論文リスト
主要論文• Kodama, T. & Arimoto, N., 1997, A&A, 320, 41–53,“Origin of the Colour-Magnitude Relation of Elliptical Galaxies”,
新しい銀河スペクトル進化モデル構築の基礎論文。また銀河団早期型銀河の作る色–等級関係の起源についても論じた。
• Kodama, T., Arimoto, N., Barger, A. J., & Aragón-Salamamca, A., 1998, A&A, 334, 99–109,“Evolution of the Colour-Magnitude Relation of Early-Type Galaxies in Distant Clusters”,
銀河団の早期型 (楕円) 銀河を構成する星への年齢制限を、色等級関係から論じたもの。
• Bower, R. G., Kodama, T., & Terlevich, A., 1998, MNRAS, 299, 1193–1208,“The Colour-Magnitude Relation as a Constraint on the Formation of Rich Cluster Galaxies”,
色等級関係の分散の小ささから銀河団銀河の星形成史と合体史に対して制限を与えたもの。
• Kodama, T., Bell, E. F., & Bower, R. G., 1999, MNRAS, 302, 152–166,“A Bayesian Classiﬁer for Photometric Redshifts: Identiﬁcation of High Redshift Clusters”,
測光学的赤方偏移のコードを、自身のスペクトル進化モデルを用いて作成した論文。さらにそれを用いて、遠方銀河団の同定を如何に効率良く行なえるかについても論じた。
• Kodama, T., Bower, R. G., & Bell, E. F., 1999a, MNRAS, 306, 561–566,“The Colour-Magnitude Relation of Early-Type Galaxies in the Hubble Deep Field”,
フィールド環境にいる早期型銀河を構成する星への年齢制限を、色等級関係から論じたもの。
• Kodama, T., & Bower, R. G., 2001, MNRAS, 321, 18–36,“Reconstructing the History of Star Formation in Rich Cluster Cores”,
銀河団領域における星形成史を、銀河の測光分光的性質の時間進化から総合的に論じたもの。銀河団銀河進化に関するランドマーク的論文。
• Kodama, T., Smail, I., Nakata, F., Okamura, S., Bower, R. G., 2001, ApJ, 562, L9–L13,“The Transformation of Galaxies within the Large Scale Structure around a z = 0.41 Cluster”,
すばる望遠鏡による広視野観測から、銀河団の大規模構造とその中の銀河の環境依存性を論じた論文。PISCES プロジェクトの端緒となる論文。
• Kodama, T., 31 authors, 2004, MNRAS, 350, 1005–1014,“Down-Sizing in Galaxy Formation at z ∼ 1 in the Subaru/XMM-Newton Deep Survey (SXDS)”,
すばる望遠鏡による広視野観測から、銀河進化の質量依存性 (ダウンサイジング) をはっきりと示した端緒的論文。
• Kodama, T., 23 authors, 2005, PASJ, 57, 309–323,“Panoramic Views of Cluster-Scale Assemblies Explored by Subaru Wide-Field Imaging”,
すばる望遠鏡で展開している、遠方銀河団の広視野観測プロジェクト (PISCES) の概略を紹介し、3 つの典型的な銀河団サンプルについて大規模構造の発展を、理論シミュレーションと比較して示
した論文。

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• Tanaka, M., Kodama, T., 6 authors, 2005, MNRAS, 362, 268–288,“The build-up of the colour-magnitude relation as a function of environment”,
PISCES のハイライト的論文で、z = 0.8 から z = 0 までの銀河の星形成活動の進化を、質量と環境の関数として定量的に示した論文。
• Kodama, T., 7 authors, 2007, MNRAS, 377, 1717–1725,“The ﬁrst appearance of the red sequence of galaxies in proto-clusters at 2 <
∼z <
∼ 3”,
近赤外線観測による 2 < z < 3 の原始銀河団の観測により、楕円銀河の祖先である重い銀河の形成
現場を間接的に捕えた、先駆的な論文。
• Koyama, Y., Kodama, T., Shimasaku, K., Hayashi, M., Okamura, S., Tanaka, I., Tokoku, C.,
2010, MNRAS, 403, 1611–1624,“Panoramic Hα and mid-infrared mapping of star formation in a z=0.8 cluster”,
すばるのナローバンドを用いた Hα 輝線マッピング観測とあかりの広視野中間赤外線データを用いて、銀河団の外側の銀河群やインフォール領域において星形成活動が活発になっていることを突き止めた論文。現在進行中の MAHALO-Subaru プロジェクトの先駆的な論文。
• Tadaki, K., Kodama, T., Tanaka, I., Hayashi, M., Koyama, Y., Shimakawa, R., 2014, ApJ,
780, 77,“The Nature of Hα selected galaxies at z > 2. II. Clumpy galaxies and compact star-forming
galaxies” すばるのナローバンドを用いた Hα 輝線マッピング観測と、ハッブル宇宙望遠鏡の高解像度画像とを組み合わせて、銀河形成最盛期 (z=2–2.5) の時代の銀河の性質や内部構造を議論した論文で、MAHALO-Subaru プロジェクトのハイライト論文の一つ。
• Shimakawa, R., Kodama, T., Tadaki, K., Hayashi, M., Koyama, Y., Tanaka, I., 2015, MNRAS,
448, 666–680,“An early phase of environmental eﬀects on galaxy properties unveiled by near-infrared spectroscopy of protocluster galaxies at z > 2” MAHALO-Subaru プロジェクトの最も遠い銀河団サンプル２つについて近赤外線分光観測を行って、銀河形成最盛期にあたる原始銀河団の重元素量や電離状態について環境依存性を議論した論文。MAHALO-Subaru プロジェクトのハイライト論
