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20002026
most citedImproved Cosmological Constraints from New, Old and Combined Supernova Datasets

1.6k citations · 12.2k across the 89 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2022★ 7 cited

Bump Morphology of the CMAGIC Diagram

L. Aldoroty, L. Wang, P. Hoeflich +38

We apply the color-magnitude intercept calibration method (CMAGIC) to the Nearby Supernova Factory SNe Ia spectrophotometric dataset. The currently existing CMAGIC parameters are t…

astro-ph.SR2017★ 19 cited

The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu

X. Huang, Z. Raha, G. Aldering +39

Correction of Type Ia Supernova brightnesses for extinction by dust has proven to be a vexing problem. Here we study the dust foreground to the highly reddened SN 2012cu, which is…

astro-ph.SR2016★ 8 cited

Optical and ultraviolet spectroscopic analysis of SN 2011fe at late times

Brian Friesen, E. Baron, Jerod T. Parrent +16

We present optical spectra of the nearby Type Ia supernova SN 2011fe at 100, 205, 311, 349, and 578 days post-maximum light, as well as an ultraviolet spectrum obtained with Hubble…

astro-ph.SR2016★ 100 cited

DES14X3taz: A Type I Superluminous Supernova Showing a Luminous, Rapidly Cooling Initial Pre-Peak Bump

M. Smith, M. Sullivan, C. B. D'Andrea +81

We present DES14X3taz, a new hydrogen-poor super luminous supernova (SLSN-I) discovered by the Dark Energy Survey (DES) supernova program, with additional photometric data provided…

astro-ph.SR2015★ 12 cited

Spectral Models for Early Time SN 2011fe Observations

E. Baron, P. Hoeflich Brian Friesen, M. Sullivan +11

We use observed UV through near IR spectra to examine whether SN 2011fe can be understood in the framework of Branch-normal SNe Ia and to examine its individual peculiarities. As a…

astro-ph.SR2014★ 35 cited

Near-infrared line identification in type Ia supernovae during the transitional phase

Brian Friesen, E. Baron, John P. Wisniewski +4

We present near-infrared synthetic spectra of a delayed-detonation hydrodynamical model and compare them to observed spectra of four normal type Ia supernovae ranging from day +56.…