[GH2008] 1 , the SIMBAD biblio

[GH2008] 1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST00:12:46

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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
2003ApJ...589..253B 27 49 Diffuse hard X-ray sources discovered with the ASCA galactic plane survey. BAMBA A., UENO M., KOYAMA K., et al.
2005ApJ...630L.157M 17 28 The INTEGRAL/IBIS source AX J1838.0-0655: a soft X-Ray-to-TeV γ-ray broadband emitter. MALIZIA A., BASSANI L., STEPHEN J.B., et al.
2008ApJ...681..515G 745   K A D S   X C       19 31 34 Discovery of a young, energetic 70.5 ms pulsar associated with the TeV gamma-ray source HESS J1837-069. GOTTHELF E.V. and HALPERN J.P.
2009PASJ...61S.183A 187   K A D     X C       5 4 6 X-Ray studies of HESS J1837-069 with Suzaku and ASCA: a VHE gamma-ray source originated from the pulsar wind nebula. ANADA T., EBISAWA K., DOTANI T., et al.
2012ApJ...745...99K 305     A D     X         9 55 6 XMM-Newton observations of two candidate supernova remnants. KARGALTSEV O., SCHMITT B.M., PAVLOV G.G., et al.
2012ApJ...756....5L 115           X C       2 61 123 Search for spatially extended Fermi large area telescope sources using two years of data. LANDE J., ACKERMANN M., ALLAFORT A., et al.
2018ApJS..235...43T viz 120           X C       2 69 12 The Massive Star-forming Regions Omnibus X-ray Catalog, second installment. TOWNSLEY L.K., BROOS P.S., GARMIRE G.P., et al.
2020MNRAS.494.3405S 305       D     X   F     7 14 ~ Diffuse γ-ray emission from the vicinity of young massive star cluster RSGC 1. SUN X.-N., YANG R.-Z. and WANG X.-Y.
2025ApJ...989..110F 93           X         2 112 ~ A Systematic Search for MeV-GeV Pulsar Wind Nebulae without Gamma-Ray Detected Pulsars. FERMI-LAT COLLABORATION, ACHARYYA A., ADELFIO A., et al.
2025ApJ...991...43P 4992     A D S   X C       106 10 ~ X-Ray Studies of PSR J1838-0655 and its Wind Nebula Associated with HESS J1837-069 and 1LHAASO J1837-0654u. PARK M., PARK J., KIM C., et al.

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