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| 1 | Zinc finger nuclease-mediated transgene deletion显示文摘 | Joseph F. Petolino Andrew Worden Krisi Curlee James Connell Tonya L. Strange Moynahan Cory Larsen Sean Russell | 2010 | Plant Molecular Biology2010，，6： | 1 |
| 2 | Restoring coastal plants to improve global carbon storage:reaping what we sow 显示文摘 | IRVING A D CONNELL S D RUSSELL B D | 2011 | Plos One2011，6，18： | 1 |
| 3 | The direct effects of increasing CO2 and temperature on non-calcifying organisms : Increasing the potential for phase shifts in kelp forests 显示文摘 | CONNELL S D RUSSELL B D | 2010 | Proceedings of the Royal Society B: Biological Sciences2010，277，1686： | 1 |
| 4 | Spontaneous clearance of hepatitis C infection after liver transplantation from IL28B rs12979860 CC donors显示文摘 | Jun Liong Chin Ross Mac Nicholas Jennifer Russell Michael Carr Jeff Connell Stephen Stewart P. Aiden McCormick | 2012 | European Journal of Gastroenterology & Hepatology2012，，9： | 1 |
| 5 | Electron, proton,and ultraviolet radiation effects on thermo physicalproperties of polymeric films显示文摘 | Russell D A Connell J W Fogdall L B | 2002 | Journal of Spacecraftand Rockets2002，39，6： | 1 |
| 6 | The LysR-type transcriptional regulator VirR is required for expression of the virulence gene vapA of Rhodococcus equi ATCC 33701 显示文摘 | RUSSELL D A BYRNE G A O'CONNELL E P | 2004 | J Baeteriol2004，186，17： | 1 |
| 7 | Towards Complex Team Behaviour in Multi- Agent Systems显示文摘 | Andrew Lucas Ralph R? nnquist Nick Howden Andrew Hodgson Russell Connell Geoffrey White Dr Jonathan Vaughan | 2001 | Proceedings of SimTecT 2001 Canberra Australia2001，，5： | 1 |
| 8 | Economic and environmental threats of alien plant,animal,and microbe invasions显示文摘 | Pimentel D McNair S Janecka J Wightman J Simmonds C O'Connell C Wong E Russel L Zern J Aquino T and Tsomondo T | | 0，，： | 1 |
| 9 | Fine-scale estimation of outcrossing in western redcedar with microsatellite assay of bulked DNA显示文摘 | O'Connell L M Russell J Ritland K | | 0，，： | 1 |
| 10 | Recovering a lost baseline: missing kelp forests from a metropolitan coast显示文摘 | Connell S D Russell B D Turner D J | 2005 | Marine Ecology Progress Series2005，360，： | 1 |
| 11 | Galaxy formation in the reionization epoch as hinted by WideField Camera 3 observations of the Hubble Ultra Deep Field显示文摘We present a large sample of candidate galaxies at z ≈ 7 - 10, selected in the Hubble Ultra Deep Field using the new observations of the Wide Field Camera 3 that was recently installed on the Hubble Space Telescope. Our sample is composed of 20 z850-dropouts (four new discoveries), 15 Y105-dropouts (nine new discoveries) and 20 J125-dropouts (all new discoveries). The surface densities of the z850-dropouts are close to what was predicted by earlier studies, however, those of the Y105- and J125-dropouts are quite unexpected. While no Y105-or J125-dropouts have been found at AB ≤ 28.0 mag, their surface densities seem to increase sharply at fainter levels. While some of these candidates seem to be close to foregroundgalaxies and thus could possibly be gravitationally lensed, the overall surface densities after excluding such cases are still much higher than what would be expected if the luminosity function does not evolve from z ~ 7 to 10. Motivated by such steep increases, we tentatively propose a set of Schechter function parameters to describe the luminosity functions at z ≈ 8 and 10. As compared to their counterpart at z ≈ 7, here L * decreases by a factor of ~ 6.5 and Φ* increases by a factor of 17-90. Although such parameters are not yet demanded by the existing observations, they are allowed and seem to agree with the data better than other alternatives. If these luminosity functions are still valid beyond our current detection limit, this would imply a sudden emergence of a large number of low-luminosity galaxies when looking back in time to z ≈ 10, which, while seemingly exotic, would naturally fit in the picture of the cosmic hydrogen reionization. These early galaxies could easily account for the ionizing photon budget required by the reionization, and they would imply that the global star formation rate density might start from a very high value at z ≈ 10, rapidly reach the minimum at z ≈ 7, and start to rise again towards z ≈ 6. In this scenario, the majority of the stellar mass that the universe assembled through the reionization epoch seems still undetected by current observations at z ≈ 6. | Hao-Jing Yan Rogier A. Windhorst Nimish E Hathi Seth H. Cohen Russell E.Ryan Robert W. O'Connell Patrick J. McCarthy | 2010 | Research in Astronomy and Astrophysics2010，10，9： | 0 |
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