All pull requests

Pull requests

• Scale the gravity drop of a decelerating meteor in the trajectory solver (builds on #156)

  #189·AstroEloy opened Nov 7, 2026Contributor·

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• Source regions of a meteoroid among the asteroid families of METEOMOD, weighted by the meteoroid flux, also at every output of REBOUND (builds on #187)

  #188·AstroEloy opened Nov 7, 2026Contributor·

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• Source regions of an orbit in NEOMOD, from a trajectory, an orbit or every output of REBOUND (builds on #170)

  #187·AstroEloy opened Nov 7, 2026Contributor·

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• Save the plots when an ignored station has NaN heights, as one whose clock is far off

  #186·AstroEloy opened Nov 7, 2026Contributor·

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• SampleTrajectoryPositions: sample the deceleration, dynamic pressure and uncertainties, and derotate the radiant with the initial velocity

  #185·AstroEloy opened Nov 6, 2026Contributor·

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• ParentBodySearch and REBOUND --parent_bodies: take the GR model, including none

  #181·AstroEloy opened Nov 5, 2026Contributor·

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• Add --dynamics_plot: a figure of the Jupiter-family dynamics of a run

  #180·AstroEloy opened Nov 5, 2026Contributor·

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• Run --dynamics shober2024 from published elements, without a trajectory pickle

  #179·AstroEloy opened Nov 5, 2026Contributor·

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• OrbitClassification --dynamics shober2024: the setup of Shober et al. (2024), validated against the paper

  #178·AstroEloy opened Nov 5, 2026Contributor·

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• OrbitClassification --dynamics: Jupiter-family dynamics from REBOUND clones

  #177·AstroEloy opened Nov 5, 2026Contributor·

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• REBOUND: --gr none, to integrate without general relativity

  #176·AstroEloy opened Nov 5, 2026Contributor·

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• REBOUND: 1.5x faster encounter tracking and lean per-clone outputs for large ensembles

  #175·AstroEloy opened Nov 5, 2026Contributor·

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• Add the Jupiter-family dynamics metrics of Shober et al. (2024) to OrbitClassification

  #174·AstroEloy opened Nov 5, 2026Contributor·

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• Search parent bodies and classify the orbit over clones within the uncertainty of the trajectory (builds on #169 and #127)

  #170·AstroEloy opened Oct 31, 2026Contributor·

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• ParentBodySearch --chance_meteoroid: how often an unrelated meteoroid lies as close to a parent-body candidate, from the Deam et al. (2026) model (builds on #146)

  #169·AstroEloy opened Oct 31, 2026Contributor·

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• Let calcPf take a trajectory, with the maximum dynamic pressure from the drag fit (or a robust alpha-beta fit)

  #165·AstroEloy opened Oct 22, 2026Contributor·

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• Simulate MetSim relative to the ground in the GUI, AutoRefineFit and DynestyMetSim (builds on #161 and #162)

  #164·AstroEloy opened Oct 22, 2026Contributor·

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• Compute DynestyMetSim's photometric mass with the luminous efficiency model along the trajectory

  #162·AstroEloy opened Oct 22, 2026Contributor·

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• Compute the GUI's photometric mass with the chosen luminous efficiency model, and rescale the initial mass when it changes

  #161·AstroEloy opened Oct 22, 2026Contributor·

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• Optional extra passes after the timing rerun, until the clocks stop moving

  #158·AstroEloy opened Oct 20, 2026Contributor·

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• ParentBodySearch --chance_neo: p-values of parent-body matches against the Granvik et al. (2018) debiased NEO population (builds on #144 and #145)

  #146·AstroEloy opened Oct 18, 2026Contributor·

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• Offer the MOID as a criterion in the parent body search, like the D criteria (builds on #128 and #143)

  #144·AstroEloy opened Oct 17, 2026Contributor·

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• One vectorised MOID for wmpl: compute it with the planets in REBOUND.py and use it in OrbitClassification

  #143·AstroEloy opened Oct 17, 2026Contributor·

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• Share one planet palette between the REBOUND figure and the solver's orbit plots

  #142·AstroEloy opened Oct 17, 2026Contributor·

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• REBOUND: redraw the orbit figure with the clones as 1σ and 2σ bands, angles within 0–360° and the predictability horizon, and give the orbit to use beyond the horizon (builds on #140)

  #141·AstroEloy opened Oct 17, 2026Contributor·

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