- UHRA Home
- Browsing by Author
Browsing by Author "Pearson, W. J."
Now showing items 1-2 of 2
-
The bright end of the infrared luminosity functions and the abundance of hyperluminous infrared galaxies
Wang, L.; Gao, F.; Best, P. N.; Duncan, K.; Hardcastle, M. J.; Kondapally, R.; Malek, K.; McCheyne, I.; Sabater, J.; Shimwell, T.; Tasse, C.; Bonato, M.; Bondi, M.; Cochrane, R. K.; Farrah, D.; Gurkan, G.; Haskell, P.; Pearson, W. J.; Prandoni, I.; Rottgering, H. J. A.; Smith, D. J. B.; Vaccari, M.; Williams, W. L. (2021-04-07)We provide the most accurate estimate yet of the bright end of the infrared (IR) luminosity functions (LFs) and the abundance of hyperluminous IR galaxies (HLIRGs) with IR luminosities > 10^13 L_solar, thanks to the ... -
Main sequence of star forming galaxies beyond the Herschel confusion limit
Pearson, W. J.; Wang, L.; Hurley, P. D.; Małek, K.; Buat, V.; Burgarella, D.; Farrah, D.; Oliver, S. J.; Smith, D. J. B.; Tak, F. F. S. van der (2018-07-30)Context. Deep far-infrared (FIR) cosmological surveys are known to be affected by source confusion, causing issues when examining the main sequence (MS) of star forming galaxies. In the past this has typically been partially ...