Abstract. Observation of the North East (NE) rim of SN1006 has been carried out using the CANGAROO-II 10m telescope in April and May 2000. The observation time is 55.2 and 48.8 hours, ON- and OFF-source runs, respectively. We have confirmed TeV Gamma-ray emission from the NE-rim. The energy threshold of the observed flux is estimated to be around 1 TeV by the Monte Carlo simulation assuming the inverse Compton like spectrum. The preliminary flux is consistent with the previous result observed by the 3.8m CAN-GAROO telescope.
We have detected sub-TeV gamma-ray emission from the direction of the Galactic center (GC) using the...
Optical images of SN 1987A show a triple-ring structure. The inner (dust) ring has recently increase...
7 pages, 8 figuresRecent theoretical predictions of the lowest very high energy (VHE) luminosity of ...
The differential spectrum of TeV gamma rays between 1.5 TeV and 20 TeV from the north-east rim of SN...
In this Letter we report the discovery of TeV gamma-ray emission from a supernova remnant made with ...
This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with ...
Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system o...
We searched for TeV gamma-rays from the remnant of SN 1987A around 5400 days after the supernova. Th...
The supernova remnant(SNR) RCW86(G315.4-2.3) has been observed as our third SNR in 2001 and 2002 wit...
Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system o...
We searched for TeV gamma rays from the remnant of SN 1987A around 5400 days after the supernova. Th...
We have detected gamma-ray emission at the 6 σ level at energies greater than 500 GeV from the super...
We have detected sub-TeV gamma-ray emission from the direction of the Galactic center (GC) using the...
Optical images of SN 1987A show a triple-ring structure. The inner (dust) ring has recently increase...
7 pages, 8 figuresRecent theoretical predictions of the lowest very high energy (VHE) luminosity of ...
The differential spectrum of TeV gamma rays between 1.5 TeV and 20 TeV from the north-east rim of SN...
In this Letter we report the discovery of TeV gamma-ray emission from a supernova remnant made with ...
This paper reports the first discovery of TeV gamma-ray emission from a supernova remnant made with ...
Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system o...
We searched for TeV gamma-rays from the remnant of SN 1987A around 5400 days after the supernova. Th...
The supernova remnant(SNR) RCW86(G315.4-2.3) has been observed as our third SNR in 2001 and 2002 wit...
Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system o...
We searched for TeV gamma rays from the remnant of SN 1987A around 5400 days after the supernova. Th...
We have detected gamma-ray emission at the 6 σ level at energies greater than 500 GeV from the super...
We have detected sub-TeV gamma-ray emission from the direction of the Galactic center (GC) using the...
Optical images of SN 1987A show a triple-ring structure. The inner (dust) ring has recently increase...
7 pages, 8 figuresRecent theoretical predictions of the lowest very high energy (VHE) luminosity of ...