Daichi Kashino

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Designated Assistant Professor

Nagoya University

Japan

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About

Daichi Kashino is a Designated Assistant Professor at Nagoya University, Japan. His research focuses on high-redshift galaxies, particularly their structural assembly, host characteristics, and the intergalactic medium. Recent publications include investigations of spiral structures in galaxies using JWST data and studies of luminous quasars at redshifts greater than 6.

Recent Grants

Grant: Close

宇宙再電離と宇宙初期の銀河進化の解明

Open Date: 2021-04-01

Close Date: 2025-03-01

Grant: Close

JSPS Research Fellow

Open Date: 2014-04-01

Close Date: 2017-03-01

Articles (17)

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2025

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2023

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2023

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2023

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2023

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2023

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2022

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2022

Collaborators (16)

Tsutomu Takeuchi

Associate Professor

Nagoya University

JAPAN

Daichi Kashino

Research Interests

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About

Recent Grants

Articles (17)

A Multiwavelength Investigation of Spiral Structures in z > 1 Galaxies with JWST

JWST and ALMA Discern the Assembly of Structural and Obscured Components in a High-redshift Starburst Galaxy

Little Red Dots

Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch (z > 10): Signature of Short Delay Time or Bright Hypernovae/Pair-instability Supernovae?

EIGER. VI. The Correlation Function, Host Halo Mass, and Duty Cycle of Luminous Quasars at z ≳ 6

EIGER. V. Characterizing the Host Galaxies of Luminous Quasars at z ≳ 6

EIGER IV. The Cool 104 K Circumgalactic Environment of High-redshift Galaxies Reveals Remarkably Efficient Intergalactic Medium Enrichment

Characterizing and understanding galaxies with two parameters

EIGER. I. A Large Sample of [O iii]-emitting Galaxies at 5.3 < z < 6.9 and Direct Evidence for Local Reionization by Galaxies

EIGER. II. First Spectroscopic Characterization of the Young Stars and Ionized Gas Associated with Strong Hβ and [O iii] Line Emission in Galaxies at z = 5–7 with JWST

EIGER. III. JWST/NIRCam Observations of the Ultraluminous High-redshift Quasar J0100+2802

Identifying Lyα emitter candidates with Random Forest: Learning from galaxies in the CANDELS survey

Elentári:a massive proto-supercluster at<scp> <i>z</i> ∼ 3.3</scp> in the <scp>cosmos</scp> field

Subhalo abundance matching using progenitor mass at varying redshift: two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering

Compact [C ii] emitters around a C iv absorption complex at redshift 5.7

Predicted future fate of COSMOS galaxy protoclusters over 11 Gyr with constrained simulations

The physical origin for spatially large scatter of IGM opacity at the end of reionization: The IGM Lyα opacity-galaxy density relation

Collaborators (16)

Tsutomu Takeuchi

Charlotte Mason

Georgios Magdis

Simon Lilly

Kai T Kono

Kimihiko Nakajima

Nozomu Tominaga

Jenny E Greene

Kei Ito

Koh Takahashi

Emanuele Daddi

Takumi S Tanaka

Shuowen Jin

Thomas Müller

John Silverman

Si-Yue Yu

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