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Astrometric Exoplanet Detection with Gaia
DOI: 10.1088/0004-637X/797/1/14 Bibcode: 2014ApJ...797...14P

Bakos, Gáspár Á.; Lindegren, Lennart; Hartman, Joel +1 more

We provide a revised assessment of the number of exoplanets that should be discovered by Gaia astrometry, extending previous studies to a broader range of spectral types, distances, and magnitudes. Our assessment is based on a large representative sample of host stars from the TRILEGAL Galaxy population synthesis model, recent estimates of the exo…

2014 The Astrophysical Journal
Gaia 280
Predicted Space Motions for Hypervelocity and Runaway Stars: Proper Motions and Radial Velocities for the Gaia Era
DOI: 10.1088/0004-637X/793/2/122 Bibcode: 2014ApJ...793..122K

Geller, Margaret J.; Brown, Warren R.; Kenyon, Scott J. +1 more

We predict the distinctive three-dimensional space motions of hypervelocity stars (HVSs) and runaway stars moving in a realistic Galactic potential. For nearby stars with distances less than 10 kpc, unbound stars are rare; proper motions alone rarely isolate bound HVSs and runaways from indigenous halo stars. At large distances of 20-100 kpc, unbo…

2014 The Astrophysical Journal
Gaia 61
The Variable Sky of Deep Synoptic Surveys
DOI: 10.1088/0004-637X/796/1/53 Bibcode: 2014ApJ...796...53R

Matheson, Thomas; Howell, Steve B.; Mighell, Kenneth J. +2 more

The discovery of variable and transient sources is an essential product of synoptic surveys. The alert stream will require filtering for personalized criteria—a process managed by a functionality commonly described as a Broker. In order to understand quantitatively the magnitude of the alert generation and Broker tasks, we have undertaken an analy…

2014 The Astrophysical Journal
Gaia 28
Microlensing Events by Proxima Centauri in 2014 and 2016: Opportunities for Mass Determination and Possible Planet Detection
DOI: 10.1088/0004-637X/782/2/89 Bibcode: 2014ApJ...782...89S

Anderson, Jay; Bond, Howard E.; Sahu, Kailash C. +1 more

We have found that Proxima Centauri, the star closest to our Sun, will pass close to a pair of faint background stars in the next few years. Using Hubble Space Telescope (HST) images obtained in 2012 October, we determine that the passage close to a mag 20 star will occur in 2014 October (impact parameter 1.''6), and to a mag 19.5 star in 2016 Feb…

2014 The Astrophysical Journal
Gaia eHST 25
The Gaia Inertial Reference Frame and the Tilting of the Milky Way Disk
DOI: 10.1088/0004-637X/789/2/166 Bibcode: 2014ApJ...789..166P

Spergel, David N.; Lindegren, Lennart; Perryman, Michael

While the precise relationship between the Milky Way disk and the symmetry planes of the dark matter halo remains somewhat uncertain, a time-varying disk orientation with respect to an inertial reference frame seems probable. Hierarchical structure formation models predict that the dark matter halo is triaxial and tumbles with a characteristic rat…

2014 The Astrophysical Journal
Gaia 23