Table 3
The ρUV and ρSFR for the different dropout samples.
| Sample | Integral limit | ρUV [1026 | ρSFR |
| erg s-1 Hz-1 Mpc-3]a | [M⊙ yr-1 Mpc-3]a,b | ||
|
|
|||
| u |
|
1.73 ± 0.09 |
|
| Schechter | 4.41 | 0.154 | |
| g |
|
1.07 ± 0.03 |
|
| Schechter | 2.62 | 0.092 | |
| r |
|
0.80 ± 0.03 |
|
| Schechter | 2.19 | 0.038 | |
Notes. The first lines for each sample correspond to sums over the
data points down to 
while the second lines
correspond to integrals over the best-fit Schechter functions.
Due to uncertainties in the redshift distributions, there is an additional error component of ~7%, ~5%, and ~4% in the estimated ρUV and ρSFR values for the u-, g-, and r-dropout samples, respectively.
Corrected for dust extinction using the luminosity dependent correction factors from Bouwens et al. (2009). Systematic errors as a result from the age-dust degeneracy are also included.
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