arcsec
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There are three possible search modes:
Observations
This mode provide the detailed information about original observations from the papers (without any modification), including single-dish and interferometric data.
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Maser groups
In this mode observations are combined into maser groups using DBSCAN method with the minimum distance between observations of 60 arcsec. |
Maser variability
Use this page to review the maser variability using the single-dish fluxes at all observed epochs. In this mode observations are combined into maser groups using DBSCAN method with the minimum distance of 10 arcsec between observations. |
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