文の一つ。
• Suzuki, L. T., Kodama, T., Tadaki, K., Hayashi, M., Koyama, Y., Tanaka, I., Minowa, Y.,
Shimakawa, R., Yamamoto, M., 2015, ApJ, 806, 208,
“Galaxy formation at z > 3 revealed by narrow-band selected [OIII] Emission Line Galaxies”• Tadaki, K., Genzel, R., Kodama, T., 24 authors, 2017, ApJ, 834, 135,
“Bulge-forming galaxies with an extended rotating disk at z ∼ 2”
• Hayashi, M., Kodama, T., et al., ApJ, 841, L21,
“Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46”• Shimakawa, R., Kodama, T., et al., 2017, MNRAS, 468, L21,
“Direct evidence for Ly-alpha depletion in the protocluster core”• Shimakawa, R., Kodama, T., et al., 2018, MNRAS, 473, 1977,“MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest
regions of a protocluster at z=2.5”
2• Tadaki, K., Kodama, T., 13 authors, 2019, PASJ, 71, 40,”Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2”
• Asano, T., Kodama, T., 18 authors, 2020, ApJ, 899, 64,”Environmental Impact on Star-forming Galaxies in a z ∼ 0.9 Cluster during the Course of
Galaxy Accretion”• Koyama, Y., 2 authors, Kodama, T., 5 authors, 2021, MNRAS, 503, L1,”A Planck-selected dusty proto-cluster at z=2.16 associated with a strong overdensity of massive
H α-emitting galaxies”• Aoyama, K., Kodama, T., 6 authors, 2022, ApJ, 924, 74,”The Environmental Dependence of Gas Properties in Dense Cores of a Protocluster at z=2.5
Revealed with ALMA”• Suzuki, T. L., Glazebrook, K., Schreiber, C., Kodama, T., 9 authors, 2022, ApJ, 936, 61,”Low Star Formation Activity and Low Gas Content of Quiescent Galaxies at z=3.5–4.0 Constrained with ALMA”• Mao, Z., Kodama, T., 4 authors, 2022, A&A, 666, 141,
”Revealing impacts of stellar mass and environment on galaxy quenching”• Pérez-Martı́nez, J. M., Dannerbauer, H., Kodama, T., 10 authors, 2023, MNRAS, 518, 1707,”Signs of environmental eﬀects on star-forming galaxies in the Spiderweb protocluster at z=2.16”• Liu, Z., Morishita, T., Kodama, T., 2023, ApJ, 955, 29,”A Multiwavelength Investigation of Dust and Stellar Mass Distributions in Galaxies: Insightsfrom High-resolution JWST Imaging”• Tadaki, K., Kodama, T., Koyama, Y., Suzuki, T., Mitsuhashi, I., Ikeda, R., 2023, ApJ, 957,
15,
”Spatial Extent of Molecular Gas, Dust, and Stars in Massive Galaxies at z=2.2–2.5 Determinedwith ALMA and JWST”

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査読論文
• van Driel, W., 13 authors, Kodama, T., 4 authors, 1995, AJ, 109, 942–959,“Polar Ring Spiral Galaxy NGC 660”
• Kodama, T. & Arimoto, N., 1997, A&A, 320, 41–53,“Origin of the Colour-Magnitude Relation of Elliptical Galaxies”• Yamada, T., Tanaka, I., Aragón-Salamanca, A., Kodama, T., Ohta, K., & Arimoto, N., 1997,
ApJ, 487, L125–128,“Clustering of Red Galaxies near the Radio-loud Quasar 1335.8+2834 at z = 1.1”
• Kodama, T., Arimoto, N., Barger, A. J., & Aragón-Salamamca, A., 1998, A&A, 334, 99–109,“Evolution of the Colour-Magnitude Relation of Early-Type Galaxies in Distant Clusters”• Gladders, M. D., Lopez-Cruz, O., Yee, H. K. C. & Kodama, T., 1998, ApJ, 501, 571–577,“The Slope of the Cluster Elliptical Red Sequence: A Probe of Cluster Evolution”• Bower, R. G., Kodama, T., & Terlevich, A., 1998, MNRAS, 299, 1193–1208,“The Colour-Magnitude Relation as a Constraint on the Formation of Rich Cluster Galaxies”• Kodama, T., & Arimoto, N., 1998, MNRAS, 300, 193–199,“Secondary Episode of Star Formation in Elliptical Galaxies”• Kodama, T., Bell, E. F., & Bower, R. G., 