You signed in with another tab or window. Reload to refresh your session.You signed out in another tab or window. Reload to refresh your session.You switched accounts on another tab or window. Reload to refresh your session.Dismiss alert
Following a similar structure to D3.3.1, the initial step of D3.3.2 is to develop the mathematical background required to answer the required questions surrounding the identification of potential matches that were missed in an initial cross-match run, and assign relative probabilities to astrophysical (or telescope/pipeine-related) origins of the reason for objects not matching, such as high proper motion, data artefact, or transient outbursts.
The text was updated successfully, but these errors were encountered:
Following a similar structure to D3.3.1, the initial step of D3.3.2 is to develop the mathematical background required to answer the required questions surrounding the identification of potential matches that were missed in an initial cross-match run, and assign relative probabilities to astrophysical (or telescope/pipeine-related) origins of the reason for objects not matching, such as high proper motion, data artefact, or transient outbursts.
The text was updated successfully, but these errors were encountered: