tests:collision:gc4
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=== M4 mass modelling challenge: method comparison === | === M4 mass modelling challenge: method comparison === | ||
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+ | This is a joint project between many participants, | ||
[[: | [[: | ||
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+ | Some preliminary results from GCIII are shown [[: | ||
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+ | The current plan is to turn this M4 challenge into one ‘Gaia Challenge' | ||
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+ | - Jeans modelling (Laura & Antonio - each with their own code) | ||
+ | - Multi-mass models with full mass function and SSP model (Vincent) | ||
+ | - Three-component multi-mass models (Mark) | ||
+ | - Single-mass models (Mark/ | ||
+ | - Single-mass models with potential escapers (Ian) | ||
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+ | The plan is to use combined datasets with increasing level of information: | ||
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+ | - The surface brightness profile and line-of-sight velocity dispersion profile | ||
+ | - Then additionally consider HST-like proper-motion dispersion profiles | ||
+ | - Finally, fits including all the previous data and including Gaia-like proper motions and distances | ||
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+ | Mock data for steps 1 and 2 are currently available. For step 3, Elena Pancino is working on producing Gaia-like observations of the M4 snapshot (with different simulated backgrounds). | ||
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+ | We want to compare how well the different methods recover or fit the following quantities/ | ||
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+ | - total cluster mass $M$ | ||
+ | - half-mass radius $r_h$ | ||
+ | - global mass-to-light ratio $M/L$ | ||
+ | - $M/L$ profile | ||
+ | - general quality of the fit to the velocity dispersion, surface brightness, and anisotropy profile | ||
+ | - constraints on the stellar mass function (where applicable) | ||
+ | - mass in dark remnants (where applicable) | ||
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+ | You can put your [[: | ||
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tests/collision/gc4.1476171990.txt.gz · Last modified: 2022/10/24 12:26 (external edit)