REsolved ALMA and SMA Observations of Nearby Stars (REASONS): Observation Logs
<p>Observation Details for millimetre-wavelength data gathered and modelled as part of the REsolved ALMA and SMA Observations of Nearby Stars (REASONS) paper (same DOI as this table). For the processed data and modelling results, see https://doi.org/10.5281/zenodo.12583396.</p> <ul> <li>Table A.1 refers to targets observed as part of the REASONS <em>Observational</em> ALMA program</li> <li>Table A.2 refers to targets observed as part of the REASONS <em>Observational</em> SMA program</li> <li>Table A.3 refers to targets previously observed whose raw data was retrieved from the ALMA archive and reanalysed as part of REASONS.</li> </ul>
ShareScore
36/100
Overall dataset sharing score
Score breakdown
These five areas show where the dataset supports — or may limit — practical reuse.
- Stewardship
- 4
- Harmonization
- 4
- Access
- 16
- Reuse readiness
- 8
- Engagement
- 4
ScienceDex for faculty
Your academic CV and NIH biosketch
Make your CV in your school's format and your NIH biosketch from it, then download both as Word files.