2026-04-18T05:04:56Zhttps://recercat.cat/oai/request

oai:recercat.cat:2445/2184532026-03-17T02:44:35Zcom_2072_1057col_2072_478823col_2072_478904col_2072_478917

00925njm 22002777a 4500 dc Jiménez Arranz, Óscar author Anders, F. author Khalatyan, A. author Queiroz, A. B. A. author Chiappini, C. author Ardèvol Guillamón, Judith author Casamiquela, L. author Figueras Siñol, Francesca author Jordi i Nebot, Carme author Monguió i Montells, Maria author Romero Gómez, Mercè author Altamirano, D. author Antoja, T. (Teresa) author Assaad, R. author Cantat Gaudin, Tristan author Castro Ginard, Alfred author Enke, H. author Girardi, L. author Guiglion, G. author Khan, S. author Luri Carrascoso, Xavier author Miglio, A. author Minchev, I. author Ramos, P. author Santiago, B. X. author Steinmetz, M. author 2025-02-03T16:24:48Z 2025-02-03T16:24:48Z 2022-02-07 2025-02-03T16:24:48Z We present a catalogue of 362 million stellar parameters, distances, and extinctions derived from Gaia's early third data release (EDR3) cross-matched with the photometric catalogues of Pan-STARRS1, SkyMapper, 2MASS, and AllWISE. The higher precision of the Gaia EDR3 data, combined with the broad wavelength coverage of the additional photometric surveys and the new stellar-density priors of the {\tt StarHorse} code allow us to substantially improve the accuracy and precision over previous photo-astrometric stellar-parameter estimates. At magnitude G=14(17), our typical precisions amount to 3% (15%) in distance, 0.13 mag (0.15 mag) in V-band extinction, and 140 K (180 K) in effective temperature. Our results are validated by comparisons with open clusters, as well as with asteroseismic and spectroscopic measurements, indicating systematic errors smaller than the nominal uncertainties for the vast majority of objects. We also provide distance- and extinction-corrected colour-magnitude diagrams, extinction maps, and extensive stellar density maps that reveal detailed substructures in the Milky Way and beyond. The new density maps now probe a much greater volume, extending to regions beyond the Galactic bar and to Local Group galaxies, with a larger total number density. We publish our results through an ADQL query interface ({\tt gaia.aip.de}) as well as via tables containing approximations of the full posterior distributions. Our multi-wavelength approach and the deep magnitude limit make our results useful also beyond the next Gaia release, DR3. Fotometria Astrometria Galàxies Photometry Astrometry Galaxies Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia EDR3 stars brighter than G=18.5