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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).&nbsp;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&nbsp;<em>Observational</em> ALMA program</li> <li>Table A.2&nbsp;refers to targets observed as part of the REASONS&nbsp;<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

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