activity
19972026
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 9.7k across the 138 of their papers we have counts for

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Showing 2013 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2013★ 53 cited

The Discovery of Cometary Activity in Near-Earth Asteroid (3552) Don Quixote

Michael Mommert, Joseph L. Hora, Alan W. Harris +8

The near-Earth object (NEO) population, which mainly consists of fragments from collisions between asteroids in the main asteroid belt, is thought to include contributions from sho…

astro-ph.EP2013★ 89 cited

De-biased Populations of Kuiper Belt Objects from the Deep Ecliptic Survey

E. R. Adams, A. A. S. Gulbis, J. L. Elliot +4

The Deep Ecliptic Survey (DES) discovered hundreds of Kuiper Belt objects from 1998-2005. Follow-up observations yielded 304 objects with good dynamical classifications (Classical,…

astro-ph.EP2013★ 32 cited

Asteroid spin-axis longitudes from the Lowell Observatory database

E. Bowell, D. A. Oszkiewicz, L. H. Wasserman +3

By analyzing brightness variation with ecliptic longitude and using the Lowell Observatory photometric database, we estimate spin-axis longitudes for more than 350 000 asteroids. H…

astro-ph.EP2013★ 73 cited

Physical Characterization of Warm Spitzer-observed Near-Earth Objects

Cristina A. Thomas, Joshua P. Emery, David E. Trilling +3

Near-infrared spectroscopy of Near-Earth Objects (NEOs) connects diagnostic spectral features to specific surface mineralogies. The combination of spectroscopy with albedos and dia…

astro-ph.EP2013★ 2 cited

TNOs are Cool: A Survey of the Transneptunian Region XI: A Herschel-PACS view of 16 Centaurs

R. Duffard, N. Pinilla-Alonso, P. Santos-Sanz +13

Centaurs are the transitional population between trans-Neptunian objects (TNOs) and Jupiter-family comets. For this reason it is possible to access the smaller ones, which is more…

astro-ph.EP2013★ 118 cited

Initial Planetesimal Sizes and the Size Distribution of Small Kuiper Belt Objects

Hilke E. Schlichting, Cesar I. Fuentes, David E. Trilling

We show, by comparing observations with theoretical models, that the observed Kuiper Belt size distribution is well matched by coagulation models, which start from an initial plane…