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Table 2
Redshifts, centroid velocities relative to z = 3.005, FWHM line widths, and integrated line fluxes in individual counter images of the Ruby.
| ID | Redshift | v | FWHM | μ I CO | ||
| [km s-1] | [km s-1] | [Jy km s-1] | ||||
|
|
||||||
| 1.1 | 3.00373 ± 0.00008 | –381 ± 25 | 374 ± 58 | 5.6 ± 1.1 | ||
| 3.00539 ± 0.00004 | 117 ± 11 | 436 ± 27 | 14.7 ± 1.2 | |||
| 1.2 | 3.00371 ± 0.00005 | –387 ± 14 | 562 ± 34 | 19.9 ± 1.6 | ||
| 3.00548 ± 0.00002 | 145 ± 6 | 358 ± 15 | 22.3 ± 1.3 | |||
| 1.3 | 3.00400 ± 0.00004 | –300.5 ± 11 | 449 ± 26 | 13.8 ± 1.1 | ||
| 3.00541 ± 0.00009 | 124 ± 28 | 495 ± 68 | 6.4 ± 1.2 | |||
| 1.4 | 3.00448 ± 0.00021 | –155 ± 63 | 414 ± 161 | 2.8 ± 1.4 | ||
| 3.00561 ± 0.00005 | 184.2 ± 16 | 345 ± 38 | 7.2 ± 1.0 | |||
|
|
||||||
| Sum | 3.00382 ± 0.00004 | –355 ± 13 | 406 ± 31 | 9.5 ± 1.0 | ||
| 3.00542 ± 0.00002 | 127 ± 6 | 359 ± 14 | 17.3 ± 0.9 | |||
|
|
||||||
| 2.1 | 3.00441 ± 0.00004 | –178 ± 12 | 525 ± 28 | 17.9 ± 1.2 | ||
| 3.00534 ± 0.00011 | 101 ± 34 | 1030 ± 81 | 17.0 ± 1.8 | |||
| 2.2 | 3.00451 ± 0.00003 | –147 ± 10 | 399 ± 24 | 21.5 ± 1.7 | ||
| 3.00556 ± 0.00007 | 169 ± 20 | 173 ± 50 | 3.6 ± 1.3 | |||
|
|
||||||
| Sum | 3.00446 ± 0.00002 | –162 ± 7 | 409 ± 16 | 20.1 ± 1.0 | ||
| 3.00553 ± 0.00005 | 158 ± 14 | 233 ± 34 | 4.3 ± 0.8 | |||
Notes. We also provide fit results for the sum of multiple images from each system as shown in Fig. 2.
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