1999, MNRAS, 302, 152–166,“A Bayesian Classiﬁer for Photometric Redshifts: Identiﬁcation of High Redshift Clusters”• Kodama, T., Bower, R. G., & Bell, E. F., 1999b, Astrophysics and Space Science, 265, 487–488,“Formation Epoch of Field Early-Type Galaxies”• Kodama, T., Bower, R. G., & Bell, E. F., 1999a, MNRAS, 306, 561–566,“The Colour-Magnitude Relation of Early-Type Galaxies in the Hubble Deep Field”• Tanaka, I., Yamada, T., Aragón-Salamanca, A., Kodama, T., Miyaji, T., Ohta, K., & Arimoto,N., 2000, ApJ, 528, 123–138,“A Rich Cluster of Galaxies Near the Quasar B2 1335+28 at z = 1.1: Colour Distribution andStar-Formation Properties”• Tamura, N., Kobayashi, C., Arimoto, N., Kodama, T., Ohta, K., 2000, AJ, 119, 2134–2145,“Origin of Color Gradients in Elliptical Galaxies in the Hubble Deep Field”• Kodama, T., & Matsushita, K., 2000, ApJ, 539, 149–154,“Homogeneity of Stellar Populations in Early-Type Galaxies with Diﬀerent X-ray Properties”• Kodama, T., Bower, R. G., 2001, Astrophysics and Space Science, 277, 597–597“Global Star Formtion History in Rich Cluster Cores”• Kodama, T., & Bower, R. G., 2001, MNRAS, 321, 18–36,“Reconstructing the History of Star Formation in Rich Cluster Cores”

4• Kodama, T., 2001, Astrophysics and Space Science, 276, 877–884,“The Colour-Magnitude Relation and the Formation of Early-Type Galaxies”• Kodama, T., Bower, R. G., Bell, E. F., 2001, Astrophysics and Space Science, 276, 979–981,“The Colour-Magnitude Relation of Early-Type Galaxies in the Hubble Deep Field North”• Smail, I., Kuntschner, H., Kodama, T., Smith, G. P., Packham, C., Fruchter, A. S., Hook, R.
N., 2001, MNRAS, 323, 839–849,“A Photometric Study of the Ages and Metallicities of Early-type Galaxies in A2218”• Kodama, T., & Smail, I., 2001, MNRAS, 326, 637–642,“Testing the Hypothesis of the Morphological Transformation from Field Spiral to Cluster S0”• Kodama, T., Smail, I., Nakata, F., Okamura, S., Bower, R. G., 2001, ApJ, 562, L9–L13,“The Transformation of Galaxies within the Large Scale Structure around a z = 0.41 Cluster”• Yamada, T., 5 authors, Kodama, T., 11 authors, 2001, PASJ, 53, 1119–1131,“Subaru Deep Near Infrared Imaging of the Field of the Possible Proto-Cluster Near the Radio
Galaxy 53W002 at z = 2.4”
• Nakata F., Kajisawa, M., Yamada, T., Kodama, T., Shimasaku, K., Tanaka, I., 2001, PASJ,53, 1139–1152,“Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C324 at z = 1.2”
• Pimbblet, K. A., Smail, I., Kodama, T., Edge, A. C., Couch, W. J., Zabludoﬀ, A. I., & O’Hely,E., 2002, MNRAS, 331, 333–350,“The Las Campanas/AAT Rich Cluster Survey: II. The Environmental Dependence of Galaxy
Colours in Clusters at z ∼ 0.1”
• Yamada, T., 4 authors, Kodama, T., 2 authors, 2002, ApJ, 577, L89–L92,“Witnessing the Hierarchical Assembly of the Brightest Cluster Galaxy in a Cluster at z=1.26”• Kawabata, K. S., 29 authors, Kodama, T., 2002, ApJ, 580, L39–L42,“Optical Spectropolarimetry of SN 2002ap: A High-Velocity Asymmetric Explosion”• Kodaira, K., 17 authors, Kodama, T., 26 authors, 2003, PASJ, 55, L17–L21,“The Discovery of Two Lymanα Emitters beyond Redshift 6 in the Subaru Deep Field”• Iye, S., 5 authors, Kodama, T., 7 authors, 2003, ApJ, 590, 770–777,“ERO R1 in the Field of CL 0939+4713: Evidence for an S0-like Galaxy at z ∼ 1.5”
