activity
19962009
most citedThe 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures

1.1k citations · 1.1k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2009★ 1.1k cited

The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures

D. Heath Jones, Mike A. Read, Will Saunders +30

We report the final redshift release of the 6dF Galaxy Survey, a combined redshift and peculiar velocity survey over the southern sky (|b|>10 deg). Its 136,304 spectra have yielded…

astro-ph2008★ 7 cited

Microstructure and kinematics of H2O masers in the massive star forming region IRAS 06061+2151

K. Motogi, Y. Watanabe, K. Sorai +14

We have made multi-epoch VLBI observations of H2O maser emission in the massive star forming region IRAS 06061+2151 with the Japanese VLBI network (JVN) from 2005 May to 2007 Octob…

astro-ph2007★ 12 cited

Multi-epoch VLBA observations of 3C 66A

H. -B. Cai, Z. -Q. Shen, H. Sudou +6

We present the results of six-epoch Very Long Baseline Array (VLBA) observations of 3C~66A. The high-resolution Very Long Baseline Interferometer (VLBI) maps obtained at multi-freq…

astro-ph2001★ 13 cited

Hubble Constant at Intermediate Redshift using the CO-Line Tully-Fisher Relation

Y. Tutui, Y. Sofue, M. Honma +2

We have determined distances and Hubble ratios for galaxies at intermediate redshifts, cz=about 10,000 to 35,000 km/s, by applying the CO-line Tully-Fisher relation to our 12CO (J=…

astro-ph2000★ 8 cited

CO Observations of Luminous IR Galaxies at Intermediate Redshift

Y. Tutui, Y. Sofue, M. Honma +2

We present new measurement of CO() emission from 16 luminous infrared galaxies (LIGs) at intermediate redshift (). These new…

astro-ph1996★ 7 cited

Distance Measurement of Galaxies to Redshift of 0.1 using the CO-Line Tully-Fisher Relation

Y. Sofue, F. Schoeniger, M. Honma +5

We report on the first results of a long-term project to derive distances of galaxies at cosmological distances by applying the CO-line width-luminosity relation. We have obtained…