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most citedMicrolens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

336 citations · 1.5k across the 30 of their papers we have counts for

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astro-ph200623 cited

The circumburst environment of a FRED GRB: study of the prompt emission and X-ray/optical afterglow of GRB 051111

C. Guidorzi, A. Gomboc, S. Kobayashi +14

We report a multi-wavelength analysis of the prompt emission and early afterglow of GRB051111 and discuss its properties in the context of current fireball models. The detection of…

astro-ph200697 cited

The Remarkable Afterglow of GRB 061007: Implications for Optical Flashes and GRB Fireballs

C. G. Mundell, A. Melandri, C. Guidorzi +18

We present a multiwavelength analysis of Swift GRB 061007. The 2-m robotic Faulkes Telescope South (FTS) began observing 137 s after the onset of the gamma-ray emission, when the o…

astro-ph200621 cited

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase

A. Evans, T. Kerr, Bin Yang +20

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombin…

astro-ph2006171 cited

An asymmetric shock wave in the 2006 outburst of the recurrent nova RS Ophiuchi

T. J. O'Brien, M. F. Bode, R. W. Porcas +6

Nova outbursts take place in binary star systems comprising a white dwarf and either a low-mass Sun-like star or, as in the case of the recurrent nova RS Ophiuchi, a red giant. Alt…

astro-ph2006336 cited

Microlens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

A. Gould, A. Udalski, D. An +33

We detect a Neptune mass-ratio (q~8e-5) planetary companion to the lens star in the extremely high-magnification (A~800) microlensing event OGLE-2005-BLG-169. If the parent is a ma…

astro-ph200632 cited

Rotational velocities of the giants in symbiotic stars: II. Are S-type symbiotics synchronized?

R. K. Zamanov, M. F. Bode, C. H. F. Melo +5

We have measured the projected rotational velocities (v sin i) of the mass donors for 29 S-type symbiotic stars using high resolution spectroscopic observations and the cross-corre…