Long-term timing observations of 374 pulsars : J/MNRAS/353/1311

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Authors : Hobbs G. orcid , Lyne A.G., Kramer M. (hide) , Lyne A.G., Kramer M. et..al

VizieR DOI : https://doi.org/10.26093/cds/vizier.73531311
Bibcode : 2004MNRAS.353.1311H (ADS) (Simbad) (Objects)
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CDS Keywords : Pulsars; Proper motions
UAT : Pulsars, Proper motions

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Inserted into VizieR : 11-Feb-2006
Last modification : 29-Jun-2024

Long-term timing observations of 374 pulsars. (2004)

Keywords : methods data analysis - astrometry - pulsars: general

Abstract:We present pulsar timing solutions for 374 pulsars. Each ephemeris was obtained by analysing archival data stored at Jodrell Bank Observatory. This data archive contains over 5600yr of pulsar rotational history with individual data-spans of up to 34yr. A new method has been developed to mitigate the effects of timing noise by whitening the pulsar timing residuals. ...(more)
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Monthly Notices policies
The majority of pulse times of arrival (TOAs) were obtained using the 76-m Lovell Radio Telescope at Jodrell Bank Observatory. Results are also included, for the brighter pulsars, from the 30-m MkII telescope also situated at Jodrell Bank. The earliest TOAs for 18 pulsars (between the years 1968 and 1981) were obtained from observations using the NASA Deep Space Network (Downs & Reichley, 1983ApJS...53..169D). 


                


                

                    

                


                

                    

                


                

                    
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