activity
19962026
most citedThe Spitzer c2d Legacy Results: Star Formation Rates and Efficiencies; Evolution and Lifetimes

1.7k citations · 13.7k across the 180 of their papers we have counts for

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Showing 2017Show all

6 papers · 1 filter

astro-ph.SR2017★ 33 cited

HST Scattered Light Imaging and Modeling of the Edge-on Protoplanetary Disk ESO-H 569

Schuyler G. Wolff, Marshall D. Perrin, Karl Stapelfeldt +6

We present new HST ACS observations and detailed models for a recently discovered edge-on protoplanetary disk around ESO H 569 (a low-mass T Tauri star in the Cha I star forming…

astro-ph.EP2017★ 74 cited

A Direct Imaging Survey of Spitzer detected debris disks: Occurrence of giant planets in dusty systems

Tiffany Meshkat, Dimitri Mawet, Marta Bryan +10

We describe a joint high contrast imaging survey for planets at Keck and VLT of the last large sample of debris disks identified by the Spitzer Space Telescope. No new substellar c…

astro-ph.EP2017★ 30 cited

The First Scattered Light Image of the Debris Disk around the Sco-Cen target HD 129590

Elisabeth Matthews, Sasha Hinkley, Arthur Vigan +7

We present the first scattered light image of the debris disk around HD 129590, a ~1.3 M G1V member of the Scorpius Centaurus association with age ~10-16 Myr. The debris di…

astro-ph.EP2017★ 326 cited

Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment

Victoria S. Meadows, Christopher T. Reinhard, Giada N. Arney +13

Here we review how environmental context can be used to interpret whether O2 is a biosignature in extrasolar planetary observations. This paper builds on the overview of current bi…

astro-ph.EP2017★ 168 cited

Exoplanet Biosignatures: Observational Prospects

Yuka Fujii, Daniel Angerhausen, Russell Deitrick +9

Exoplanet hunting efforts have revealed the prevalence of exotic worlds with diverse properties, including Earth-sized bodies, which has fueled our endeavor to search for life beyo…

astro-ph.SR2017★ 35 cited

The Inner 25 AU Debris Distribution in the epsilon Eri System

Kate Y. L. Su, James M. De Buizer, George H. Rieke +6

Debris disk morphology is wavelength dependent due to the wide range of particle sizes and size-dependent dynamics influenced by various forces. Resolved images of nearby debris di…