Table 1.
Flux or flux densities of two LRDs from multiwavelength observations.
| Instrument | λref | Units | ID2756 | ID9094 |
|---|---|---|---|---|
| Chandraa | 0.5–7 keV | erg s−1 cm−2 | < 1.1 × 10−16 | < 1.1 × 10−16 |
| 2–7 keV | erg s−1 cm−2 | < 1.8 × 10−16 | < 1.8 × 10−16 | |
| 0.5–2 keV | erg s−1 cm−2 | < 3.6 × 10−17 | < 3.6 × 10−17 | |
| HST/ACS F435W | 0.43 μm | nJy | < 19.4 | < 17.7 |
| HST/ACS F606W | 0.59 μm | nJy | < 12.3 | < 9.4 |
| HST/ACS F775W | 0.77 μm | nJy | < 13.6 | < 17.7 |
| HST/ACS F814W | 0.80 μm | nJy | < 17.1 | < 13.5 |
| HST/ACS F850LP | 0.90 μm | nJy | < 19.5 | < 24.4 |
| HST/WFC3 F105W | 1.06 μm | nJy | 33.0 ± 8.4 | … |
| HST/WFC3 F125W | 1.25 μm | nJy | 87.5 ± 10.8 | 75.7 ± 9.8 |
| HST/WFC3 F140W | 1.40 μm | nJy | 84.7 ± 6.6 | … |
| HST/WFC3 F160W | 1.54 μm | nJy | 91.3 ± 7.8 | 109.7 ± 10.4 |
| JWST/NIRCam F090W | 0.90 μm | nJy | < 14.3 | < 21.0 |
| JWST/NIRCam F115W | 1.15 μm | nJy | 79.2 ± 4.4 | 64.8 ± 6.2 |
| JWST/NIRCam F150W | 1.50 μm | nJy | … | 93.7 ± 12.9 |
| JWST/NIRCam F182M | 1.85 μm | nJy | 80.0 ± 4.0 | 99.3 ± 6.7 |
| JWST/NIRCam F200W | 1.99 μm | nJy | … | 109.6 ± 11.5 |
| JWST/NIRCam F210M | 2.10 μm | nJy | 117.8 ± 5.9 | 130.2 ± 8.8 |
| JWST/NIRCam F356W | 3.57 μm | nJy | 225.8 ± 11.3 | 443.8 ± 22.2 |
| JWST/NIRCam F444W | 4.40 μm | nJy | 372.4 ± 18.6 | 887.7 ± 44.4 |
| Spitzer/IRAC | 3.6 μm | nJy | 191.0 ± 15.4 | 400.4 ± 13.0 |
| 4.5 μm | nJy | 340.2 ± 17.6 | 592.7 ± 16.5 | |
| 5.8 μm | nJy | 933.7 ± 243.5 | < 676.5 | |
| 8.0 μm | nJy | 351.2 ± 284.8 | 2683.0 ± 289.4 | |
| Spitzer/MIPSb | 24 μm | μJy | < 21 | < 21 |
| 70 μm | mJy | < 2.4 | < 2.4 | |
| Herschel/PACSb | 100 μm | mJy | < 1.1 | < 1.1 |
| 160 μm | mJy | < 2.7 | < 2.7 | |
| Herschel/SPIREb | 250 μm | mJy | < 5.7 | < 5.7 |
| 350 μm | mJy | < 7.2 | < 7.2 | |
| 500 μm | mJy | < 9 | < 9 | |
| SCUBA-2c | 850 μm | mJy | < 1.2 | < 1.2 |
| NOEMA | 1.3 mm | μJy | < 151 | < 91 |
| [C II]158 μm | Jy km s−1 | < 0.310 | < 0.157 | |
| NIKA-2d | 1.2 mm | μJy | < 510 | < 510 |
| 2.0 mm | μJy | < 144 | < 144 | |
| VLA 1.5 GHze | 20 cm | uJy | < 6.6 | < 6.6 |
Notes. We use 1σ for uncertainties and 3σ upper limits for non-detections. (a) We calculate 3σ upper limits based on the mean sensitivity limits achieved in the central ∼1 arcmin2 area at the average aim point from 2 Ms Chandra Deep Field-North survey (Xue et al. 2016). (b) Sources are not detected, we adopt 3σ upper limits from the GOODS-Herschel survey (Elbaz et al. 2011). (c) We adopt the confusion limit for a 3σ detection in the central region of GOODS-N from Cowie et al. (2017). (d) We adopt 3σ upper limits according to the N2CLS depth from Bing et al. (2023). (e) Calculated based on the rms noise for a 1
6 resolution in the field center from Owen (2018).
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.