中文
相关论文

相关论文: Astrometry Survey Missions Beyond the Magnitude Li…

200 篇论文

FAME is designed to perform an all-sky, astrometric survey with unprecedented accuracy. It will create a rigid astrometric catalog of 4x10^7 stars with 5 < m_V < 15. For bright stars, 5 < m_V < 9, FAME will determine positions and…

We run numerical simulations of the disruption of satellite galaxies in a Galactic potential to build up the entire stellar halo, in order to investigate what the next generation of astrometric satellites will reveal by observing the halo…

天体物理学 · 物理学 2009-10-31 Amina Helmi , P. Tim de Zeeuw

According to current plans, the SIM/NASA mission will be launched just after the end of operations for the Gaia/ESA mission. This is a new situation which enables long term astrometric projects that could not be achieved by either mission…

天体物理仪器与方法 · 物理学 2015-05-13 G. Anglada-Escude , J. H. Debes

We evaluate the potential of the ESA Cornerstone Mission GAIA in helping populate the database of nearby stars ($d < 25$ pc) for subsequent target selection for DARWIN/TPF. The GAIA high-precision astrometric measurements will make it an…

天体物理学 · 物理学 2007-05-23 A. Sozzetti , S. Casertano , M. G. Lattanzi , A. Spagna

The proposed global astrometry mission {\it GAIA}, recently recommended within the context of ESA's Horizon 2000 Plus long-term scientific program, appears capable of surveying the solar neighborhood within $\sim$ 200 pc for the astrometric…

天体物理学 · 物理学 2009-10-31 M. G. Lattanzi , A. Spagna , A. Sozzetti , S. Casertano

In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint objects in the Universe. Theia is primarily designed to…

天体物理仪器与方法 · 物理学 2017-07-06 The Theia Collaboration , Celine Boehm , Alberto Krone-Martins , Antonio Amorim , Guillem Anglada-Escude , Alexis Brandeker , Frederic Courbin , Torsten Ensslin , Antonio Falcao , Katherine Freese , Berry Holl , Lucas Labadie , Alain Leger , Fabien Malbet , Gary Mamon , Barbara McArthur , Alcione Mora , Michael Shao , Alessandro Sozzetti , Douglas Spolyar , Eva Villaver , Conrado Albertus , Stefano Bertone , Herve Bouy , Michael Boylan-Kolchin , Anthony Brown , Warren Brown , Vitor Cardoso , Laurent Chemin , Riccardo Claudi , Alexandre C. M. Correia , Mariateresa Crosta , Antoine Crouzier , Francis-Yan Cyr-Racine , Mario Damasso , Antonio da Silva , Melvyn Davies , Payel Das , Pratika Dayal , Miguel de Val-Borro , Antonaldo Diaferio , Adrienne Erickcek , Malcolm Fairbairn , Morgane Fortin , Malcolm Fridlund , Paulo Garcia , Oleg Gnedin , Ariel Goobar , Paulo Gordo , Renaud Goullioud , Nigel Hambly , Nathan Hara , David Hobbs , Erik Hog , Andrew Holland , Rodrigo Ibata , Carme Jordi , Sergei Klioner , Sergei Kopeikin , Thomas Lacroix , Jacques Laskar , Christophe Le Poncin-Lafitte , Xavier Luri , Subhabrata Majumdar , Valeri Makarov , Richard Massey , Bertrand Mennesson , Daniel Michalik , Andre Moitinho de Almeida , Ana Mourao , Leonidas Moustakas , Neil Murray , Matthew Muterspaugh , Micaela Oertel , Luisa Ostorero , Angeles Perez-Garcia , Imants Platais , Jordi Portell i de Mora , Andreas Quirrenbach , Lisa Randall , Justin Read , Eniko Regos , Barnes Rory , Krzysztof Rybicki , Pat Scott , Jean Schneider , Jakub Scholtz , Arnaud Siebert , Ismael Tereno , John Tomsick , Wesley Traub , Monica Valluri , Matt Walker , Nicholas Walton , Laura Watkins , Glenn White , Dafydd Wyn Evans , Lukasz Wyrzykowski , Rosemary Wyse

