HESS J1800-240C , the SIMBAD biblio

HESS J1800-240C , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:21:36


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Title First 3 Authors
2008A&A...481..401A 636     A D     X         18 34 246 Discovery of very high energy gamma-ray emission coincident with molecular clouds in the W 28 (G6.4-0.1) field. AHARONIAN F., AKHPERJANIAN A.G., BAZER-BACHI A.R., et al.
2009ApJ...694L..16H 37           X         1 86 54 Discovery of new interacting supernova remnants in the inner Galaxy. HEWITT J.W. and YUSEF-ZADEH F.
2009A&A...508.1331L viz 75           X         2 9 2 CO J=1-0 observations of gas near the galactic supernova remnants G5.4-1.2, G5.55+0.32 and G5.71-0.08. LISZT H.S.
2010ApJ...718..348A 344           X C F     7 19 200 Fermi Large Area Telescope observations of the supernova remnant W28 (G6.4-0.1). ABDO A.A., ACKERMANN M., AJELLO M., et al.
2010MNRAS.409L..35L 133       D     X   F     3 7 72 γ-rays from molecular clouds illuminated by accumulated diffusive protons from supernova remnant W28. LI H. and CHEN Y.
2011MNRAS.411.1367N viz 189           X C       4 38 20 12 mm line survey of the dense molecular gas towards the W28 field TeV gamma-ray sources. NICHOLAS B., ROWELL G., BURTON M.G., et al.
2011APh....35...33Y 10 11 Neutrino emission of Fermi supernova remnants. YUAN Q., YIN P.-F. and BI X.-J.
2011MNRAS.417.3072T 38           X         1 18 10 Cosmic rays in the surroundings of SNR G35.6-0.4. TORRES D.F., LI H., CHEN Y., et al.
2012MNRAS.419..251N 801     A D S   X C F     19 29 29 A 7 mm line survey of the shocked and disrupted molecular gas towards the W28 field TeV gamma-ray sources. NICHOLAS B.P., ROWELL G., BURTON M.G., et al.
2014ApJ...786..145H 929     A D     X C       24 16 21 Detailed investigation of the gamma-ray emission in the vicinity of SNR W28 with FERMI-LAT. HANABATA Y., KATAGIRI H., HEWITT J.W., et al.
2014MNRAS.443..474P 15       D               1 108 87 Are both BL Lacs and pulsar wind nebulae the astrophysical counterparts of IceCube neutrino events? PADOVANI P. and RESCONI E.
2016ApJ...816...63J 275           X C       6 18 3 Fermi-LAT observations of supernova remnant G5.7-0.1, believed to be interacting with molecular clouds. JOUBERT T., CASTRO D., SLANE P., et al.
2016ApJS..224....8A viz 39           X         1 300 196 The first Fermi LAT supernova remnant catalog. ACERO F., ACKERMANN M., AJELLO M., et al.
2017MNRAS.468.2093D 95       D         F     3 85 9 Dense molecular gas at 12 mm towards Galactic TeV gamma-ray sources. DE WILT P., ROWELL G., WALSH A.J., et al.
2018ApJ...860...69C 105     A     X C       2 14 23 Leaked GeV CRs from a broken shell: explaining 9 years of Fermi-LAT data of SNR W28. CUI Y., YEUNG P.K.H., TAM P.H.T., et al.
2018ApJ...867..120H 201           X         5 16 1 High-energy and very high energy emission from stellar-mass black holes moving in gaseous clouds. HIROTANI K., PU H.-Y., OUTMANI S., et al.
2019MNRAS.482.3843T 463       D     X   F     11 29 4 Gamma-ray emission from middle-aged supernova remnants interacting with molecular clouds: the challenge for current models. TANG X.
2020MNRAS.495.1093H 82           X         2 45 ~ Searches for pulsar-like candidates from unidentified objects in the Third Catalog of Hard Fermi-LAT Sources with machine learning techniques. HUI C.Y., LEE J., LI K.L., et al.
2020MNRAS.495.2909R 206           X C       4 25 ~ High-velocity interstellar absorption associated with the supernova remnant W28. RITCHEY A.M.
2020ApJ...905...76A viz 42           X         1 89 89 3HWC: the third HAWC catalog of very-high-energy gamma-ray sources. ALBERT A., ALFARO R., ALVAREZ C., et al.
2021ApJ...923..106Z 42           X         1 13 ~ Fermi-LAT detection of extended gamma-ray emission in the vicinity of SNR G045.7-00.4: evidence of escaping cosmic rays interacting with the surrounding molecular clouds. ZHANG H.-M., LIU R.-Y., SU Y., et al.
2024RAA....24f5020W 18       D               1 20 ~ The Influence of the Sun and Moon on the Observation of Very High Energy Gamma-ray Sources Using EAS Arrays. WEN T., CHEN S. and DAI B.

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