output
19972024
most citedThe 105 month Swift-BAT all-sky hard X-ray survey

414 citations

25 papers

physics.optics2024★ 14 cited

Quasi-real-time dual-comb spectroscopy with 750-MHz Yb:fiber combs

Haochen Tian, Runmin Li, Lukasz A. Sterczewski +3

We present quasi-real-time dual-comb spectroscopy (DCS) using two Yb:fiber combs with ~750 MHz repetition rates. A computational coherent averaging technique is employed to correct…

quant-ph2023★ 2 cited

Logical Characterization of Contextual Hidden-Variable Theories based on Quantum Set Theory

Masanao Ozawa

While non-contextual hidden-variable theories are proved to be impossible, contextual ones are possible. In a contextual hidden-variable theory, an observable is called a beable if…

astro-ph.HE2020★ 15 cited

Analytic properties of electromagnetic field of binary compact stars and electromagnetic precursors to gravitational waves

Tomoki Wada, Masaru Shibata, Kunihito Ioka

We analytically study the properties of the electromagnetic field in vacuum around close binary compact stars containing at least one neutron star. We show that the orbital motion…

math.NA2019★ 6 cited

Recent advances in higher order quasi-Monte Carlo methods

Takashi Goda, Kosuke Suzuki

In this article we review some of recent results on higher order quasi-Monte Carlo (HoQMC) methods. After a seminal work by Dick (2007, 2008) who originally introduced the concept…

math.OA2018★ 5 cited

E-semigroups over closed convex cones

Anbu Arjunan, R. Srinivasan, S. Sundar

We initiate a study of E-semigroups over convex cones. We prove a structure theorem for E-semigroups which leave the algebra of compact operators invariant. Then we study in detail…

math.AP2018

Carleman estimates for a magnetohydrodynamics system and application to inverse source problems

Xinchi Huang, Masahiro Yamamoto

In this article, we consider a linearized magnetohydrodynamics system for incompressible flow in a three-dimensional bounded domain. We first prove two kinds of Carleman estimates.…

astro-ph.HE2018★ 414 cited

The 105 month Swift-BAT all-sky hard X-ray survey

Kyuseok Oh, Michael Koss, Craig B. Markwardt +10

We present a catalog of hard X-ray sources detected in the first 105 months of observations with the Burst Alert Telescope (BAT) coded mask imager on board the Swift observatory. T…

eess.SY2017★ 3 cited

Bounding Errors Due to Switching Delays in Incrementally Stable Switched Systems (Extended Version)

Kengo Kido, Sean Sedwards, Ichiro Hasuo

Time delays pose an important challenge in networked control systems, which are now ubiquitous. Focusing on switched systems, we introduce a framework that provides an upper bound…

eess.SY2017★ 7 cited

Causality-Aided Falsification

Takumi Akazaki, Yoshihiro Kumazawa, Ichiro Hasuo

Falsification is drawing attention in quality assurance of heterogeneous systems whose complexities are beyond most verification techniques' scalability. In this paper we introduce…

cs.LO2017★ 1 cited

Categorical Liveness Checking by Corecursive Algebras

Natsuki Urabe, Masaki Hara, Ichiro Hasuo

Final coalgebras as "categorical greatest fixed points" play a central role in the theory of coalgebras. Somewhat analogously, most proof methods studied therein have focused on gr…

eess.SY2015★ 1 cited

Time Robustness in MTL and Expressivity in Hybrid System Falsification (Extended Version)

Takumi Akazaki, Ichiro Hasuo

Building on the work by Fainekos and Pappas and the one by Donze and Maler, we introduce AvSTL, an extension of metric interval temporal logic by averaged temporal operators. Its e…

astro-ph.SR2009★ 3 cited

Period-Luminosity Relation for Type II Cepheids

Noriyuki Matsunaga, Michael W. Feast, John W. Menzies

We have estimated JHKs magnitudes corrected to mean intensity for LMC type II Cepheids found in the OGLE-III survey. Period-luminosity relations (PLRs) are derived in JHKs as well…

astro-ph2007★ 31 cited

The Subaru/XMM-Newton Deep Survey (SXDS) - V. Optically Faint Variable Object Survey

