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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: ZENODO
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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MeerTime MSP Census

Authors: Spiewak, Renee; Bailes, Matthew; Miles, Matthew T; Parthasarathy, Aditya; Reardon, Daniel J; Shamohammadi, Mohsen; Shannon, Ryan M; +12 Authors

MeerTime MSP Census

Abstract

Data table and PSRFITS-format files associated with Spiewak et al. 2022, "The MeerTime Pulsar Timing Array -- A Census of Emission Properties and Timing Potential" (doi:10.1017/pasa.2022.19). The zipped tar file contains one PSRFITS-format file per pulsar, containing a profile, summed from multiple observations with varying lengths, with 1024 phase bins across the profile, 1 subintegration, 8 frequency channels across the 775.75-MHz band, and 4 polarization channels (with the up-to-date rotation measures and dispersion measures in the headers). The columns in the data table (in csv format) are as follows: PSRJ : the pulsar name (J2000) PTA_SCR : boolean indicating whether the pulsar is part of the MPTA REF_SH : short form of the reference (psrcat-style) GL, GB : Galactic longitude and latitude P0, P1 : pulse period and period derivative in (s) and (s/s), respectively DM, DM_ERR, DMEPOCH : the dispersion measure of a single epoch, with 1-sigma uncertainty, and the MJD for that epoch RM, RM_ERR : the rotation measure, as described in the paper, with uncertainty RM_SNG : boolean indicating whether the RM was measured from the summed archive (True indicates the RM_ERR is the 1-sigma uncertainty from `rmfit` and False indicates the RM_ERR is the standard deviation of all measured RMs after outlier removal) L_FRAC, L_FRAC_ERR : the fractional linear polarization and uncertainty V_FRAC, V_FRAC_ERR : the fractional circular polarization and uncertainty ABS_V_FRAC, ABS_V_FRAC_ERR : the fractional absolute circular polarization (from `psrchive`) and uncertainty TOA_ERR_NEW : the median ToA uncertainty, as described in the paper SPIND, SPIND_ERR : the spectral index from a power law fit to the flux density per band and uncertainty NOBS : number of unique observations of the pulsar included in this analysis S1400, S1400_ERR : the flux density at 1400 MHz from a power law fit to the flux density per band, and uncertainty FLUX_n_VAL, FLUX_n_ERR, FLUX_n_FRQ : flux density information per frequency band (n=0-7), the mean value, the formal error on the mean, and the mean frequency of the band html, body, table, thead, input, textarea, select {color: #bab5ab!important; background: #35393b;} input[type="text"], textarea, select {color: #bab5ab!important; background: #35393b;} [data-darksite-inline-background-image-gradient] {background: linear-gradient(rgba(0, 0, 0, 0.5), rgba(0, 0, 0, 0.5))!important; -webkit-background-size: cover!important; -moz-background-size: cover!important; -o-background-size: cover!important; background-size: cover!important;} [data-darksite-force-inline-background] * {background-color: rgba(0,0,0,0.7)!important;} [data-darksite-inline-background] {background-color: rgba(0,0,0,0.7)!important;} [data-darksite-inline-color] {color: #fff!important;} [data-darksite-inline-background-image] {background-image: linear-gradient(rgba(0,0,0,0.3), rgba(0,0,0,0.3))!important}

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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