[46] "The Halo Occupation Distribution Modeling of the X-ray Selected AGNs at 0.6 < z < 2.6 in the COSMOS field", 

         Ikeda et al., 2024, submitted to AAS journal

[45] "Chandra Survey in the AKARI North Ecliptic Pole Deep Field", 

          Miyaji and Ikeda (6/20) et al., 2024, A&A, submitted

[44] "Quasar Luminosity Function at z = 7", 

          Matsuoka and Ikeda (17/44) et al., 2023, ApJL, Volume 949, Issue 2, id.L42, 8 pp.

[43] "Combining the CLAUDS & HSC-SSP surveys: U+grizy(+YJHKs) photometry and photometric redshifts 

          for 18M galaxies in the 20 deg2 of the HSC-SSP Deep and ultraDeep fields", 

          Desprez and Ikeda (12/24) et al., 2023, A&A, Volume 670, id.A82, 25 pp.

[42] "Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0", 

          Matsuoka and Ikeda (17/44) et al., 2022, ApJ, Volume 259, Issue 1, id.18, 19 pp.

[41] "Third Data Release of the Hyper Suprime-Cam Subaru Strategic Program", 

          Aihara and Ikeda (12/67) et al., 2022, PASJ, Volume 74, Issue 2, pp.247-272

[40] "The evolution of merger fraction of galaxies at z < 0.6 depending on the star formation  

          mode in the AKARI NEP Wide field", 

          Kim and Ikeda (16/22) et al., 2021, MNRAS, Volume 507, Issue 3, pp.3113-3124

[39] "Optically-detected galaxy cluster candidates in the  AKARI  North Ecliptic Pole field 

          based on photometric redshift from Subaru Hyper Suprime-Cam", 

          Huang and Ikeda (8/26) et al., 2021, MNRAS, Volume 506, Issue 4, pp.6063-6080

[38] "Hyper Suprime-Cam Legacy Archive", 

          Tanaka and Ikeda (2/8) et al., 2021, PASJ,  Volume 73, Issue 3

[37] "Identification of AKARI infrared sources by the Deep HSC Optical Survey: 

        construction of a new band-merged catalogue in the North Ecliptic Pole Wide field", 

          Kim and Ikeda (4/24) et al., 2021, MNRAS, Volume 500, Issue 3

[36] "CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview", 

          Inoue and Ikeda (13/31) et al., 2020, PASJ, psaa100

[35] "The Faint End of the Quasar Luminosity Function at  z∼5  from the Subaru Hyper Suprime-Cam Survey", 

          Niida and Ikeda (3/20) et al., 2020, ApJ, 904, 89

[34] "Extinction-free Census of AGNs in the AKARI/IRC North Ecliptic Pole Field from 23-band Infrared Photometry from Space Telescopes", 

         Wang and Ikeda (12/24) et al., 2020, MNRAS, Volume 499, Issue 3

[33] "A high redshift population of galaxies at the North Ecliptic Pole: unveiling the main sequence of dusty galaxies", 

         Barrufet and Ikeda (16/19) et al., 2020, A&A, 641, 129

[32] " Search for Optically Dark Infrared Galaxies without Counterparts of Subaru Hyper Suprime-Cam in the AKARI   

         North Ecliptic Pole Wide Survey Field", 

         Toba and Ikeda (12/28) et al., 2020, ApJ, 899, 35

[31] " Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). III. Discovery of a z = 4.72 Radio  

         Galaxy with Lyman Break Technique", 

         Yamashita and Ikeda (3/20) et al., 2020, AJ, 160, 60

[30] "Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 ≤ z ≤ 7.0", 

         Matsuoka and Ikeda (16/46) et al., 2019, ApJ, 883, 183

[29] "A Catastrophic Failure to Build a Massive Galaxy around a Supermassive Black Hole at z = 3.84",  

         Schramm and Ikeda (7/9) et al., 2019, ApJ, 881, 145

[28] "Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program",

          Aihara and Ikeda (15/64) et al., 2019, PASJ, 71, 114

[27] "Infrared luminosity functions based on 18 mid-infrared bands: revealing cosmic star formation history with AKARI 

         and Hyper Suprime-Cam,"  

        Goto and Ikeda (24/24) et al., 2019, PASJ, 71, 30 

[26] "Discovery of the First Low-Luminosity Quasar at z > 7", 

         Matsuoka and Ikeda (16/49) et al., 2018, ApJL, 872, 2

[25] "Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). V.

         Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6",

         Matsuoka and Ikeda (17/47) et al., 2018, ApJ, 869, 150

[24] "A Wide and Deep Exploration of Radio Galaxies with the Subaru HSC (WERGS).  I: the Optical Counterparts of   

         FIRST Radio Sources", 

         Yamashita and Ikeda (5/15) et al., 2018, ApJ, 866, 140

[23] "The mass-metallicity relation of high-z type-2 active galactic nuclei", 

         Matsuoka and Ikeda (8/8) et al., 2018, A&A, 616, 4

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

         Matsuoka and Ikeda (16/53) et al., 2018, ApJs, 237S, 5M

[21] "Hyper Suprime-Cam: System design and verification of image quality",

          Miyazaki and Ikeda (8/85) et al., 2018, PASJ, 70S, 1M

[20] "The Hyper Suprime-Cam Software Pipeline",

         Bosch and Ikeda (5/35), et al., 2018, PASJ, 70S, 5B

[19] "Clustering of quasars in a wide luminosity range at redshift 4 with  Subaru Hyper Suprime-Cam wide field imaging",

        He and Ikeda (6/28), et al., 2018, PASJ, 70S, 33H

[18] "The Quasar Luminosity Function at Redshift 4 with Hyper Suprime-Cam Wide Survey",

         Akiyama and Ikeda (3/27), et al., 2018, PASJ, 70S, 34A

[17] "Subaru high-z exploration of low-luminosity quasars (SHELLQs).  II. Discovery of 32 Quasars and Luminous 

       Galaxies at 5.7 < z < 6.8",  

        Matsuoka and Ikeda (17/46), et al., 2018, PASJ, 70S, 35M

[16] "The Hyper Suprime-Cam SSP Survey: Overview and Survey Design",

          Aihara and Ikeda (38/143), et al., 2018, PASJ, 70S, 4A

[15] "First Data Release of the Hyper Suprime-Cam Subaru Strategic Program",

          Aihara and Ikeda (8/107), et al., 2018, PASJ, 70S, 8A

[14] "An Optically Faint Quasar Survey at z~5 in the CFHTLS Wide Field:  Estimates of the Black Hole Masses and  

       Eddington Ratios", 

         Ikeda et al., 2017, ApJ, 846, 57

[13] "Clustering of infrared-bright dust-obscured galaxies revealed  by the Hyper Suprime-Cam and WISE",

         Toba and Ikeda (6/23), et al., 2017, ApJ, 835, 36

[12] "Near-infrared spectroscopy of nearby Seyfert galaxies: Is there evidence for the shock excitation in narrow-line  

         regions? ", 

         Terao and Ikeda (7/8), et al., 2016, ApJ, 833, 190

[11] "Revisiting the Completeness and the Luminosity Function in High-Redshift Low-Luminosity Quasar Surveys",

          Niida and Ikeda (3/7), et al., 2016, ApJ, 832, 208

[10] "Subaru high-z exploration of low-luminosity quasars (SHELLQs). I. Discovery of 15 quasars and bright galaxies 

         at 5.7 < z < 6.9", 

         Matsuoka and Ikeda (18/39), et al., 2016, ApJ, 828, 26

[9]  "An Effective Selection Method for Low-Mass Active Black Holes and First Spectroscopic Identification",

        Morokuma and Ikeda (12/16), et al. 2016, PASJ, 68, 40

[8]  "The Quasar-LBG Two-Point Angular Cross-Correlation Function at z〜4  in the COSMOS Field",

        Ikeda et al., 2015, ApJ, 809, 138

[7]  "Constraints on the Faint End of the Quasar Luminosity Function at z〜5 in the COSMOS Field",

        Ikeda et al., 2012, ApJ, 756, 160

[6]  "Near-infrared spectroscopy of a nitrogen-loud quasar SDSS J1707+6443",

        Araki and Ikeda (6/9), et al., 2012, A&A, 543, 143

[5]  "Evolution of the Quasar Luminosity Function over 3 < z < 5 in the COSMOS Survey" ,

        Masters and Ikeda (11/13), et al., 2012, ApJ, 755, 169

[4]  "Dissecting Photometric Redshift for AGN using XMM- and Chandra- COSMOS Samples" ,

        Mara and Ikeda (35/66), et al., 2011, ApJ, 742, 61

[3] "The Population of High-redshift Active Galactic Nuclei in the Chandra-COSMOS Survey",

       Civao and Ikeda (11/22), et al, 2011, ApJ, 741, 91

[2]  "Spectropolarimetric Evidence for Radiatively Inefficient Accretion in an Optically Dull Active Galaxy",

         Trump and Ikeda (3/12), et al., 2011, ApJ, 732, 23

[1]  "Probing the Faint End of the Quasar Luminosity Function at z〜4 in the COSMOS Field",

        Ikeda et al. 2011, ApJ, 728, L25