PSR J1018-1523 , the SIMBAD biblio

PSR J1018-1523 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST02:27:15


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Title First 3 Authors
2023ApJ...944..154S 609     A D S   X C       13 16 2 The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions. SWIGGUM J.K., PLEUNIS Z., PARENT E., et al.
2023A&A...678A.187C 17       D               1 25 ~ The MPIfR-MeerKAT Galactic Plane Survey II. The eccentric double neutron star system PSR J1208-5936 and a neutron star merger rate update. COLOM I BERNADICH M., BALAKRISHNAN V., BARR E., et al.
2023ApJ...958L..17W 44           X         1 17 ~ PSR J2150+3427: A Possible Double Neutron Star System. WU Q.D., WANG N., YUAN J.P., et al.
2024MNRAS.530.1506S 90             C       1 12 ~ The FAST Galactic Plane Pulsar Snapshot Survey - V. PSR J1901+0658 in a double neutron star system. SU W.Q., HAN J.L., YANG Z.L., et al.
2024MNRAS.532.3893Y 18       D               1 209 ~ High-priority targets for transient gravitational waves from glitching pulsars. YIM G., SHAO L. and XU R.
2024PASP..136k4202Z 18       D               1 30 ~ Be X-Ray Binaries as Progenitors of Double Neutron Stars: Evidence of Similar bi-modal Classifications. ZHOU Y.-G., WANG D.-H. and ZHANG C.-M.
2025ApJ...982..179M 19       D               1 22 ~ The Neutron Star Merger Delay-time Distribution, R-process “Knees,” and the Metal Budget of the Galaxy. MAOZ D. and NAKAR E.
2025A&A...701A.180W 47           X         1 14 ~ A deep search for radio pulsations from the 1.3 M⊙ compact-object binary companion of young pulsar PSR J1906+0746. WANG Y. and VAN LEEUWEN J.
2025MNRAS.543..233N 19       D               1 37 ~ Formation of heavy double neutron stars - I. Eddington-limited accretion for a 1.4 M⊙ neutron star at solar metallicity. NAIR A. and STEVENSON S.
2026ApJ...997...52C 20       D               1 34 ~ Forming Double Neutron Stars Using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems. CHATTARAJ A., ANDREWS J.J., BAVERA S.S., et al.

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