Tomoki Morokuma, Mamoru Doi, Naoki Yasuda +19

We present our survey for optically faint variable objects using multi-epoch (8-10 epochs over 2-4 years) -band imaging data obtained with Subaru Suprime-Cam over 0.918 deg…

astro-ph2007★ 19 cited

The Subaru/XMM-Newton Deep Survey (SXDS) - VI. Properties of Active Galactic Nuclei Selected by Optical Variability

Tomoki Morokuma, Mamoru Doi, Naoki Yasuda +11

We present the properties of active galactic nuclei (AGN) selected by optical variability in the Subaru/XMM-Newton Deep Field (SXDF). Based on the locations of variable components…

astro-ph2007★ 21 cited

The Effect of Poloidal Magnetic Field on Type I Planetary Migration: Significance of Magnetic Resonance

Takayuki Muto, Masahiro N. Machida, Shu-ichiro Inutsuka

We study the effect of poloidal magnetic field on type I planetary migration by linear perturbation analysis in the shearing-sheet approximation and the analytic results are compar…

cond-mat.mtrl-sci2006★ 16 cited

Magnetic Properties and Metastable States in Spin-Crossover Transition of Co-Fe Prussian Blue Analogues

Y. Konishi, H. Tokoro, M. Nishino +1

The combination of spin transitions and magnetic ordering provides an interesting structure of phase transitions in Prussian blue analogues (PBAs). To understand the structure of s…

cond-mat.dis-nn2006★ 11 cited

Replica analysis of a preferential urn model

Jun Ohkubo, Muneki Yasuda, Kazuyuki Tanaka

We analyse a preferential urn model with randomness using the replica method. The preferential urn model is a stochastic model based on the concept "the rich get richer." The repli…

astro-ph2005★ 59 cited

The Elongations and Supersonic Motions of Molecular Clouds

Jin Koda, Tsuyoshi Sawada, Tetsuo Hasegawa +1

New 13CO data from the BU-FCRAO Milky Way Galactic Ring Survey (GRS) are analyzed to understand the shape and internal motions of molecular clouds. For a sample of more than five h…

astro-ph2005★ 41 cited

On Heating of Cluster Cooling Flows by Sound Waves

Yutaka Fujita, Takeru Ken Suzuki

We investigate heating of the cool core of a galaxy cluster through the dissipation of sound waves excited by the activities of the central active galactic nucleus (AGN). Using a w…

astro-ph2005★ 283 cited

Making the corona and the fast solar wind: a self-consistent simulation for the low-frequency Alfven waves from photosphere to 0.3AU

Takeru K. Suzuki, Shu-ichiro Inutsuka

We show that the coronal heating and the fast solar wind acceleration in the coronal holes are natural consequence of the footpoint fluctuations of the magnetic fields at the photo…

astro-ph2005★ 15 cited

The Reionization History and Early Metal Enrichment inferred from the Gamma-Ray Burst Rate

T. Murakami, D. Yonetoku, M. Umemura +2

Based on the gamma-ray burst (GRB) event rate at redshifts of , which is assessed by the spectral peak energy-to-luminosity relation recently found by Yonetoku et…

astro-ph2003★ 30 cited

Tsunamis in Galaxy Clusters: Heating of Cool Cores by Acoustic Waves

Yutaka Fujita, Takeru Ken Suzuki, Keiichi Wada

Using an analytical model and numerical simulations, we show that acoustic waves generated by turbulent motion in intracluster medium effectively heat the central region of a so-ca…

astro-ph2002★ 57 cited

NMA CO (J=1-0) Observations of the Halpha/Radio Lobe Galaxy NGC 3079: Gas Dynamics in a Weak Bar Potential and Central Massive Core

J. Koda, Y. Sofue, K. Kohno +4

within 24 lines with 80 characters) We present ^12CO (1-0) observations in the central 4.5 kpc (1 arcmin) of the Halpha/Radio lobe galaxy NGC 3079 with the Nobeyama Millimeter Arra…

astro-ph1998★ 47 cited

Detecting z > 10 objects through carbon, nitrogen and oxygen emission lines

Maki Suginohara, Tatsushi Suginohara, David N. Spergel

By redshift of 10, star formation in the first objects should have produced considerable amounts of Carbon, Nitrogen and Oxygen. The submillimeter lines of C, N and O redshift into…