activity
20062023
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations · 5.3k across the 67 of their papers we have counts for

collaborators
Showing 2014Show all

7 papers · 1 filter

astro-ph.EP2014★ 5 cited

A Quick Study of the Characterization of Radial Velocity Giant Planets in Reflected Light by Forward and Inverse Modeling

Mark Marley, Roxana Lupu, Nikole Lewis +3

We explored two aspects of the problem of characterizing cool extrasolar giant planets in scattered optical light with a space based coronagraph. First, for a number of the known r…

astro-ph.EP2014★ 372 cited

Gaseous Mean Opacities for Giant Planet and Ultracool Dwarf Atmospheres over a Range of Metallicities and Temperatures

Richard S. Freedman, Jacob Lustig-Yaeger, Jonathan J. Fortney +3

We present new calculations of Rosseland and Planck gaseous mean opacities relevant to the atmospheres of giant planets and ultracool dwarfs. Such calculations are used in modeling…

astro-ph.GA2014★ 45 cited

Herschel-ATLAS and ALMA: HATLAS J142935.3-002836, a lensed major merger at redshift 1.027

Hugo Messias, Simon Dye, Neil Nagar +29

[Abridged] Aims: This work focuses on one lensed system, HATLAS J142935.3-002836 (H1429-0028), selected in the Herschel-ATLAS field. Gathering a rich, multi-wavelength dataset, we…

astro-ph.SR2014★ 78 cited

Spectral Variability from the Patchy Atmospheres of T and Y Dwarfs

Caroline V. Morley, Mark S. Marley, Jonathan J. Fortney +1

Brown dwarfs of a variety of spectral types have been observed to be photometrically variable. Previous studies have focused on objects at the L/T transition, where the iron and si…

astro-ph.SR2014★ 1 cited

Cloud structure of brown dwarfs from spectroscopic variability observations

Esther Buenzli, Mark S. Marley, Daniel Apai +1

Recent discoveries of variable brown dwarfs have provided us with a new window into their three-dimensional cloud structure. The highest variables are found at the L/T transition,…

astro-ph.SR2014★ 190 cited

Water Clouds in Y Dwarfs and Exoplanets

Caroline V. Morley, Mark S. Marley, Jonathan J. Fortney +4

The formation of clouds affects brown dwarf and planetary atmospheres of nearly all effective temperatures. Iron and silicate condense in L dwarf atmospheres and dissipate at the L…