Table 4
Physical parameters for MUSE C III] emitters in the HDFS and udf-10 .
| ID | log LUV | log SFR | log M⋆ | log Age | A V | β | log ne |
| (L⊙) | (M⊙ yr-1) | (M⊙) | (yr) | (mag) | (cm-3) | ||
|
|
|||||||
| HDFS-74 | 10.0 | 0.072+0.000-0.000 | 8.07+0.000-0.000 | 7.79+0.000-0.000 | 0.088+0.000-0.000 | ... | ... |
| HDFS-87 | 10.2 | 0.212+0.000-0.000 | 8.21+0.000-0.000 | 7.79+0.000-0.000 | 0.088+0.000-0.000 | ... | ... |
| HDFS-97 | 9.71 | –0.068+0.045-0.035 | 8.73+0.155-0.290 | 8.69+0.195-0.230 | 0.013+0.025-0.000 | ... | 3.0 ± 0.90 |
| HDFS-100 | 9.41 | 0.422+0.390-0.505 | 9.71+0.205-0.220 | 9.08+0.205-0.360 | 1.04+0.575-0.625 | ... | 4.4 ± 0.60 |
| HDFS-126 | 9.92 | 0.152+0.000-0.080 | 8.26+0.000-0.000 | 7.92+0.000-0.000 | 0.038+0.000-0.000 | –1.99 ± 0.004 | ... |
| UDF10-22 | 11.2 | 1.43+0.000-0.000 | 10.1+0.000-0.010 | 8.43+0.000-0.000 | 0.463+0.000-0.000 | –1.18 ± 0.035 | 2.9 ± 0.47 |
| UDF10-41 | 10.4 | 0.637+0.020-0.045 | 9.08+0.050-0.050 | 8.36+0.060-0.090 | 0.138+0.050-0.025 | –1.61 ± 0.038 | <3 |
| UDF10-42 | 10.2 | 0.427+0.370-0.000 | 9.06+0.000-0.140 | 8.60+0.000-0.610 | 0.038+0.375-0.000 | –1.97 ± 0.038 | 3.5 ± 0.31 |
| UDF10-51 | 10.2 | 0.397+0.000-0.000 | 9.30+0.000-0.000 | 8.80+0.000-0.000 | 0.038+0.000-0.000 | –1.91 ± 0.110 | 3.9 ± 0.20 |
| UDF10-64 | 10.0 | 0.202+0.035-0.010 | 8.67+0.035-0.000 | 8.41+0.000-0.020 | 0.038+0.025-0.000 | –2.34 ± 0.058 | ... |
| UDF10-99 | 10.0 | 0.177+0.000-0.000 | 8.09+0.000-0.000 | 7.55+0.000-0.000 | 0.363+0.000-0.000 | –1.69 ± 0.421 | ... |
| UDF10-164 | 9.36 | –0.413+0.015-0.000 | 8.42+0.000-0.315 | 8.69+0.000-0.225 | 0.013+0.000-0.000 | –2.93 ± 0.474 | 3.4 ± 0.56 |
| UDF10-231 | 9.34 | –0.388+0.070-0.055 | 8.07+0.195-0.250 | 8.46+0.145-0.535 | 0.038+0.075-0.025 | –2.50 ± 0.532 | ... |
| UDF10-6664 | 10.7 | 0.882+0.000-0.005 | 9.02+0.000-0.000 | 8.01+0.000-0.000 | 0.713+0.000-0.000 | –1.84 ± 0.091 | ... |
| UDF10-6668 | 9.73 | –0.043+0.110-0.000 | 8.79+0.000-0.090 | 8.69+0.000-0.085 | 0.013+0.025-0.000 | –2.23 ± 0.091 | 2.9 ± 0.32 |
| UDF10-6670 | 9.75 | –0.023+0.000-0.080 | 8.89+0.000-0.160 | 8.88+0.000-0.195 | 0.113+0.000-0.100 | –2.19 ± 0.316 | <3 |
| UDF10-6674 | 10.2 | 0.047+0.255-0.055 | 8.52+0.150-0.055 | 8.41+0.195-0.325 | 0.038+0.175-0.025 | –1.22 ± 0.360 | 4.1 ± 0.78 |
Notes. With the exception of ne, all parameters are derived from broadband SED fits using MAGPHYS (da Cunha et al. 2008). Ultraviolet luminosities are the unattenuated values at rest-frame 1900 Å, as measured from the best-fit MAGPHYS SED. Values and quoted uncertainties for MAGPHYS parameters (SFR, M⋆, Age, and AV) denote the median and shortest 68% confidence interval centered on the median. Star formation rates are averaged over the past 0.1 Gyr and ages are mass weighted. The value ne is the electron density measured from the ratio of C III] 1907 to 1909 Å (Osterbrock & Ferland 2006) at T = 10 000 K when the signal to noise in each of the individual components is >3σ; a measured 1907/1909 ratio in excess of the value in the low-density limit of 1.53 implies that the actual electron density is <103 cm -3.
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