HAWC J0635+070 , the SIMBAD biblio

HAWC J0635+070 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST04:55:51


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Title First 3 Authors
2020MNRAS.493.1874D 206           X C       4 17 ~ XMM-Newton observations of a gamma-ray pulsar J0633+0632: pulsations, cooling and large-scale emission. DANILENKO A., KARPOVA A., OFENGEIM D., et al.
2020A&A...636A.113G 124           X         3 49 59 Halo fraction in TeV-bright pulsar wind nebulae. GIACINTI G., MITCHELL A.M.W., LOPEZ-COTO R., et al.
2018ATel12013....1B 161 T         X         3 2 ~ HAWC detection of TeV source
HAWC J0635+070.
BRISBOIS C., RIVIERE C., FLEISCHHACK H., et al.
2020ApJ...905...76A viz 59       D     X         2 89 89 3HWC: the third HAWC catalog of very-high-energy gamma-ray sources. ALBERT A., ALFARO R., ALVAREZ C., et al.
2022MNRAS.513.2884L 17       D               1 26 3 Prospect of detecting X-ray haloes around middle-aged pulsars with eROSITA. LI B., ZHANG Y., LIU T., et al.
2023ApJ...956...20A 17       D               2 35 ~ Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube. ABBASI R., ACKERMANN M., ADAMS J., et al.
2024ApJS..271...25C viz 18       D               1 176 ~ The First LHAASO Catalog of Gamma-Ray Sources. CAO Z., AHARONIAN F., AN Q., et al.
2024A&A...683A.180K 90               F     1 21 ~ Searching for X-ray counterparts of degree-wide TeV halos around middle-aged pulsars with SRG/eROSITA. KHOKHRIAKOVA A., BECKER W., PONTI G., et al.
2024ApJ...968..117Z 45           X         1 34 ~ Finding Candidate TeV Halos among Very-high-energy Sources. ZHENG D. and WANG Z.
2024A&A...689A.258C 45           X         1 29 ~ Detection prospects of very and ultra high-energy gamma rays from extended sources with ASTRI, CTA, and LHAASO. CELLI S. and PERON G.
2024ApJ...976....8A 108       D         F     5 34 ~ Search for Joint Multimessenger Signals from Potential Galactic Cosmic-Ray Accelerators with HAWC and IceCube. ALFARO R., ALVAREZ C., ARTEAGA-VELAZQUEZ J.C., et al.
2024ApJ...977L...3K 18       D               1 70 ~ Quantitative Constraint on the Contribution of Resolved Gamma-Ray Sources to the Sub-PeV Galactic Diffuse Gamma-Ray Flux Measured by the Tibet ASγ Experiment. KATO S., ANZORENA M., CHEN D., et al.

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