activity
20092024
most citedA statistical relation between the X-ray spectral index and Eddington ratio of active galactic nuclei in deep surveys

214 citations · 1.6k across the 43 of their papers we have counts for

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28 papers · 1 filter

astro-ph.GA2024

Ongoing and fossil large-scale outflows detected in a high-redshift radio galaxy: [C II] observations of TN J09242201 at

Kianhong Lee, Masayuki Akiyama, Kotaro Kohno +13

We present Atacama Large Millimeter/submillimeter Array observations of the [C II] 158 m line and the underlying continuum emission of TN J09242201, which is one of the most…

astro-ph.GA2022★ 10 cited

Multi-line assessment of narrow-line regions in 3 radio galaxies

Koki Terao, Tohru Nagao, Kyoko Onishi +4

In this paper, we utilize high-quality rest-UV spectra of three radio galaxies at 3 observed with VLT/FORS2 to measure the flux of several emission lines including relativ…

astro-ph.GA2021★ 92 cited

The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements

B. Garilli, R. McLure, L. Pentericci +94

VANDELS is an ESO Public Spectroscopic Survey designed to build a sample of high signal to noise, medium resolution spectra of galaxies at redshift between 1 and 6.5. Here we prese…

astro-ph.GA2020★ 73 cited

The Faint End of the Quasar Luminosity Function at from the Subaru Hyper Suprime-Cam Survey

Mana Niida, Tohru Nagao, Hiroyuki Ikeda +17

We present the quasar luminosity function at derived from the optical wide-field survey data obtained as a part of the Subaru strategic program (SSP) with Hyper Suprime-…

astro-ph.GA2020★ 46 cited

Metal enrichment in the circumgalactic medium and Lyα haloes around quasars at z 3

Yucheng Guo, Roberto Maiolino, Linhua Jiang +8

Deep observations have detected extended Ly emission nebulae surrounding tens of quasars at redshift 2 to 6. However, the metallicity of such extended haloes is still poorly und…

astro-ph.GA2019★ 7 cited

A NuSTAR and XMM-Newton Study of the Two Most Actively Star-forming Green Pea Galaxies (SDSS J0749+3337 and SDSS J0822+2241)

Taiki Kawamuro, Yoshihiro Ueda, Kohei Ichikawa +4

We explore X-ray evidence for the presence of active galactic nuclei (AGNs) in the two most actively star-forming Green Pea galaxies (GPs), SDSS J0749+3337 and SDSS J0822+2241, whi…

astro-ph.GA2018★ 39 cited

Does the mid-infrared-hard X-ray luminosity relation for active galactic nuclei depend on Eddington ratio?

Yoshiki Toba, Yoshihiro Ueda, Kenta Matsuoka +5

We revisit the correlation between the mid-infrared (6 m) and hard X-ray (2--10 keV) luminosities of active galactic nuclei (AGNs) to understand the physics behind it. We constr…

astro-ph.GA2018★ 14 cited

Ratio of black hole to galaxy mass of an extremely red dust-obscured galaxy at z = 2.52

Kenta Matsuoka, Yoshiki Toba, Megumi Shidatsu +7

We present a near-infrared (NIR) spectrum of WISE J1042+1641, an extremely red dust-obscured galaxy (DOG), which has been observed with the LIRIS on the 4.2m William Hershel Telesc…

astro-ph.GA2018★ 27 cited

Discovery of Dying Active Galactic Nucleus in Arp 187: Experience of Drastic Luminosity Decline within years

Kohei Ichikawa, Junko Ueda, Hyun-Jin Bae +4

Arp 187 is one of the fading active galactic nuclei (AGN), whose AGN activity is currently decreasing in luminosity. We investigate the observational signatures of AGN in Arp 187,…

astro-ph.GA2018★ 116 cited

MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and photoionization in the Seyfert galaxy NGC 1365

G. Venturi, E. Nardini, A. Marconi +24

Ionized outflows, revealed by broad asymmetric wings of the [OIII] line, are commonly observed in AGN but the low intrinsic spatial resolution of observations has generally prevent…

astro-ph.GA2018★ 40 cited

The mass-metallicity relation of high-z type-2 active galactic nuclei

Kenta Matsuoka, Tohru Nagao, Alessandro Marconi +5

The mass-metallicity relation (MZR) of type-2 active galactic nuclei (AGNs) at 1.2 < z < 4.0 is investigated by using high-z radio galaxies (HzRGs) and X-ray selected radio-quiet A…

astro-ph.GA2018★ 134 cited

The VANDELS ESO public spectroscopic survey: observations and first data release

L. Pentericci, R. J. McLure B. Garilli, O. Cucciati +93

This paper describes the observations and the first data release (DR1) of the ESO public spectroscopic survey "VANDELS, a deep VIMOS survey of the CANDELS CDFS and UDS fields". VAN…

