21
Grant note: 2009468 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001) 1430284 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001) 2020265 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001) 0968296 / National Science Foundation (NSF) (https://doi.org/10.13039/100000001)
Identifiers: 991019676496807081
Academic Unit: Physics
Language: English
Resource Type: Journal article