Evidence for VHE emission from SNR G22.7-0.2 region with H.E.S.S

Andre-Claude Clapson (for the H.E.S.S. collaboration); Arache Djannati-Ata\"i; Bruno Kh\'elifi; Fabio Acero; Francois Brun; Gerd P\"uhlhofer; H\'el\`ene Laffon; J\'er\'emie M\'ehault; Marek Jamrozy; Peter Eger

REVIEW

Evidence for VHE emission from SNR G22.7-0.2 region with H.E.S.S

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1110.6890 v2 pith:YXHPX4NE submitted 2011-10-31 astro-ph.HE

Hélène Laffon , Bruno Khélifi , Francois Brun , Fabio Acero , Jérémie Méhault , Gerd Pühlhofer , Peter Eger , Marek Jamrozy

show 2 more authors

Arache Djannati-Ataï Andre-Claude Clapson (for the H.E.S.S. collaboration)

This is my paper · ORCID

classification astro-ph.HE

keywords emissionevidenceobservationsregionalthougharrayassociatedbrought

verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments

read the original abstract

Observations of the supernova remnant G22.7-0.2 in the field of view of W41 with the H.E.S.S. telescope array have resulted in evidence for a very high energy (VHE) gamma-ray emission from the direction of the object. The emission region is spatially coincident with molecular clouds visible in 13CO data, suggesting a hadronic origin of the TeV emission, although other scenarios brought by X-ray observations with the XMM-Newton satellite are also discussed. The latest results obtained on this SNR with H.E.S.S. and associated multi-wavelength information are presented here.

Discussion (0). Continue with ORCID to comment.

Pith tools