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相关论文: Gaia: 3-dimensional census of the Milky Way Galaxy

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The ESA cornerstone mission Gaia was successfully launched in 2013, and is now scanning the sky to accurately measure the positions and motions of about two billion point-like sources of 3<V<20.5 mag, with the main goal of reconstructing…

太阳与恒星天体物理 · 物理学 2020-01-08 E Pancino

Gaia is a satellite mission of the European Space Agency which is creating a catalogue of extremely accurate positions, distances and space motions of two billion stars in our Galaxy, along with more than one hundred thousand solar system…

天体物理仪器与方法 · 物理学 2025-09-16 Michael Perryman

GAIA is a short-listed candidate for the ESA Cornerstone mission C5, meeting the ESA Survey Committee requirement for an observatory mission, dedicated to astrometry, providing 10 micro-arcsecond accuracy at 15th magnitude. The GAIA mission…

天体物理学 · 物理学 2015-06-24 Gerry Gilmore , Michael Perryman , L Lindegren , F Favata , E Hoeg , M Lattanzi , X Luri , F Mignard , S Roeser , P. T. deZeeuw

Gaia is an ambitious ESA space mission which will provide photometric and astrometric measurements with the accuracies needed to produce a kinematic census of almost one billion stars in our Galaxy. These data will revolutionize our…

星系天体物理 · 物理学 2012-09-27 Benoit Famaey

Gaia is an all sky, high precision astrometric and photometric satellite of the European Space Agency (ESA) due for launch in 2010-2011. Its primary mission is to study the composition, formation and evolution of our Galaxy. Gaia will…

天体物理学 · 物理学 2009-11-10 C. A. L. Bailer-Jones

The GAIA Observatory, ESA's Cornerstone 6 mission, addresses the origin and evolution of our Galaxy, and a host of other scientific challenges. GAIA will provide unprecedented positional and radial velocity measurements with the accuracies…

天体物理学 · 物理学 2007-05-23 Gerard Gilmore

Access to microarcsecond astrometry is now routine in the radio, infrared, and optical domains. In particular the publication of the second data release from the Gaia mission made it possible for every astronomer to work with easily…

天体物理仪器与方法 · 物理学 2021-09-17 Anthony G. A. Brown

In its all-sky survey, the ESA global astrometry mission Gaia will perform high-precision astrometry and photometry for 1 billion stars down to $V = 20$ mag. The data collected in the Gaia catalogue, to be published by the end of the next…

地球与行星天体物理 · 物理学 2015-05-14 A. Sozzetti

Gaia is a fully-approved all-sky astrometric and photometric survey due for launch in 2011. It will measure accurate parallaxes and proper motions for everything brighter than G=20 (ca. 10^9 stars). Its primary objective is to study the…

天体物理学 · 物理学 2007-05-23 Coryn A. L. Bailer-Jones

The measurement of the positions, distances, motions and luminosities of stars represents the foundations of modern astronomical knowledge. Launched at the end of the eighties, the ESA Hipparcos satellite was the first space mission…

天体物理仪器与方法 · 物理学 2015-06-04 L. Eyer , P. Dubath , S. Saesen , D. W. Evans , L. Wyrzykowski , S. Hodgkin , N. Mowlavi

The Gaia mission is expected to provide highly accurate astrometric, photometric, and spectroscopic measurements for about $10^9$ objects. Automated classification of detected sources is a key part of the data processing. Here a few aspects…

天体物理学 · 物理学 2008-12-02 A. Vallenari , R. Sordo

Gaia is the next astrometry mission of the European Space Agency (ESA), following up on the success of the Hipparcos mission. With a focal plane containing 106 CCD detectors, Gaia will survey the entire sky and repeatedly observe the…

天体物理仪器与方法 · 物理学 2015-06-03 J. H. J. de Bruijne

Gaia is a satellite mission of the ESA, aiming at absolute astrometric measurements of about one billion stars (all stars down to 20th magnitude, with unprecedented accuracy. Additionally, magnitudes and colors will be obtained for all…

天体物理学 · 物理学 2008-12-18 Stefan Jordan

The Gaia space project, planned for launch in 2011, is one of the ESA cornerstone missions, and will provide astrometric, photometric and spectroscopic data of very high quality for about one billion stars brighter than V=20. This will…

天体物理学 · 物理学 2015-05-13 Carla Cacciari

Gaia will be ESA's milestone astrometric mission, and is due for launch at the end of 2013. Gaia will repeatedly map the whole sky measuring about one billion sources to V=20-22 mag. Its data products will be {\mu}as accuracy astrometry,…

太阳与恒星天体物理 · 物理学 2015-06-22 Carla Cacciari

The {\Gaia} astrometric mission was approved by the European Space Agency in 2000 and the construction of the spacecraft and payload is on-going for a launch in late 2012. {\Gaia} will continuously scan the entire sky for 5 years, yielding…

天体物理仪器与方法 · 物理学 2011-06-01 C. Jordi

The GAIA space observatory was recently approved as Cornerstone 6 of ESA's science program, to be launched no later than mid-2012. It will provide a stereoscopic and kinematic census of about 10^9 stars throughout our Galaxy (and into the…

天体物理学 · 物理学 2007-05-23 P. T. de Zeeuw

GAIA (originally the acronym for Global Astrometric Interferometer for Astrophysics) is a mission of the European Space Agency (ESA) which will make the largest, most precise three dimensional map of our Galaxy by an unparalleled survey of…

科普物理 · 物理学 2021-06-10 Priya Hasan

The Gaia space astrometry mission is measuring accurate distances and space motions of more than two billion stars throughout our Galaxy and beyond. This is a first look at how Gaia is contributing to fundamental physics, and in particular…

星系天体物理 · 物理学 2021-06-30 Michael Perryman , Konstantin Zioutas

The Gaia astrometric mission - the Hipparcos successor - is described in some detail, with its three instruments: the two (spectro)photometers (BP and RP) covering the range 330-1050 nm, the white light (G-band) imager dedicated to…

天体物理仪器与方法 · 物理学 2010-09-24 E. Pancino
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