Table 1.
Position, spectroscopic redshift, and (F438W − F160W) color for the BGG and multiple images used in the modeling.
| ID | RA | Dec | zspec | Color | a [″] | b [″] |
|---|---|---|---|---|---|---|
| BGG | 9:21:25.738 | 18:10:17.70 | 0.6828 | … | … | … |
| S0(a) | 9:21:25.040 | 18:10:12.27 | 1.4869 | 4.69±0.90 | 0.14 | 0.07 |
| S0(b) | 9:21:25.858 | 18:10:07.24 | 1.4869 | 5.53±2.13 | 0.14 | 0.07 |
| S0(c) | 9:21:26.439 | 18:10:13.60 | 1.4869 | 4.35±1.67 | 0.14 | 0.07 |
| S0(d) | 9:21:25.781 | 18:10:24.64 | 1.4869 | 4.19±0.53 | 0.14 | … |
| S1(a) | 9:21:25.987 | 18:10:07.84 | 1.4869 | 1.37±0.08 | 0.14 | 0.07 |
| S1(b) | 9:21:26.376 | 18:10:12.58 | 1.4869 | 1.32±0.08 | 0.14 | 0.07 |
| S2(a) | 9:21:25.851 | 18:10:34.05 | 1.4874 | … | 0.14 | 0.07 |
| S2(b) | 9:21:26.252 | 18:10:31.13 | 1.4874 | … | 0.14 | 0.07 |
| S2(c) | 9:21:26.323 | 18:10:31.04 | 1.4874 | … | 0.14 | 0.07 |
| S3(a) | 9:21:24.159 | 18:10:16.03 | 2.763 | 3.13±0.24 | 0.14 | 0.07 |
| S3(b) | 9:21:26.517 | 18:10:21.73 | 2.763 | 3.37±0.17 | 0.28 | 0.07 |
| S4(a) | 9:21:25.105 | 18:10:17.76 | 3.4280 | … | 0.21 | … |
| S4(b) | 9:21:25.531 | 18:10:17.62 | 3.4280 | … | 0.21 | … |
| S4(c) | 9:21:27.395 | 18:10:18.65 | 3.4280 | … | 0.21 | … |
| S5(a) | 9:21:24.634 | 18:10:06.47 | 4.205 | … | 0.27 | 0.14 |
| S5(b) | 9:21:25.418 | 18:09:59.46 | 4.205 | 2.33±0.69 | 0.27 | 0.14 |
| S5(c) | 9:21:27.085 | 18:10:13.39 | 4.205 | 2.23±0.85 | 0.27 | 0.14 |
| S5(d) | 9:21:25.670 | 18:10:35.81 | 4.205 | … | 0.27 | 0.14 |
Notes. The right ascension and declination are measured with SExtractor in our HST F160W image, except for images of source 4 (S4), which are only detected by MUSE. All spectroscopic redshifts are secure and measured with MUSE. The (F438W − F160W) colors of multiple images in each set are consistent with each other given the 1σ uncertainties. Multiple images without color values either fall into the WFC3 UVIS chip gaps or are undetected in both bands (for S4), and they are all confirmed by MUSE. The last two columns show the positional uncertainties along the elliptical major a and minor b axes that we used for the image position modeling (Sect. 4). Images with a single listed value have circular positional uncertainties.
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