activity
19972026
most citedIlluminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

822 citations · 4.5k across the 68 of their papers we have counts for

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Showing 2010Show all

6 papers · 1 filter

astro-ph.SR2010★ 84 cited

Exquisite Nova Light Curves from the Solar Mass Ejection Imager (SMEI)

R. Hounsell, M. F. Bode, P. P. Hick +10

We present light curves of three classical novae (KT Eridani, V598 Puppis, V1280 Scorpii) and one recurrent nova (RS Ophiuchi) derived from data obtained by the Solar Mass Ejection…

astro-ph.SR2010★ 35 cited

OGLE-2005-BLG-153: Microlensing Discovery and Characterization of A Very Low Mass Binary

K. -H. Hwang, A. Udalski, C. Han +77

The mass function and statistics of binaries provide important diagnostics of the star formation process. Despite this importance, the mass function at low masses remains poorly kn…

astro-ph.HE2010★ 44 cited

GRB 090902B: afterglow observations and implications

S. B. Pandey, C. A. Swenson, D. A. Perley +30

The optical-infrared afterglow of the LAT-detected long duration burst, GRB 090902B, has been observed by several instruments. The earliest detection by ROTSE-IIIa occurred 80 minu…

astro-ph.CO2010★ 9 cited

Gamma Ray Bursts in the Era of Rapid Followup

C. G. Mundell, C. Guidorzi, I. A. Steele

We present a status report on the study of gamma-ray bursts (GRB) in the era of rapid follow-up using the world's largest robotic optical telescopes - the 2-m Liverpool and Faulkes…

astro-ph.EP2010★ 33 cited

An ingress and a complete transit of HD 80606 b

M. G. Hidas, Y. Tsapras, R. A. Street +11

We have used four telescopes at different longitudes to obtain near-continuous lightcurve coverage of the star HD 80606 as it was transited by its \sim 4-MJup planet. The observati…

astro-ph.EP2010★ 217 cited

A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common

T. Sumi, D. P. Bennett, I. A. Bond +104

We present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q=[9.5 +/- 2.1] x 10^{-5} via gravitational microlensing. The planetary devia…