| dc.contributor.author | Conselice, C. J. | en_US |
| dc.contributor.author | Bluck, A. F. L. | en_US |
| dc.contributor.author | Buitrago, F. | en_US |
| dc.contributor.author | Bauer, A. E. | en_US |
| dc.contributor.author | Grützbauch, R. | en_US |
| dc.contributor.author | Bouwens, R. J. | en_US |
| dc.contributor.author | Bevan, S. | en_US |
| dc.contributor.author | Mortlock, A. | en_US |
| dc.contributor.author | Dickinson, M. | en_US |
| dc.contributor.author | Daddi, E. | en_US |
| dc.contributor.author | Yan, H. | en_US |
| dc.contributor.author | Scott, Douglas | en_US |
| dc.contributor.author | Chapman, S. C. | en_US |
| dc.contributor.author | Chary, R. -R | en_US |
| dc.contributor.author | Ferguson, H. C. | en_US |
| dc.contributor.author | Giavalisco, M. | en_US |
| dc.contributor.author | Grogin, N. | en_US |
| dc.contributor.author | Illingworth, G. | en_US |
| dc.contributor.author | Jogee, S. | en_US |
| dc.contributor.author | Koekemoer, A. M. | en_US |
| dc.contributor.author | Lucas, Ray A. | en_US |
| dc.contributor.author | Mobasher, B. | en_US |
| dc.contributor.author | Moustakas, L. | en_US |
| dc.contributor.author | Papovich, C. | en_US |
| dc.contributor.author | Ravindranath, S. | en_US |
| dc.contributor.author | Siana, B. | en_US |
| dc.contributor.author | Teplitz, H. | en_US |
| dc.contributor.author | Trujillo, I. | en_US |
| dc.contributor.author | Urry, M. | en_US |
| dc.contributor.author | Weinzirl, T. | en_US |
| dc.date.accessioned | 2014-03-12T19:20:49Z | |
| dc.date.available | 2014-03-12T19:20:49Z | |
| dc.date.issued | 2010-10-06 | en_US |
| dc.identifier.citation | Conselice, C. J., A. F. L. Bluck, F. Buitrago, A. E. Bauer, et al. 2010. "The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3." Monthly Notices of the Royal Astronomical Society 413:80. | en_US |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/10222/45277 | |
| dc.identifier.uri | http://dx.doi.org/10.1111/j.1365-2966.2010.18113.x | |
| dc.description.abstract | We present the details and early results from a deep near-infrared survey utilising the NICMOS instrument on the Hubble Space Telescope centred around massive M_* > 10^11 M_0 galaxies at 1.7 10^11 M_0, whereby we find an increase of a factor of eight between z = 3 and z = 1.5, demonstrating that this is an epoch when massive galaxies establish most of their mass. | en_US |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3 | en_US |
| dc.title.alternative | arXiv:1010.1164 [astro-ph] | en_US |
| dc.type | article | en_US |
| dc.identifier.volume | 413 | |
| dc.identifier.startpage | 80 | en_US |
