Lista de obras - Tohru Nagao - Dominio Público Uruguay

NuSTAR Discovery of a Compton-thick, Dust-obscured Galaxy: WISE J0825+3002

artículo científico publicado en 2019

A Lyα EMITTER WITH AN EXTREMELY LARGE REST-FRAME EQUIVALENT WIDTH OF ∼900 Å ATz= 6.5: A CANDIDATE POPULATION III-DOMINATED GALAXY? ⬇️

artículo científico publicado en 2012

A Photometric Survey for Lyα–HeiiDual Emitters: Searching for Population III Stars in High‐Redshift Galaxies ⬇️

scholarly article

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). I. The Optical Counterparts of FIRST Radio Sources

scientific article published in the Astrophysical Journal

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z = 0.3–1.4

artículo científico publicado en 2022

ALMA 26 Arcmin2 Survey of GOODS-S at One Millimeter (ASAGAO): Average Morphology of High-z Dusty Star-forming Galaxies in an Exponential Disk (n ≃ 1)

artículo científico publicado en 2018

ALMA Reveals Strong $[{\bf{C}}\,{\bf{II}}]$ Emission in a Galaxy Embedded in a Giant LyαBlob atz= 3.1 ⬇️

scholarly article

ALMA deep field in SSA22: Blindly detected CO emitters and [C ii] emitter candidates

artículo científico publicado en 2017

ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy atz= 4.8 ⬇️

artículo científico publicado en 2014

Accretion properties of high- and low-excitation young radio galaxies ⬇️

scientific article published in the Astrophysical Journal

Accretion rate and the physical nature of unobscured active galaxies ⬇️

artículo científico publicado en 2011

An FMOS Survey of Moderate-luminosity, Broad-line AGNs in COSMOS, SXDS, and E-CDF-S

artículo científico publicado en 2018

CHORUS. II. Subaru/HSC Determination of the Lyα Luminosity Function at z = 7.0: Constraints on Cosmic Reionization Model Parameter

artículo científico publicado en 2018

Circumnuclear Molecular Gas in Low-redshift Quasars and Matched Star-forming Galaxies

artículo científico publicado en 2020

Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE ⬇️

artículo científico publicado en 2017

Completing the census of Ly{alpha} emitters at the reionization epoch ⬇️

artículo científico publicado en 2011

Discovery of a protocluster at z ~ 6 ⬇️

artículo científico publicado en 2012

Discovery of dramatic optical variability in SDSS J1100+4421: a peculiar radio-loud narrow-line Seyfert 1 galaxy? ⬇️

artículo científico publicado en 2014

Discovery of massive, mostly star formation quenched galaxies with extremely large Ly{alpha} equivalent widths at z ~ 3 ⬇️

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

artículo científico publicado en 2019

EMPRESS. XI. SDSS and JWST Search for Local and z 4-5 Extremely Metal-poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs

artículo científico publicado en 2023

EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely Metal-poor Galaxies

artículo científico publicado en 2024

Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph

article

First data release of the Hyper Suprime-Cam Subaru Strategic Program

Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4–7 derived with the half-million dropouts on the 100 deg2 sky†

article by Yoshiaki Ono et al published 1 November 2017 in Publications of the Astronomical Society of Japan

Keck spectroscopy of lyman-break galaxies and its implications for the UV-continuum and Ly{alpha} luminosity functions at z > 6 ⬇️

scientific article published in the Astrophysical Journal

Large Population of ALMA Galaxies at z > 6 with Very High [O iii] 88 μm to [C ii] 158 μm Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

artículo científico publicado en 2020

Minor Contribution of Quasars to Ionizing Photon Budget at z ∼ 6: Update on Quasar Luminosity Function at the Faint End with Subaru/Suprime-Cam ⬇️

artículo científico publicado en 2017

Morphological properties of Ly{alpha} emitters at redshift 4.86 in the cosmos field: clumpy star formation or merger? ⬇️

scientific article published in the Astrophysical Journal

Near-IR Spectroscopy of Luminous LoBAL Quasars at 1 < z < 2.5

artículo científico publicado en 2017

Near-infrared spectroscopy of quasars at z ∼ 3 and estimates of their supermassive black hole masses ⬇️

artículo científico publicado en 2016

No Sign of Strong Molecular Gas Outflow in an Infrared-bright Dust-obscured Galaxy with Strong Ionized-gas Outflow

artículo científico publicado en 2017

Observational limits on type 1 active galactic nucleus accretion rate in COSMOS ⬇️

artículo científico publicado en 2009

On the observed distributions of black hole masses and Eddington ratios from radiation pressure corrected virial indicators ⬇️

scholarly article by Alessandro Marconi et al published 29 May 2009 in The Astrophysical Journal

SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC

artículo científico publicado en 2018

SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies

artículo científico publicado en 2019

SUBARU HIGH-zEXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7 <z< 6.9 ⬇️

artículo científico publicado en 2016

Spectropolarimetric evidence for radiatively inefficient accretion in an optically dull active galaxy ⬇️

artículo científico publicado en 2011

Star formation at 4 < z < 6 from the Spitzer large area survey with Hyper-Suprime-Cam (SPLASH) ⬇️

artículo científico publicado en 2014

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 ≤ z ≤ 6.9

artículo científico publicado en 2018

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6

artículo científico publicado en 2018

The AGN-Starburst Connection traced by the Nitrogen Abundance

The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field,

artículo científico publicado en 2003

The Effect of Radiation Pressure on Virial Black Hole Mass Estimates and the Case of Narrow‐Line Seyfert 1 Galaxies ⬇️

article

The FMOS-COSMOS Survey of Star-forming Galaxies at Z ∼ 1.6. V: Properties of Dark Matter Halos Containing Hα Emitting Galaxies

artículo científico publicado en 2017

The Fe ii/Mg ii Flux Ratio of Low-luminosity Quasars at z ∼ 3

scholarly article

The Hyper Suprime-Cam SSP Survey: Overview and survey design

The Metal Abundances across Cosmic Time (MACT) survey. II. Evolution of the mass-metallicity relation over 8 billion years, using [OIII]4363AA-based metallicities ⬇️

artículo científico publicado en 2016

The Subaru COSMOS 20: Subaru optical imaging of the HST COSMOS field with 20 filters ⬇️

scholarly article

The nature of optically dull active galactic nuclei in COSMOS ⬇️

artículo científico publicado en 2009

Truth or Delusion? A Possible Gravitational Lensing Interpretation of the Ultraluminous Quasar SDSS J010013.02+280225.8 at z = 6.30

artículo científico publicado en 2020

Lista de obras de Tohru Nagao

<i>NuSTAR</i> Discovery of a Compton-thick, Dust-obscured Galaxy: WISE J0825+3002

A Lyα EMITTER WITH AN EXTREMELY LARGE REST-FRAME EQUIVALENT WIDTH OF ∼900 Å ATz= 6.5: A CANDIDATE POPULATION III-DOMINATED GALAXY? ⬇️

A Photometric Survey for Lyα–HeiiDual Emitters: Searching for Population III Stars in High‐Redshift Galaxies ⬇️

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). I. The Optical Counterparts of FIRST Radio Sources

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VII. Redshift Evolution of Radio Galaxy Environments at z = 0.3–1.4

ALMA 26 Arcmin2 Survey of GOODS-S at One Millimeter (ASAGAO): Average Morphology of High-z Dusty Star-forming Galaxies in an Exponential Disk (n ≃ 1)

ALMA Reveals Strong $[{\bf{C}}\,{\bf{II}}]$ Emission in a Galaxy Embedded in a Giant LyαBlob atz= 3.1 ⬇️

ALMA deep field in SSA22: Blindly detected CO emitters and [C ii] emitter candidates

ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy atz= 4.8 ⬇️

Accretion properties of high- and low-excitation young radio galaxies ⬇️

Accretion rate and the physical nature of unobscured active galaxies ⬇️

An FMOS Survey of Moderate-luminosity, Broad-line AGNs in COSMOS, SXDS, and E-CDF-S

CHORUS. II. Subaru/HSC Determination of the Lyα Luminosity Function at z = 7.0: Constraints on Cosmic Reionization Model Parameter

Circumnuclear Molecular Gas in Low-redshift Quasars and Matched Star-forming Galaxies