astro-ph.GA2018★ 130 cited

The VANDELS ESO public spectroscopic survey

R. J. McLure, L. Pentericci, A. Cimatti +92

VANDELS is a uniquely-deep spectroscopic survey of high-redshift galaxies with the VIMOS spectrograph on ESO's Very Large Telescope (VLT). The survey has obtained ultra-deep optica…

astro-ph.GA2017★ 21 cited

Chemical enrichment and accretion of nitrogen-loud quasars

Kenta Matsuoka, Tohru Nagao, Roberto Maiolino +3

We present rest-frame optical spectra of 12 nitrogen-loud quasars at z ~ 2.2, whose rest-frame ultraviolet (UV) spectra show strong nitrogen broad emission lines. To investigate th…

astro-ph.GA2017★ 6 cited

An Optically Faint Quasar Survey at z~5 in the CFHTLS Wide Field: Estimates of the Black Hole Masses and Eddington Ratios

H. Ikeda, T. Nagao, K. Matsuoka +5

We present the result of our spectroscopic follow-up observation for faint quasar candidates at z~5 in a part of the Canada-France-Hawaii Telescope Legacy Survey wide field. We sel…

astro-ph.GA2017★ 19 cited

Active Galactic Nuclei with a Low-Metallicity Narrow-Line Region

Kota Kawasaki, Tohru Nagao, Yoshiki Toba +2

Low-metallicity active galactic nuclei (AGNs) are interesting to study the early phase of the AGN evolution. However most AGNs are chemically matured and accordingly low-metallicit…

astro-ph.GA2017★ 2 cited

Nature of hard X-ray (3-24 keV) detected luminous infrared galaxies in the COSMOS field

Kenta Matsuoka, Yoshihiro Ueda

We investigate the nature of far-infrared (70 um) and hard X-ray (3-24 keV) selected galaxies in the COSMOS field detected with both Spitzer and Nuclear Spectroscopic Telescope Arr…

astro-ph.GA2016★ 105 cited

The Complete Infrared View of Active Galactic Nuclei from the 70-month Swift/BAT Catalog

Kohei Ichikawa, Claudio Ricci, Yoshihiro Ueda +5

We systematically investigate the near- (NIR) to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGN) detected in the Swift/B…

astro-ph.GA2016★ 15 cited

Near-infrared spectroscopy of nearby Seyfert galaxies: Is there evidence for the shock excitation in narrow-line regions?

Koki Terao, Tohru Nagao, Tetsuya Hashimoto +5

One of the unsettled, important problems in active galactic nuclei (AGNs) is the major ionization mechanism of gas clouds in their narrow-line regions (NLRs). In order to investiga…

astro-ph.GA2016★ 12 cited

Revisiting the Completeness and the Luminosity Function in High-Redshift Low-Luminosity Quasar Surveys

Mana Niida, Tohru Nagao, Hiroyuki Ikeda +4

Recent studies have derived quasar luminosity functions (QLFs) at various redshifts. However, the faint side of the QLF at high redshifts is still too uncertain. An accurate estima…

astro-ph.GA2015★ 12 cited

Rest-frame UV single-epoch black hole mass estimates of low-luminosity AGN at intermediate redshifts

Marios Karouzos, Jong-Hak Woo, Kenta Matsuoka +6

The ability to accurately derive black hole (BH) masses at progressively higher redshifts and over a wide range of continuum luminosities has become indispensable in the era of lar…

astro-ph.GA2015★ 15 cited

The sign of active galactic nucleus quenching in a merger remnant with radio jets

Kohei Ichikawa, Junko Ueda, Megumi Shidatsu +2

We investigate optical, infrared, and radio active galactic nucleus (AGN) signs in the merger remnant Arp 187, which hosts luminous jets launched in the order of yr ago but…

astro-ph.GA2015★ 9 cited

Near-Infrared Spectroscopy of Quasars at z~3 and Estimates of Their Supermassive Black Hole Masses

Yuriko Saito, Masatoshi Imanishi, Yosuke Minowa +8

We present the results of new infrared spectroscopic observations of 37 quasars at z~3, selected based on the optical r'-band magnitude and the availability of nearby bright stars…

astro-ph.GA2015★ 15 cited

The Quasar-LBG Two-point Angular Cross-correlation Function at z ~ 4 in the COSMOS Field

H. Ikeda, T. Nagao, Y. Taniguchi +15

In order to investigate the origin of quasars, we estimate the bias factor for low-luminosity quasars at high redshift for the first time. In this study, we use the two-point angul…