Publication data of Toshikawa, Jun: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20122014201620182020202220240100200300400500600
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201220142016201820202022202404812162000.81.62.43.24
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion201220142016201820202022202402468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersNarrowband Imaging of a z=3.24 Protocluster: Insights from [O III] Emitting GalaxiesNarrowband Imaging of a z=3.24 Protocluster: Insights from [O III] Emitting …A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X. The Massive and Passive Nature of Radio Galaxies at z ∼ 4A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X.…Nature versus Nurture: Revisiting the Environmental Impact on Star Formation Activities of GalaxiesNature versus Nurture: Revisiting the Environmental Impact on Star Formati…Extended Lyman-alpha emission from a high-z DLA at z=3.115Accelerated Galaxy Growth and Environmental Quenching in a Protocluster at $z$ = 3.24Accelerated Galaxy Growth and Environmental Quenching in a Protocluster a…A Detailed Study of Massive Galaxies in a Protocluster at $z$ = 3.13Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program SurveyEnhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on …How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massive Protocluster at $Z = 3.13$How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massi…The redshift selected sample of long gamma-ray burst host galaxies: the overall metallicity distribution at $z < 0.4$The redshift selected sample of long gamma-ray burst host galaxies: the over…The Subaru HSC Galaxy Clustering with Photometric Redshift. I. Dark Halo Masses versus Baryonic Properties of Galaxies at 0.3 ≤ z ≤ 1.4The Subaru HSC Galaxy Clustering with Photometric Redshift. I. Dark Halo Ma…A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protoclu…The Galaxy–Halo Connection in High-redshift Universe: Details and Evolution of Stellar-to-halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep FieldsThe Galaxy–Halo Connection in High-redshift Universe: Details and Evolution …A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of …A Systematic Survey of Protoclusters at $zsim3mathrm{-}6$ in the CFHTLS Deep FieldsA Systematic Survey of Protoclusters at $zsim3mathrm{-}6$ in the CFHTLS …Discovery of a protocluster at z~6A New Constraint on Reionization from Evolution of the Ly$alpha$ Luminosity Function at $zsim6-7$ Probed by a Deep Census of $z=7.0$ Ly$alpha$ Emitter Candidates to 0.3 $L^*$A New Constraint on Reionization from Evolution of the Ly$alpha$ Luminosity…GOLDRUSH. II. Clustering of galaxies at z ∼ 4–6 revealed with the half-million dropouts over the 100 deg2 area corresponding to 1 Gpc3GOLDRUSH. II. Clustering of galaxies at z ∼ 4–6 revealed with the half-million …Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey DataEvolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analy…Completing the Census of Ly-alpha Emitters at the Reionization Epoch20122014201620182020202220240100200300400500600
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Narrowband Imaging of a z=3.24 Protocluster: Insights from [O III] Emitting GalaxiesNarrowband Imaging of a z=3.24 Protocluster: Insights from [O III] Emitting …A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X. The Massive and Passive Nature of Radio Galaxies at z ∼ 4A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). X.…Nature versus Nurture: Revisiting the Environmental Impact on Star Formation Activities of GalaxiesNature versus Nurture: Revisiting the Environmental Impact on Star Formati…Extended Lyman-alpha emission from a high-z DLA at z=3.115Accelerated Galaxy Growth and Environmental Quenching in a Protocluster at $z$ = 3.24Accelerated Galaxy Growth and Environmental Quenching in a Protocluster a…A Detailed Study of Massive Galaxies in a Protocluster at $z$ = 3.13Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program SurveyEnhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on …How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massive Protocluster at $Z = 3.13$How Do Galaxies Trace a Large-scale Structure? A Case Study around a Massi…The redshift selected sample of long gamma-ray burst host galaxies: the overall metallicity distribution at $z < 0.4$The redshift selected sample of long gamma-ray burst host galaxies: the over…The Subaru HSC Galaxy Clustering with Photometric Redshift. I. Dark Halo Masses versus Baryonic Properties of Galaxies at 0.3 ≤ z ≤ 1.4The Subaru HSC Galaxy Clustering with Photometric Redshift. I. Dark Halo Ma…A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protoclu…The Galaxy–Halo Connection in High-redshift Universe: Details and Evolution of Stellar-to-halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep FieldsThe Galaxy–Halo Connection in High-redshift Universe: Details and Evolution …A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of ~900A at z=6.5: A Candidate of Population III-dominated Galaxy?A Ly-alpha Emitter with an Extremely Large Rest-frame Equivalent Width of …A Systematic Survey of Protoclusters at $zsim3mathrm{-}6$ in the CFHTLS Deep FieldsA Systematic Survey of Protoclusters at $zsim3mathrm{-}6$ in the CFHTLS …Discovery of a protocluster at z~6A New Constraint on Reionization from Evolution of the Ly$alpha$ Luminosity Function at $zsim6-7$ Probed by a Deep Census of $z=7.0$ Ly$alpha$ Emitter Candidates to 0.3 $L^*$A New Constraint on Reionization from Evolution of the Ly$alpha$ Luminosity…GOLDRUSH. II. Clustering of galaxies at z ∼ 4–6 revealed with the half-million dropouts over the 100 deg2 area corresponding to 1 Gpc3GOLDRUSH. II. Clustering of galaxies at z ∼ 4–6 revealed with the half-million …Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey DataEvolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analy…Completing the Census of Ly-alpha Emitters at the Reionization Epoch20122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2012201420162018202020222024020406080