activity
20092023
most citedThree Hypervelocity White Dwarfs in Gaia DR2: Evidence for Dynamically Driven Double-Degenerate Double-Detonation Type Ia Supernovae

249 citations · 3.9k across the 110 of their papers we have counts for

collaborators

112 papers

astro-ph.HE2023★ 2 cited

SN~2015da: Late-time observations of a persistent superluminous Type~IIn supernova with post-shock dust formation

Nathan Smith, Jennifer E. Andrews, Peter Milne +5

We present photometry and spectroscopy of the slowly evolving superluminous Type IIn SN2015da. SN2015da is extraordinary for its very high peak luminosity, and also for sustaining…

astro-ph.HE2023

Strong Carbon Features and a Red Early Color in the Underluminous Type Ia SN 2022xkq

Jeniveve Pearson, David J. Sand, Peter Lundqvist +85

We present optical, infrared, ultraviolet, and radio observations of SN 2022xkq, an underluminous fast-declining type Ia supernova (SN Ia) in NGC 1784 ( Mpc),…

astro-ph.HE2023

Serendipitous detection of the dusty Type IIL SN 1980K with JWST/MIRI

Szanna Zsíros, Tamás Szalai, Ilse De Looze +39

We present mid-infrared (mid-IR) imaging of the Type IIL supernova (SN) 1980K with the James Webb Space Telescope (JWST) more than 40 yr post-explosion. SN 1980K, located in the ne…

astro-ph.IM2023

SpectAcLE: An Improved Method for Modeling Light Echo Spectra

Roee Partoush, Armin Rest, Jacob E. Jencson +17

Light echoes give us a unique perspective on the nature of supernovae and non-terminal stellar explosions. Spectroscopy of light echoes can reveal details on the kinematics of the…

astro-ph.HE2023

Evidence of weak circumstellar medium interaction in the Type II SN 2023axu

Manisha Shrestha, Jeniveve Pearson, Samuel Wyatt +34

We present high-cadence photometric and spectroscopic observations of SN~2023axu, a classical Type II supernova with an absolute -band peak magnitude of mag. SN~…

astro-ph.HE2023★ 13 cited

Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties

Yize Dong, Stefano Valenti, Chris Ashall +52

We present optical and near-infrared observations of SN~2022crv, a stripped envelope supernova in NGC~3054, discovered within 12 hrs of explosion by the Distance Less Than 40 Mpc S…

astro-ph.HE2023

Ground-based and JWST Observations of SN 2022pul: I. Unusual Signatures of Carbon, Oxygen, and Circumstellar Interaction in a Peculiar Type Ia Supernova

Matthew R. Siebert, Lindsey A. Kwok, Joel Johansson +79

Nebular-phase observations of peculiar Type Ia supernovae (SNe Ia) provide important constraints on progenitor scenarios and explosion dynamics for both these rare SNe and the more…

astro-ph.SR2023★ 1 cited

Evidence for late-time dust formation in the ejecta of supernova SN~1995N from emission-line asymmetries

R. Wesson, A. M. Bevan, M. J. Barlow +4

We present a study of the dust associated with the core-collapse supernova SN~1995N. Infrared emission detected 14--15 years after the explosion was previously attributed to therma…

astro-ph.SR2023★ 83 cited

A Luminous Red Supergiant and Dusty Long-period Variable Progenitor for SN 2023ixf

Jacob E. Jencson, Jeniveve Pearson, Emma R. Beasor +23

We analyze pre-explosion near- and mid-infrared (IR) imaging of the site of SN 2023ixf in the nearby spiral galaxy M101 and characterize the candidate progenitor star. The star dis…

astro-ph.SR2023★ 3 cited

The SN 2023ixf Progenitor in M101: II. Properties

Schuyler D. Van Dyk, Sundar Srinivasan, Jennifer E. Andrews +12

We follow our first paper with an analysis of the ensemble of the extensive pre-explosion ground- and space-based infrared observations of the red supergiant (RSG) progenitor candi…

astro-ph.HE2023★ 25 cited

Ground-based and JWST Observations of SN 2022pul: II. Evidence from Nebular Spectroscopy for a Violent Merger in a Peculiar Type-Ia Supernova

Lindsey A. Kwok, Matthew R. Siebert, Joel Johansson +78

We present an analysis of ground-based and JWST observations of SN~2022pul, a peculiar "03fg-like" (or "super-Chandrasekhar") Type Ia supernova (SN Ia), in the nebular phase at 338…

astro-ph.HE2023★ 1 cited

A comprehensive optical search for pre-explosion outbursts from the quiescent progenitor of SN~2023ixf

