| Typicality: | 0.250 |
| Saliency: | 0.000 |
| with infrared spectroscopy | 2 | other |
| to confirm the galaxy’s distance | 2 | purpose |
| astronomer → conduct → follow-up observations | 3 |
| negative | neutral | positive |
| 0.007 | 0.909 | 0.084 |
| Raw frequency | 3 |
| Normalized frequency | 0.000 |
| Modifier score | 0.500 |
| Perplexity | 60.589 |