[abridged] We carry out numerical simulations to gauge the Gaia potential for precision astrometry of exoplanets orbiting a sample of known dM stars within 30 pc from the Sun. (1) It will be possible to accurately determine orbits and…

地球与行星天体物理 · 物理学 2015-06-17 A. Sozzetti , P. Giacobbe , M. G. Lattanzi , G. Micela , R. Morbidelli , G. Tinetti

Europe's Gaia spacecraft will soon embark on its five-year mission to measure the absolute parallaxes of the complete sample of 1,000 million objects down to 20 mag. It is expected that thousands of nearby brown dwarfs will have their…

太阳与恒星天体物理 · 物理学 2014-04-16 J. H. J. de Bruijne

The second data release of ESA's Gaia satellite (Gaia DR2) revolutionised astronomy by providing accurate distances, proper motions, apparent magnitudes, and in many cases temperatures and radial velocities for an unprecedented number of…

天体物理仪器与方法 · 物理学 2018-12-18 Tomaž Zwitter

One of the most promising space missions of ESA is the astrometric satellite Gaia, which will provide very precise astrometry and multicolour photometry, for all 1.3 billion objects to V~20, and radial velocities with accuracies of a few…

天体物理学 · 物理学 2009-11-11 S. Torres , E. Garcia-Berro , J. Isern , F. Figueras

Gaia is an astrometric mission that will be launched in spring 2013. There are many scientific outcomes from this mission and as far as our Solar System is concerned, the satellite will be able to map thousands of main belt asteroids (MBAs)…

地球与行星天体物理 · 物理学 2016-08-30 D. Bancelin , D. Hestroffer , W. Thuillot

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

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the revised mission design are presented. Next we estimate the…

天体物理学 · 物理学 2007-05-23 Tomaz Zwitter , Ulisse Munari

(Abridged) A consequence of the Earth's motion with respect to the CMB is that over a 10 year period it will travel a distance of ~800 AU. As first noted by Kardashev in 1986, this baseline can be used to carry out astrometric measurements…

宇宙学与河外天体物理 · 物理学 2015-05-13 Fiona Ding , Rupert A. C. Croft

High precision astrometry aims at source position determination to a very small fraction of the diffraction image size, in high SNR regime. One of the key limitations to such goal is the optical response variation of the telescope over a…

Aims. We use near-infrared, ground-based data from the VISTA Variables in the Via Lactea (VVV) survey to indirectly extend the astrometry provided by the Gaia catalog to objects in heavily-extincted regions towards the Galactic bulge and…

星系天体物理 · 物理学 2024-07-03 M. Griggio , M. Libralato , A. Bellini , L. R. Bedin , J. Anderson , L. C. Smith , D. Minniti

Launch of the Gaia space observatory started a new era in astrometry when the accuracy of star coordinates increased by thousands of times. Significant improvement of accuracy was also expected for the coordinates of the Solar system…

地球与行星天体物理 · 物理学 2023-04-05 Nikolay V. Emelyanov , Mikhail Kovalev , Maxim I. Varfolomeev

Future astrometric satellites, such as SIM (NASA's Space Interferometric Mission) and GAIA (ESA's Global Astrometric Interferometer for Astrophysics), hold the promise of mapping out the detailed phase space structure of the Galactic halo…

天体物理学 · 物理学 2009-09-25 HongSheng Zhao , Kathryn Johnston , David Spergel , Lars Hernquist

We present the results of realistic end-to-end simulations of observations of nearby stars with the proposed global astrometry mission GAIA, recently recommended within the context of ESA's Horizon 2000 Plus long-term scientific program. We…

天体物理学 · 物理学 2016-08-30 M. G. Lattanzi , A. Spagna , A. Sozzetti , S. Casertano

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
‹ 上一页 1 2 3 10 下一页 ›