Table 2.
Submillimetre point sources fluxes and their corresponding names in Herschel SPIRE or PACS catalogue.
| Source | Herschel name | 150 GHz | 150 GHz | 260 GHz | 260 GHz |
|---|---|---|---|---|---|
| [extrap. AO] | [extrap. TO] | [AO] | [TO] | ||
| [mJy] | [mJy] | [mJy] | [mJy] | ||
| PS1 | HSPSC250A_J1227.00+3332.5 | 2.8 ± 0.3 | 2.7 ± 2.3 | 8.2 ± 0.5 | 8.1 ± 0.5 |
| PS2 | HSPSC250A_J1226.86+3334.7 | 1.1 ± 0.3 | 1.0 ± 0.3 | 3.7 ± 0.6 | 3.6 ± 0.6 |
| PS3 | HSPSC250A_J1227.12+3331.9 | 1.4 ± 0.4 | 1.4 ± 0.4 | 3.9 ± 0.6 | 3.8 ± 0.6 |
| PS4 | HSPSC250A_J1226.85+3333.2 | 0.5 ± 0.2 | 0.4 ± 0.2 | 2.6 ± 0.5 | 2.5 ± 0.5 |
| PS5 | HSPSC250A_J1227.13+3332.4 | 0.6 ± 0.2 | 0.5 ± 0.2 | 3.5 ± 0.6 | 3.4 ± 0.6 |
| PS6 | 0.4 ± 2.0 | 0.4 ± 2.0 | 3.1 ± 0.5 | 2.9 ± 0.5 | |
| PS7 | HPPSC160A_J122654.1+333253 | 1.2 ± 0.2(a) | 1.2 ± 0.2(a) | 3.2 ± 0.5 | 3.1 ± 0.5 |
| PS8 | HSPSC250A_J1226.78+3332.8 | 0.5 ± 0.2 | 0.5 ± 0.2 | 3.4 ± 0.6 | 3.3 ± 0.6 |
Notes. Fluxes at 260 GHz are estimated from the NIKA2 maps and fluxes at 150 GHz obtained from the extrapolation of the fitted spectral energy distributions.
For PS7 the extrapolated 150 GHz fluxes are too high, and we take these values as upper limits of flat priors for the fit in Sect. 4.1.1.
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.