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20132023
most citedThe pattern speed of the Milky Way bar from transverse velocities

151 citations · 465 across the 19 of their papers we have counts for

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Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2021★ 24 cited

Variable star classification across the Galactic bulge and disc with the VISTA Variables in the Vía Láctea survey

Thomas A. Molnar, Jason L. Sanders, Leigh C. Smith +3

We present VIVACE, the VIrac VAriable Classification Ensemble, a catalogue of variable stars extracted from an automated classification pipeline for the Vista Variables in the Vía…

astro-ph.SR2021★ 15 cited

VVV-WIT-08: the giant star that blinked

Leigh C. Smith, Sergey E. Koposov, Philip W. Lucas +11

We report the serendipitous discovery of a late-type giant star that exhibited a smooth, eclipse-like drop in flux to a depth of 97 per cent. Minimum flux occurred in April 2012 an…

astro-ph.SR2020★ 17 cited

Predictions of Gaia's prize microlensing events are flawed

Peter McGill, Andrew Everall, Douglas Boubert +1

Precision astrometry from the second Gaia data release has allowed astronomers to predict 5,787 microlensing events, with 528 of these having maximums within the extended Gaia miss…

astro-ph.SR2019★ 27 cited

The asymptotic evolution of the stellar merger V1309 Sco: a Blue Straggler in the making?

Thiago Ferreira, Roberto K. Saito, Dante Minniti +4

Stellar mergers are estimated to be common events in the Galaxy. The best studied stellar merger case to date is V1309 Sco (= Nova Scorpii 2008) which was originally misclassified…

astro-ph.SR2014★ 22 cited

High Proper Motion Objects from the UKIDSS Galactic Plane Survey

L. Smith, P. W. Lucas, R. Bunce +12

The UKIDSS Galactic Plane Survey (GPS) began in 2005 as a 7 year effort to survey ~1800 square degrees of the northern Galactic plane in the J, H, and K passbands. The survey inclu…

astro-ph.SR2013★ 2 cited

The Kinematic Age of the Coolest T Dwarfs

Leigh Smith, Philip Lucas, Ben Burningham +5

Surprisingly, current atmospheric models suggest that the coolest T dwarfs (T8.5 to T10) are young and very low mass (0.06-2Gyr, 5-20Mjup, Leggett et al.2009, 2010, 2012). Studies…