ZFOURGE/CANDELS: ON THE EVOLUTION OF M * GALAXY PROGENITORS FROM z = 3 TO 0.5
dc.creator | Papovich, C. | |
dc.creator | Labbé, I. | |
dc.creator | Quadri, R. | |
dc.creator | Tilvi, V. | |
dc.creator | Behroozi, P. | |
dc.creator | Bell, E. F. | |
dc.creator | Glazebrook, K. | |
dc.creator | Spitler, L. | |
dc.creator | Straatman, C. M. S. | |
dc.creator | Tran, K.-V. | |
dc.creator | Cowley, M. | |
dc.creator | Davé, R. | |
dc.creator | Dekel, A. | |
dc.creator | Dickinson, M. | |
dc.creator | Ferguson, H. C. | |
dc.creator | Finkelstein, S. L. | |
dc.creator | Gawiser, E. | |
dc.creator | Inami, H. | |
dc.creator | Faber, S. M. | |
dc.creator | Kacprzak, G. G. | |
dc.creator | Kawinwanichakij, L. | |
dc.creator | Kocevski, D. | |
dc.creator | Koekemoer, A. | |
dc.creator | Koo, D. C. | |
dc.creator | Kurczynski, P. | |
dc.creator | Lotz, J. M. | |
dc.creator | Lu, Y. | |
dc.creator | Lucas, R. A. | |
dc.creator | McIntosh, D. | |
dc.creator | Mehrtens, N. | |
dc.creator | Mobasher, B. | |
dc.creator | Monson, A. | |
dc.creator | Morrison, G. | |
dc.creator | Nanayakkara, T. | |
dc.creator | Persson, S. E. | |
dc.creator | Salmon, B. | |
dc.creator | Simons, R. | |
dc.creator | Tomczak, A. | |
dc.creator | van Dokkum, P. | |
dc.creator | Weiner, B. | |
dc.creator | Willner, S. P. | |
dc.date.accessioned | 2019-10-09T18:50:22Z | |
dc.date.available | 2019-10-09T18:50:22Z | |
dc.date.issued | 2015 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.issn | 1538-4357 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/181207 | |
dc.format.extent | 1 | en |
dc.publisher | The Astrophysical Journal | |
dc.relation.ispartof | 1foldr Import 2019-10-08 Batch 6 | en |
dc.relation.uri | 10.1088/0004-637X/803/1/26 | en |
dc.title | ZFOURGE/CANDELS: ON THE EVOLUTION OF M * GALAXY PROGENITORS FROM z = 3 TO 0.5 | en |