activity
20192026
most citedSupernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries

9 citations · 18 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

Disco in the Dust: Reflected light at the bow shock around Betelgeuse's companion explains its observed luminosity

Jared A. Goldberg, Meridith Joyce, Anna J. G. O'Grady +6

Recent detections of Orionis B, the putative companion to Betelgeuse, have been reported using multiple instruments and techniques. These include, most recently, a detect…

astro-ph.HE2026

Pinning Down the Geometry of the Type Ic Broad-Line Supernova 2026gzf

Xudong Wen, Yi Yang, Jing Lu +11

Type Ic broad-line supernovae (SNe Ic-BL) are often associated with energetic explosions that display a prompt outburst of high-energy emission. Since their progenitor lost the H a…

cs.IR2026

Traditional statistical representations outperform generative AI in identifying expert peer reviewers

Vicente Amado Olivo, Tereza Jerabkova, Jakub Klencki +5

The exponential growth of scientific submissions has strained the peer review system. Despite the rapidly expanding global pool of researchers, this unprecedented scale has rendere…

astro-ph.HE2026

Type Ib supernovae are bluer than Type Ic supernovae

Harim Jin, Selma E. de Mink, Sebastian Holzner +5

Type Ib and Ic supernovae (SNe Ib/Ic) are the bright finale of massive stars that have lost their hydrogen envelopes, making them powerful probes of mass stripping in massive star…

astro-ph.HE2026

Traces of Helium Detected in Type Ic Supernova 2014L

Jing Lu, Wolfgang E. Kerzendorf, John T. O'Brien +6

The absence of helium features in optical spectra is one of the classification criteria for Type Ic supernovae (SNe Ic). However, it is highly debated whether helium is truly absen…

astro-ph.IM2025

Practical Author Name Disambiguation under Metadata Constraints: A Contrastive Learning Approach for Astronomy Literature

Vicente Amado Olivo, Wolfgang Kerzendorf, Bangjing Lu +3

The ability to distinctly and properly collate an individual researcher's publications is crucial for ensuring appropriate recognition, guiding the allocation of research funding a…

astro-ph.HE2025

Effect of positronium on the -ray spectra and energy deposition in Type Ia supernovae

Anirban Dutta, Andrew Fullard, Wolfgang Kerzendorf +5

Type Ia supernovae (SNe Ia) are powered by the radioactive decay of isotopes such as Ni and Co, making their -ray spectra useful probes of the explosion mechanism…

astro-ph.SR2025

Introducing STARDIS: An Open and Modular Stellar Spectral Synthesis Code

Joshua V. Shields, Wolfgang Kerzendorf, Isaac G. Smith +7

We introduce a new 1D stellar spectral synthesis Python code called stardis. stardis is a modular, open-source radiative transfer code that is capable of spectral synthesis from ne…

astro-ph.SR2025

Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors

Aldana Grichener, Mathieu Renzo, Wolfgang E. Kerzendorf +7

One of the main challenges in modeling massive stars to the onset of core collapse is the computational bottleneck of nucleosynthesis during advanced burning stages. The number of…

astro-ph.HE2024

Physics-driven Explosions of Stripped High-Mass Stars: Synthetic Light Curves and Spectra of Stripped-Envelope Supernovae with Broad Lightcurves

Jing Lu, Brandon L. Barker, Jared Goldberg +5

Stripped-envelope supernovae (SESNe) represent a significant fraction of core-collapse supernovae, arising from massive stars that have shed their hydrogen and, in some cases, heli…

astro-ph.IM2024

Identifying Telescope Usage in Astrophysics Publications: A Machine Learning Framework for Institutional Research Management at Observatories

Vicente Amado Olivo, Wolfgang Kerzendorf, Brian Cherinka +3

Large scientific institutions, such as the Space Telescope Science Institute, track the usage of their facilities to understand the needs of the research community. Astrophysicists…

astro-ph.SR2024★ 9 cited

Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries

Aakash Bhat, Evan B. Bauer, Rüdiger Pakmor +5

Recent observations have found a growing number of hypervelocity stars with speeds of km\,s which could have only been produced through thermonuclear su…

astro-ph.SR2023★ 9 cited

Scalable stellar evolution forecasting: Deep learning emulation vs. hierarchical nearest neighbor interpolation

K. Maltsev, F. R. N. Schneider, F. K. Roepke +5

Many astrophysical applications require efficient yet reliable forecasts of stellar evolution tracks. One example is population synthesis, which generates forward predictions of mo…

astro-ph.IM2019

Astro2020 APC White Paper: Elevating the Role of Software as a Product of the Research Enterprise

Arfon M. Smith, Dara Norman, Kelle Cruz +42

Software is a critical part of modern research, and yet there are insufficient mechanisms in the scholarly ecosystem to acknowledge, cite, and measure the impact of research softwa…