output
19932026
most citedThe Hyper Suprime-Cam SSP Survey: Overview and Survey Design

1.1k citations

Showing 2006Show all

8 papers · 1 filter

astro-ph2006★ 11 cited

Underground Water Cherenkov Muon Detector Array with the Tibet Air Shower Array for Gamma-Ray Astronomy in the 100 TeV Region

The Tibet AS Gamma Collaboration, M. Amenomori

We propose to build a large water-Cherenkov-type muon-detector array (Tibet MD array) around the 37,000 m Tibet air shower array (Tibet AS array) already constructed at 4,300…

astro-ph2006★ 12 cited

Erratum: Detection of diffuse TeV gamma-ray emission from the nearby starburst galaxy NGC 253

C. Itoh, R. Enomoto, S. Yanagita +1

The CANGAROO-II telescope observed sub-TeV gamma-ray emission from the nearby starburst galaxy NGC 253. The emission region was extended with a radial size of 0.3-0.6 degree. On th…

nucl-th2006★ 4 cited

Pre-scission neutron multiplicity associated with the dynamical process in superheavy mass region

Y. Aritomo, M. Ohta, F. Hanappe

The fusion-fission process accompanied by neutron emission is studied in the superheavy-mass region on the basis of the fluctuation-dissipation model combined with a statistical mo…

astro-ph2006★ 38 cited

CANGAROO-III Observations of the supernova remnant RX J0852.04622

R. Enomoto, S. Watanabe, T. Tanimori et al

Sub-TeV gamma-ray emission from the North-West rim of the supernova remnant RX J0852.04622 was detected with the CANGAROO-II telescope and recently confirmed by the H.E.S.S. gro…

nucl-ex2006★ 101 cited

The Giant Monopole Resonance in the Sn Isotopes: Why is Tin so "Fluffy"?

U. Garg

The isoscalar giant monopole resonance (GMR) has been investigated in a series of Sn isotopes (A=112--124) using inelstic scattering of 400-MeV alpha particles at extremely forward…

nucl-ex2006★ 50 cited

Measurement of the Gamow-Teller Strength Distribution in 58Co via the 58Ni(t,3He) reaction at 115 MeV/nucleon

A. L. Cole, H. Akimune, Sam M. Austin +18

Electron capture and beta decay play important roles in the evolution of pre-supernovae stars and their eventual core collapse. These rates are normally predicted through shell-mod…