activity
19952022
most citedMultiwavelength Monitoring of the BL Lacertae Object PKS 2155-304 in May 1994. III. Probing the Inner Jet through Multiwavelength Correlations

117 citations · 387 across the 17 of their papers we have counts for

collaborators

17 papers

hep-ph2022★ 6 cited

Axion-photon multimessenger astronomy with giant flares

Javier De Miguel, Chiko Otani

We treat prospects for multimessenger astronomy with giant flares (GFs), a rare transient event featured by magnetars that can be as luminous as a hundred of the brightest supernov…

astro-ph.HE2021★ 2 cited

Superdense beaming of axion dark matter in the vicinity of the light cylinder of pulsars

Javier De Miguel, Chiko Otani

In this article we treat the non-adiabatic photon-to-axion resonant conversion of curvature radiation, synchrotron emission and inverse Compton scattering dominating the spectral d…

physics.ins-det2021★ 5 cited

Characterization of two-level system noise for microwave kinetic inductance detector comprising niobium film on silicon substrate

Yoshinori Sueno, Shunsuke Honda, Hiroki Kutsuma +5

A microwave kinetic inductance detector (MKID) is a cutting-edge superconducting detector. It comprises a resonator circuit constructed with a superconducting film on a dielectric…

cond-mat.mes-hall2021

Hot carrier dynamics and electron-optical phonon coupling in photoexcited graphene via time-resolved ultrabroadband terahertz spectroscopy

Sho Ikeda, Chiko Otani, Masatsugu Yamashita

Electron-electron (e-e) interaction is known as a source of logarithmic renormalizations for Dirac fermions in quantum field theory. The renormalization of electron--optical phonon…

cond-mat.mes-hall2020★ 3 cited

Intrinsic and extrinsic effects on intraband optical conductivity of hot carriers in photoexcited graphene

Masatsugu Yamashita, Chiko Otani

We present a numerical study on the intraband optical conductivity of hot carriers at quasi-equilibria in photoexcited graphene based on the semiclassical Boltzmann transport equat…

physics.ins-det2020

A method to measure superconducting transition temperature of microwave kinetic inductance detector by changing power of readout microwaves

Hiroki Kutsuma, Yoshinori Sueno, Makoto Hattori +5

A microwave kinetic inductance detector (MKID) is a cutting-edge superconducting detector, and its principle is based on a superconducting resonator circuit. The superconducting tr…

physics.optics2017★ 1 cited

Closed-form formulae of hyperbolic metamaterial made by stacked hole-array layers working at terahertz or microwave radiation

Piyawath Tapsanit, Masatsugu Yamashita, Chiko Otani +2

A metamaterial made by stacked hole-array layers known as a fishnet metamaterial behaves as a hyperbolic metamaterial at wavelength much longer than hole-array period. However, the…

physics.optics2016★ 3 cited

Quasi-analytical solutions of hybrid platform and the optimization of highly sensitive thin-film sensors for terahertz radiation

Piyawath Tapsanit, Masatsugu Yamashita, Teruya Ishihara +1

We present quasi-analytical solutions (QANS) of hybrid platform (HP) comprising metallic grating (MG) and stacked-dielectric layers for terahertz (THz) radiation. The QANS are vali…

astro-ph2001★ 57 cited

A Possible Emission Feature in an X-ray Afterglow of GRB970828 as a Radiative Recombination Edge

A. Yoshida, M. Namiki, D. Yonetoku +6

A gamma-ray burst of 28 August 1997 was localized by the All-Sky Monitor on the Rossi XTE satellite and its coordinates were promptly disseminated. An ASCA followup started 1.17 da…

astro-ph2001★ 4 cited

RE J2248-511 - Not all variable, ultrasoft, X-ray AGN have narrow Balmer lines

A. A. Breeveld, E. M. Puchnarewicz, C. Otani

We present ASCA data on RE J2248-511, extending existing optical and soft X-ray coverage to 10 keV, and monitoring the soft component. These data show that, despite a very strong u…

astro-ph1998★ 29 cited

ASCA Observations of the Seyfert 2 Galaxy NGC 7582: An Obscured and Scattered View of the Hidden Nucleus

S. -J. Xue, C. Otani, T. Mihara +2

ASCA observations of the Seyfert 2 galaxy NGC 7582 revealed it was highly variable on the timescale of s in the hard X-ray (2-10 keV) band, while the soft X-ray (…

astro-ph1997★ 2 cited

BeppoSAX observation of NGC 7674: a new reflection-dominated Seyfert 2 galaxy

G. Malaguti, G. G. C. Palumbo, M. Cappi +6

The Seyfert 2 galaxy NGC 7674 has been observed within the BeppoSAX Core Programme with the onboard narrow field instruments between 0.1 and 100 keV. The broad-band spectrum shows…

astro-ph1997★ 117 cited

Multiwavelength Monitoring of the BL Lacertae Object PKS 2155-304 in May 1994. III. Probing the Inner Jet through Multiwavelength Correlations

C. Megan Urry, A. Treves, L. Maraschi +16

In May 1994 the BL Lac object PKS 2155-304 was observed continuously for ~10 d with IUE and EUVE and for 2 d with ASCA, as well as with ROSAT and with ground- based radio, IR, and…

astro-ph1997★ 21 cited

The ASCA X-ray spectrum of the powerful radio galaxy 3C109

S. W. Allen, A. C. Fabian, E. Idesawa +3

We report the results from an ASCA X-ray observation of the powerful Broad Line Radio Galaxy, 3C109. The ASCA spectra confirm our earlier ROSAT detection of intrinsic X-ray absorpt…

astro-ph1996★ 58 cited

Spectral Variability and iron line emission in the ASCA Observations of the Seyfert 1 Galaxy NGC4051

Matteo Guainazzi, Tatehiro Mihara, Chiko Otani +1

We present the results of an extensive analysis of the ``ASCA'' AO2 observation of the Seyfert 1 galaxy NGC4051. The target exhibits broadband [0.5--10 keV] variability by a factor…

astro-ph1996★ 54 cited

ASCA Observations of the Composite Warm Absorber in NGC 3516

G. A. Kriss, J. H. Krolik, C. Otani +11

We obtained X-ray spectra of the Seyfert 1 galaxy NGC~3516 in March 1995 using ASCA. Simultaneous far-UV observations were obtained with HUT on the Astro-2 shuttle mission. The ASC…

astro-ph1995★ 25 cited

Warm absorber, reflection and Fe K line in the X-ray spectrum of IC 4329A

M. Cappi, T. Mihara, M. Matsuoka +3

Results from the X-ray spectral analysis of the ASCA PV phase observation of the Seyfert 1 galaxy IC 4329A are presented. We find that the 0.4 - 10 keV spectrum of IC 4329A is best…