activity
20002026
most citedProgenitors of core-collapse supernovae

1.2k citations · 25.3k across the 314 of their papers we have counts for

collaborators
Showing 2017Show all

15 papers · 1 filter

astro-ph.SR2017★ 50 cited

SN 2017dio: a type-Ic supernova exploding in a hydrogen-rich circumstellar medium

Hanindyo Kuncarayakti, Keiichi Maeda, Christopher J. Ashall +42

SN 2017dio shows both spectral characteristics of a type-Ic supernova (SN) and signs of a hydrogen-rich circumstellar medium (CSM). Prominent, narrow emission lines of H and He are…

astro-ph.HE2017★ 83 cited

A population of highly energetic transient events in the centres of active galaxies

E. Kankare, R. Kotak, S. Mattila +25

Recent all-sky surveys have led to the discovery of new types of transients. These include stars disrupted by the central supermassive black hole, and supernovae that are 10-100 ti…

astro-ph.CO2017★ 32 cited

Euclid: Superluminous supernovae in the Deep Survey

C. Inserra, R. C. Nichol, D. Scovacricchi +31

In the last decade, astronomers have found a new type of supernova called `superluminous supernovae' (SLSNe) due to their high peak luminosity and long light-curves. These hydrogen…

astro-ph.HE2017★ 888 cited

A kilonova as the electromagnetic counterpart to a gravitational-wave source

S. J. Smartt, T. -W. Chen, A. Jerkstrand +118

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to…

astro-ph.CO2017★ 151 cited

Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters

D. O. Jones, D. M. Scolnic, A. G. Riess +25

We use 1169 Pan-STARRS supernovae (SNe) and 195 low- () SNe Ia to measure cosmological parameters. Though most Pan-STARRS SNe lack spectroscopic classifications, in a p…

astro-ph.GA2017★ 45 cited

Spatially resolved MaNGA observations of the host galaxy of superluminous supernova 2017egm

Ting-Wan Chen, Patricia Schady, Lin Xiao +6

Superluminous supernovae (SLSNe) are found predominantly in dwarf galaxies, indicating that their progenitors have a low metallicity. However, the most nearby SLSN to date, SN 2017…