( en | de | ru )

 

Disambiguation of "Ouchi, Masami"

Author of the publication

copydeleteadd this publication to your clipboard
GOLDRUSH. II. Clustering of Galaxies at $z4-6$ Revealed with the Half-Million Dropouts Over the 100 deg$^2$ Area Corresponding to 1 Gpc$^3$

, , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1704.06535Comment: 31 pages, 25 figures, submitted to a special issue of PASJ.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

Masami Th Nagatomo

Luise Masami Schmidt

 

Other publications of authors with the same name

Ly$\alpha$ Emitters with Very Large Ly$\alpha$ Equivalent Widths, EW$_0$(Ly$\alpha$) $200-400$ \AA, at $z2$, , , , , , , , and . (2016)cite arxiv:1611.00777Comment: Accepted for publication in MNRAS; 23 pages with 16 figures.Luminous Quasars Do Not Live in the Most Overdense Regions of Galaxies at z~4, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1704.06050Comment: 14 pages, 11 figures.Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program Survey, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1704.06051Comment: 21 pages, 9 figures, 6 tables, submitted to PASJ special issue.SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1705.00733Comment: 24 pages, 11 figures, submitted to PASJ special issue.Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). X. Discovery of 35 Quasars and Luminous Galaxies at 5.7 $łe$ z $łe$ 7.0, , , , , , , , , and 37 other author(s). (2019)cite arxiv:1908.07910Comment: ApJ, in press. arXiv admin note: text overlap with arXiv:1803.01861.3D Distribution Map of HI Gas and Galaxies Around an Enormous Ly$\alpha$ Nebula and Three QSOs at $z=2.3$ Revealed by the HI Tomographic Mapping Technique, , , , , , , , , and 15 other author(s). (2019)cite arxiv:1910.02962Comment: 14 pages, 7 figures, submitted to ApJ.Average Metallicity and Star Formation Rate of Lya Emitters Probed by a Triple Narrow-Band Survey, , , , , , , , , and 2 other author(s). (2011)cite arxiv:1105.2824 Comment: 17 pages, 16 figures. Submitted to ApJ.Faint LAEs near z>4.7 CIV absorbers revealed by MUSE, , , , , , , and . (2020)cite arxiv:2001.04453Comment: 21 pages, 23 figures, 3 tables. Submitted to MNRAS.SILVERRUSH. XI. Intensity Mapping for Lya Emission Extending over $100-1000$ comoving kpc around $z\sim2-7$ LAEs with Subaru HSC-SSP and CHORUS Data, , , , , , , , , and 7 other author(s). (2021)cite arxiv:2108.09288.Gaia 400,894 QSO constraint on the energy density of low-frequency gravitational waves, , , and . (2021)cite arxiv:2105.04039Comment: Submitted to Physical Review D.