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Jun Toshikawa

Identifiers

  • name variant Jun Toshikawa 0.60 · backfill

Papers (25)

  1. EPISODE II: Variability in the CO and H$_2$O rovibrational absorption lines in a periodically variable protostar EC 53 astro-ph.GA · 2026 · author #19
  2. The Evolution of the SFR-M_* relation at 0.1<z<4: Environmental and Morphological Dependencies astro-ph.GA · 2026 · author #3
  3. How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at $z=3.13$ astro-ph.GA · 2019 · author #4
  4. The brightest UV-selected galaxies in protoclusters at $z\sim4$: Ancestors of Brightest Cluster Galaxies? astro-ph.GA · 2019 · author #3
  5. Environmental impacts on molecular gas in protocluster galaxies at z~2 astro-ph.GA · 2019 · author #14
  6. Large Scale Environment of a $z=6.61$ Luminous Quasar Probed by Ly$\alpha$ Emitters and Lyman Break Galaxies astro-ph.GA · 2018 · author #11
  7. SILVERRUSH. VII. Subaru/HSC Identifications of 42 Protocluster Candidates at z~6-7 with the Spectroscopic Redshifts up to z=6.574: Implications for Cosmic Reionization astro-ph.GA · 2018 · author #5
  8. Minor Contribution of Quasars to Ionizing Photon Budget at z~6: Update on Quasar Luminosity Function at the Faint-end with Subaru/Suprime-Cam astro-ph.GA · 2017 · author #18
  9. GOLDRUSH. III. A Systematic Search of Protoclusters at $z\sim4$ Based on the $>100\,\mathrm{deg^2}$ Area astro-ph.GA · 2017 · author #1
  10. GOLDRUSH. II. Clustering of Galaxies at $z\sim 4-6$ Revealed with the Half-Million Dropouts Over the 100 deg$^2$ Area Corresponding to 1 Gpc$^3$ astro-ph.GA · 2017 · author #8
  11. Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program Survey astro-ph.GA · 2017 · author #15
  12. Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at $z \sim 4-7$ Derived with the Half-Million Dropouts on the 100 deg$^2$ Sky astro-ph.GA · 2017 · author #4
  13. A New Constraint on Reionization from Evolution of the Ly$\alpha$ Luminosity Function at $z\sim6-7$ Probed by a Deep Census of $z=7.0$ Ly$\alpha$ Emitter Candidates to 0.3 $L^*$ astro-ph.GA · 2017 · author #10
  14. The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields astro-ph.GA · 2016 · author #3
  15. The redshift selected sample of long gamma-ray burst host galaxies: the overall metallicity distribution at $z < 0.4$ astro-ph.HE · 2016 · author #9
  16. A Systematic Survey of Protoclusters at $z\sim3\mathrm{-}6$ in the CFHTLS Deep Fields astro-ph.GA · 2016 · author #1
  17. The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z \sim 2$ and their host haloes based upon HOD modelling astro-ph.GA · 2016 · author #4
  18. The very wide-field $gzK$ galaxy survey -- I. Details of the clustering properties of star-forming galaxies at $z \sim 2$ astro-ph.GA · 2016 · author #3
  19. 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 Data astro-ph.GA · 2015 · author #18
  20. The Subaru high-z quasar survey: discovery of faint z~6 quasars astro-ph.GA · 2014 · author #7
  21. A First Site of Galaxy Cluster Formation: Complete Spectroscopy of a Protocluster at $z=6.01$ astro-ph.GA · 2014 · author #1
  22. Extended Lyman-alpha emission from a high-z DLA at z=3.115 astro-ph.CO · 2013 · author #6
  23. 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? astro-ph.CO · 2012 · author #3
  24. Discovery of a protocluster at z~6 astro-ph.CO · 2012 · author #1
  25. Completing the Census of Ly-alpha Emitters at the Reionization Epoch astro-ph.CO · 2011 · author #19

Mentions

  • 2606.06628 #19 · arxiv_oai · confidence 0.70 Jun Toshikawa
  • 1511.07873 #18 · backfill · confidence 0.70 Jun Toshikawa
  • 1410.7401 #7 · backfill · confidence 0.70 Jun Toshikawa
  • 1407.1851 #1 · backfill · confidence 0.70 Jun Toshikawa
  • 1311.5534 #6 · backfill · confidence 0.70 Jun Toshikawa
  • 1210.4933 #3 · backfill · confidence 0.70 Jun Toshikawa
  • 1203.1326 #1 · backfill · confidence 0.70 Jun Toshikawa
  • 1104.2330 #19 · backfill · confidence 0.70 Jun Toshikawa

Frequent Coauthors