grss.fit.fit_optical#
Optical observation handling for the GRSS orbit determination code
Functions
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Assemble the optical observations for a given body from Gaia DR3. |
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Assemble the optical observations for a given body into an array for an orbit fit, from the ADES PSV observation file. |
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Apply the Eggl et al. (2020) debiasing scheme to the observation array. |
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Apply the station-specific weight rules to the observation data. |
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Apply the weights from Vereš et al. (2017) to the observation array. |
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Get optical observation data from the Minor Planet Center for a desired small body and assemble the optical observations for the given body into an array for an orbit fit. |
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Calculate the bias on an optical observation given the epoch and the star catalog. |
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Deweight observations that occur on the same night at the same observatory. |
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Limit the number of observations that occur on the same night at the same observatory. |
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Get observation data from MPC observations API for desired small body |
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Assemble the optical observations for a given body into an array for an orbit fit. |
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Get the packed program ID from the ADES data. |
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Get the unpacked program ID for the ADES data. |