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Reference93 articles.
1. Abraham, R. G., Tanvir, N. R., Santiago, B., et al. (1996). Galaxy morphology to I = 25 mag in the Hubble Deep Field. Monthly Notices of the Royal Astronomical Society, 279, L47–L52.
2. Aragón-Salamanca, A., Ellis, R. S., Couch, W. J., & Carter, D. (1993). Evidence for systematic evolution in the properties of galaxies in distant clusters. Monthly Notices of the Royal Astronomical Society, 262, 764–794.
3. Beckwith, S. V. W., Stiavelli, M., Koekemoer, A. M., et al. (2006). The Hubble Ultra Deep Field. Astronomical Journal, 132, 1729–1755.
4. Berta, S., Magnelli, B., Nordon, R., et al. (2011). Herschel/PEP dissects the cosmic infrared background. In W. Wang, J. Lu, Z. Luo, et al. (Eds.), Galaxy evolution: Infrared to millimeter wavelength perspective. Astronomical Society of the Pacific Conference Series (Vol. 446, pp. 309–314).
5. Blain, A. W., & Longair, M. S. (1993). Sub-millimetre cosmology. Monthly Notices of the Royal Astronomical Society, 264, 509–521.