activity
20022026
most citedMid-Infrared Photometry of Cold Brown Dwarfs: Diversity in Age, Mass and Metallicity

179 citations · 1.5k across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.IM2026★ 8 cited

Quasi-automatic software support for Gaia ground based optical tracking

S. Bouquillon, C. Barache, T. Carlucci +6

The ESA Gaia satellite mission will create a catalog of 1 billion stars with unprecedented astrometric precision. To achieve its aim in terms of astrometric precision, a ground bas…

astro-ph.SR2018★ 20 cited

Parallaxes of southern extremely cool objects III: 118 L \& T dwarfs

R. L. Smart, B. Bucciarelli, H. R. A. Jones +17

We present new results from the Parallaxes of Southern Extremely Cool dwarfs program to measure parallaxes, proper motions and multi-epoch photometry of L and early T dwarfs. The o…

astro-ph.SR2017★ 155 cited

VIRAC: The VVV Infrared Astrometric Catalogue

L. C. Smith, P. W. Lucas, R. Kurtev +12

We present VIRAC version 1, a near-infrared proper motion and parallax catalogue of the VISTA VVV survey for 312,587,642 unique sources averaged across all overlapping pawprint and…

astro-ph.SR2015★ 58 cited

Methane and Ammonia in the near-infrared spectra of late T dwarfs

J. I. Canty, P. W. Lucas, Sergei N. Yurchenko +7

Analysis of T dwarfs using model atmospheres has been hampered by the absence of reliable line lists for methane and ammonia. Newly computed high temperature line lists for both of…

astro-ph.SR2013★ 28 cited

A 1500 deg Near Infrared Proper Motion Catalogue from the UKIDSS Large Area Survey

L. Smith, P. W. Lucas, B. Burningham +5

The UKIDSS Large Area Survey (LAS) began in 2005, with the start of the UKIDSS program as a 7 year effort to survey roughly 4000 deg at high galactic latitudes in Y, J, H and K…

astro-ph.EP2012★ 26 cited

Photometric transit search for planets around cool stars from the western Italian Alps: A pilot study

P. Giacobbe, M. Damasso, A. Sozzetti +7

[ABRIDGED] In this study, we set out to a) demonstrate the sensitivity to <4 R_E transiting planets with periods of a few days around our program stars, and b) improve our knowledg…