Subaru Hyper Suprime-Cam Survey for An Optical Counterpart of GW170817

We perform a $z$-band survey for an optical counterpart of a binary neutron star coalescence GW170817 with Subaru/Hyper Suprime-Cam. Our untargeted transient search covers $23.6$ deg$^2$ corresponding to the $56.6\%$ credible region of GW170817 and reaches the $50\%$ completeness magnitude of $20.6$ mag on average. As a result, we find 60 candidates of extragalactic transients, including J-GEM17btc (a.k.a. SSS17a/DLT17ck). While J-GEM17btc is associated with NGC 4993 that is firmly located inside the 3D skymap of GW170817, the other 59 candidates do not have distance information in the GLADE v2 catalog or NASA/IPAC Extragalactic Database (NED). Among 59 candidates, 58 are located at the center of extended objects in the Pan-STARRS1 catalog, while one candidate has an offset. We present location, $z$-band apparent magnitude, and time variability of the candidates and evaluate the probabilities that they are located inside of the 3D skymap of GW170817. The probability for J-GEM17btc is $64\%$ being much higher than those for the other 59 candidates ($9.3\times10^{-3}-2.1\times10^{-1}\%$). Furthermore, the possibility, that at least one of the other 59 candidates is located within the 3D skymap, is only $3.2\%$. Therefore, we conclude that J-GEM17btc is the most-likely and distinguished candidate as the optical counterpart of GW170817.Comment: 14 pages, 9 figures. Accepted for publication in PASJ (Publications of the Astronomical Society of Japan

Synthetic Seismograms Near a Finite Fault System

We developed computer codes to synthesize seismograms near a finite fault system with the discrete wave-number method. Besides we synthesized seismograms in two dimensional space, formulations in three dimension are also provided. The discrete wave-number method which regarded circular wave from epicenter as a sum of plane waves propagating any direction is useful in introducing a rectangular fault source and a stratified medium. 1

MOESM2 of Infrasonic wave accompanying a crack opening during the 2015 Hakone eruption

Additional file 2. Calibration test for the microphone at the OWD station

MOESM3 of Infrasonic wave accompanying a crack opening during the 2015 Hakone eruption

Additional file 3. Shift in the peaks and node of the seismic-infrasonic correlation resulting from background seismic oscillation

MOESM4 of Infrasonic wave accompanying a crack opening during the 2015 Hakone eruption

Additional file 4. Strain changes using the open crack model estimated by InSAR data