activity
19962026
most citedFirst-year Sloan Digital Sky Survey-II (SDSS-II) Supernova Results: Hubble Diagram and Cosmological Parameters

696 citations · 2.8k across the 40 of their papers we have counts for

collaborators

41 papers

astro-ph.HE2026

Fast and furious -- High-velocity features of Ca and Si in the spectra of Type Ia supernovae

Zsófia Bora, József Vinkó, J. Craig Wheeler +2

High velocity absorption lines of Ca II and Si II (high-velocity features, HVFs) are common in the early spectra of Type Ia supernovae (SNe Ia), but their physical origin is still…

astro-ph.SR2025★ 2 cited

SN 2022ngb: A faint, slowly evolving Type IIb supernova with a low-mass envelope

J. -W. Zhao, S. Benetti, Y. -Z. Cai +35

An extensive photometric and spectroscopic follow-up campaign of the Type IIb SN 2022ngb is presented in the article. Through detailed modeling of this dataset, we aim to constrain…

astro-ph.GA2025

North+Lone Star Supernova Host Survey I: Local Host-Galaxy H Surface Brightness and the Hubble Residuals of Type Ia Supernovae

Ann M. Isaacs, Patrick Kelly, J. Craig Wheeler

We present optical integral-field unit (IFU) spectroscopy acquired with the George and Cynthia Mitchell Spectrograph on the Harlan J. Smith telescope at McDonald Observatory of 94…

astro-ph.HE2024★ 12 cited

Luminous Type II Short-Plateau SN 2023ufx: Asymmetric Explosion of a Partially-Stripped Massive Progenitor

Aravind P. Ravi, Stefano Valenti, Yize Dong +34

We present supernova (SN) 2023ufx, a unique Type IIP SN with the shortest known plateau duration ( 47 days), a luminous V-band peak ( = 18.42 0…

astro-ph.HE2024

Optical Spectroscopy of Type Ia Supernovae by the Carnegie Supernova Projects I and II

N. Morrell, M. M. Phillips, G. Folatelli +57

We present the second and final release of optical spectroscopy of Type Ia Supernovae (SNe Ia) obtained during the first and second phases of the Carnegie Supernova Project (CSP-I…

astro-ph.GA2023

The Pre-explosion Environments and The Progenitor of SN 2023ixf from the Hobby Eberly Telescope Dark Energy Experiment (HETDEX)

Chenxu Liu, Xinlei Chen, Xinzhong Er +20

Supernova (SN) 2023ixf was discovered on May 19th, 2023. The host galaxy, M101, was observed by the Hobby Eberly Telescope Dark Energy Experiment (HETDEX) collaboration over the pe…

astro-ph.HE2023★ 3 cited

SN 2022oqm: A Bright and Multi-peaked Calcium-rich Transient

S. Karthik Yadavalli, V. Ashley Villar, Luca Izzo +60

We present the photometric and spectroscopic evolution of SN 2022oqm, a nearby multi-peaked hydrogen- and helium-weak calcium-rich transient (CaRT). SN 2022oqm was detected 13.1 kp…

astro-ph.GA2021★ 15 cited

The Stars of the HETDEX Survey. I. Radial Velocities and Metal-Poor Stars from Low-Resolution Stellar Spectra

Keith Hawkins, Greg Zeimann, Chris Sneden +18

The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) is an unbiased, massively multiplexed spectroscopic survey, designed to measure the expansion history of the universe thr…

astro-ph.HE2020★ 18 cited

The Exotic Type Ic Broad-Lined Supernova SN 2018gep: Blurring the Line Between Supernovae and Fast Optical Transients

T. A. Pritchard, Katarzyna Bensch, Maryam Modjaz +28

In the last decade a number of rapidly evolving transients have been discovered that are not easily explained by traditional supernovae models. We present optical and UV data on on…

astro-ph.HE2018★ 15 cited

Optical Observations of the Young Type Ic Supernova SN 2014L in M99

Jujia Zhang, Xiaofeng Wang, József Vinkó +22

We present optical spectroscopic and photometric observations of the nearby type Ic supernova (SN Ic) SN 2014L. This SN was discovered by the Tsinghua-NAOC Transient Survey (TNTS)…

astro-ph.SR2018★ 28 cited

The double-peaked radio light curve of PTF11qcj

N. T. Palliyaguru, A. Corsi, D. A. Frail +6

We present continued radio follow-up observations of PTF11qcj, a highly energetic broad-lined Type Ic supernova (SN), with a radio peak luminosity comparable to that of the -ray…

