<script type="text/javascript">
<!--
document.write('<div id="oa_widget"></div>');
document.write('<script type="text/javascript" src="https://beta.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=undefined&type=result"></script>');
-->
</script>

COPY SCRIPT

For further information contact us at helpdesk@openaire.eu

On the spectrum of gamma-rays ranging from multi TeV to sub PeV emitted from the MGRO J1908+06 observed by the Tibet-AS+MD array

Name: On the spectrum of gamma-rays ranging from multi TeV to sub PeV emitted from the MGRO J1908+06 observed by the Tibet-AS+MD array
Creator: Chen Ding
Keywords: 13. Climate action, 7. Clean energy

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 22 Jul 2019Publisher:Sissa MedialabJournal:Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)

Authors: Chen Ding;

doi: 10.22323/1.358.0648

On the spectrum of gamma-rays ranging from multi TeV to sub PeV emitted from the MGRO J1908+06 observed by the Tibet-AS+MD array

- Summary
- Related research
  (16)
- Metrics

Abstract

We have built a large water Cherenkov muon detector array (Tibet-MD) under the existing Tibet air shower array (Tibet-AS) at 4,300 m above sea level, to observe 10-1000 TeV gamma rays from cosmic-ray accelerators in our Galaxy with wide field of view at very low background level. The Tibet-MD array will improve the sensitivity to gamma-ray sources by an order of magnitude around 100 TeV. In this paper, we will report on the gamma-ray emission from the TeV pulsar wind nebula MGRO J1908+06 observed in the energy region from multi TeV to sub PeV with the Tibet-AS+MD array using data accumulated from 2014.

Related Organizations

Institute of High Energy Physics
China (People's Republic of)
Chinese Academy of Sciences
China (People's Republic of)
Institute of High Energy Physics
China (People's Republic of)
Chinese Academy of Sciences
China (People's Republic of)

16 Research products, page 1 of 2

The Ultra-High-Energy Source MGRO J1908+06
2021IsAmongTopNSimilarDocuments
Multiwavelength investigation of the candidate Galactic PeVatron MGRO J1908+06
2021IsAmongTopNSimilarDocuments
Reevaluation of the prospect of observing neutrinos from Galactic sources in the light of recent results in gamma ray and neutrino astronomy
2014IsAmongTopNSimilarDocuments
HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06
2022IsAmongTopNSimilarDocuments
The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters
2008IsAmongTopNSimilarDocuments
H.E.S.S. Galactic Plane Survey unveils a Milagro Hotspot
2007IsAmongTopNSimilarDocuments
The unidentified source HESS J1908+063∕MGRO J1908+06
2008IsAmongTopNSimilarDocuments
Search for Galactic Pevatron candidates in a population of unidentifiedγ-ray sources
2020IsAmongTopNSimilarDocuments
Gamma ray sources observed with ARGO-YBJ
2013IsAmongTopNSimilarDocuments
OBSERVATION OF THE TeV GAMMA-RAY SOURCE MGRO J1908+06 WITH ARGO-YBJ
2012IsAmongTopNSimilarDocuments

chevron_left
1
2
chevron_right

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	0
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average