• Kodama, T., Bower, R. G., 2003, MNRAS, 346, 1–12,“The Ks -band Luminosity and Stellar Mass Functions of Galaxies in z ∼ 1 Clusters”• Miyazaki, M., Shimasaku, K., Kodama, T., +23 authors, 2003, PASJ, 55, 1079–1103,“Evolution of Elliptical Galaxies at z >∼ 1 Revealed from a Large, Multicolor Sample of Extremely
Red Objects”• Bundy, K., Fukugita, M., Ellis, R. S., Kodama, T., Conselice, C. J., 2004, ApJ, 601, L123–L126“A Slow Merger History of Field Galaxies Since z ∼ 1”
5

• Kodama, T., 31 authors, 2004, MNRAS, 350, 1005–1014,“Down-Sizing in Galaxy Formation at z ∼ 1 in the Subaru/XMM-Newton Deep Survey (SXDS)”• Nagao, T., 16 authors, Kodama, T., 22 authors, 2004, ApJ, 613, L9–L12“A Strong Lyα Emitter at z=6.33 in the Subaru Deep Field Selected as an i′ -Dropout”• Kodama, T., Balogh, M. L., Smail, I., Bower, R. G., Nakata, F., 2004, MNRAS, 354, 1103–
1119,“A panoramic Hα imaging survey of the z = 0.4 cluster Cl0024.0+1652 with Subaru”• Kashikawa, N., 15 authors, Kodama, T., 21 authors, 2004, PASJ, 56, 1011–1023,“The Subaru Deep Field: The Optical Imaging Data”• Ouchi, M., 7 authors, Kodama, T., 8 authors, 2005, ApJ, 620, L1–L4,“The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6”• Taniguchi, Y., 18 authors, Kodama, T., 20 authors, 2005, PASJ, 57, 165–182,“The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6”
• Nakata, F., Kodama, T., 12 authors, 2005, MNRAS, 357, 1357–1362,“Discovery of a Large Scale Structure towards the Lynx Supercluster at z ∼ 1.27”• Kodama, T., 23 authors, 2005, PASJ, 57, 309–323,“Panoramic Views of Cluster-Scale Assemblies Explored by Subaru Wide-Field Imaging”• Tanaka, M., Kodama, T., 6 authors, 2005, MNRAS, 362, 268–288,“The build-up of the colour-magnitude relation as a function of environment”• Yamada, T., Kodama, T., 11 authors, 2005, ApJ, 634, 861–878,“The Number Density of Old Passively Evolving Galaxies at z = 1 in the Subaru/XMM-Newton
Deep Survey Field”• Umetsu, K., Tanaka, M., Kodama, T., 4 authors, 2005, PASJ, 57, 877–880,“Discovery of a Strongly Lensed Galaxy at z = 3.9 behind a z = 0.83 Galaxy Cluster”• Kashikawa, N., 19 authors, Kodama, T., 19 authors, 2006, ApJ, 637, 631–647,“Clustering of Lyman Break Galaxies at z = 4 and 5 in the Subaru Deep Field: Luminosity
Dependence of the Correlation Function Slope”• Tanaka, M., Kodama, T., Arimoto, N., Tanaka, I, 2006, MNRAS, 365, 1392–1404,“Spectroscopically conﬁrmed large-scale structures associated to a z=0.83 cluster”• Hamana, T., Yamada, T., Ouchi, M., Iwata, I., Kodama, T., 2006, MNRAS, 369, 1929–1938,“Masses of high-z galaxy hosting haloes from angular clustering and their evolution in the cold
dark matter model”• Matsuhara, H., 13 authors, Kodama, T., 14 authors, 2006, PASJ, 58, 673–694,“Deep Extragalactic Surveys around the Ecliptic Poles with AKARI (ASTRO-F)”• Intema, H. T., Venemans, B. P., Kurk, J. D., Ouchi, M., Kodama, T., 3 authors, 2006, A&A,
456, 433–437,“Large-scale structure of Lyman break galaxies around a radio galaxy protocluster at z ∼ 4”
6

• Kajisawa, M., Kodama, T., 3 authors, 2006, MNRAS, 371, 577–582,“Protoclusters with evolved populations around radio galaxies at z ∼ 2.5”
• Geach, J. E., 7 authors, Kodama, T., 2006, ApJ, 649, 661–672,“A Panoramic Mid-Infrared Survey of Two Distant Clusters”• Yoshida, M., 16 authors, Kodama, T., 20 authors, 2006, ApJ, 653, 988–1003,“Luminosity Functions of Lyman Break Galaxies at ∼ 4 and z ∼ 5 in the Subaru Deep Field”• Ly, C., 6 arthors, Kodama, T., 2 authors, 2007, ApJ, 657, 738–759,“The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for
