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

collaborators

15 papers

cs.CL2018

Measuring Similarity: Computationally Reproducing the Scholar's Interests

Ashley Lee, Jo Guldi, Andras Zsom

Computerized document classification already orders the news articles that Apple's "News" app or Google's "personalized search" feature groups together to match a reader's interest…

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…