activity
19982020
most citedChemistry and Star Formation in the Host Galaxies of Type Ia Supervovae

166 citations · 821 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2020★ 28 cited

The Slow Demise of the Long-Lived SN 2005ip

Ori D. Fox, Claes Fransson, Nathan Smith +16

The Type IIn supernova (SN) 2005ip is one of the most well-studied and long-lasting examples of a SN interacting with its circumstellar environment. The optical light curve plateau…

astro-ph.SR2016★ 25 cited

Hubble Tarantula Treasury Project V. The star cluster Hodge 301: the old face of 30 Doradus

M. Cignoni, E. Sabbi, R. P. van der Marel +10

Based on color-magnitude diagrams (CMDs) from the Hubble Space Telescope Hubble Tarantula Treasury Project (HTTP) survey, we present the star formation history (SFH) of Hodge~301,…

astro-ph.HE2015★ 33 cited

What Powers the 3000-Day Light Curve of SN 2006gy?

Ori D. Fox, Nathan Smith, S. Mark Ammons +11

SN 2006gy was the most luminous SN ever observed at the time of its discovery and the first of the newly defined class of superluminous supernovae (SLSNe). The extraordinary energe…

astro-ph.GA2013★ 66 cited

Hubble Tarantula Treasury Project: Unraveling Tarantula's Web. I. Observational overview and first results

E. Sabbi, J. Anderson, D. J. Lennon +18

The Hubble Tarantula Treasury Project (HTTP) is an ongoing panchromatic imaging survey of stellar populations in the Tarantula Nebula in the Large Magellanic Cloud that reaches int…

astro-ph.CO2012★ 23 cited

Optical and Infrared Analysis of Type II SN 2006BC

Joseph S. Gallagher, B. E. K. Sugerman, Geoffrey C. Clayton +8

We present nebular phase optical imaging and spectroscopy and near/mid-IR imaging of the Type II SN 2006bc. Observations reveal the central wavelength of the symmetric H line pr…

astro-ph.CO2012★ 73 cited

The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101

T. Matheson, R. R. Joyce, L. E. Allen +42

We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light cur…