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sim:development_plan [2018/06/05 11:23] leo |
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| - | ===== Development plan / Milestones ===== | ||
| - | for each milestone, the minimum required points to release that version are given; additional goals (best effort basis) are printed in // | ||
| - | === 0.1 (June 2018) === | ||
| - | * Simcado with bug fixes to support simulations at 3-20 microns | ||
| - | * Configuration files for METIS L and N band imaging | ||
| - | * Transmission curves (sky emission / absorption, mirror reflectivity, | ||
| - | * iPython notebooks with example use cases for both LM and NQ band imaging | ||
| - | * output fluxes in L and N band imaging verified against Roy’s fluxes document | ||
| - | |||
| - | === 0.2 (July 2018) === | ||
| - | * bug fixes | ||
| - | * properly implement cold stop(s) in METIS | ||
| - | * all filter curves | ||
| - | * M band | ||
| - | * //Q band// | ||
| - | * //create pickled OpticalTrain objects for all METIS imaging observing modes for faster operation// | ||
| - | |||
| - | === 0.3 (aim: September 2018, dependent on core SimCADO development) === | ||
| - | * Long-slit mode with sensitivities verified against Roy’s fluxes document | ||
| - | * bug fixes | ||
| - | * updates for instrument configuration files | ||
| - | |||
| - | === 0.4 (aim: October 2018, dependent on core SimCADO development) === | ||
| - | * IFU mode implemented with sensitivities verified against Roy’s fluxes document | ||
| - | * bug fixes | ||
| - | * updates for instrument configuration files | ||
| - | |||
| - | === 1.0 (aim: December 2018, dependent on Simcado development and humanpower available at NOVA) === | ||
| - | * Aquarius noise generator included (including ELFN, non-linear gain curve, correlated noise) | ||
| - | * All METIS modes implemented, | ||
| - | * Example notebooks available and reproducibly executable for all METIS modes | ||