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most citedThe Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

2.7k citations · 5.9k across the 35 of their papers we have counts for

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astro-ph.CO2017★ 2.7k cited

The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

D. M. Scolnic, D. O. Jones, A. Rest +37

We present optical light curves, redshifts, and classifications for 365 spectroscopically confirmed Type Ia supernovae (SNe Ia) discovered by the Pan-STARRS1 (PS1) Medium Deep Surv…

astro-ph.CO2013★ 272 cited

Slowly fading super-luminous supernovae that are not pair-instability explosions

M. Nicholl, S. J. Smartt, A. Jerkstrand +57

Super-luminous supernovae that radiate more than 10^44 ergs per second at their peak luminosity have recently been discovered in faint galaxies at redshifts of 0.1-4. Some evolve s…

astro-ph.CO2013★ 170 cited

Systematic Uncertainties Associated with the Cosmological Analysis of the First Pan-STARRS1 Type Ia Supernova Sample

D. Scolnic, A. Rest, A. Riess +46

We probe the systematic uncertainties from 113 Type Ia supernovae (SNIa) in the Pan-STARRS1 (PS1) sample along with 197 SN Ia from a combination of low-redshift surveys. The compan…

astro-ph.CO2012★ 18 cited

An Independent Measurement of the Incidence of MgII Absorbers along Gamma-Ray Burst Sightlines: the End of the Mystery?

A. Cucchiara, J. X. Prochaska, G. Zhu +15

In 2006, Prochter et al. reported a statistically significant enhancement of very strong Mg II absorption systems intervening the sightlines to gamma-ray bursts (GRBs) relative to…

astro-ph.CO2012★ 65 cited

Ultra-Luminous Supernovae as a New Probe of the Interstellar Medium in Distant Galaxies

E. Berger, R. Chornock, R. Lunnan +27

We present the Pan-STARRS1 discovery and light curves, and follow-up MMT and Gemini spectroscopy of an ultra-luminous supernova (ULSN; dubbed PS1-11bam) at a redshift of z=1.566 wi…