activity
20112026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 7.5k across the 112 of their papers we have counts for

collaborators
Showing 2020Show all

12 papers · 1 filter

astro-ph.IM2020★ 29 cited

The ZTF Source Classification Project: II. Periodicity and variability processing metrics

Michael W. Coughlin, Kevin Burdge, Dmitry A. Duev +22

The current generation of all-sky surveys is rapidly expanding our ability to study variable and transient sources. These surveys, with a variety of sensitivities, cadences, and fi…

astro-ph.HE2020★ 104 cited

Optical follow-up of the neutron star-black hole mergers S200105ae and S200115j

Shreya Anand, Michael W. Coughlin, Mansi M. Kasliwal +46

LIGO and Virgo's third observing run (O3) revealed the first neutron star-black hole (NSBH) merger candidates in gravitational waves. These events are predicted to synthesize r-pro…

astro-ph.HE2020★ 168 cited

A large fraction of hydrogen-rich supernova progenitors experience elevated mass loss shortly prior to explosion

Rachel J. Bruch, Avishay Gal-Yam, Steve Schulze +43

Spectroscopic detection of narrow emission lines traces the presence of circumstellar mass distributions around massive stars exploding as core-collapse supernovae. Transient emiss…

astro-ph.HE2020★ 34 cited

A non-equipartition shockwave traveling in a dense circumstellar environment around SN2020oi

Assaf Horesh, Itai Sfaradi, Mattias Ergon +34

We report the discovery and panchromatic followup observations of the young Type Ic supernova, SN2020oi, in M100, a grand design spiral galaxy at a mere distance of Mpc. We fo…

astro-ph.SR2020★ 30 cited

Helium-rich Superluminous Supernovae From the Zwicky Transient Facility

Lin Yan, D. Perley, S. Schulze +39

Helium is expected to be present in the ejecta of some hydrogen-poor superluminous supernovae (SLSN-I). However, so far only one event, PTF10hgi has been identified with He feature…

astro-ph.CO2020★ 66 cited

Redshift evolution of the underlying type Ia supernova stretch distribution

N. Nicolas, M. Rigault, Y. Copin +7

The detailed nature of type Ia supernovae (SNe Ia) remains uncertain, and as survey statistics increase, the question of astrophysical systematic uncertainties arises, notably that…