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20142026
most citedThe Zwicky Transient Facility: System Overview, Performance, and First Results

2.1k citations · 8.4k across the 119 of their papers we have counts for

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Showing 2019Show all

13 papers · 1 filter

astro-ph.HE2019★ 54 cited

Monte Carlo radiative transfer for the nebular phase of Type Ia supernovae

L. J. Shingles, S. A. Sim, M. Kromer +9

We extend the range of validity of the ARTIS 3D radiative transfer code up to hundreds of days after explosion, when Type Ia supernovae are in their nebular phase. To achieve this,…

astro-ph.HE2019★ 106 cited

ZTF Early Observations of Type Ia Supernovae I: Properties of the 2018 Sample

Yuhan Yao, Adam A. Miller, S. R. Kulkarni +32

Early-time observations of Type Ia supernovae (SNe Ia) are essential to constrain their progenitor properties. In this paper, we present high-quality light curves of 127 SNe Ia dis…

astro-ph.HE2019★ 109 cited

GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-Infrared Counterpart to a Neutron Star-Black Hole Merger

Igor Andreoni, Daniel A. Goldstein, Mansi M. Kasliwal +49

On 2019 August 14, the Advanced LIGO and Virgo interferometers detected the high-significance gravitational wave (GW) signal S190814bv. The GW data indicated that the event resulte…

astro-ph.HE2019★ 93 cited

Implications of the search for optical counterparts during the first six months of the Advanced LIGO's and Advanced Virgo's third observing run: possible limits on the ejecta mass and binary properties

Michael W. Coughlin, Tim Dietrich, Sarah Antier +6

GW170817 showed that neutron star mergers not only emit gravitational waves but also can release electromagnetic signatures in multiple wavelengths. Within the first half of the th…

astro-ph.HE2019★ 76 cited

Linear spectropolarimetry of 35 Type Ia Supernovae with VLT/FORS: An analysis of the Si II line polarization

Aleksandar Cikota, Ferdinando Patat, Lifan Wang +9

Spectropolarimetry enables us to measure the geometry and chemical structure of the ejecta in supernova explosions, which is fundamental for the understanding of their explosion me…

astro-ph.HE2019★ 57 cited

On standardizing kilonovae and their use as standard candles to measure the Hubble constant

Michael W. Coughlin, Tim Dietrich, Jack Heinzel +6

The detection of GW170817 is revolutionizing many areas of astrophysics with the joint observation of gravitational waves and electromagnetic emissions. These multi-messenger event…

astro-ph.HE2019★ 33 cited

The aspherical explosion of the Type IIP SN 2017gmr

T. Nagao, A. Cikota, F. Patat +7

Type IIP supernovae (SNe IIP), which represent the most common class of core-collapse (CC) SNe, show a rapid increase in continuum polarization just after entering the tail phase.…

astro-ph.HE2019★ 39 cited

GROWTH on S190510g: DECam Observation Planning and Follow-Up of a Distant Binary Neutron Star Merger Candidate

Igor Andreoni, Daniel A. Goldstein, Shreya Anand +23

The first two months of the third Advanced LIGO and Virgo observing run (2019 April-May) showed that distant gravitational wave (GW) events can now be readily detected. Three candi…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…

astro-ph.SR2019★ 49 cited

On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion

Lluís Galbany, Chris Ashall, Peter Hoeflich +46

We present a comprehensive dataset of optical and near-infrared photometry and spectroscopy of type~Ia supernova (SN) 2016hnk, combined with integral field spectroscopy (IFS) of it…

astro-ph.IM2019★ 102 cited

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.IM2019★ 850 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.IM2019★ 2.1k 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…