Narrowband Emitters in the Subaru Deep Field”• Tanaka, M., Kodama, T., 6 authors, 2007, MNRAS, 377, 1206–1214,“A deﬁcit of faint red galaxies in the possible large-scale structures around the RDCS J1252.9–
2927 cluster at z = 1.24”• Kodama, T., 7 authors, 2007, MNRAS, 377, 1717–1725,“The ﬁrst appearance of the red sequence of galaxies in proto-clusters at 2 <
∼z <
∼ 3”
• Tanaka, M., Hoshi, T., Kodama, T., Kashikawa, N., 2007, MNRAS, 379, 1546–1556,“A huge ﬁlamentary structure at z = 0.55 and star formation histories of galaxies at z < 1”
• Koyama, Y., Kodama, T., 3 authors, 2007, MNRAS, 382, 1719–1728,“Dependence of the Build-up of the Colour-Magnitude Relation on Cluster Richness at z ∼ 0.8”
• Furusawa, H., 22 authors, Kodama, T., 12 authors, 2008, ApJS, 176, 1–18,“The Subaru/XMM-Newton Deep Survey (SXDS). II. Optical Imaging and Photometric Catalogs”• Ouchi, M., 8 authors, Kodama, T., 6 authors, 2008, ApJS, 176, 301–330,“The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z=3.1
to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN”
• Tanaka, M., Finoguenov, A., Kodama T., 6 authors, 2008, A&A, 489, 571–581,“The environmental dependence of properties of galaxies around the RDCSJ0910+54 cluster at
z=1.1”• Koyama, Y., Kodama, T., 9 authors, 2008, MNRAS, 391, 1758–1770,“Mapping dusty star formation in and around a cluster at z=0.81 by wide-ﬁeld imaging withAKARI”• Ouchi, M., 20 authors, Kodama, T., 5 authors, 2009, ApJ, 696, 1164–1175,“Discovery of a Giant Lyα Emitter Near the Reionization Epoch”• Bundy, K., Fukugita, M., Ellis, R. S., Targett, T. A., Belli, S., Kodama, T., 2009, ApJ, 697,
1369–1383,“The Greater Impact of Mergers on the Growth of Massive Galaxies: Implications for Mass
Assembly and Evolution since z ∼ 1”

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• Matsuura, M., 7 suthors, Kodama, T., 4 authors, 2009, ApJ, 396, 918–934,“The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae,
and the impact on the ISM evolution”• Tanaka, M., Finoguenov, A., Kodama, T., Koyama, Y., Maughan, B., Nakata, F., 2009, A&A,
505, L9–L12,“The spectroscopically conﬁrmed huge cosmic structure at z=0.55”• Tanaka, M., Lidman, C., Bower, R. G., Demarco, R., Finoguenov, A., Kodama, T., Nakata,F., Rosati, P., 2009, A&A, 507, 671–682,“Star formation activities of galaxies in the large-scale structures at z=1.2”• Matsuda, Y., 5 authors, Kodama, T., 11 authors, 2009, MNRAS, 400, L66–L70,“Lyα blobs like company: the discovery of a candidate 100kpc Lyα blob near to a radio galaxy
with a giant Lyα halo B3J2330+3927 at z=3.1”• Doherty, M., Tanaka, M., De Breuck, C., Ly, C., Kodama, T., 7 authors, 2010, A&A, 509,
A83,
“Optical and near-IR spectroscopy of candidate red galaxies in two z ∼ 2.5 proto-clusters”• Hayashi, M., Kodama, T., Koyama, Y., Tanaka, I., Shimasaku, K., Okamura, S., 2010, MNRAS, 402, 1980–1990,“High star formation activity in the central region of a distant cluster at z=1.46”• Wardlow, J. L., 13 authors, Kodama, T., 5 authors, 2010, MNRAS, 401, 2299–2317,“An AzTEC 1.1-mm survey for ULIRGs in the ﬁeld of the Galaxy Cluster MS0451.6-0305”• Goto, T., 13 authors, Kodama, T., 8 authors, 2010, A&A, 514, A7,“Environmental dependence of 8um luminosity functions of galaxies at z ∼ 0.8: Comparison
between RXJ1716.4+6708 and the AKARI NEP deep ﬁeld”• Koyama, Y., Kodama, T., Shimasaku, K., Hayashi, M., Okamura, S., Tanaka, I., Tokoku, C.,