Clustering of infrared-bright dust-obscured galaxies revealed by the Hyper Suprime-Cam and WISE ⬇️

Completing the census of Ly{alpha} emitters at the reionization epoch ⬇️

Discovery of a protocluster at z ~ 6 ⬇️

Discovery of dramatic optical variability in SDSS J1100+4421: a peculiar radio-loud narrow-line Seyfert 1 galaxy? ⬇️

Discovery of massive, mostly star formation quenched galaxies with extremely large Ly{alpha} equivalent widths at z ~ 3 ⬇️

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

EMPRESS. XI. SDSS and JWST Search for Local and z 4-5 Extremely Metal-poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs

EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely Metal-poor Galaxies

Extragalactic science, cosmology, and Galactic archaeology with the Subaru Prime Focus Spectrograph

First data release of the Hyper Suprime-Cam Subaru Strategic Program

Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4–7 derived with the half-million dropouts on the 100 deg2 sky†

Keck spectroscopy of lyman-break galaxies and its implications for the UV-continuum and Ly{alpha} luminosity functions at z > 6 ⬇️

Large Population of ALMA Galaxies at <i>z</i> &gt; 6 with Very High [O iii] 88 <i>μ</i>m to [C ii] 158 <i>μ</i>m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?

Minor Contribution of Quasars to Ionizing Photon Budget at z ∼ 6: Update on Quasar Luminosity Function at the Faint End with Subaru/Suprime-Cam ⬇️

Morphological properties of Ly{alpha} emitters at redshift 4.86 in the cosmos field: clumpy star formation or merger? ⬇️

Near-IR Spectroscopy of Luminous LoBAL Quasars at 1 < z < 2.5

Near-infrared spectroscopy of quasars at z ∼ 3 and estimates of their supermassive black hole masses ⬇️

No Sign of Strong Molecular Gas Outflow in an Infrared-bright Dust-obscured Galaxy with Strong Ionized-gas Outflow

Observational limits on type 1 active galactic nucleus accretion rate in COSMOS ⬇️

On the observed distributions of black hole masses and Eddington ratios from radiation pressure corrected virial indicators ⬇️

SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC

SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at <i>z</i> ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies

SUBARU HIGH-zEXPLORATION OF LOW-LUMINOSITY QUASARS (SHELLQs). I. DISCOVERY OF 15 QUASARS AND BRIGHT GALAXIES AT 5.7 <z< 6.9 ⬇️

Spectropolarimetric evidence for radiatively inefficient accretion in an optically dull active galaxy ⬇️

Star formation at 4 < z < 6 from the Spitzer large area survey with Hyper-Suprime-Cam (SPLASH) ⬇️

Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). IV. Discovery of 41 Quasars and Luminous Galaxies at 5.7 ≤ z ≤ 6.9

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6

The AGN-Starburst Connection traced by the Nitrogen Abundance

The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field,

The Effect of Radiation Pressure on Virial Black Hole Mass Estimates and the Case of Narrow‐Line Seyfert 1 Galaxies ⬇️

The FMOS-COSMOS Survey of Star-forming Galaxies at Z ∼ 1.6. V: Properties of Dark Matter Halos Containing Hα Emitting Galaxies

The Fe ii/Mg ii Flux Ratio of Low-luminosity Quasars at z ∼ 3

The Hyper Suprime-Cam SSP Survey: Overview and survey design

The Metal Abundances across Cosmic Time (MACT) survey. II. Evolution of the mass-metallicity relation over 8 billion years, using [OIII]4363AA-based metallicities ⬇️

The Subaru COSMOS 20: Subaru optical imaging of the HST COSMOS field with 20 filters ⬇️

The nature of optically dull active galactic nuclei in COSMOS ⬇️

Truth or Delusion? A Possible Gravitational Lensing Interpretation of the Ultraluminous Quasar SDSS J010013.02+280225.8 at z = 6.30

X-ray-bright optically faint active galactic nuclei in the Subaru Hyper Suprime-Cam wide survey

Large Population of ALMA Galaxies at <i>z</i> > 6 with Very High [O iii] 88 <i>μ</i>m to [C ii] 158 <i>μ</i>m Flux Ratios: Evidence of Extremely High Ionization Parameter or PDR Deficit?