Table 2
Input parameters for each of the umax grids are shown, with the parameter ranges shown in square brackets.
| umax grid type | Input parameters |
|---|---|
| Signal-to-noise | ms [16,24.9], × [0.01,1.0]†, ρ* [0,5] |
| Parallax | mW [16,24.9], mE [16,24.9], πE [10−4,1]†, tE [0.02,6],  , ρ, [0,5] |
| Finite Source | ms [16,24.9], × [0.01,1]†, ρ* [10−5,5]† |
Notes. The parameters flagged with † are distributed logarithmically; all the others are distributed linearly. All parameters have a grid resolution of 10 points, other than ϕ and ρ*, for the parallax grid which have a grid resolution of 5 points. The parameters used throughout are ms, an arbitrary source magnitude; mW, a W146 magnitude; mE, a magnitude in either Euclid VIS or NISP(H) filters; tE, the Einstein radius crossing time; x, the cadence of a telescope normalized to tE; ρ*, the source radius normalized to θE; πE, the magnitude of the microlensing parallax; and ϕ, the angle between the lens-source proper motion vector and the projected baseline vector.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.