zenodoopen
The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. I. Carbon-Chain Chemistry of Intermediate-Mass Protostars
<p>These figures show spectra obtained by the Yebes 40m telescope toward eleven intermediate-mass protostars. Black lines indicate the observational spectra and red curves indicate the best-fitting models with the MCMC method. Blue curves show the results of the Gaussian fitting.</p>
ShareScore
32/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 12
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 0
- Engagement
- 0