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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

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

We investigate the possibility of detecting planetary or stellar companions orbiting white dwarf binaries using the LISA gravitational radiation detector. Specifically, we consider the acceleration of the barycenter of the white dwarf…

地球与行星天体物理 · 物理学 2018-12-11 Jason H. Steffen , Dong-Hong Wu , Shane L. Larson

The frequency of planets in binaries is an important issue in the field of extrasolar planet studies because of its relevance in the estimation of the global planet population of our galaxy and the clues it can give to our understanding of…

地球与行星天体物理 · 物理学 2020-02-28 Mariangela Bonavita , Silvano Desidera

Astrometry is a powerful technique to study the populations of extrasolar planets around nearby stars. It gives access to a unique parameter space and is therefore required for obtaining a comprehensive picture of the properties,…

太阳与恒星天体物理 · 物理学 2015-06-17 J. Sahlmann , P. F. Lazorenko , A. Mérand , D. Queloz , D. Ségransan , J. Woillez

We discuss the synergy of Gaia and the Large Synoptic Survey Telescope (LSST) in the context of Milky Way studies. LSST can be thought of as Gaia's deep complement because the two surveys will deliver trigonometric parallax, proper-motion,…

天体物理仪器与方法 · 物理学 2015-02-24 Željko Ivezić , Steven M. Kahn , Patricia Eliason

To date more than 3500 exoplanets have been discovered orbiting a large variety of stars. Due to the sensitivity limits of the currently used detection techniques, these planets populate zones restricted either to the solar neighbourhood or…

地球与行星天体物理 · 物理学 2019-09-16 Nicola Tamanini , Camilla Danielski

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

We use detailed numerical simulations and the $\upsilon$ Andromedae, planetary system as a template to evaluate the capability of the ESA Cornerstone Mission GAIA in detecting and measuring multiple planets around solar-type stars in the…

天体物理学 · 物理学 2009-11-06 A. Sozzetti , S. Casertano , M. G. Lattanzi , A. Spagna

Observations of binaries containing pairs of neutron stars using the upcoming space-based gravitational wave observatory, LISA, have the potential to improve our understanding of neutron star physics and binary evolution. In this work we…

高能天体物理现象 · 物理学 2023-03-08 Anatole Storck , Ross Church

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 power of micro-arcsecond ($\mu$as) astrometry is about to be unleashed. ESA's Gaia mission, now headed towards the end of the first year of routine science operations, will soon fulfil its promise for revolutionary science in countless…

地球与行星天体物理 · 物理学 2016-02-03 A. Sozzetti , M. Bonavita , S. Desidera , R. Gratton , M. G. Lattanzi

The ESA Cornerstone Mission GAIA, to be launched prior to 2012 and with a nominal lifetime of 5 years, will improve the accuracy of Hipparcos astrometry by more than two orders of magnitude. GAIA high-precision global astrometric…

天体物理学 · 物理学 2015-06-24 M. G. Lattanzi , S. Casertano , A. Sozzetti , A. Spagna

As the most ancient branch of astronomy, astrometry has been developed for thousands of years. However, it has only recently become possible to utilize astrometry for the detection of exoplanets. Gaia, an astrometric surveyor of 1 billion…

地球与行星天体物理 · 物理学 2024-03-14 Fabo Feng

Double white dwarf (DWD) binaries are expected to be very common in the Milky Way, but their intrinsic faintness challenges the detection of these systems. Currently, only a few tens of detached DWDs are know. Such systems offer the best…

高能天体物理现象 · 物理学 2017-07-26 Valeriya Korol , Elena M. Rossi , Paul J. Groot , Gijs Nelemans , Silvia Toonen , Anthony G. A. Brown

The ESA Gaia mission uses two telescopes to create the most ambitious survey of the Galaxy. The angle between them must be known with exquisite precision and accuracy. An interferometer: the Basic Angle Monitoring system measures its…

Distant objects in the solar system are crucial to better understand the history and evolution of its outskirts. The stellar occultation technique allows the determination of their sizes and shapes with kilometric accuracy, a detailed…

ESA and NASA are studying projects having a tremendous return on variable star research. Other national space agencies are also studying or developing projects of smaller costs but with impressive returns. The projects range from global…

天体物理学 · 物理学 2007-05-23 Laurent Eyer

In the last two decades, thousands of extrasolar planets were discovered based on different observational techniques, and their number must increase substantially in virtue of the ongoing and near-future approved missions and facilities. It…

地球与行星天体物理 · 物理学 2018-08-01 J. V. Cunha , F. E. Silva , J. A. S. Lima

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