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20132026
most citedDoes the Hubble constant tension call for new physics?

280 citations · 2.9k across the 59 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

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.GA2019★ 32 cited

Magnification, dust and time-delay constraints from the first resolved strongly lensed Type Ia supernova

S. Dhawan, J. Johansson, A. Goobar +14

We report lensing magnifications, extinction, and time-delay estimates for the first resolved, multiply-imaged Type Ia supernova iPTF16geu, at , using $Hubble\,Space\,Te…

astro-ph.CO2019★ 27 cited

Lens modelling of the strongly lensed Type Ia supernova iPTF16geu

E. Mörtsell, J. Johansson, S. Dhawan +3

In 2016, the first strongly lensed Type Ia supernova, iPTF16geu at redshift with four resolved images arranged symmetrically around the lens galaxy at , was dis…

astro-ph.CO2019★ 7 cited

The Next Generation of Cosmological Measurements with Type Ia Supernovae

Dan Scolnic, Saul Perlmutter, Greg Aldering +56

While Type Ia Supernovae (SNe Ia) are one of the most mature cosmological probes, the next era promises to be extremely exciting in the number of different ways SNe Ia are used to…

astro-ph.IM2019★ 43 cited

: 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…