output
20022011
most citedHeavy quarkonium: progress, puzzles, and opportunities

1.8k citations

Showing 2006 · astro-phShow all

82 papers · 2 filters

astro-ph200617 cited

The Angstrom Project Alert System: real-time detection of extragalactic microlensing

M. J. Darnley, E. Kerins, A. Newsam +9

The Angstrom Project is undertaking an optical survey of stellar microlensing events across the bulge region of the Andromeda Galaxy (M31) using a distributed network of two-meter…

astro-ph200631 cited

The Fe-Line Feature In The X-Ray Spectrum of Solar Flares: First Results From The SOXS Mission

Rajmal Jain, Anil K. Pradhan, Vishal Joshi +5

We present the first results from the "Low Energy Detector" payload of the "Solar X-ray Spectrometer (SOXS)" mission, which was launched onboard the GSAT-2 Indian spacecraft on 08…

astro-ph2006

The Sources of the CDF-N : broadband spectral analyses, absorption measurements and the alpha_ox - L_UV relation

S. Frank, Patrick S. Osmer, S. Mathur

We present broadband properties of sources in the Chandra Deep Field-North with spectroscopic redshifts. The high luminosity and redshift bins are dominated by typical quasars. The…

astro-ph2006

Early Results from the KELT Transit Survey

Joshua Pepper, Richard Pogge, D. L. DePoy +5

The Kilodegree Extremely Little Telescope (KELT) project is a small-aperture transit survey of bright stars. The project has completed commissioning runs searching for transits in…

astro-ph20062 cited

Statistics and Simulations of Transit Surveys for Extrasolar Planets

B. Scott Gaudi

The yields from transit surveys can be used to constrain the frequency and statistical properties of extrasolar planets. Conversely, planet frequencies can be used to estimate expe…

astro-ph200633 cited

Strongly Variable z=1.48 FeII and MgII Absorption in the Spectra of z=4.05 GRB 060206

H. Hao, K. Z. Stanek, A. Dobrzycki +9

We report on the discovery of strongly variable FeII and MgII absorption lines seen at z=1.48 in the spectra of the z=4.05 GRB 060206 obtained between 4.13 to 7.63 hours (observer…