This shows you the differences between two versions of the page.
| Next revision | Previous revision | ||
|
sim:development_plan [2018/06/05 10:39] leo created |
— (current) | ||
|---|---|---|---|
| Line 1: | Line 1: | ||
| - | **As of 12 April 2018** | ||
| - | ===== 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 (at METIS science team meeting, 2-4 May 2018) === | ||
| - | * Simcado with bug fixes to support simulations at 3-20 microns | ||
| - | * Configuration files for METIS LM and NQ 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 LM and NQ band imaging verified against Roy’s fluxes document// | ||
| - | |||
| - | === 0.2 (before summer break) === | ||
| - | * output fluxes in LM and NQ band imaging verified against Roy’s fluxes document | ||
| - | * //create pickled OpticalTrain objects for all METIS imaging observing modes for faster operation// | ||
| - | |||
| - | === 0.3 (dependent on Simcado development) === | ||
| - | * Long-slit mode implemented | ||
| - | * Sensitivities verified against Roy’s fluxes document | ||
| - | |||
| - | === 0.4 (dependent on Simcado development) === | ||
| - | * IFU mode implemented | ||
| - | * Sensitivities verified against Roy’s fluxes document | ||
| - | |||
| - | === ... (dependent on Simcado development) === | ||
| - | |||
| - | === 1.0 (dependent on Simcado development and humanpower available at NOVA) === | ||
| - | * All METIS modes implemented, | ||
| - | * Example notebooks available and reproducibly executable for all METIS modes | ||
| - | * Adapt Simcado for VISIR and verify against actual observations | ||
| - | |||
| - | |||
| - | ===== Future developments by Simcado classes ===== | ||
| - | * '' | ||
| - | * include time-resolved jitter effects | ||
| - | * include sub-pixel shifts for spectro-spatial effects for Vortex coronagraphy | ||
| - | * instrument-internal emission (possibly requiring a different treatment of the global transmission/ | ||
| - | * List of transmissive elements (e.g. multiple dichroics currently not supported) | ||
| - | * Implement fixed ADCs (give residuals of the partial atmospheric dispersion correction as static input?) | ||
| - | * '' | ||
| - | * Aquarius noise generator (including ELFN, non-linear gain curve, correlated noise) | ||
| - | * Chopping and nodding (including chop-difference residuals?) | ||
| - | |||