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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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22 papers · 1 filter

astro-ph.HE2025

ZTF SN Ia DR2 follow-up: Characterization of subluminous Type Ia supernovae in the ZTF DR2 full sample

Alaa Alburai, Lluís Galbany, Umut Burgaz +19

The Zwicky Transient Facility Data Release 2 (ZTF DR2) includes a total of 3,628 Type Ia supernovae (SNe~Ia), providing the largest and most complete sample of spectroscopically co…

astro-ph.HE2023★ 5 cited

Early-time spectroscopic modelling of the transitional Type Ia Supernova 2021rhu with TARDIS

Luke Harvey, Kate Maguire, Mark R. Magee +15

An open question in SN Ia research is where the boundary lies between 'normal' Type Ia supernovae (SNe Ia) that are used in cosmological measurements and those that sit off the Phi…

astro-ph.HE2022★ 96 cited

The prevalence and influence of circumstellar material around hydrogen-rich supernova progenitors

Rachel J. Bruch, Avishay Gal-Yam, Ofer Yaron +44

Narrow transient emission lines (flash-ionization features) in early supernova (SN) spectra trace the presence of circumstellar material (CSM) around the massive progenitor stars o…

astro-ph.HE2022★ 49 cited

The Young Supernova Experiment Data Release 1 (YSE DR1): Light Curves and Photometric Classification of 1975 Supernovae

P. D. Aleo, K. Malanchev, S. Sharief +80

We present the Young Supernova Experiment Data Release 1 (YSE DR1), comprised of processed multi-color Pan-STARRS1 (PS1) griz and Zwicky Transient Facility (ZTF) gr photometry of 1…

astro-ph.HE2022

SN 2020jgb: A Peculiar Type Ia Supernova Triggered by a Helium-Shell Detonation in a Star-Forming Galaxy

Chang Liu, Adam A. Miller, Abigail Polin +25

The detonation of a thin () helium shell (He-shell) atop a white dwarf (WD) is a promising mechanism to explain normal…

astro-ph.HE2022★ 1 cited

Multi-messenger constraints on the Hubble constant through combination of gravitational waves, gamma-ray bursts and kilonovae from neutron star mergers

Mattia Bulla, Michael W. Coughlin, Suhail Dhawan +1

The simultaneous detection of gravitational waves and light from the binary neutron star merger GW170817 led to independent measurements of distance and redshift, providing a direc…

astro-ph.HE2022★ 14 cited

The detection efficiency of type Ia supernovae from the Zwicky Transient Facility: Limits on the intrinsic rate of early flux excesses

M. R. Magee, C. Cuddy, K. Maguire +8

Samples of young type Ia supernovae have shown `early excess' emission in a few cases. Similar excesses are predicted by some explosion and progenitor scenarios and hence can provi…

astro-ph.HE2022★ 209 cited

The Final Season Reimagined: 30 Tidal Disruption Events from the ZTF-I Survey

Erica Hammerstein, Sjoert van Velzen, Suvi Gezari +30

Tidal disruption events (TDEs) offer a unique way to study dormant black holes. While the number of observed TDEs has grown thanks to the emergence of wide-field surveys in the pas…

astro-ph.HE2021★ 16 cited

Supernova Siblings and their Parent Galaxies in the Zwicky Transient Facility Bright Transient Surve

M. L. Graham, C. Fremling, D. A. Perley +19

Supernova (SN) siblings -- two or more SNe in the same parent galaxy -- are useful tools for exploring progenitor stellar populations as well as properties of the host galaxies suc…

astro-ph.HE2021★ 28 cited

Less than 1% of Core-Collapse Supernovae in the local universe occur in elliptical galaxies

I. Irani, S. J. Prentice, S. Schulze +39

We present observations of three Core-collapse supernovae (CCSNe) in elliptical hosts, detected by the Zwicky Transient Facility Bright Transient Survey (BTS). SN 2019ape is a SN I…

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★ 50 cited

The Spectacular Ultraviolet Flash From the Peculiar Type Ia Supernova 2019yvq

A. A. Miller, M. R. Magee, A. Polin +42

Early observations of Type Ia supernovae (SNeIa) provide essential clues for understanding the progenitor system that gave rise to the terminal thermonuclear explosion. We pres…

astro-ph.HE2020★ 40 cited

ZTF Early Observations of Type Ia Supernovae III: Early-Time Colors as a Test for Explosion Models and Multiple Populations

Mattia Bulla, Adam A. Miller, Yuhan Yao +22

Colors of Type Ia supernovae in the first few days after explosion provide a potential discriminant between different models. In this paper, we present colors of 65 Type Ia s…

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.HE2018★ 13 cited

Characterising the secondary maximum in the r-band for Type Ia Supernovae: Diagnostic for the ejecta mass

Seméli Papadogiannakis, Suhail Dhawan, Roberta Morosin +1

An increase in the number of studied Type Ia supernovae (SNe~Ia) has demonstrated that this class of explosions has a greater diversity in its observables than was previously assum…

astro-ph.HE2018★ 23 cited

R-band light-curve properties of Type Ia supernovae from the (intermediate) Palomar Transient Factory

S. Papadogiannakis, A. Goobar, R. Amanullah +15

We present the best 265 sampled R-band light curves of spectroscopically identified Type Ia supernovae (SNe) from the Palomar Transient Factory (PTF; 2009-2012) survey and the inte…

astro-ph.HE2018★ 17 cited

Limits on stable iron in TypeIa supernovae from NIR spectroscopy

A. Flörs, J. Spyromilio, K. Maguire +3

We obtained optical and near-infrared spectra of TypeIa supernovae (SNeIa) at epochs ranging from 224 to 496 days after the explosion. The spectra show emission lines from…

astro-ph.HE2018★ 20 cited

iPTF16abc and the population of Type Ia supernovae: Comparing the photospheric, transitional and nebular phases

S. Dhawan, M. Bulla, A. Goobar +6

Key information about the progenitor system and the explosion mechanism of Type Ia supernovae (SNe~Ia) can be obtained from early observations, within a few days from explosion. iP…

astro-ph.HE2018★ 29 cited

Nebular spectroscopy of SN 2014J: Detection of stable nickel in near infrared spectra

S. Dhawan, A. Flörs, B. Leibundgut +5

We present near infrared (NIR) spectroscopy of the nearby supernova 2014J obtained 450 d after explosion. We detect the [Ni II] 1.939 m line in the spectra indicating the…

astro-ph.HE2018★ 31 cited

Shedding light on the Type Ia supernova extinction puzzle: dust location found

M. Bulla, A. Goobar, S. Dhawan

The colour evolution of reddened Type Ia supernovae can place strong constraints on the location of dust and help address the question of whether the observed extinction stems from…

astro-ph.HE2017★ 63 cited

Early Observations of the Type Ia Supernova iPTF 16abc: A Case of Interaction with Nearby, Unbound Material and/or Strong Ejecta Mixing

A. A. Miller, Y. Cao, A. L. Piro +19

Early observations of Type Ia supernovae (SNe Ia) provide a unique probe of their progenitor systems and explosion physics. Here we report the intermediate Palomar Transient Factor…