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19972026
most citedSN 2003du: 480 days in the Life of a Normal Type Ia Supernova

182 citations · 1.2k across the 29 of their papers we have counts for

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astro-ph2007★ 182 cited

SN 2003du: 480 days in the Life of a Normal Type Ia Supernova

V. Stanishev, A. Goobar, S. Benetti +29

An extensive set of optical and NIR photometry and low-resolution spectra the Type Ia supernova (SN Ia) 2003du was obtained using a number of facilities. The observations started 1…

astro-ph2007★ 105 cited

Signatures of Delayed Detonation, Asymmetry, and Electron Capture in the Mid-Infrared Spectra of Supernovae 2003hv and 2005df

Christopher L. Gerardy, W. P. S. Meikle, Rubina Kotak +10

We present the first mid-infrared (5.2-15.2 micron) spectra of Type Ia supernovae (SNe 2003hv and 2005df). The detection of Ni emission in SN 2005df 135 days after the explosion pr…

astro-ph2005★ 21 cited

The Near-UV Pulse Profile and Spectrum of the Pulsar PSR B0656+14

Yu. A. Shibanov, J. Sollerman, P. Lundqvist +2

We have observed the middle-aged pulsar PSR B0656+14 with the prism and the NUV MAMA detector of the Space Telescope Imaging Spectrograph (STIS) to measure the pulsar spectrum and…

astro-ph2003★ 47 cited

The Vela Pulsar in the Near-Infrared

Y. A. Shibanov, A. B. Koptsevich, J. Sollerman +1

We report on the first detection of the Vela pulsar in the near-infrared with the VLT/ISAAC in the Js and H bands. The pulsar magnitudes are Js=22.71 +/- 0.10 and H=22.04 +/- 0.16.…

astro-ph2002★ 107 cited

Spectropolarimetry of the Type Ic SN 2002ap in M74: More Evidence for Asymmetric Core Collapse

Lifan Wang, Dietrich Baade, Peter Hoeflich +3

High-quality spectropolarimetric data of SN 2002ap were obtained with the ESO Very Large Telescope Melipal (+ FORS1) at 3 epochs that correspond to -6, -2, and +1 days for a V maxi…

astro-ph2001★ 27 cited

ISO/SWS observations of SN 1987A: II. A refined upper limit on the mass of Ti-44 in the ejecta of SN 1987A

P. Lundqvist, C. Kozma, J. Sollerman +1

ISO/SWS observations of SN 1987A on day 3425 show no emission in [Fe I] 24.05 microns and [Fe II] 25.99 microns down to the limits of roughly 0.39 Jy and 0.64 Jy, respectively. Ass…