Open Access
Table 1.
Global properties of SDP.81.
| Basic properties | ||
|---|---|---|
| RA | [J2000] | 09:03:11.57 |
| Dec | [J2000] | +00:39:06.5 |
| zs | 3.042 | |
| zL | 0.299 | |
 |
[L⊙] | (43 ± 0.5)×1012 |
 |
[K km s−1 pc2] | (54 ± 9)×1010 |
| FWHMCO(1 − 0) | [km s−1] | 435 ± 54 |
| μ160 μm | 18.2 ± 1.2 | |
| ALMA Band 3 continuum | ||
 |
[mJy] | 0.510 ± 0.031 |
| Jupp = 1 lines (Rybak et al. 2022) | ||
 |
[K km s−1 pc2] | ≤3.7 × 1010 |
 |
[K km s−1 pc2] | ≤4.2 × 1010 |
 |
[K km s−1 pc2] | ≤2.4 × 1010 |
| Jupp = 4 lines (This work) | ||
| SΔvHCN(4 − 3) | [Jy km s−1] | ≤0.302 |
| SΔvHCO+(4 − 3) | [Jy km s−1] | 0.357 ± 0.056 |
| SΔvHNC(4 − 3) | [Jy km s−1] | ≤0.207 |
 |
[K km s−1 pc2] | ≤7.2 × 109 |
 |
[K km s−1 pc2] | (16.0 ± 4.3)×109 |
 |
[K km s−1 pc2] | ≤7.1 × 109 |
Notes. Individual columns list the source position, source and lens redshift (zs, zL), sky-plane (observed) FIR and CO(1–0) luminosities, CO(1–0) FWHM (Valtchanov et al. 2011), and FIR continuum magnification (Rybak et al. 2020). LFIR is integrated over 8–1000 μm.
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