Free Access
Table 3.
Sensitivity of MIRI filters in 10 ks at S/N = 10 (Col. 2) and the Cosmic Evolution Early Release Science Survey (CEERS, Finkelstein et al. 2017, Col. 3).
| Sensitivity of MIRI filters | ||
|---|---|---|
| Filter | Sensitivity at S/N = 10 | CEERS |
| (μJy) | (μJy) | |
| (1) | (2) | (3) |
| F560 | 0.13 | |
| F770 | 0.24 | 0.23 |
| F1000W | 0.52 | 0.43 |
| F1130W | 1.22 | |
| F1280W | 0.92 | 0.7 |
| F1500W | 1.45 | 1.1 |
| F1800W | 2.97 | 2.5 |
| F2100W | 5.14 | 2.75 |
| F2550W | 17.3 | |
Notes. (1) MIRI filters; (2) Detection limit at S/N = 10 in 10 ks; (3) 5σ sensitivity for CEERS program.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.