output
20032011
most citedDust Masses, PAH Abundances, and Starlight Intensities in the SINGS Galaxy Sample

1.1k citations

Showing 2011Show all

12 papers · 1 filter

cs.AI201187 cited

Collective Intelligence, Data Routing and Braess' Paradox

K. Tumer, D. H. Wolpert

We consider the problem of designing the the utility functions of the utility-maximizing agents in a multi-agent system so that they work synergistically to maximize a global utili…

astro-ph.EP201178 cited

Faint young Sun paradox remains

Colin Goldblatt, Kevin J. Zahnle

The Sun was fainter when the Earth was young, but the climate was generally at least as warm as today; this is known as the `faint young Sun paradox'. Rosing et al. [1] claim that…

astro-ph.CO201187 cited

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS

Ivan Valtchanov, J. Virdee, R. J. Ivison +51

We present Herschel-SPIRE Fourier Transform Spectrometer (FTS) and radio follow-up observations of two Herschel-ATLAS (H-ATLAS) detected strongly lensed distant galaxies. In one of…

cs.AI201122 cited

Synthesizing Robust Plans under Incomplete Domain Models

Tuan Nguyen, Subbarao Kambhampati, Minh Do

Most current planners assume complete domain models and focus on generating correct plans. Unfortunately, domain modeling is a laborious and error-prone task. While domain experts…

astro-ph.HE2011

Swift observations of black hole candidate XTE J1752-223 during outburst

P. A. Curran, P. Casella, T. J. Maccarone +5

Here we summarise the Swift broadband observations of the recently discovered X-ray transient and black hole candidate, XTE J1752-223,obtained over the period of outburst from Octo…

astro-ph.GA201199 cited

Using H-alpha Morphology and Surface Brightness Fluctuations to Age-Date Star Clusters in M83

Bradley C. Whitmore, Rupali Chandar, Hwihyun Kim +21

We use new WFC3 observations of the nearby grand design spiral galaxy M83 to develop two independent methods for estimating the ages of young star clusters. The first method uses t…