The central compact object 1E 1207.4-5209 emits pulsed radio waves at its 0.4-second spin period, revealing it as a faint radio pulsar.
PSRCHIVE and PSRFITS An Open Approach to Radio Pulsar Data Storage and Analysis
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
abstract
A new set of software applications and libraries for use in the archival and analysis of pulsar astronomical data is introduced. Known collectively as the PSRCHIVE scheme, the code was developed in parallel with a new data storage format called PSRFITS, which is based on the Flexible Image Transport System (FITS). Both of these projects utilise a modular, object-oriented design philosophy. PSRCHIVE is an open source development environment that incorporates an extensive range of C++ object classes and pre-built command line and graphical utilities. These deal transparently and simultaneously with multiple data storage formats, thereby enhancing data portability and facilitating the adoption of the PSRFITS file format. Here, data are stored in a series of modular header-data units that provide flexibility and scope for future expansion. As it is based on FITS, various standard libraries and applications may be used for data input/output and visualisation. Both PSRCHIVE and PSRFITS are made publicly available to the academic community in the hope that this will promote their widespread use and acceptance.
representative citing papers
First detection of relativistic angular deformation δ_θ in PSR J1757−1854 via MeerKAT-enhanced timing, ruling out two of four prior geometric solutions while confirming GR consistency for orbital decay.
toa_sp applies multiple single-pulse timing strategies to 688 pulses from RRAT J1913+1330, yielding 1.33 ms weighted RMS residuals (24% better than PSRCHIVE) while keeping all pulses.
Bayesian fitting of an eccentric Keplerian orbit to the radio light curve of PKS 2131-021 gives e = 0.053 ± 0.015 without red noise but favors a circular orbit plus DRW noise with e < 0.15.
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.
citing papers explorer
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Detection of relativistic orbital deformation from improved timing of PSR J1757$-$1854
First detection of relativistic angular deformation δ_θ in PSR J1757−1854 via MeerKAT-enhanced timing, ruling out two of four prior geometric solutions while confirming GR consistency for orbital decay.
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TOA_SP: A Multi-Strategy Framework for Single-Pulse Timing
toa_sp applies multiple single-pulse timing strategies to 688 pulses from RRAT J1913+1330, yielding 1.33 ms weighted RMS residuals (24% better than PSRCHIVE) while keeping all pulses.
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Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211
Bayesian fitting of an eccentric Keplerian orbit to the radio light curve of PKS 2131-021 gives e = 0.053 ± 0.015 without red noise but favors a circular orbit plus DRW noise with e < 0.15.
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Searching for links between energetic millisecond pulsars and repeating fast radio bursts
Wideband observations show M28A giant pulses differ from FRB 20200120E bursts in duration, luminosity, timing statistics, and spectral structure, yielding no strong evidence for a direct link.