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

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12 papers · 1 filter

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.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.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.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.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.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.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…