activity
20152019
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.5k across the 16 of their papers we have counts for

collaborators

15 papers

astro-ph.SR201933 cited

The Evolution of Luminous Red Nova AT 2017jfs in NGC 4470

A. Pastorello, T. -W. Chen, Y. -Z. Cai +43

We present the results of our photometric and spectroscopic follow-up of the intermediate-luminosity optical transient AT 2017jfs. At peak, the object reaches an absolute magnitude…

astro-ph.HE201783 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.CO201732 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.HE2017888 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.SR2017

Hydrogen-rich supernovae beyond the neutrino-driven core-collapse paradigm

G. Terreran, M. L. Pumo, T. -W. Chen +41

We present our study of OGLE-2014-SN-073, one of the brightest Type II SN ever discovered, with an unusually broad lightcurve combined with high ejecta velocities. From our hydrody…

astro-ph.GA201745 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…