OmniSky v1
Collection
Crossmatched, normalized multimodal astronomy: 20.4M DESI DR1 objects x 24 catalogs, 822 GB. Start with mmu-norm-index. • 20 items • Updated
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_healpix_29 int64 3.12B 3,458,764,065B | photometry dict | astrometry dict | radial_velocity dict | gspphot dict | flags dict | corrections dict | ra float64 0 360 | dec float64 -27.2 84.6 | healpix int64 0 3.07k | object_id int64 4.3B 6,917,528,100B | xp_coefficients dict |
|---|---|---|---|---|---|---|---|---|---|---|---|
3,456,512,695,685,715,000 | {
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} | 44.823741 | 0.85587 | 0 | 124,901,944,696,960 | {
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End of preview. Expand in Data Studio
Gaia DR3 astrometry, photometry, and XP spectra — L1 (release v1)
This L1 repository contains 809,882 sources matched across the release, in seven shards.
Schema
xp_coefficientsstruct:bp_coeff[55],rp_coeff[55],bp_coeff_error[55], andrp_coeff_error[55]. The upstream 110-element vector is split into Gaia DR3 basis components. Empty arrays indicate that XP data are unavailable for that source.astrometrystruct: positions, parallax, proper motions, and their uncertainties and correlations. Negative parallaxes are valid measurements; do not treat1/parallaxas a distance (Bailer-Jones 2015).photometry,radial_velocity,gspphot,flags,correctionsstructs: native Gaia DR3 values.
Data notes
- The upstream data did not retain XP coefficient correlations or covariance. The provided coefficient errors form a diagonal approximation.
- GSP-Phot quantities are model-dependent posteriors.
- XP coefficients are basis-dependent. Keep the physical representation when scaling them for a model.
The L2 scaling statistics, fit on the training split, are in l2_stats/v1/gaia_gaia.json. Credit: ESA Gaia DR3 (Gaia Collaboration 2023). Sourced via Multimodal Universe.
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