The SCUBA-2 Cosmology Legacy Survey : the submillimetre properties of Lyman-break galaxies at z = 3-5
                
    Coppin, Kristen, Geach, J.E., Almaini, O., Arumugam, V., Dunlop, James S., Hartley, W.G., Ivison, Rob J., Simpson, C.J., Smith, Daniel, Swinbank, A.M., Blain, Andrew W., Bourne, N., Bremer, M., Conselice, C., Harrison, C. M., Mortlock, A., Chapman, S.C., Davies, L.J.M., Farrah, D., Gibb, A., Jenness, T., Karim, A., Knudsen, K., Ibar, E., Michalowski, M. J., Peacock, J.A., Rigopoulou, D., Robson, E.I., Scott, D., Stevens, J. and van der Werf, P.
  
(2015)
The SCUBA-2 Cosmology Legacy Survey : the submillimetre properties of Lyman-break galaxies at z = 3-5.
    Monthly Notices of the Royal Astronomical Society (MNRAS), 446 (2).
     pp. 1293-1304.
     ISSN 0035-8711
  
  
              
            
We present detections at 850 μm of the Lyman-break galaxy (LBG) population at z ≈ 3, 4, and 5 using data from the Submillimetre Common User Bolometer Array 2 Cosmology Legacy Survey in the United Kingdom Infrared Deep Sky Survey ‘Ultra Deep Survey’ field
| Item Type | Article | 
|---|---|
| Identification Number | 10.1093/mnras/stu2185 | 
| Additional information | This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record [MNRAS (January 11, 2015) 446(2): 1293-1304 is available online at: DOI: 10.1093/mnras/stu2185, first published online November 19, 2014. | 
| Keywords | galaxies: evolution - galaxies: formation, galaxies: high-redshift, galaxies: star formation, submillimetre: galaxies, ultraviolet: galaxies | 
| Date Deposited | 15 May 2025 12:53 | 
| Last Modified | 22 Oct 2025 19:25 | 
- 
            picture_as_pdf 
- Coppin_et_al_Accepted_Manuscript.pdf
- 
            subject 
- Submitted Version
Share this file
            
				Downloads
			  
			  ?
                    Total file downloads from UHRA since January 2020. For more information on metrics see the IRUS guide.