2010, MNRAS, 403, 1611–1624,“Panoramic Hα and mid-infrared mapping of star formation in a z=0.8 cluster”• Kuiper, E., 8 authors, Kodama, T., 5 authors, 2010, MNRAS, 405, 969–986,“A Galaxy populations study of a radio-selected protocluster at z ∼ 3.1”
• Galametz, A., 4 authors, Kodama, T., 7 authors, 2010, A&A, 522, A58,
“A Galaxy populations study of a radio-selected protocluster at z ∼ 3.1”
• Ouchi, M., 10 authors, Kodama, T., 3 authors, 2010, ApJ, 723, 869,
“Statistics of 207 Ly α Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy
Formation Models”• Hatch, N. A., 6 authors, Kodama, T., 5 authors, 2011, MNRAS, 410, 1537–1549,“Galaxy protocluster candidates around z ∼ 2.4 radio galaxies”• Tanaka, I., 3 authors, Kodama, T., 10 authors, 2011, PASJ, 63, 415–435,“Discovery of an Excess of Hα Emitters around 4C 23.56 at z=2.4”
8• Tadaki, K., Kodama, T., Koyama, Y., Hayashi, M., Tanaka, I., Tokoku, C., 2011, PASJ, 63,
437–446,“Cosmic Star-Formation Activity at z=2.2 Probed by Hα Emission-Line Galaxies”• Raichoor, A., 13 authors, Kodama, T., 2 authors, 2011, ApJ, 745, 130“Early-type Galaxies at z 1.3. II. Masses and Ages of Early-type Galaxies in Diﬀerent Environments and Their Dependence on Stellar Population Model Assumptions”• Rettura, A., 17 authors, Kodama, T., 3 authors, 2011, ApJ, 732, 94“Early-type Galaxies at z 1.3. III. On the Dependence of Formation Epochs and Star Formation
Histories on Stellar Mass and Environment”• Koyama, Y., Kodama, T., Nakata, F., Shimasaku, K., Okamura, S., 2011, ApJ, 734, 66“Red Star-forming Galaxies and Their Environment at z=0.4 Revealed by Panoramic Hα Imaging”• Hayashi, M., Kodama, T., Koyama, Y., Tadaki, K., Tanaka, I., 2011, MNRAS, 415, 2670–2687,“Properties of star-forming galaxies in a cluster and its surrounding structure at z=1.46”• Matsuda, Y., 13 authors, Kodama, T., 3 authors, 2011, MNRAS, 416, 2041–2059,“An Hα search for overdense regions at z=2.23”• Raichoor, A., 10 authors, Kodama, T., 6 authors, 2012, ApJ, 745, 130,
“Early-type Galaxies at z∼1.3. IV. Scaling Relations in Diﬀerent Environments”• Tadaki, K., Kodama, T., Ota, K., Hayashi, M., Koyama, Y., Papovich, C., Brodwin, M.,
Tanaka, M., Iye, M., 2012, MNRAS, 423, 2617
“A large-scale structure traced by [OII] emitters hosting a distant cluster at z=1.62”• Simona, M., 8 authors, Kodama, T., 11 authors, 2012, ApJ, 754, 141,
“Early-type Galaxies at z=1.3. I. The Lynx Supercluster: Cluster and Groups at z=1.3. Morphology and Color-Magnitude Relation”• Iono, D., 5 authors, Kodama, T., 34 authors, 2012, PASJ, 64, L2,“Initial Results from Nobeyama Molecular Gas Observations of Distant Bright Galaxies”• Hayashi, M., Kodama, T., Tadaki, K., Koyama, Y., Tanaka I., 2012, ApJ, 757, 15,“A Starbursting Proto-cluster in Making Associated with a Radio Galaxy at z=2.53 Discoveredby Hα Imaging”• Crossﬁeld, I. J. M., Barman, T., Hansen, B. M. S., Tanaka, I., Kodama, T., 2012, ApJ, 760,
140,
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9• Gu, L., Gandhi, P., Inada, N., Kawaharada, M., Kodama, T., Konami, S., Nakazawa, K.,
Shimasaku, K., Xu, H., Makishima, K., 2013, ApJ, 767, 157,
“Probing of the Interactions between the Hot Plasmas and Galaxies in Clusters from z=0.1 to
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“On the Formation Timescale of Massive Cluster Ellipticals Based on Deep Near-infrared Spectroscopy at z ∼ 2”
