@@ -194,11 +194,11 @@ def load_data(self, ids, *, data_release=None, data_structure='INDIVIDUAL', retr
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retrieval type identifier. For GAIA DR2 possible values are ['EPOCH_PHOTOMETRY']
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For GAIA DR3, possible values are ['EPOCH_PHOTOMETRY', 'RVS', 'XP_CONTINUOUS', 'XP_SAMPLED',
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'MCMC_GSPPHOT' or 'MCMC_MSC']
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- For GAIA DR4, possible values will be ['EPOCH_PHOTOMETRY', 'RVS', 'XP_CONTINUOUS', 'XP_SAMPLED',
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- 'MCMC_GSPPHOT', 'MCMC_MSC', 'EPOCH_ASTROMETRY', 'RV_EPOCH_SINGLE', 'RV_EPOCH_DOUBLE', 'RVS_EPOCH' or
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- 'RVS_TRANSIT', 'EPOCH_ASTROMETRY_CROWDED_FIELD ', 'EPOCH_IMAGE ', 'EPOCH_PHOTOMETRY_CCD ',
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- 'XP_EPOCH_SPECTRUM_SSO ', 'XP_EPOCH_CROWDING ', 'XP_MEAN_SPECTRUM ', 'XP_EPOCH_SPECTRUM ',
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- 'CROWDED_FIELD_IMAGE'] . Note that for 'CROWDED_FIELD_IMAGE' only the format 'fits' can be used,
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+ For GAIA DR4, possible values will be ['EPOCH_PHOTOMETRY', 'RVS', 'XP_CONTINUOUS', 'XP_SAMPLED',
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+ 'MCMC_GSPPHOT', 'MCMC_MSC', 'EPOCH_ASTROMETRY', 'RVS_EPOCH_DATA_SINGLE',
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+ 'RVS_EPOCH_DATA_DOUBLE','RVS_EPOCH_SPECTRUM ', 'RVS_TRANSIT ', 'EPOCH_ASTROMETRY_CROWDED_FIELD ',
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+ 'EPOCH_IMAGE ', 'EPOCH_PHOTOMETRY_CCD ', 'XP_EPOCH_SPECTRUM_SSO ', 'XP_EPOCH_CROWDING', 'XP_MEAN_SPECTRUM ',
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+ 'XP_EPOCH_SPECTRUM', ' CROWDED_FIELD_IMAGE', 'EPOCH_ASTROMETRY_BRIGHT']. . Note that for 'CROWDED_FIELD_IMAGE' only the format 'fits' can be used,
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and that its image, in the principal header, will not be available in the returned dictionary. Set
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'output_file' to retrieve all data: image + tables.
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linking_parameter : str, optional, default SOURCE_ID, valid values: SOURCE_ID, TRANSIT_ID, IMAGE_ID
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