Yize Dong, David J. Sand, Stefano Valenti +13

We perform a comprehensive search for optical precursor emission at the position of SN~2023ixf using data from the DLT40, ZTF and ATLAS surveys. By comparing the current data set w…

astro-ph.SR2023★ 3 cited

The SN 2023ixf Progenitor in M101: I. Infrared Variability

Monika D. Soraisam, Tamás Szalai, Schuyler D. Van Dyk +6

Observational evidence points to a red supergiant (RSG) progenitor for SN 2023ixf. The progenitor candidate has been detected in archival images at wavelengths (>0.6 micron) where…

astro-ph.HE2023★ 90 cited

Early Spectroscopy and Dense Circumstellar Medium Interaction in SN 2023ixf

K. Azalee Bostroem, Jeniveve Pearson, Manisha Shrestha +53

We present the optical spectroscopic evolution of SN~2023ixf seen in sub-night cadence spectra from 1.18 to 14 days after explosion. We identify high-ionization emission features,…

astro-ph.HE2023★ 80 cited

Shock Cooling and Possible Precursor Emission in the Early Light Curve of the Type II SN 2023ixf

Griffin Hosseinzadeh, Joseph Farah, Manisha Shrestha +28

We present the densely sampled early light curve of the Type II supernova (SN) 2023ixf, first observed within hours of explosion in the nearby Pinwheel Galaxy (Messier 101; 6.7 Mpc…

astro-ph.HE2023★ 6 cited

Observational properties of a bright type Iax SN 2018cni and a faint type Iax SN 2020kyg

Mridweeka Singh, Devendra. K. Sahu, Raya Dastidar +29

We present the optical photometric and spectroscopic analysis of two type Iax SNe 2018cni and 2020kyg. SN 2018cni is a bright type Iax SN (M = 17.810.21 mag) whe…

astro-ph.HE2023★ 2 cited

A Low-Mass Helium Star Progenitor Model for the Type Ibn SN 2020nxt

Qinan Wang, Anika Goel, Luc Dessart +55

A growing number of supernovae (SNe) are now known to exhibit evidence for significant interaction with a dense, pre-existing, circumstellar medium (CSM). SNe Ibn comprise one such…

astro-ph.HE2023★ 17 cited

The Early Light Curve of SN 2023bee: Constraining Type Ia Supernova Progenitors the Apian Way

Griffin Hosseinzadeh, David J. Sand, Sumit K. Sarbadhicary +39

We present very early photometric and spectroscopic observations of the Type Ia supernova (SN Ia) 2023bee, starting about 8 hr after the explosion, which reveal a strong excess in…

astro-ph.HE2023★ 24 cited

SN 2022acko: the First Early Far-Ultraviolet Spectra of a Type IIP Supernova

K. Azalee Bostroem, Luc Dessart, D. John Hillier +41

We present five far- and near-ultraviolet spectra of the Type II plateau supernova, SN 2022acko, obtained 5, 6, 7, 19, and 21 days after explosion, all observed with the Hubble Spa…

astro-ph.HE2023

Multi-Epoch Spectropolarimetry for a Sample of Type IIn Supernovae: Persistent Asymmetry in Dusty Circumstellar Material

Christopher Bilinski, Nathan Smith, G. Grant Williams +5

We present multi-epoch spectropolarimetry and spectra for a sample of 14 Type IIn supernovae (SNe IIn). We find that after correcting for likely interstellar polarization, SNe IIn…

astro-ph.SR2023★ 7 cited

Don't believe the hype(r): The Yellow Supergiants of Westerlund 1

Emma R. Beasor, Nathan Smith, Jennifer E. Andrews

Yellow hypergiants (YHGs) are often presumed to represent a transitional post-red supergiant (RSG) phase for stars 30-40 \msun. Here we present visual-wavelength echelle spec…

astro-ph.HE2023★ 26 cited

Limit on Supernova Emission in the Brightest Gamma-ray Burst, GRB 221009A

Manisha Shrestha, David J. Sand, Kate D. Alexander +30

We present photometric and spectroscopic observations of the extraordinary gamma-ray burst (GRB) 221009A in search of an associated supernova. Some past GRBs have shown bumps in th…

astro-ph.HE2023★ 29 cited

JWST Low-Resolution MIRI Spectral Observations of SN~2021aefx: High-density Burning in a Type Ia Supernova

J. M. DerKacy, C. Ashall, P. Hoeflich +38

We present a JWST/MIRI low-resolution mid-infrared (MIR) spectroscopic observation of the normal Type Ia supernova (SN Ia) SN 2021aefx at +323 days past rest-frame B-band maximum l…

astro-ph.SR2023★ 2 cited

The Superluminous Type IIn Supernova ASASSN-15ua: Part of a continuum in extreme precursor mass loss

Danielle Dickinson, Nathan Smith, Jennifer E. Andrews +3

We present a series of ground-based photometry and spectroscopy of the superluminous Type IIn supernova (SN) ASASSN-15ua, which shows evidence for strong interaction with pre-exist…