X-Ray and Near-Infrared Observations of the Middle-aged Pulsar B1055–52, Its Multiwavelength Spectrum, and Proper Motion* * Based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. Based also on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #15676.
The Astrophysical Journal American Astronomical Society 952:2 (2023) 134
The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: A boundary layer-jet coupling?
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No redshift evolution in the rest-frame ultraviolet emission line properties of quasars from z = 1.5 to z = 4.0
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 524:4 (2023) 5497-5513
Rotational and radio emission properties of PSR J0738−4042 over half a century
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 524:4 (2023) 5904-5917
Pulsar polarization: a partial-coherence model
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