activity
20042009
most citedExploring the substellar temperature regime down to ~550K

124 citations · 652 across the 9 of their papers we have counts for

collaborators
Showing astro-phShow all

9 papers · 1 filter

astro-ph200817 cited

HD 179949b: A Close Orbiting Extrasolar Giant Planet with a stratosphere?

J. R. Barnes, Travis S. Barman, H. R. A. Jones +4

We have carried out a search for the 2.14 micron spectroscopic signature of the close orbiting extrasolar giant planet, HD 179949b. High cadence time series spectra were obtained w…

astro-ph2008124 cited

Exploring the substellar temperature regime down to ~550K

Ben Burningham, D. J. Pinfield, S. K. Leggett +15

We report the discovery of three very late T dwarfs in the UKIRT Infrared Deep Sky Survey (UKIDSS) Third Data Release: ULAS J101721.40+011817.9 (ULAS1017), ULAS J123828.51+095351.3…

astro-ph2008122 cited

Metallicities & Activities of Southern Stars

J. S. Jenkins, H. R. A. Jones, Y. Pavlenko +3

We present the results from high-resolution spectroscopic measurements to determine metallicities and activities of bright stars in the southern hemisphere. We have measured the ir…

astro-ph200740 cited

Limits on the 2.2 microns contrast ratio of the close orbiting planet HD 189733b

J. R. Barnes, Travis S. Barman, L. Prato +5

We obtained 238 spectra of the close orbiting extrasolar giant planet HD 189733b with resolution R ~ 15,000 during one night of observations with the near infrared spectrograph, NI…

astro-ph200723 cited

Near infrared spectroscopic search for the close orbiting planet HD 75289b

J. R. Barnes, C. J. Leigh, H. R. A. Jones +4

We present a search for the near infrared spectroscopic signature of the close orbiting extrasolar giant planet HD 75289b. We obtained ~230 spectra in the wavelength range 2.18 - 2…

astro-ph200661 cited

New, nearby bright southern ultracool dwarfs

T. R. Kendall, H. R. A. Jones, D. J. Pinfield +5

We report the discovery of twenty-one hitherto unknown bright southern ultracool dwarfs with spectral types in the range M7 to L5.5, together with new observations of a further thr…