PSR J2042+0246 , the SIMBAD biblio

PSR J2042+0246 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:05:29


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Title First 3 Authors
2015ApJS..218...23A viz 16       D               1 3140 1411 Fermi Large Area Telescope third source catalog. ACERO F., ACKERMANN M., AJELLO M., et al.
2016ApJ...819...34C 16       D               2 39 33 Six new millisecond pulsars from Arecibo searches of Fermi gamma-ray sources. CROMARTIE H.T., CAMILO F., KERR M., et al.
2016ApJ...820....8S viz 16       D               1 3047 91 Classification and ranking of Fermi LAT gamma-ray sources from the 3FGL catalog using machine learning techniques. SAZ PARKINSON P.M., XU H., YU P.L.H., et al.
2018ApJS..237...32A viz 16       D               1 2605 130 The search for spatial extension in high-latitude sources detected by the Fermi Large Area Telescope. ACKERMANN M., AJELLO M., BALDINI L., et al.
2018MNRAS.481.3966B 16       D               1 154 15 Bayesian model comparison and analysis of the Galactic disc population of gamma-ray millisecond pulsars. BARTELS R.T., EDWARDS T.D.P. and WENIGER C.
2019ApJ...879...10A viz 16       D               1 225 87 Searches for gravitational waves from known pulsars at two harmonics in 2015-2017 LIGO data. ABBOTT B.P., ABBOTT R., ABBOTT T.D., et al.
2020MNRAS.492.3032K 1029   K A D S   X C       24 11 ~ Searching for optical companions to four binary millisecond pulsars with the Gran Telescopio Canarias. KIRICHENKO A.Y., KARPOVA A.V., ZYUZIN D.A., et al.
2020ApJS..247...33A viz 16       D               1 5175 880 Fermi Large Area Telescope fourth source catalog. ABDOLLAHI S., ACERO F., ACKERMANN M., et al.
2021MNRAS.505.5853G 17       D               2 5834 ~ Artificial Neural Network classification of 4FGL sources. GERMANI S., TOSTI G., LUBRANO P., et al.
2021ApJ...916..100R viz 17       D               1 422 2 Analyzing the Galactic pulsar distribution with machine learning. RONCHI M., GRABER V., GARCIA-GARCIA A., et al.
2022MNRAS.510.6011W 17       D               1 53 15 Formation of millisecond pulsars with long orbital periods by accretion-induced collapse of white dwarfs. WANG B., LIU D. and CHEN H.
2022A&A...660A..87B viz 17       D               2 6191 10 Machine learning methods for constructing probabilistic Fermi-LAT catalogs. BHAT A. and MALYSHEV D.
2022ApJS..260...53A viz 17       D               1 6710 133 Incremental Fermi Large Area Telescope Fourth Source Catalog. ABDOLLAHI S., ACERO F., BALDINI L., et al.
2022ApJ...934...65K 17       D               1 191 3 The Fundamental Plane Relation for Gamma-Ray Pulsars Implied by 4FGL. KALAPOTHARAKOS C., WADIASINGH Z., HARDING A.K., et al.
2023ApJ...958..191S 17       D               4 502 ~ The Third Fermi Large Area Telescope Catalog of Gamma-Ray Pulsars. SMITH D.A., ABDOLLAHI S., AJELLO M., et al.
2023RAA....23j4002W viz 17       D               1 530 ~ FAST Pulsar Database. I. Polarization Profiles of 682 Pulsars. WANG P.F., HAN J.L., XU J., et al.
2024MNRAS.530.3552L 18       D               4 129 ~ The effect of pulsar geometry on the observed gamma-ray spectrum of millisecond pulsars. LLOYD S.J., CHADWICK P.M. and BROWN A.M.
2024MNRAS.532.2196W 18       D               1 49 ~ Formation of millisecond pulsars with wide orbits. WANG B., LIU D., GUO Y., et al.
2024MNRAS.532.3893Y 18       D               2 209 ~ High-priority targets for transient gravitational waves from glitching pulsars. YIM G., SHAO L. and XU R.
2024MNRAS.533.3637C 18       D               1 33 ~ Spin evolution of neutron stars in transient low-mass X-ray binaries. CUI Z. and LI X.-D.
2025ApJ...985...58A 19       D               1 297 ~ Prediction of Radio-quiet Gamma-Ray Pulsar Distances Using the Fundamental Plane Relation. ANGUNER E.O.
2025MNRAS.541..806I 112       D         F     2 230 ~ Synchro-curvature description of γ-ray light curves and spectra of pulsars: concurrent fitting. INIGUEZ-PASCUAL D., TORRES D.F. and VIGANO D.
2025ApJ...992..116M 19       D               1 181 ~ Irradiated Pulsar Planets and Companions as 511 keV Positron Annihilation Line Sources. METZLER Z. and WADIASINGH Z.

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