HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4
dc.creator | Viero, M. P. | |
dc.creator | Moncelsi, L. | |
dc.creator | Quadri, R. F. | |
dc.creator | Béthermin, M. | |
dc.creator | Bock, J. | |
dc.creator | Burgarella, D. | |
dc.creator | Chapman, S. C. | |
dc.creator | Clements, D. L. | |
dc.creator | Conley, A. | |
dc.creator | Conversi, L. | |
dc.creator | Duivenvoorden, S. | |
dc.creator | Dunlop, J. S. | |
dc.creator | Farrah, D. | |
dc.creator | Franceschini, A. | |
dc.creator | Halpern, M. | |
dc.creator | Ivison, R. J. | |
dc.creator | Lagache, G. | |
dc.creator | Magdis, G. | |
dc.creator | Marchetti, L. | |
dc.creator | Álvarez-Márquez, J. | |
dc.creator | Marsden, G. | |
dc.creator | Oliver, S. J. | |
dc.creator | Page, M. J. | |
dc.creator | Pérez-Fournon, I. | |
dc.creator | Schulz, B. | |
dc.creator | Scott, Douglas | |
dc.creator | Valtchanov, I. | |
dc.creator | Vieira, J. D. | |
dc.creator | Wang, L. | |
dc.creator | Wardlow, J. | |
dc.creator | Zemcov, M. | |
dc.date.accessioned | 2019-10-08T20:04:50Z | |
dc.date.available | 2019-10-08T20:04:50Z | |
dc.date.issued | 2015 | |
dc.identifier.issn | 2041-8205 | |
dc.identifier.issn | 2041-8213 | |
dc.identifier.uri | https://hdl.handle.net/1969.1/178400 | |
dc.format.extent | 1 | en |
dc.publisher | Letters of the Astrophysical Journal | |
dc.relation.ispartof | 1foldr Import 2019-10-08 Batch 1 | en |
dc.relation.uri | 10.1088/2041-8205/809/2/L22 | en |
dc.title | HERMES: CURRENT COSMIC INFRARED BACKGROUND ESTIMATES CAN BE EXPLAINED BY KNOWN GALAXIES AND THEIR FAINT COMPANIONS AT z < 4 | en |