579 citations
- RIKEN Nishina CenterJP4 papers
- Kyoto UniversityJP3 papers
- Kyushu UniversityJP3 papers
- Osaka Electro-Communication UniversityJP3 papers
- The University of TokyoJP3 papers
- Brookhaven National LaboratoryUS2 papers
- Chiba Keizai CollegeJP2 papers
- High Energy Accelerator Research OrganizationJP2 papers
- Hosei UniversityJP2 papers
- Kyoto Sangyo UniversityJP2 papers
- National Astronomical Observatory of JapanJP2 papers
- Radboud University NijmegenNL2 papers
18 papers
Hyper-spectral NIR and MIR data and optimal wavebands for detection of apple tree diseases
Dmitrii Shadrin, Mariia Pukalchik, Anastasia Uryasheva +4
Plant diseases can lead to dramatic losses in yield and quality of food, becoming a problem of high priority for farmers. Apple scab, moniliasis, and powdery mildew are the most si…
Possible lightest Hypernucleus with Modern Interactions
E. Hiyama, K. Sasaki, T. Miyamoto +4
Experimental evidence exists that the -nucleus interaction is attractive. We search for and bound systems on the basis of the AV8 potential combined with eithe…
Inversion angle of phase-polarization curve of near-Earth asteroid (3200) Phaethon
Yoshiharu Shinnaka, Toshihiro Kasuga, Reiko Furusho +5
The linear polarization degree (referred to the scattering plane, P_r) as a function of the solar phase angle, α, of solar system objects is a good diagnostic to understand the sca…
Note on families of pairing-friendly elliptic curves with small embedding degree
Keiji Okano
Pairing-based cryptographic schemes require so-called pairing-friendly elliptic curves, which have special properties. The set of pairing-friendly elliptic curves that are generate…
Initial Speed of Knots in the Plasma Tail of C/2013 R1(Lovejoy)
Masafumi Yagi, Jin Koda, Reiko Furusho +3
We report short-time variations in the plasma tail of C/2013 R1(Lovejoy). A series of short (two to three minutes) exposure images with the 8.2-m Subaru telescope shows faint detai…
Neutrino masses from CMB B-mode polarization and cosmic growth rate
Koichi Hirano
Constraints on neutrino masses are estimated based on future observations of the cosmic microwave background (CMB), which includes the B-mode polarization produced by CMB lensing f…