Zobrazeno 1 - 10
of 19
pro vyhledávání: '"L. Racero"'
Context. This work is part of the Gaia Data Processing and Analysis Consortium papers published with the Gaia Early Data Release 3 (EDR3). It is one of the demonstration papers aiming to highlight the improvements and quality of the newly published d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::e0f077702248166858b69752e4c86b3d
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068457
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068457
Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quality five-parameter astrometric solutions. Aims. The proper motions of Q
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::403709634f34b4d406a46c6f7a485941
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068453
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068453
Context. We present the early installment of the third Gaia data release, Gaia EDR3, consisting of astrometry and photometry for 1.8 billion sources brighter than magnitude 21, complemented with the list of radial velocities from Gaia DR2. Aims. A su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::7a1bc7533881ab72620ae95d116985e6
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3196272
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3196272
Aims. We produce a clean and well-characterised catalogue of objects within 100 pc of the Sun from the Gaia Early Data Release 3. We characterise the catalogue through comparisons to the full data release, external catalogues, and simulations. We car
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::c9e381641333c57f3b6ba68a83fffd85
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068455
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068455
Aims. We aim to demonstrate the scientific potential of the Gaia Early Data Release 3 (EDR3) for the study of different aspects of the Milky Way structure and evolution and we provide, at the same time, a description of several practical aspects of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::d23af374b5f7950706de65fe2ad2574b
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068451
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068451
This is a corrigendum to Gaia Collaboration (2018). It corrects errors in Appendix B, which describes the modelling of the Large and Small Magellanic Clouds (LMC and SMC). One of these errors also affects Fig. 18 of the paper, which shows the rotatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::68e2f3ba802570e24a8a765ccb8e0a91
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068627
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3068627
An error occurred during the production process of the original published version. The following names were omitted from the author list: R. Haigron, D. Hatzidimitriou, M. Hauser, M. Haywood, U. Heiter, J. Heu, T. Hilger. The original published versi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::182344b46bb6736eb925f3798848cf28
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3074572
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3074572
Context. The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ≲ 21 mag. Aims. We showcase stellar variability in the Galactic colour-absolute magnitude diagram (CaMD). We focus on pulsating, eruptiv
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::c4b52d603d30727b192ad2c9d3a63ad6
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069019
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069019
Context. The second Gaia data release (Gaia DR2) contains high-precision positions, parallaxes, and proper motions for 1.3 billion sources as well as line-of-sight velocities for 7.2 million stars brighter than GRVS = 12 mag. Both samples provide a f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______2127::1dabdbd690e29bfdc26ad07b40e05175
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069317
https://pergamos.lib.uoa.gr/uoa/dl/object/uoadl:3069317