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20072026
most citedLight Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

839 citations · 5.3k across the 62 of their papers we have counts for

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Showing 2015Show all

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astro-ph.HE2015★ 71 cited

Almost Gone: SN~2008S and NGC~300 2008OT-1 are Fainter than their Progenitors

S. M. Adams, C. S. Kochanek, J. L. Prieto +3

We present late-time Hubble and Spitzer Space Telescope imaging of SN 2008S and NGC 300 2008OT-1, the prototypes of a common class of stellar transients whose true nature is debate…

astro-ph.SR2015★ 31 cited

Massive stars exploding in a He-rich circumstellar medium - VII. The metamorphosis of ASASSN-15ed from a narrow line Type Ibn to a normal Type Ib Supernova

A. Pastorello, J. L. Prieto, N. Elias-Rosa +39

We present the results of the spectroscopic and photometric monitoring campaign of ASASSN-15ed. The transient was discovered quite young by the All Sky Automated Survey for SuperNo…

astro-ph.HE2015★ 324 cited

Six Months of Multi-Wavelength Follow-up of the Tidal Disruption Candidate ASASSN-14li and Implied TDE Rates from ASAS-SN

T. W. -S. Holoien, C. S. Kochanek, J. L. Prieto +21

We present ground-based and Swift photometric and spectroscopic observations of the candidate tidal disruption event (TDE) ASASSN-14li, found at the center of PGC 043234 ($d\simeq9…

astro-ph.HE2015★ 48 cited

Optical observations of the luminous Type IIn Supernova 2010jl for over 900 days

J. E. Jencson, J. L. Prieto, C. S. Kochanek +3

The luminous Type IIn Supernova (SN) 2010jl shows strong evidence for the interaction of the SN ejecta with dense circumstellar material (CSM). We present observations of SN 2010jl…

astro-ph.SR2015★ 45 cited

Massive stars exploding in a He-rich circumstellar medium. V. Observations of the slow-evolving SN Ibn OGLE-2012-SN-006

A. Pastorello, L. Wyrzykowski, S. Valenti +36

We present optical observations of the peculiar Type Ibn supernova (SN Ibn) OGLE-2012-SN-006, discovered and monitored by the OGLE-IV survey, and spectroscopically followed by PESS…