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We need to assemble the content for the nodes of a dark matter graph. The initial idea is that each entry would have at least these parameters:
Probe - The physical parameter that is sensitive to deviations from cold, collisionless dark matter (e.g., minimum halo mass, substructure abundance, dark matter density profile, etc.)
Target - The astrophysical object that will be measured (e.g., Milky Way satellite galaxies, cluster strong lenses, stellar light curves, etc.)
Measurement - The observable that LSST will contribute to (e.g., dwarf galaxy luminosity function, gaps in stellar streams, etc.)
As an initial step, we will build this content and a Google Spreadsheet. To start, columns correspond to Probe, Target, Measurement and each row will be a unique combination. There will eventually be more information associated with each entry (e.g., sensitivity, particle physics model, etc.).
For a somewhat more complete (though still known to be incomplete) table of probes, check out the table.md
The text was updated successfully, but these errors were encountered:
Very nice! One DM probe missing: microlensing of stars by black holes. If much of the dark matter is composed of the population of 2-100 M_solar BHs which we now know exists, LSST will find hundreds of ~year-long microlensing events in part of the low latitude survey.
Another is weak lensing statistical (stacked) mass mapping of the population of ~100,000 dark matter dominated dwarf galaxies. Simulation shows good S/N.
We need to assemble the content for the nodes of a dark matter graph. The initial idea is that each entry would have at least these parameters:
Probe
- The physical parameter that is sensitive to deviations from cold, collisionless dark matter (e.g., minimum halo mass, substructure abundance, dark matter density profile, etc.)Target
- The astrophysical object that will be measured (e.g., Milky Way satellite galaxies, cluster strong lenses, stellar light curves, etc.)Measurement
- The observable that LSST will contribute to (e.g., dwarf galaxy luminosity function, gaps in stellar streams, etc.)As an initial step, we will build this content and a Google Spreadsheet. To start, columns correspond to
Probe
,Target
,Measurement
and each row will be a unique combination. There will eventually be more information associated with each entry (e.g., sensitivity, particle physics model, etc.).For a somewhat more complete (though still known to be incomplete) table of probes, check out the table.md
The text was updated successfully, but these errors were encountered: