eHWC J1825-134 , the SIMBAD biblio

eHWC J1825-134 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST11:24:46

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2020MNRAS.498.4901F 41           X         1 10 ~ Investigating the multiband non-thermal emission of the 100 TeV source eHWC J2019+368 with a pulsar wind nebula scenario. FANG J., WEN L., YU H., et al.
2020A&A...644A.112H 207           X C       4 12 12 An extreme particle accelerator in the Galactic plane: HESS J1826-130. HESS COLLABORATION, ABDALLA H., ADAM R., et al.
2021ApJ...907L..30A viz 378           X C       8 13 38 Evidence of 200 TeV photons from HAWC J1825-134. ALBERT A., ALFARO R., ALVAREZ C., et al.
2021MNRAS.503.3522M 125           X         3 71 11 Using interstellar clouds to search for Galactic PeVatrons: gamma-ray signatures from supernova remnants. MITCHELL A.M.W., ROWELL G.P., CELLI S., et al.
2021ApJ...911L..27A 43           X         1 28 29 Evidence that ultra-high-energy gamma rays are a universal feature near powerful pulsars. ALBERT A., ALFARO R., ALVAREZ C., et al.
2021Natur.594...33C 52     A D               9 20 207 Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 gam-ray Galactic sources. CAO Z., AHARONIAN F.A., AN Q., et al.
2022ApJ...925...85H 468     A D     X C       11 44 6 Constraints on Hadronic Contributions to LHAASO Sources with Neutrino Observations. HUANG T.-Q. and LI Z.
2022A&A...660A...8B 299       S   X C       5 14 15 Pulsar wind nebula origin of the LHAASO-detected ultra-high energy γ-ray sources. BREUHAUS M., REVILLE B. and HINTON J.A.
2022ApJ...930L...2D 17       D               2 32 13 On the Potential of Bright, Young Pulsars to Power Ultrahigh Gamma-Ray Sources. DE ONA WILHELMI E., LOPEZ-COTO R., AMATO E., et al.
2022ApJ...930..148B 128           X         3 23 7 The Eel Pulsar Wind Nebula: A PeVatron-candidate Origin for HAWC J1826-128 and HESS J1826-130. BURGESS D.A., MORI K., GELFAND J.D., et al.
2022MNRAS.514..852H 528       D S   X C       11 35 7 Neutrino observations of LHAASO sources: Present constraints and future prospects. HUANG T.-Q. and LI Z.
2022MNRAS.516.4916C 536 T   A     X C       11 10 1 Pulsars as candidates of LHAASO sources J2226+6057, J1908+0621, and
J1825-1326. 		CHANG Z., ZHANG X. and ZHOU J.-Z.
2023ApJ...945L...8A 61       D     X         2 21 5 Searches for Neutrinos from Large High Altitude Air Shower Observatory Ultra-high-energy γ-Ray Sources Using the IceCube Neutrino Observatory. ABBASI R., ACKERMANN M., ADAMS J., et al.
2023MNRAS.521.1144S 104       D         F     2 22 4 Probing LHAASO galactic PeVatrons through gamma-ray and neutrino correspondence. SARMAH P., CHAKRABORTY S. and JOSHI J.C.
2023ApJ...954....9W 17       D               1 27 ~ Hard X-Ray Observation and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula “Dragonfly”. WOO J., AN H., GELFAND J.D., 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.
2023NatAs...7.1497Y 87             C       1 4 ~ A multi-cubic-kilometre neutrino telescope in the western Pacific Ocean. YE Z.P., HU F., TIAN W., et al.
2024MNRAS.528.2749C 179             C F     4 10 ~ A 3D diffusive and advective model of electron transport applied to the pulsar wind nebula HESS J1825 - 137. COLLINS T., ROWELL G., EINECKE S., et al.
2024ApJ...965...44F 242       D     X         6 53 ~ Probing Lorentz Invariance Violation with Absorption of Astrophysical γ-Rays by Solar Photons. FINKE J.D. and PATEL P.
2025ApJ...987L..42A 47           X         1 9 ~ Orbital Modulation of Gamma Rays up to 100 TeV from LS 5039. ALFARO R., ARAYA M., ARTEAGA-VELAZQUEZ J.C., et al.
2025ApJ...991..192A 47           X         1 7 ~ HAWC, VERITAS, Fermi-LAT, and XMM-Newton Follow-up Observations of the Unidentified Ultra-high-energy Gamma-Ray Source LHAASO J2108+5157. ADAMS C.B., BANGALE P., BENBOW W., et al.

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