3FGL J2051.8-5535 , the SIMBAD biblio

3FGL J2051.8-5535 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.08.18CEST22:16:50


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Title First 3 Authors
2018ApJ...867...90N 280           X C       5 6 ~ Evidence on the orbital modulated gamma-ray emissions from the redback candidate 3FGL J2039.6-5618. NG C.W., TAKATA J., STRADER J., et al.
2018ApJS..235...39C viz 19       D               1 1394 5 On the jet properties of γ-ray-loud active galactic nuclei. CHEN L.
2017A&A...602A..86L viz 18       D               1 1081 1 Research and characterisation of blazar candidates among the Fermi/LAT 3FGL catalogue using multivariate classifications. LEFAUCHEUR J. and PITA S.
2016A&A...588A.141G viz 17       D               1 213 12 High-energy sources at low radio frequency: the Murchison Widefield Array view of Fermi blazars. GIROLETTI M., MASSARO F., D'ABRUSCO R., et al.
2016ApJ...820....8S viz 17       D               1 3052 22 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.
2016ApJS..226...20F viz 17       D               1 1392 28 The spectral energy distributions of Fermi blazars. FAN J.H., YANG J.H., LIU Y., et al.
2016MNRAS.462.3180C viz 17       D               1 579 11 Blazar flaring patterns (B-FlaP) classifying blazar candidate of uncertain type in the third Fermi-LAT catalogue by artificial neural networks. CHIARO G., SALVETTI D., LA MURA G., et al.
2015ATel.8096....1C 85           X         2 2 ~ Fermi-LAT Detection of a Hard Spectrum and Enhanced Gamma-ray Emission from the Blazar PMN J2052-5533. CARPENTER B., MAGILL J. and OJHA R.
2015ApJ...810...14A viz 17       D               1 1898 269 The third catalog of active galactic nuclei detected by the Fermi large area telescope. ACKERMANN M., AJELLO M., ATWOOD W.B., et al.
2015ApJS..218...23A viz 17       D               1 3128 873 Fermi Large Area Telescope third source catalog. ACERO F., ACKERMANN M., AJELLO M., et al.

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2019.08.18-22:16:50

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