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20162024
most citedX-Ray Spectral Model from Clumpy Torus and Its Application to Circinus Galaxy

92 citations · 649 across the 27 of their papers we have counts for

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16 papers · 1 filter

astro-ph.HE2023

Circumnuclear Multi-phase Gas in the Circinus Galaxy. V. The Origin of the X-Ray Polarization in the Circinus Galaxy

Atsushi Tanimoto, Keiichi Wada, Yuki Kudoh +3

The Imaging X-ray Polarimetry Explorer (IXPE) detected X-ray polarization in the nearest Seyfert 2 galaxy, the Circinus galaxy, for the first time. To reproduce the IXPE results, w…

astro-ph.HE2023★ 8 cited

A broadband X-ray imaging spectroscopy in the 2030s: the FORCE mission

Koji Mori, Takeshi G. Tsuru, Kazuhiro Nakazawa +49

In this multi-messenger astronomy era, all the observational probes are improving their sensitivities and overall performance. The Focusing on Relativistic universe and Cosmic Evol…

astro-ph.HE2023★ 14 cited

A different view of wind in X-ray binaries: The Accretion Disc Corona source 2S 0921-630

Ryota Tomaru, Chris Done, Hirokazu Odaka +1

Accretion disc coronae (ADC) sources are very high inclination neutron star or black hole binaries, where the outer accretion flow blocks a direct view of the central source. The w…

astro-ph.HE2022★ 10 cited

Orbital- and spin-phase variability in the X-ray emission from the accreting pulsar Cen X-3

Tsubasa Tamba, Hirokazu Odaka, Atsushi Tanimoto +3

We analyzed 39 ks NuSTAR observation data of the high mass X-ray binary Cen X-3 in order to investigate the orbital- and spin-phase spectral variability. The observation covers the…

astro-ph.HE2022★ 10 cited

Broadband X-ray Spectral Analysis of the Dual AGN System Mrk 739

Koki Inaba, Yoshihiro Ueda, Satoshi Yamada +4

We present the result of a broadband (0.5-70 keV) X-ray spectral analysis of the late-merger galaxy Mrk 739, which contains a dual active galactic nucleus (AGN), Mrk 739E and Mrk 7…

astro-ph.HE2022★ 44 cited

NuSTAR Observations of 52 Compton-thick Active Galactic Nuclei Selected by the Swift/BAT All-sky Hard X-Ray Survey

Atsushi Tanimoto, Yoshihiro Ueda, Hirokazu Odaka +2

We present the systematic broadband X-ray spectral analysis of 52 Compton-thick () active galactic nucleus (CTAGN) cand…

astro-ph.HE2022★ 5 cited

Absorption Variability of the Highly Obscured Active Galactic Nucleus NGC 4507

Arghajit Jana, Claudio Ricci, Sachindra Naik +6

We present a detailed study of the highly obscured active galaxy NGC 4507, performed using four Nuclear Spectroscopic Telescope Array (NuSTAR) observations carried out between May…

astro-ph.HE2020★ 48 cited

Systematic Study of AGN Clumpy Tori with Broadband X-ray Spectroscopy: Updated Unified Picture of AGN Structure

Shoji Ogawa, Yoshihiro Ueda, Atsushi Tanimoto +1

We present the results of a systematic, broadband X-ray spectral analysis of nearby active galactic nuclei (AGNs) with the X-ray clumpy torus model (XCLUMPY; Tanimoto et al. 2019).…

astro-ph.HE2020★ 31 cited

Application of X-Ray Clumpy Torus Model (XCLUMPY) to 10 Obscured Active Galactic Nuclei Observed with Suzaku and NuSTAR

Atsushi Tanimoto, Yoshihiro Ueda, Hirokazu Odaka +4

We apply XCLUMPY, an X-ray spectral model from a clumpy torus in an active galactic nucleus (AGN), to the broadband X-ray spectra of 10 obscured AGNs observed with both Suzaku and…

astro-ph.HE2020★ 22 cited

Nature of Compton-thick Active Galactic Nuclei in "Non-merging'' Luminous Infrared Galaxies UGC 2608 and NGC 5135 Revealed with Broadband X-ray Spectroscopy

Satoshi Yamada, Yoshihiro Ueda, Atsushi Tanimoto +4

We have analyzed the broadband X-ray spectra of active galactic nuclei (AGNs) in two "non-merging" luminous infrared galaxies (LIRGs) UGC 2608 and NGC 5135, utilizing the data of N…

astro-ph.HE2019★ 92 cited

X-Ray Spectral Model from Clumpy Torus and Its Application to Circinus Galaxy

Atsushi Tanimoto, Yoshihiro Ueda, Hirokazu Odaka +3

We construct an X-ray spectral model from the clumpy torus in an active galactic nucleus (AGN), designated as "XCLUMPY", utilizing the Monte Carlo simulation for Astrophysics and C…

astro-ph.HE2019★ 14 cited

Luminosity Ratio between [O IV] 25.89 um Line and Nuclear Continuum 12 um as Diagnostic for "Buried" AGN

Satoshi Yamada, Yoshihiro Ueda, Atsushi Tanimoto +3

We propose new diagnostics that utilize the [O IV] 25.89 m and nuclear (subarcsecond scale) 12 m luminosity ratio for identifying whether an AGN is deeply `buried' in their s…

astro-ph.HE2019★ 24 cited

Application of Clumpy Torus Model to Broadband X-ray Spectra of Two Seyfert 1 Galaxies: IC 4329A and NGC 7469

Shoji Ogawa, Yoshihiro Ueda, Satoshi Yamada +2

We apply a new X-ray clumpy torus model called XCLUMPY (Tanimoto et al. 2019), where the clump distribution is assumed to be the same as in the infrared clumpy torus model (CLUMPY)…

astro-ph.HE2018★ 25 cited

The 7-year MAXI/GSC X-ray Source Catalog in the High Galactic-Latitude Sky (3MAXI)

Taiki Kawamuro, Yoshihiro Ueda, Megumi Shidatsu +28

We present the third MAXI/GSC catalog in the high Galactic-latitude sky () based on the 7-year data from 2009 August 13 to 2016 July 31, complementary to that in th…

astro-ph.HE2018★ 18 cited

Broadband X-ray Spectral Analysis of the Double-Nucleus Luminous Infrared Galaxy Mrk 463

Satoshi Yamada, Yoshihiro Ueda, Saeko Oda +4

We present a broadband (0.4-70 keV) X-ray spectral analysis of the luminous infrared galaxy (LIRG) system Mrk 463 observed with Nuclear Spectroscopic Telescope Array (NuSTAR), Chan…

astro-ph.HE2018★ 35 cited

Suzaku Observations of Heavily Obscured (Compton-thick) Active Galactic Nuclei selected by Swift/BAT Hard X-ray Survey

Atsushi Tanimoto, Yoshihiro Ueda, Taiki Kawamuro +3

We present a uniform broadband X-ray (0.5-100.0 keV) spectral analysis of 12 Swift/Burst Alert Telescope (BAT) selected Compton-thick ($\log N_{\mathrm{H}}/\mathrm{cm}^{-2} \geq 24…