activity
20182020
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 3.1k across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2020

Seventeen Tidal Disruption Events from the First Half of ZTF Survey Observations: Entering a New Era of Population Studies

Sjoert van Velzen, Suvi Gezari, Erica Hammerstein +34

While tidal disruption events (TDEs) have long been heralded as laboratories for the study of quiescent black holes, the small number of known TDEs and uncertainties in their emiss…

astro-ph.IM2019

Transient processing and analysis using : Alert Management, Photometry and Evaluation of Lightcurves

J. Nordin, V. Brinnel, J. van Santen +18

Both multi-messenger astronomy and new high-throughput wide-field surveys require flexible tools for the selection and analysis of astrophysical transients. We here introduce the A…

astro-ph.IM2019148 cited

A Fully Automated Integral Field Spectrograph Pipeline for the SEDMachine: pysedm

M. Rigault, J. D. Neill, N. Blagorodnova +8

Current time domain facilities are discovering hundreds of new galactic and extra-galactic transients every week. Classifying the ever-increasing number of transients is challengin…

astro-ph.IM2019850 cited

The Zwicky Transient Facility: Science Objectives

Matthew J. Graham, S. R. Kulkarni, Eric C. Bellm +114

The Zwicky Transient Facility (ZTF), a public-private enterprise, is a new time domain survey employing a dedicated camera on the Palomar 48-inch Schmidt telescope with a 47 deg$^2…

astro-ph.IM20192.1k cited

The Zwicky Transient Facility: System Overview, Performance, and First Results

Eric C. Bellm, Shrinivas R. Kulkarni, Matthew J. Graham +112

The Zwicky Transient Facility (ZTF) is a new optical time-domain survey that uses the Palomar 48-inch Schmidt telescope. A custom-built wide-field camera provides a 47 deg fiel…

astro-ph.IM2019

: Estimating Transient Discovery Rates for the Zwicky Transient Facility

Ulrich Feindt, Jakob Nordin, Mickael Rigault +4

When planning a survey for astronomical transients, many factors such as cadence, filter choice, sky coverage, and depth of observations need to be balanced in order to optimize th…