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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 2013Show all

6 papers · 1 filter

astro-ph.IM2013★ 4 cited

The Debris Disk Explorer: a balloon-borne coronagraph for observing debris disks

Lewis C. Roberts, Geoffrey Bryden, Wesley Traub +9

The Debris Disk Explorer (DDX) is a proposed balloon-borne investigation of debris disks around nearby stars. Debris disks are analogs of the Asteroid Belt (mainly rocky) and Kuipe…

astro-ph.EP2013★ 76 cited

Herschel's "Cold Debris Disks": Background Galaxies or Quiescent Rims of Planetary Systems?

A. V. Krivov, C. Eiroa, T. Löhne +24

(abridged) Infrared excesses associated with debris disk host stars detected so far peak at wavelengths around ~100μm or shorter. However, six out of 31 excess sources in the Hersc…

astro-ph.IM2013★ 51 cited

WFIRST-2.4: What Every Astronomer Should Know

D. Spergel, N. Gehrels, J. Breckinridge +43

The Astro2010 Decadal Survey recommended a Wide Field Infrared Survey Telescope (WFIRST) as its top priority for a new large space mission. The report of the WFIRST-AFTA Science De…

astro-ph.SR2013★ 220 cited

DUst Around NEarby Stars. The survey observational results

C. Eiroa, J. P. Marshall, A. Mora +47

Debris discs are a consequence of the planet formation process and constitute the fingerprints of planetesimal systems. Their solar system's counterparts are the asteroid and Edgew…

astro-ph.SR2013★ 50 cited

Vertical settling and radial segregation of large dust grains in the circumstellar disk of the Butterfly Star

Christian Gräfe, Sebastian Wolf, Stephane Guilloteau +4

Context: Circumstellar disks are considered to be the environment for the formation of planets. The growth of dust grains in these disks is the first step in the core accretion-gas…

astro-ph.EP2013★ 182 cited

Asteroid Belts in Debris Disk Twins: VEGA and FOMALHAUT

Kate Y. L. Su, G. H. Rieke, R. Malhotra +8

Vega and Fomalhaut, are similar in terms of mass, ages, and global debris disk properties; therefore, they are often referred as "debris disk twins". We present Spitzer 10-35 um sp…