astro-ph.HE2017★ 69 cited

GW170817 Most Likely Made a Black Hole

David Pooley, Pawan Kumar, J. Craig Wheeler +1

There are two outstanding issues regarding the neutron-star merger event GW170817: the nature of the compact remnant and the interstellar shock. The mass of the remnant of GW170817…

astro-ph.HE2016★ 9 cited

Differentially Rotating White Dwarfs I: Regimes of Internal Rotation

Pranab Ghosh, J. Craig Wheeler

Most viable models of Type Ia supernovae (SN~Ia) require the thermonuclear explosion of a carbon/oxygen white dwarf that has evolved in a binary system. Rotation could be an import…

astro-ph.HE2016★ 36 cited

Extreme Supernova Models for the Superluminous Transient ASASSN-15lh

E. Chatzopoulos, J. C. Wheeler, J. Vinko +3

The recent discovery of the unprecedentedly superluminous transient ASASSN-15lh (or SN 2015L) with its UV-bright secondary peak challenges all the power-input models that have been…

astro-ph.HE2015★ 27 cited

Supernova 2013fc in a circumnuclear ring of a luminous infrared galaxy: the big brother of SN 1998S

T. Kangas, S. Mattila, E. Kankare +30

We present photometric and spectroscopic observations of SN 2013fc, a bright type II supernova (SN) in a circumnuclear star-forming ring in the luminous infrared galaxy ESO 154-G01…

astro-ph.SR2015★ 64 cited

Extensive Spectroscopy and Photometry of the Type IIP Supernova 2013ej

G. Dhungana, R. Kehoe, J. Vinko +32

We present extensive optical (, , and open CCD) and near-infrared () photometry for the very nearby Type IIP SN ~2013ej extending from +1 to +461 days after…

astro-ph.HE2014★ 3 cited

The Optical Luminosity Function of Gamma-ray Bursts deduced from ROTSE-III Observations

X. H. Cui, X. F. Wu, J. J. Wei +16

We present the optical luminosity function (LF) of gamma-ray bursts (GRBs) estimated from a uniform sample of 58 GRBs from observations with the Robotic Optical Transient Search Ex…

astro-ph.GA2014★ 225 cited

Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies

G. Leloudas, S. Schulze, T. Kruehler +16

Superluminous supernovae (SLSNe) are very bright explosions that were only discovered recently and that show a preference for occurring in faint dwarf galaxies. Understanding why s…

astro-ph.SR2014★ 26 cited

The Role of the Magnetorotational Instability in the Sun

Daniel Kagan, J. Craig Wheeler

We calculate growth rates for nonaxisymmetric instabilities including the magnetorotational instability (MRI) throughout the Sun. We first derive a dispersion relation for nonaxisy…

astro-ph.CO2014★ 213 cited

The Data Release of the Sloan Digital Sky Survey-II Supernova Survey

Masao Sako, Bruce Bassett, Andrew C. Becker +46

This paper describes the data release of the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey conducted between 2005 and 2007. Light curves, spectra, classifications, and anc…

astro-ph.CO2013★ 104 cited

The Very Young Type Ia Supernova 2013dy: Discovery, and Strong Carbon Absorption in Early-Time Spectra

WeiKang Zheng, Jeffrey M. Silverman, Alexei V. Filippenko +20

The Type Ia supernova (SN Ia) 2013dy in NGC 7250 (d ~ 13.7 Mpc) was discovered by the Lick Observatory Supernova Search. Combined with a prediscovery detection by the Italian Super…

astro-ph.SR2012★ 59 cited

The morphology of the ejecta in Supernova 1987A: a study over time and wavelength

Josefin Larsson, Claes Fransson, Karina Kjaer +9

We present a study of the morphology of the ejecta in Supernova 1987A based on images and spectra from the HST as well as integral field spectroscopy from VLT/SINFONI. The HST obse…

astro-ph.HE2012★ 6 cited

The Unusually Luminous Extragalactic Nova SN 2010U

Ian Czekala, E. Berger, R. Chornock +10

We present observations of the unusual optical transient SN 2010U, including spectra taken 1.03 days to 15.3 days after maximum light that identify it as a fast and luminous Fe II…

astro-ph.SR2012★ 58 cited

White Dwarf/M Dwarf Binaries as Single Degenerate Progenitors of Type Ia Supernovae

J. Craig Wheeler

Limits on the companions of white dwarfs in the single degenerate scenario for the origin of Type Ia supernovae (SNIa) have gotten increasingly tight. The only type of non-degenera…