A Giant Step: From Milli- to Micro- Arcsecond Astrometry (IAU S248)The Proceedings of IAU S248 reflect the state-of-the-art in the field of astrometry, summarizing the scientific achievements at the tenth anniversary of the Hipparcos and Tycho Catalogue release. It shows the latest achievements in ground-based astrometry and details the progress of second-generation astrometric satellites. Currently, the highest accuracies at a micro-arc-second level are reached by interferometric techniques, especially at radio wavelengths. Establishing and maintaining the celestial reference frame at this level, within a relativistic framework, has been identified as one of astrometry's main tasks. The era of large surveys and virtual observatories brings inevitable changes to the role of astrometry in astronomy. For instance, galactic structure and evolution can be fully understood only by combining astrometric and astrophysical parameters. Finally, due attention is given to astrometric education in astronomy curricula for the twenty-first century. These Proceedings convincingly demonstrate the ever growing role played by astrometry in understanding the Universe. |
Avis des internautes - Rédiger un commentaire
Aucun commentaire n'a été trouvé aux emplacements habituels.
Table des matières
| 8 | |
| 14 | |
| 20 | |
| 30 | |
| 36 | |
| 44 | |
| 52 | |
| 59 | |
Simulating Gaia observations and onground reconstruction | 278 |
Development of a very small telescope for a milliarcsec space astrometry | 284 |
testing General Relativity with | 290 |
the UKs contribution to Gaia data | 292 |
UCAC and URAT | 310 |
VLBI observations of weak extragalactic radio sources for the alignment of | 324 |
The second realization of the ICRF with VLBI | 337 |
Multiwavelength VLBI phasedelay astrometry of a complete sample of radio | 352 |
| 66 | |
| 74 | |
Towards a better understanding of Hipparcos | 82 |
Solution of Earth orientation parameters in 20th century based on optical astrom | 89 |
Influence of the astrometric accuracy of observation on the extrapolated ephemerides | 96 |
Brown Dwarf Kinematics Project BDKP | 102 |
Nontidal vertical variations and the past star catalogs | 108 |
A compiled catalogue of reference stars around the selected ERS in the northern | 122 |
A method of accurate guiding for LAMOST | 137 |
Microarcsecond astrometry with the VLBA | 141 |
Astrometric observations of neutron stars | 156 |
a giant step from 0 1 arcsecond to 0 1 milliarcsecond | 170 |
VLBA determinations of the distances to nearby starforming regions | 186 |
Distance and kinematics of IRAS 19134+2131 revealed by H2O maser observations | 200 |
The 3mm flux density monitoring of Sagittarius A with the ATCA | 204 |
science organization and present status | 217 |
Astrometry with SIM PlanetQuest | 231 |
Measuring proper motions of galactic dwarf galaxies with Hubble Space Telescope | 244 |
A Gaia oriented analysis of a large sample of quasars | 260 |
Reference frame linking and tests of GR with Gaia astrometry of asteroids | 266 |
CTE in Space Astrometry | 272 |
Definition and realization of the celestial intermediate reference system | 367 |
Radio interferometric tests of general relativity | 383 |
The RAMOD astrometric observable and the relativistic astrometric catalogs | 397 |
Direct contribution of the surface layers to the Earths dynamical flattening | 403 |
narrowangle astrometry with VLTIPRIMA | 417 |
their kinematics and metallicities | 433 |
Precision astrometry galactic mergers halo substructure and local dark matter | 450 |
years of high precision astrometry in the Galactic Center | 466 |
Microarcsecond astrometry in the Local Group | 474 |
Calibration of stellar parameters using highprecision parallaxes | 488 |
Galactic kinematics near the sun from open clusters | 502 |
The globular cluster tidal radii | 512 |
A project of teaching groundbased astrometry | 521 |
Astrometric education in SaintPetersburg State University Russia | 527 |
Hipparcos data supporting the IB school curriculum | 533 |
Astrometric data for NEAs extracted from the infrared DENIS survey | 544 |
Y Protsyuk A Mazhaev | 550 |
PMOE planetarylunar ephemeris framework | 560 |
IAUS248position | 576 |
Expressions et termes fréquents
2008 International Astronomical 2MASS Abstract accuracy analysis angular arcseconds asteroids astrometric astrometric data astrometric observations Astronomical Union W. J. Astrophysics baseline binary black hole brown dwarfs calibration catalogue celestial China components coordinates detection determination disk distance dynamical ephemerides epoch estimate field Figure Gaia Gaia mission Galactic center Galaxy globular clusters gravitational ground-based Hipparcos Hipparcos catalogue ICRF images interferometer International Astronomical Union Keywords kinematics km s_1 luminosity M. A. C. Perryman magnitude maser mass measurements method mission MNRAS objects obtained open clusters optical orbit parameters phase photometric pixel planets Platais & M. A. C. positions precision Proceedings IAU Symposium processing proper motions radial velocity reference frame reference systems relative relativistic rotation sample satellite Science SDSS Shanghai Astronomical Observatory simulations solar system space stellar subdwarfs survey target techniques telescope Union W. J. Jin VLBA VLBI VLTI