• Koyama, Y., 4 authors, Kodama, T., 5 authors, 2013, MNRAS, 434, 423,
“On the evolution and environmental dependence of the star formation rate versus stellar mass
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• Stott, J., 7 authors, Kodama, T., 2013, MNRAS, 436, 1130
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780, 77,“The Nature of Hα selected galaxies at z > 2. II. Clumpy galaxies and compact star-forming
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Cluster”• Santos, J. S., 6 authors, Kodama, T., 2 authors, 2014, MNRAS, 438, 2565,“Star formation in the cluster CLG0218.3–0510 at z=1.62 and its large-scale environment: theinfrared perspective”• Hayashi, M., Kodama, T., 8 authors, 2014, MNRAS, 439, 2571,“Mapping the large scale structure around a z=1.46 galaxy cluster in 3-D using two adjacentnarrow-band ﬁlters”• Shimakawa, R., Kodama, T., Tadaki, K., Tanaka, I., Hayashi, M., Koyama, Y., 2014, MNRAS,
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10

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“Evidence for a gas-rich merger in a proto-cluster at z=2.5”• Dannerbauer, H., 11 authors, Kodama, T., 6 authors, A&A, 570, A55,
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• Ma, C.-J., 9 authors, Kodama, T., 2015, ApJ, 806, 257,
Dusty starbursts and the formation of elliptical galaxies: A SCUBA-2 survey of a z=1.46 cluster• Shimakawa, R., Kodama, T., Steidel, C. C.., Tadaki, K., Tanaka, I., Strom, A. L., Hayashi,M., Koyama, Y., Suzuki, T. L., Yamamoto, M., 2015, MNRAS, 451, 1284–1289,“Correlation between star formation activity and electron density of ionized gas at z = 2.5”
• Suzuki, L. T., Kodama, T., Tadaki, K., Hayashi, M., Koyama, Y., Tanaka, I., Minowa, Y.,
Shimakawa, R., Yamamoto, M., 2015, ApJ, 806, 208,
“Galaxy formation at z > 3 revealed by narrow-band selected [OIII] Emission Line Galaxies”• Murata, K., Koyama, Y., Tanaka, M., Matsuhara, H., Kodama, T., 2015, A&A, accepted,“Environmental dependence of polycyclic aromatic hydrocarbon emission at z ∼ 0.8. Investigation by observin g the RX J0152.7-1357 with AKARI”• Tadaki, K., Kohno, K., Kodama, T., 23 authors, 2015, ApJ, 811, L3,“SXDF-ALMA 1.5 arcmin2 deep survey. A compact dusty star-forming galaxy at z = 2.5”
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11

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• Tadaki, K., Genzel, R., Kodama, T., 24 authors, 2017, ApJ, 834, 135,
“Bulge-forming galaxies with an extended rotating disk at z ∼ 2”
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“Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46”• Tadaki, K., Kodama, T., et al., 2017, ApJ, 841, L25,
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”A Universal Correlation between Star Formation Activity and Molecular Gas Properties AcrossEnvironments”• Suzuki, T. L., Kodama, T., et al., 2017, ApJ, 849, 39,“The interstellar medium in [OIII]-selected star-forming galaxies at z ∼ 3.2”
• Wang, W.-H., ; Lin, 6 authors, Kodama, T., 35 authors, 2017, ApJ, 850, 37,”SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μ m”
• Dannerbauer, H., 6 authors, Kodama, T., 13 authors, 2017, A&A, 608, 48,”The implications of the surprising existence of a large, massive CO disk in a distant protocluster”
12• Lin, Y.-T., 7 authors, Kodama, T., 6 authors, 2017, ApJ, 851, L139,”First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey.
