output
20022009
most citedPolynomial-time quantum algorithm for the simulation of chemical dynamics

399 citations

Showing 2009Show all

6 papers · 1 filter

astro-ph.CO200925 cited

Wide-Field Imaging and Polarimetry for the Biggest and Brightest in the 20GHz Southern Sky

S. Burke-Spolaor, R. D. Ekers, M. Massardi +4

We present wide-field imaging and polarimetry at 20GHz of seven of the most extended, bright (Stot >= 0.50 Jy), high-frequency selected radio sources in the southern sky with decli…

astro-ph.CO200943 cited

The ~0.9 mJy sample: A mid-infrared spectroscopic catalog of 150 infrared-luminous, 24 micron selected galaxies at 0.3<z<3.5

Kalliopi M. Dasyra, Lin Yan, George Helou +6

We present a catalog of mid-infrared (MIR) spectra of 150 infrared (IR) luminous galaxies in the Spitzer extragalactic first look survey obtained with IRS on board Spitzer. The sam…

astro-ph.CO200990 cited

The Star Formation History and Extended Structure of the Hercules Milky Way Satellite

D. J. Sand, E. W. Olszewski, B. Willman +5

We present imaging of the recently discovered Hercules Milky Way satellite and its surrounding regions to study its structure, star formation history and to thoroughly search for s…

astro-ph.GA2009347 cited

The Dual Origin of Stellar Halos

Adi Zolotov, Beth Willman, Alyson M. Brooks +5

We investigate the formation of the stellar halos of four simulated disk galaxies using high resolution, cosmological SPH + N-Body simulations. These simulations include a self-con…

astro-ph.CO20094 cited

Dwarf Galaxies in 2010: Revealing Galaxy Formation's Threshold and Testing the Nature of Dark Matter

James S. Bullock, Manoj Kaplinghat, Andrew Fruchter +4

Over the past five years, searches in Sloan Digital Sky Survey data have more than doubled the number of known dwarf satellite galaxies of the Milky Way, and have revealed a popula…

astro-ph.GA20091 cited

Detection of the 3.3um PAH feature as well as water ice and HAC absorption in z~2 ULIRGs

A. Sajina, L. Yan, H. Spoon +1

We present preliminary results from the highest available signal-to-noise rest-frame 2-8um spectra of z~2 ULIRGs. Our 10 targets are selected for their deep silicate absorption fea…