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19992022
most citedInteracting Supernovae and Supernova Impostors. SN 2009ip, is this the end?

271 citations · 1.3k across the 29 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008★ 32 cited

The CHilean Automatic Supernova sEarch (CHASE)

G. Pignata, J. Maza, M. Hamuy +16

The CHASE project started in 2007 with the aim of providing young southern supernovae (SNe) to the Carnegie Supernova Project (CSP) and Millennium Center for Supernova Studies (MCS…

astro-ph2008★ 61 cited

GRB 070714B - Discovery of the Highest Spectroscopically Confirmed Short Burst Redshift

J. F. Graham, A. S. Fruchter, A. J. Levan +10

We detect the optical afterglow and host galaxy of GRB 070714B. Our observations of the afterglow show an initial plateau in the lightcurve for approximately the first 5 to 25 minu…

astro-ph2008★ 34 cited

The Rapidly Flaring Afterglow of the Very Bright and Energetic GRB 070125

Adria C. Updike, Joshua B. Haislip, Melissa C. Nysewander +52

We report on multi-wavelength observations, ranging from the X-ray to radio wave bands, of the IPN-localized gamma-ray burst GRB 070125. Spectroscopic observations reveal the prese…

astro-ph2007★ 32 cited

PROMPT Observations of the Early-Time Optical Afterglow of GRB 060607A

M. Nysewander, D. E. Reichart, J. A. Crain +5

PROMPT (Panchromatic Robotic Optical Monitoring and Polarimetry Telescopes) observed the early-time optical afterglow of GRB 060607A and obtained a densely sampled multiwavelength…

astro-ph2007★ 67 cited

GRB051022: physical parameters and extinction of a prototype dark burst

Evert Rol, Alexander van der Horst, Klaas Wiersema +19

GRB051022 was undetected to deep limits in early optical observations, but precise astrometry from radio and X-ray showed that it most likely originated in a galaxy at z~0.8. We re…

astro-ph2005★ 119 cited

Discovery and identification of the very high redshift afterglow of GRB 050904

J. Haislip, M. Nysewander, D. Reichart +39

In 2000, Lamb and Reichart predicted that gamma-ray bursts (GRBs) and their afterglows occur in sufficient numbers and at sufficient brightnesses at very high redshifts (z > 5) to…