activity
20082018
most citedThe outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals? II. Introducing the bouncing barrier

591 citations · 2.3k across the 15 of their papers we have counts for

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Showing astro-ph.EPShow all

13 papers · 1 filter

astro-ph.EP2015★ 16 cited

A population-based Habitable Zone perspective

Andras Zsom

What can we tell about exoplanet habitability if currently only the stellar properties, planet radius, and the incoming stellar flux are known? A planet is in the Habitable Zone (H…

astro-ph.EP2013★ 290 cited

Inference of Inhomogeneous Clouds in an Exoplanet Atmosphere

Brice-Olivier Demory, Julien de Wit, Nikole Lewis +11

We present new visible and infrared observations of the hot Jupiter Kepler-7b to determine its atmospheric properties. Our analysis allows us to 1) refine Kepler-7b's relatively la…

astro-ph.EP2013

Searching for Terrestrial Planets Orbiting in the Habitable Zone of Ultra-Cool Stars and Brown Dwarfs

Brice-Olivier Demory, Sara Seager, Jack Lissauer +11

We propose to use Kepler in 2-wheel mode to conduct a detailed search for Earth-sized planets orbiting ultra-cool stars and brown dwarfs (spectral types from M7 to L3). This popula…

astro-ph.EP2013★ 59 cited

Search for a habitable terrestrial planet transiting the nearby red dwarf GJ 1214

M. Gillon, B. -O. Demory, N. Madhusudhan +12

High-precision eclipse spectrophotometry of transiting terrestrial exoplanets represents a promising path for the first atmospheric characterizations of habitable worlds and the se…

astro-ph.EP2013★ 149 cited

Towards the Minimum Inner Edge Distance of the Habitable Zone

Andras Zsom, Sara Seager, Julien de Wit +1

We explore the minimum distance from a host star where an exoplanet could potentially be habitable in order not to discard close-in rocky exoplanets for follow-up observations. We…

astro-ph.EP2012★ 144 cited

Spectral Fingerprints of Earth-like Planets Around FGK Stars

Sarah Rugheimer, Lisa Kaltenegger, Andras Zsom +2

We present model atmospheres for an Earth-like planet orbiting the entire grid of main sequence FGK stars with effective temperatures ranging from Teff = 4250K to Teff = 7000K in 2…