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regions of a protocluster at z=2.5”• Toshikawa, J., 7 authors, Kodama, T., 9 authors, 2018, PASJ, 70, 12,”GOLDRUSH. III. A systematic search for protoclusters at z ∼ 4 based on the >100 deg2 area”• Hayashi, M., 6 authors, Kodama, T., 10 authors, 2018, PASJ, 70, 17,”A 16 deg2 survey of emission-line galaxies at z < 1.5 in HSC-SSP Public Data Release 1”• Koyama, Y., 2 authors, Kodama, T., 12 authors, 2018, PASJ, 70, 21,”The nature of Hα-selected galaxies along the large-scale structure at z = 0.4 revealed by Subaru
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• Hayashi, M., Tadaki, K., Kodama, T., 7 authors, 2018, ApJ, 856, 118,
”Molecular Gas Reservoirs in Cluster Galaxies at z=1.46”• Zeballos, M., 12 authors, Kodama, T., 9 authors, 2018, MNRAS, 479, 4577,”AzTEC 1.1 mm observations of high-z protocluster environments: SMG overdensities and misalignment between AGN jets and SMG distribution”• Wang, T., Elbaz, D., Daddi, E., Liu, D., Kodama, T., 11 authors, 2018, ApJ, 867, L29,
”Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Clusterat z = 2.51”• Shimakawa, R., Koyama, Y., Röttgering, H. J. A., Kodama, T., 2018, MNRAS, 481, 5630,”MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb
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• Hatsukade, B., 16 authors, Kodama, T., 14 authors, 2018, PASJ, 70, 105,
”ALMA twenty-six arcmin2 survey of GOODS-S at one millimeter (ASAGAO): Source catalog
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2019, ApJ, 874, 54,”The Fraction of Active Galactic Nuclei in the USS 1558-003 Protocluster at z = 2.53”
13

• Koyama, S., 8 authors, Kodama, T., 4 authors, 2019, ApJ, 874, 142,
”Do Galaxy Morphologies Really Aﬀect the Eﬃciency of Star Formation During the Phase of
Galaxy Transition?”• Tadaki, K., Kodama, T., 13 authors, 2019, PASJ, 71, 40,”Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2”
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”A Spectroscopic Study of a Rich Cluster at z = 1.52 with Subaru and LBT: The Environmental
Impacts on the Mass-Metallicity Relation”• Yamaguchi, Y., 12 authors, Kodama, T., 10 authors, 2019, ApJ, 878, 73,”ALMA 26 arcmin2 Survey of GOODS-S at 1 mm (ASAGAO): Near-infrared-dark Faint ALMA
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”The whole picture of the large-scale structure of the CL1604 supercluster at z ∼ 0.9”
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”Redshift Evolution of Green Valley Galaxies in Diﬀerent Environments from the Hyper SuprimeCam Survey”• Gu, L., 5 authors, Kodama, T., 2 authors, 2020, A&A, 638, 138,
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Galaxy Accretion”• Yamaguchi, Y., 11 authors, Kodama, T., 9 authors, 2020, PASJ, 72, 69,”ALMA twenty-six arcmin2 survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies”
14• Tadaki, K., 7 authors, Kodama, T., 12 authors, 2020, ApJ, 901, 74,”Structural Evolution in Massive Galaxies at z ∼ 2”
• Onodera, M., 5 authors, Kodama, T., 3 authors, 2020, ApJ, 904, 180,
”Broadband Selection, Spectroscopic Identiﬁcation, and Physical Properties of a Population ofExtreme Emission-line Galaxies at 3 < z < 3.7”
• Inoue, A., 26 authors, Kodama, T., 3 authors, 2020, PASJ, 72, 101,
”CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview”• Suzuki, T., Onodera, M., Kodama, T., 8 authors, 2021, ApJ, 908, 15,”Dust, Gas, and Metal Content in Star-forming Galaxies at z ∼ 3.3 Revealed with ALMA and
Near-IR Spectroscopy”• Lee, M. M., 3 authors, Kodama, T., 3 authors, 2021, ApJ, 909, 181,
”Revisited Cold Gas Content with Atomic Carbon [C I] in z = 2.5 Protocluster Galaxies”• Shimakawa, R., 8 authors, Kodama, T., 1 author, 2021, MNRAS, 503, 3896,”Subaru Hyper Suprime-Cam excavates colossal over- and underdense structures over 360 deg2
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• Koyama, Y, 2 author, Kodama, T., 5 authors, 2021, MNRAS, 503, L1,”A Planck-selected dusty proto-cluster at z = 2.16 associated with a strong overdensity of massive
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”A Phase-space View of Cold-gas Properties of Virgo Cluster Galaxies: Multiple Quenching
Processes at Work?”• Jin, S., 17 authors, Kodama, T., 9 authors, 2021, A&A, 652, 11,”COALAS. I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at
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Gas Properties in Dense Cores of a Protocluster at z=2.5 Revealed with ALMA”• Yajima, H., 4 authors, Kodama, T., 11 authors, 2022, MNRAS, 509, 407,
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”Star Formation Properties of Sloan Digital Sky Survey BOSS Void Galaxies in the Hyper
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15• Ikeda, R., 2 authors, Kodama, T., 10 authors, 2022, ApJ, 933, 11,”High-resolution ALMA Study of CO J = 2–1 Line and Dust Continuum Emissions in Cluster
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”Environmental Impacts on the Rest-frame UV Size and Morphology of Star-forming Galaxies
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