activity
19992026
most citedDetection of an ultra-bright submillimeter galaxy in the Subaru/XMM-Newton Deep Field using AzTEC/ASTE

52 citations · 180 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

ALMA 2D super-resolution imaging survey of Ophiuchus Class I/flat spectrum/II disks. II. Statistical analysis of stellar and disk properties

Ayumu Shoshi, Masayuki Yamaguchi, Takayuki Muto +5

We present a statistical study of stellar and dust disk properties for young stellar objects in the Ophiuchus star-forming region. Building on our previous paper (Shoshi et al. 202…

astro-ph.GA2019★ 32 cited

Testing Star Formation Laws on Spatially Resolved Regions in a Starburst Galaxy

Piyush Sharda, Elisabete da Cunha, Christoph Federrath +6

We probe the star formation properties of the gas in AzTEC-1 in the COSMOS field, one of the best resolved and brightest starburst galaxies at , forming stars at a r…

astro-ph.GA2016★ 16 cited

SXDF-ALMA 2 Arcmin^2 Deep Survey: Resolving and Characterizing the Infrared Extragalactic Background Light Down to 0.5 mJy

Yuki Yamaguchi, Yoichi Tamura, Kotaro Kohno +22

We present a multi-wavelength analysis of five submillimeter sources (S_1.1mm = 0.54-2.02 mJy) that were detected during our 1.1-mm-deep continuum survey in the SXDF-UDS-CANDELS fi…

astro-ph.CO2010★ 52 cited

Detection of an ultra-bright submillimeter galaxy in the Subaru/XMM-Newton Deep Field using AzTEC/ASTE

S. Ikarashi, K. Kohno, J. E. Aguirre +40

We report the detection of an extremely bright (37 mJy at 1100 m and 91 mJy at 880 m) submillimeter galaxy (SMG), AzTEC-ASTE-SXDF1100.001 (hereafter referred to a…

astro-ph.CO2010★ 28 cited

Unveiling the Nature of Submillimeter Galaxy SXDF850.6

B. Hatsukade, D. Iono, T. Yoshikawa +22

We present an 880 micron Submillimeter Array (SMA) detection of the submillimeter galaxy SXDF850.6. SXDF850.6 is a bright source (S(850 micron) = 8 mJy) detected in the SCUBA Half…

astro-ph1999★ 52 cited

Sensitive Radio Observations of High Redshift Dusty QSOs

M. S. Yun, C. L. Carilli, R. Kawabe +3

We present sensitive radio continuum imaging at 1.4 GHz and 4.9 GHz of seven high redshift QSOs selected for having a 240 GHz continuum detection, which is thought to be thermal du…