Table 2.
Summary of the photometry and emission line fluxes used in the SED fitting analysis of the integrated E and W galaxies of SPT0311-58.
| Instrument/filter | E galaxy | W galaxy |
|---|---|---|
| WPFC3/F125W | 0.22±0.01 μJy | < 0.05 μJy |
| WPFC3/F160W | 0.35±0.01 μJy | < 0.07 μJy |
| IRAC/3.6 μm | 0.6±0.2 μJy | — |
| IRAC/4.5 μm | 0.6±0.2 μJy | — |
| MIRIM/F1000W | 1.6±0.3 μJy | 2.2±0.4 μJy |
| SPIRE/250 μm | 2.5±0.8 mJy | 27±9 mJy |
| SPIRE/350 μm | 3.3±0.7 mJy | 35±7 mJy |
| SPIRE/500 μm | 4.6±0.8 mJy | 48±9 mJy |
| ALMA/710 μm | 4.0±0.3 mJy | 41.8±0.7 mJy |
| ALMA/869 μm | 3.8±0.4 mJy | 33.4±0.6 mJy |
| ALMA/1.26 mm | 1.5±0.1 mJy | 20.5±0.4 mJy |
| ALMA/3 mm | < 0.12 mJy | 1.60±0.05 mJy |
| MRS/Hα | < 0.70 | < 0.86 |
| MRS/Paα | 1.07±0.11 | 1.09±0.14 |
Notes. The WPFC3 and MIRI photometry were obtained using the same aperture (see Sects. 2.4 and 3.2). The IRAC, SPIRE, and ALMA photometry are from Marrone et al. (2018). The Hα and Paα fluxes are in units of 10−17 erg s−1 cm−2 (see Sect. 3.3).
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.