activity
19972009
most citedThe DENIS Point Source Catalogue towards the Magellanic Clouds

136 citations · 382 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2009★ 11 cited

The Science Case for PILOT III: the Nearby Universe

J. S. Lawrence, M. C. B. Ashley, J. Bailey +20

PILOT (the Pathfinder for an International Large Optical Telescope is a proposed 2.5 m optical/infrared telescope to be located at DomeC on the Antarctic plateau. The atmospheric c…

astro-ph.IM2009★ 16 cited

The Science Case for PILOT I: Summary and Overview

J. S. Lawrence, M. C. B. Ashley, J. Bailey +40

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5 m optical/infrared telescope to be located at Dome C on the Antarctic plateau. Conditions at D…

astro-ph2005★ 19 cited

Discovery of a nearby M9 dwarf

N. Phan-Bao, M. S. Bessell, E. L. Martin +8

We report the discovery of a new M9.0 dwarf at only 8.2 pc, which we identified in our search for nearby ultracool dwarf (I-J >= 3.0, later than M8.0) in the DENIS database. We mea…

astro-ph2003★ 85 cited

ISOGAL: A deep survey of the obscured inner Milky Way with ISO at 7 and 15 micron and with DENIS in the near-infrared

A. Omont, G. Gilmore, C. Alard +38

The ISOGAL project is an infrared survey of specific regions sampling the Galactic Plane selected to provide information on Galactic structure,stellar populations,stellar mass-loss…

astro-ph2001★ 58 cited

New neighbours: IV. 30 DENIS late-M dwarfs between 15 and 30 parsecs

N. Phan-Bao, J. Guibert, F. Crifo +6

We present 30 new nearby (d<30 pc) red dwarf candidates, with estimated spectral types M6 to M8. 26 were directly selected from the DENIS database, and another 4 were first extract…

astro-ph2001★ 26 cited

Low mass T Tauri and young brown dwarf candidates in the Chamaeleon II dark cloud found by DENIS

My Ha Vuong, Laurent Cambresy, Nicolas Epchtein

We define a sample designed to select low-mass T Tauri stars and young brown dwarfs using DENIS data in the Chamaeleon II molecular cloud. We use a star count method to construct a…